M31 - Andromeda Galaxy · RGB Session 1 · 2026-10-16

Observing conditions

Saved context for this physical observing session. Separate time spans remain visible below.

RGB · 2026-10-16 19:53:16 CEST (UTC+0200) → 2026-10-16 21:07:28 CEST (UTC+0200)

Moon · calculated

32.5%

Illuminated · Waxing

Altitude 2.7°

Reference: 2026-10-16T18:30:22.601 UTC

Observing site

—

Location not recorded, or withheld in this read-only share.

Weather · model context

ECMWF IFS archive · Open-Meteo

Cloud cover
0.0–0.0 %
Dew point
2.4–3.8 °C
Relative humidity
52.0–54.0 %
Air temperature
11.3–13.1 °C
Wind at 10 m
1.6–2.4 m/s

Ranges of hourly model samples. Air temperature is not sensor temperature.

Hourly values and coverage
UTCAir temperature · °CRelative humidity · %Dew point · °CCloud cover · %Wind at 10 m · m/s
2026-10-16T17:00:00+00:0013.153.03.80.02.4
2026-10-16T18:00:00+00:0012.452.02.70.02.1
2026-10-16T19:00:00+00:0011.354.02.40.01.6

Hourly gridded model context, not measurements at the telescope. Hourly samples bounding this exposure-group interval; no minute interpolation.

Cloud cover: 3/3 samples; Dew point: 3/3 samples; Relative humidity: 3/3 samples; Air temperature: 3/3 samples; Wind at 10 m: 3/3 samples

Retrieved 2026-10-20T16:42:34.499914+00:00

Provider and model documentation
Context provenance and limits

Recorded DATE-OBS time interpretation retained; if TIMESYS is absent it is provisionally UTC.

Saved calculation at this exposure group's midpoint. Geometric altitude assumes sea level, no terrain or refraction. Schematic orientation, not a sky photograph.

Weather does not establish seeing, transparency at the telescope, a Bortle class or a photometric correction. Missing values do not imply clear skies.

Saved context SHA-256: 7f569a1027bf6b6140c93a0bb5c972913fa4f702e9b80d05de8aaaa0a058a91d

RGB · 2026-10-16 21:24:51 CEST (UTC+0200) → 2026-10-17 02:40:38 CEST (UTC+0200)

Moon · calculated

33.8%

Illuminated · Waxing

Altitude -25.7° · below the geometric horizon

Reference: 2026-10-16T22:02:45.140 UTC

Observing site

—

Location not recorded, or withheld in this read-only share.

Weather · model context

ECMWF IFS archive · Open-Meteo

Cloud cover
0.0–5.0 %
Dew point
1.8–2.4 °C
Relative humidity
54.0–63.0 %
Air temperature
8.4–11.3 °C
Wind at 10 m
0.6–1.6 m/s

Ranges of hourly model samples. Air temperature is not sensor temperature.

Hourly values and coverage
UTCAir temperature · °CRelative humidity · %Dew point · °CCloud cover · %Wind at 10 m · m/s
2026-10-16T19:00:00+00:0011.354.02.40.01.6
2026-10-16T20:00:00+00:0010.557.02.40.01.3
2026-10-16T21:00:00+00:009.959.02.35.01.2
2026-10-16T22:00:00+00:009.560.02.14.01.0
2026-10-16T23:00:00+00:009.362.02.40.00.6
2026-10-17T00:00:00+00:008.463.01.80.00.6

Hourly gridded model context, not measurements at the telescope. Hourly samples bounding this exposure-group interval; no minute interpolation.

Cloud cover: 6/6 samples; Dew point: 6/6 samples; Relative humidity: 6/6 samples; Air temperature: 6/6 samples; Wind at 10 m: 6/6 samples

Retrieved 2026-10-20T16:42:34.113337+00:00

Provider and model documentation
Context provenance and limits

Recorded DATE-OBS time interpretation retained; if TIMESYS is absent it is provisionally UTC.

Saved calculation at this exposure group's midpoint. Geometric altitude assumes sea level, no terrain or refraction. Schematic orientation, not a sky photograph.

Weather does not establish seeing, transparency at the telescope, a Bortle class or a photometric correction. Missing values do not imply clear skies.

Saved context SHA-256: 4f793ecf28409dec0da69e95c9c243e00c84d381bfef8dd01ba9bb29ab4e7d09

Separate exposure, camera-orientation or calibration groups within this observing session. Their images and measurements remain separate.

Group 1 · RGB · 300 s · 13 Lights

1 h 05 min · 13 exposures available.

Session
Preview image · up to 2560 px

Selected input exposures

Image quality at a glance

Selected inputs against your whole archive · RGB and DNB remain separate.

RGB · all contributing sessions

Star width / FWHM
2.71 sensor pixels
Current archive average3.00 sensor pixels
Difference -0.29
13/13 selected · archive 865/865 exposures · 11 sessions · 8 objects
Star shape / eccentricity
0.43 dimensionless
Current archive average0.45 dimensionless
Difference -0.02
13/13 selected · archive 865/865 exposures · 11 sessions · 8 objects
Background
1,091.85 ADU
Current archive average749.61 ADU
Difference +342.24
13/13 selected · archive 865/865 exposures · 11 sessions · 8 objects
Background scatter
68.59 ADU
Current archive average34.26 ADU
Difference +34.33
13/13 selected · archive 865/865 exposures · 11 sessions · 8 objects
Stellar model SNR
150.72 dimensionless
Current archive average138.73 dimensionless
Difference +11.99
13/13 selected · archive 865/865 exposures · 11 sessions · 8 objects
Stellar model estimate · different fields
Star width / FWHM
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Star shape / eccentricity
Star shape / eccentricity
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Background
Background
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Background scatter
Background scatter
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Stellar model SNR
Stellar model SNR
Selected exposure values · whole-archive RGB mean · physical sessions separated.
How this archive average is calculated

Each unique original exposure contributes once per valid saved metric. Arithmetic mean across all objects; RGB and DNB separate. Missing or invalid values are excluded, never zero. This descriptive reference includes the selected exposures and later nights.

Exposure, camera settings, field brightness, sampling and stellar populations may differ. Background and stellar model SNR are not normalized measures of sky quality, master SNR or detection sensitivity. A difference is not a grade.

Stored per-frame medians of stellar fits are averaged; stars are not pooled. SNR requires a positive recorded effective gain and at least five stellar estimates. Units remain separate. Unknown method versions are recorded, not invented. Small, undersampled stars may bias shape measurements.

Archive version ab3717b4ec376ea87d5261c94fe6dbbd42a97237e09422490b5844921d286006

Matched acquisition settings · original session-weighted comparison

Selected input exposures

Image quality at a glance

Measurements of the selected input exposures, not the finished master.

RGB · 300.0 s · 13 Lights

Acquisition settings & contributing sessions

300.0 s · Gain 100.0 · Archive snapshot 2026-11-09T03:24:34.927460+00:00

Recorded focal length: 611.0 mm · separate header/settings cohorts, not additional observing sessions.

Acquisition · 2026-10-16 · recorded DATE-OBS

Execution version was not saved: this comparison is limited to the same observing session.

Star width (FWHM)
2.71 sensor pixels
Current archive average2.71 sensor pixels
Difference 0.00 sensor pixels
13/13 frames · archive: 1 Sessions
Star shape
0.43 dimensionless
Current archive average0.43 dimensionless
Difference 0.00 dimensionless
13/13 frames · archive: 1 Sessions
Eccentricity of stellar model fits
Background
1,091.85 ADU
Current archive average1,091.85 ADU
Difference 0.00 ADU
13/13 frames · archive: 1 Sessions
Background scatter
68.59 ADU
Current archive average68.59 ADU
Difference 0.00 ADU
13/13 frames · archive: 1 Sessions
Stellar SNR
150.72 dimensionless
Current archive average150.72 dimensionless
Difference 0.00 dimensionless
13/13 frames · archive: 1 Sessions
Model estimate · same target field
Star width (FWHM) over time
Star width (FWHM) · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Star shape · Trend
Star shape over time
Star shape · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Background · Trend
Background over time
Background · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Background scatter · Trend
Background scatter over time
Background scatter · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Stellar SNR · Trend
Stellar SNR over time
Stellar SNR · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.

Provisional star fits · stellar SNR is a model estimate, not master SNR.

Reading these values

Provisional stellar models: undersampled stars can bias the measurements. Differences are not quality grades. Stellar SNR is not nebular or master-image SNR.

Processing and calibration record

Processing for this session

  1. Calibrationsuccess
  2. Registrationsuccess
  3. Stackingsuccess
  4. ReportSaved results

13/13 Lights calibrated; {'bias': 82, 'dark': 40, 'flat': 40} calibration frames. Unknown compatibility fields: device_id, filter, optical_configuration, physical_camera_to_optics_orientation, readout_mode.

Calibration and processing evidence
{
  "calibrated": 13,
  "calibration_state": "success",
  "crop": {
    "area_fraction": 0.9828110512605414
  },
  "integration_s": 3900.0,
  "planned": 13,
  "ready": 13,
  "registered": 13,
  "registration_state": "success",
  "selected_calibrations": {
    "bias": 82,
    "dark": 40,
    "flat": 40
  },
  "stacked": 13,
  "stacking_state": "success",
  "unknown_fields": [
    "device_id",
    "filter",
    "optical_configuration",
    "physical_camera_to_optics_orientation",
    "readout_mode"
  ],
  "warnings": [
    "Bias is used for flat correction only; exposure/linearity suitability remains unvalidated",
    "Flat exposure is not matched to light exposure; flat dark current, illumination and physical optical-state continuity remain unvalidated",
    "Physical camera-to-optics orientation unknown; no fabricated match and no angle-only veto.",
    "Raw ROTATOR/angle semantics are unverified; differences are not evidence of physical rotation.",
    "Short-Flat/Light temperature tolerance: +/-2 C; Dark and Bias tolerances unchanged. Flat diagnostics and optical-history approval remain required.",
    "device_id: compatibility unknown; permitted only by explicit warning policy",
    "filter: compatibility unknown; permitted only by explicit warning policy",
    "optical_configuration: compatibility unknown; permitted only by explicit warning policy",
    "readout_mode: compatibility unknown; permitted only by explicit warning policy"
  ]
}

Explore stars in the image

Verified image · RGB · 2026-10-16

571 verified identities; 12 spatially distributed highlights. Query: G < 16, at most 5000 sources; fainter neighbours may be absent.

Farb-Helligkeits-Diagramm · Gaia G / BP−RP

Scheinbare Kataloghelligkeit, kein HR-Diagramm; Staub und Distance wirken mit.

G (mag)BP−RP (mag)
Identity, data and limitations

Holdout residual: median 0.6443380545539815 px; 95 % 1.5874343915070486 px. G<16; fainter neighbours may be absent. Historical solver training set is unknown.

Temperature, mass and radius are catalogue model estimates, not stellar parameters measured from this photograph.

Exact catalogue values and geometry

Science & measurements

Experimental photometry · no confirmed transit. 1 unresolved technical review items.

Histograms, light curves & event evidence

Intensity histograms

RGB · 13/13 original exposures measured.

RGB · Raw pixel values

ADU · decoded digital value · Pixel count per bin; not a wavelength spectrum.

-0.56.554e+047.574e+07BG1G2R

All saved bins, including negative values.

Exact counts and measured valuesWerte und Darstellungsbins · Complete unchanged bins (NPZ)

Histogram of this display product is unavailable.

Events · technical review

Searched · technical review pending

1 unresolved technical review items · 16 Gaia IDs searched · 96 tested windows. Windows are not independent events.

No confirmed transit. Short artifact clusters and time-correlated errors can pass this screening. Real periodic search: insufficient coverage; no globally calibrated false-alarm probability is available.

Saved event evidenceTest windows, supporting exposures and limitations

Gaia 375307715639087616 · 19.74 % relative depth · 15 min · cause unresolved.

Photometry precision and sampling · experimental

Photometry & transit readiness

Individual native exposures, independent of the final display/HDR image. Conditional measurement errors include the comparison ensemble; shared systematics remain outside that model.

M31 — Andromeda Galaxy · RGB · 300 s · 13 frames

measured diagnostics · 13 timed frames; 0 timing exclusions.

Separate segment 9c342b8e: 1.24 h span · 303.3 s median cadence · 87.6% exposure duty · 1 large gap(s); 0 overlapping recorded intervals (bins unavailable when present).

0.6181.3762.1332.890Robust scatter (%)12.713.3Gaia G magnitude (catalogue)

Brightness comparison is observational: sources share sky and calibration; points are not independent trials.

Gaia 381203189614455680 · G 12.69

13/13 valid epochs · robust scatter 0.90% · median conditional error 0.88%. single-event diagnostics only.

0.9560.9821.0081.035Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.62% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.81% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.32% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381184944593395968 · G 12.89

13/13 valid epochs · robust scatter 1.06% · median conditional error 0.95%. single-event diagnostics only.

0.9660.9871.0081.029Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.46% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.88% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.76% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381135986260425984 · G 13.02

13/13 valid epochs · robust scatter 2.73% · median conditional error 1.42%. single-event diagnostics only.

0.9420.9831.0231.063Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 3.44% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 2.33% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.17% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381214498262497920 · G 13.05

13/13 valid epochs · robust scatter 0.82% · median conditional error 1.12%. single-event diagnostics only.

0.9410.9721.0041.035Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.82% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.60% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 1.06% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381141758696449280 · G 13.07

13/13 valid epochs · robust scatter 1.68% · median conditional error 0.89%. single-event diagnostics only.

0.9610.9901.0201.049Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.68% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 1.64% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 1.39% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 369243256178304128 · G 13.09

13/13 valid epochs · robust scatter 0.84% · median conditional error 0.88%. single-event diagnostics only.

0.9680.9901.0111.033Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.00% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 1.17% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.14% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381183333980030336 · G 13.14

13/13 valid epochs · robust scatter 1.53% · median conditional error 1.37%. single-event diagnostics only.

0.9200.9731.0261.079Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 3.42% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 1.11% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 3.28% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 369147255067950720 · G 13.16

13/13 valid epochs · robust scatter 0.77% · median conditional error 0.98%. single-event diagnostics only.

0.9600.9901.0201.050Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.97% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 1.27% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 1.51% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 369222193658888320 · G 13.16

13/13 valid epochs · robust scatter 1.21% · median conditional error 0.98%. single-event diagnostics only.

0.9660.9911.0161.041Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.56% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.29% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.78% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 369127395139218560 · G 13.18

13/13 valid epochs · robust scatter 1.08% · median conditional error 1.38%. single-event diagnostics only.

0.9610.9911.0201.050Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.08% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.36% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.04% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 375307715639087616 · G 13.24

13/13 valid epochs · robust scatter 1.08% · median conditional error 1.02%. single-event diagnostics only.

0.7100.8360.9611.087Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.68% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 1.80% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 10.32% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 369291256732926336 · G 13.25

13/13 valid epochs · robust scatter 1.14% · median conditional error 1.17%. single-event diagnostics only.

0.9690.9941.0181.043Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.25% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.50% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.46% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381152272776336640 · G 13.26

13/13 valid epochs · robust scatter 0.86% · median conditional error 1.09%. single-event diagnostics only.

0.9790.9961.0131.030Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.33% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.27% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 0.75% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381165810513518720 · G 13.28

13/13 valid epochs · robust scatter 1.55% · median conditional error 1.09%. single-event diagnostics only.

0.9670.9901.0121.034Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.68% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.95% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 1.25% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 381173472735157120 · G 13.28

13/13 valid epochs · robust scatter 1.47% · median conditional error 1.17%. single-event diagnostics only.

0.9670.9921.0171.042Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 2.68% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 0.87% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 1.32% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.
Gaia 369252739466052352 · G 13.30

13/13 valid epochs · robust scatter 0.78% · median conditional error 1.27%. single-event diagnostics only.

0.9570.9901.0231.056Raw / own medianReference ensembleDifferential2.571.7Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.00% · 1 usable bins · 12 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 100–100% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.47% · 5 usable bins · 7 native points outside this binned view · descriptive only; 1–1 exposures/bin, 300–300 s integrated, 50–50% coverage. Single-frame bins do not demonstrate averaging.
  • 15 min: 1.23% · 4 usable bins · 4 native points outside this binned view · descriptive only; 1–2 exposures/bin, 300–600 s integrated, 33–67% coverage.
  • 30 min: 1.53% · 2 usable bins · 2 native points outside this binned view · descriptive only; 1–5 exposures/bin, 300–1500 s integrated, 17–83% coverage.

Recommended next acquisition: characterize unsaturated stars with matched short-exposure Darks and same-session Flats, then keep one exposure/filter configuration through a dedicated known-host event and its before/after baseline. There is no real 60/120 s improvement demonstrated here.

Timing, uncertainty and applicability
  • Not calibrated standard magnitudes. Native G1+G2 response/Flat/pixel-phase and shared errors remain unbounded.
  • Recorded header start times support relative intervals; TIMESYS and clock accuracy are not established. No BJD_TDB.
  • References exclude each target but share sky/calibration systematics. Conditional errors hold median normalizations fixed.
  • No new search is run here. Existing event evidence and eligibility are retained; review scores are not calibrated false-alarm probabilities.
  • No new aperture is promoted. Mixed exposures, passbands, nights and calibration/angle segments stay separate.
Exact native-photometry diagnosticsConditional errors, rates, source/reference IDs and precision support
Comparison-star evidence · experimental

Comparison-star robustness check

Could a more robust reference ensemble improve these light curves? This controlled experiment reuses the original native fluxes. Your published scientific curves and event results remain unchanged.

RGB · 300.0 s · 0 supported source/segment tests

Insufficient contiguous data or independent references for the blocked comparison.

2 contiguous blocks are too short; no test is forced across the gap.

Scientific baseline retained. No promotion from scatter alone; independent control observations and a calibrated uncertainty model are still required.

Validation design and limits

Four contiguous held-out folds per sufficiently long uninterrupted block, with one purged epoch on each side. Reference medians are learned only from training epochs; each target is excluded from its references. Fixed Huber cutoff 1.5, at least six references. No hyperparameter search or target-based refitting.

  • Blocked epoch checks within existing calibration/orientation segments, not independent new-night validation.
  • Stars share references and are not independent trials; no p-values or discovery probability are inferred.
  • Lower scatter may remove reference contamination but does not prove better physical accuracy.
  • Existing shared-master, flat, centroid, sampling and clock uncertainties remain unresolved.
  • Artificial dimming checks algebraic signal transfer only, not transit detection or recovery efficiency.
  • No re-fitting, smoothing or interpolation of target flux; gaps and unavailable measurements remain gaps.
Reference comparison evidenceHeld-out folds, reference membership, unchanged baseline and signal-transfer checks

Example measured light curve

2026-10-16 · RGB · Gaia 369127395139218560. First available session and source ID; not selected for apparent variability.

Relative brightness1.0290.98070.04 — 1.20 hours since the first recorded header start · exposure midpoints
Native G1+G2 measurements · separate calibration segments · no connecting lines.
All saved stellar light curves
Appendix · measurement methods & observing conditions
Observing nights and Moon

RGB

2026-10-16 19:53:16 CEST (UTC+0200) → 2026-10-16 21:07:28 CEST (UTC+0200)

32.5% Moon illumination · saved calculation

Altitude 2.7°Target separation —

Mitte des Aufnahmezeitraums

Original saved observation note

Time assumption: DATE-OBS interpreted as UTC because TIMESYS is missing. Astronomical context is provisional.

Original saved observation note

Moon altitude is approximate; local Earth-orientation data may be incomplete.

Original saved observation note

Geometric Moon altitude, without terrain or refraction; site elevation assumed to be 0 m.

Saved time assumptions are unchanged. Site and weather are shown on the session pages.

Explain this comparison

Comparison with your current archive: each physical observing session has equal weight. Valid per-exposure values are first averaged within each session, then the session means are averaged. Later sessions and the exposures shown here may be included. This is neither an independent test nor a formal quality grade.

Selected data use the exact input IDs of this product. RGB and DNB, methods, units, sampling and recorded acquisition settings remain separate. Unknown setup metadata do not establish physical compatibility. A few sessions form only a small descriptive reference. Missing values do not count as zero.

FWHM and star shape are saved medians of the stellar fits in each exposure; the display averages these per-exposure values. Stellar SNR is the saved median of model estimates from at least five stars per exposure. Model: source Poisson noise, background variance and uncertainty in the mean local sky. Circular aperture radius 3, sky annulus 5–7 sampling pixels, 3σ clipping. EGAIN in electrons/ADU is required. Different star selections remain a limitation even within the same field.

Background and scatter are raw green-grid ADU under compatible acquisition conditions. Field emission, gradients and stellar populations limit comparison. These are not measurements of pure seeing, nebular SNR or transit sensitivity. The previous grading rule requiring eight other nights has not changed.

RGB · Stellar SNR: 13/13 valid selected exposures; archive 13/13 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Star width (FWHM): 13/13 valid selected exposures; archive 13/13 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Background: 13/13 valid selected exposures; archive 13/13 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Star shape: 13/13 valid selected exposures; archive 13/13 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Background scatter: 13/13 valid selected exposures; archive 13/13 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

Archive version ab3717b4ec376ea87d5261c94fe6dbbd42a97237e09422490b5844921d286006. This export is a frozen snapshot; it does not update without a new export.

All measurements and frozen archive comparison

Individual-frame quality review · advisory

Image-quality assistant

2 selected frames worth reviewing · 13/13 inputs have enough same-session support. All frames remain selected exactly as before.

Separate raw measurements, compared with the median of the same session and recorded setup. No overall score, automatic rejection or diagnosis.

Review suggestions · 2 frames
Saved header time / input IDMeasurementThis frameSession medianWhy review?
2026-10-16T17:53:16.269942
c725d667acb2
Stellar SNR estimate105.5 dimensionless155.7Lower model SNR in the sampled stars; changing star selection may contribute.
2026-10-16T18:44:21.218131
519598cde10c
Star eccentricity0.537 dimensionless0.413More elongated than this session; inspect tracking and field position. This is not a guiding measurement.
2026-10-16T18:44:21.218131
519598cde10c
Star width (FWHM)2.904 sensor pixels2.679Broader than this session; inspect focus, tracking and sampling. The cause is not identified.
Method, coverage and limitations

Review distance = (value − session median) / (1.4826 × MAD). The threshold 3.5 is an advisory rule, not statistical significance. At least 12 valid frames and 75% coverage are required; zero MAD is unavailable. SNR requires the existing gain and star-count checks. Background changes are flagged in either direction.

Shared tracking/focus problems can affect an entire night without producing an outlier. No independent validation labels exist yet. Raw-green sampling and changing star populations limit interpretation. RGB/DNB, exposure, method and recorded orientation remain separate; unknown metadata do not establish compatibility.

RGB · 300.0 s · session acq_6c03bd1f: Background level 13/13; Background scatter 13/13; Detected sources 0/13: too few valid session frames; Star eccentricity 13/13; Star width (FWHM) 13/13; Stellar SNR estimate 13/13. Unknown: device_id, filter, optical_configuration, readout_mode, recorded_orientation_deg.

Method session-quality-assistant-1. Saved measurements and existing archive comparisons are unchanged.

Group 2 · RGB · 180 s · 88 Lights

4 h 24 min · 89 exposures available.

Session
Preview image · up to 2560 px

Selected input exposures

Image quality at a glance

Selected inputs against your whole archive · RGB and DNB remain separate.

RGB · all contributing sessions

Star width / FWHM
2.74 sensor pixels
Current archive average3.00 sensor pixels
Difference -0.26
88/88 selected · archive 865/865 exposures · 11 sessions · 8 objects
Star shape / eccentricity
0.50 dimensionless
Current archive average0.45 dimensionless
Difference +0.05
88/88 selected · archive 865/865 exposures · 11 sessions · 8 objects
Background
734.02 ADU
Current archive average749.61 ADU
Difference -15.59
88/88 selected · archive 865/865 exposures · 11 sessions · 8 objects
Background scatter
43.22 ADU
Current archive average34.26 ADU
Difference +8.96
88/88 selected · archive 865/865 exposures · 11 sessions · 8 objects
Stellar model SNR
130.60 dimensionless
Current archive average138.73 dimensionless
Difference -8.14
88/88 selected · archive 865/865 exposures · 11 sessions · 8 objects
Stellar model estimate · different fields
Star width / FWHM
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Star shape / eccentricity
Star shape / eccentricity
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Background
Background
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Background scatter
Background scatter
Selected exposure values · whole-archive RGB mean · physical sessions separated.
Stellar model SNR
Stellar model SNR
Selected exposure values · whole-archive RGB mean · physical sessions separated.
How this archive average is calculated

Each unique original exposure contributes once per valid saved metric. Arithmetic mean across all objects; RGB and DNB separate. Missing or invalid values are excluded, never zero. This descriptive reference includes the selected exposures and later nights.

Exposure, camera settings, field brightness, sampling and stellar populations may differ. Background and stellar model SNR are not normalized measures of sky quality, master SNR or detection sensitivity. A difference is not a grade.

Stored per-frame medians of stellar fits are averaged; stars are not pooled. SNR requires a positive recorded effective gain and at least five stellar estimates. Units remain separate. Unknown method versions are recorded, not invented. Small, undersampled stars may bias shape measurements.

Archive version ab3717b4ec376ea87d5261c94fe6dbbd42a97237e09422490b5844921d286006

Matched acquisition settings · original session-weighted comparison

Selected input exposures

Image quality at a glance

Measurements of the selected input exposures, not the finished master.

RGB · 180.0 s · 88 Lights

Acquisition settings & contributing sessions

180.0 s · Gain 100.0 · Archive snapshot 2026-11-09T03:24:34.927460+00:00

Recorded focal length: 611.0 mm · separate header/settings cohorts, not additional observing sessions.

Acquisition · 2026-10-16–2026-10-17 · recorded DATE-OBS

Execution version was not saved: this comparison is limited to the same observing session.

Star width (FWHM)
2.74 sensor pixels
Current archive average2.75 sensor pixels
Difference -0.02 sensor pixels
88/88 frames · archive: 1 Sessions
Star shape
0.50 dimensionless
Current archive average0.51 dimensionless
Difference -0.00 dimensionless
88/88 frames · archive: 1 Sessions
Eccentricity of stellar model fits
Background
734.02 ADU
Current archive average733.80 ADU
Difference +0.22 ADU
88/88 frames · archive: 1 Sessions
Background scatter
43.22 ADU
Current archive average43.21 ADU
Difference +0.01 ADU
88/88 frames · archive: 1 Sessions
Stellar SNR
130.60 dimensionless
Current archive average130.10 dimensionless
Difference +0.50 dimensionless
88/88 frames · archive: 1 Sessions
Model estimate · same target field
Star width (FWHM) over time
Star width (FWHM) · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Star shape · Trend
Star shape over time
Star shape · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Background · Trend
Background over time
Background · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Background scatter · Trend
Background scatter over time
Background scatter · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.
Stellar SNR · Trend
Stellar SNR over time
Stellar SNR · saved per-exposure values and current archive average. Sessions are separate; gaps are not joined.

Provisional star fits · stellar SNR is a model estimate, not master SNR.

Reading these values

Provisional stellar models: undersampled stars can bias the measurements. Differences are not quality grades. Stellar SNR is not nebular or master-image SNR.

Processing and calibration record

Processing for this session

  1. Calibrationsuccess
  2. Registrationsuccess
  3. Stackingsuccess
  4. ReportSaved results

89/89 Lights calibrated; {'bias': 82, 'dark': 58, 'flat': 40} calibration frames. Unknown compatibility fields: device_id, filter, optical_configuration, physical_camera_to_optics_orientation, readout_mode.

Calibration and processing evidence
{
  "calibrated": 89,
  "calibration_state": "success",
  "crop": {
    "area_fraction": 0.9347634921335747
  },
  "integration_s": 15840.0,
  "planned": 89,
  "ready": 89,
  "registered": 88,
  "registration_state": "success",
  "selected_calibrations": {
    "bias": 82,
    "dark": 58,
    "flat": 40
  },
  "stacked": 88,
  "stacking_state": "success",
  "unknown_fields": [
    "device_id",
    "filter",
    "optical_configuration",
    "physical_camera_to_optics_orientation",
    "readout_mode"
  ],
  "warnings": [
    "Bias is used for flat correction only; exposure/linearity suitability remains unvalidated",
    "Flat exposure is not matched to light exposure; flat dark current, illumination and physical optical-state continuity remain unvalidated",
    "Physical camera-to-optics orientation unknown; no fabricated match and no angle-only veto.",
    "Raw ROTATOR/angle semantics are unverified; differences are not evidence of physical rotation.",
    "Short-Flat/Light temperature tolerance: +/-2 C; Dark and Bias tolerances unchanged. Flat diagnostics and optical-history approval remain required.",
    "device_id: compatibility unknown; permitted only by explicit warning policy",
    "filter: compatibility unknown; permitted only by explicit warning policy",
    "optical_configuration: compatibility unknown; permitted only by explicit warning policy",
    "readout_mode: compatibility unknown; permitted only by explicit warning policy"
  ]
}

Explore stars in the image

Verified image · RGB · 2026-10-16

573 verified identities; 12 spatially distributed highlights. Query: G < 16, at most 5000 sources; fainter neighbours may be absent.

Farb-Helligkeits-Diagramm · Gaia G / BP−RP

Scheinbare Kataloghelligkeit, kein HR-Diagramm; Staub und Distance wirken mit.

G (mag)BP−RP (mag)
Identity, data and limitations

Holdout residual: median 0.5632635246806421 px; 95 % 1.219086762916769 px. G<16; fainter neighbours may be absent. Historical solver training set is unknown.

Temperature, mass and radius are catalogue model estimates, not stellar parameters measured from this photograph.

Exact catalogue values and geometry

Science & measurements

Experimental photometry · no confirmed transit. 2 unresolved technical review items.

Histograms, light curves & event evidence

Intensity histograms

RGB · 88/88 original exposures measured.

RGB · Raw pixel values

ADU · decoded digital value · Pixel count per bin; not a wavelength spectrum.

-0.56.554e+045.607e+08BG1G2R

All saved bins, including negative values.

Exact counts and measured valuesWerte und Darstellungsbins · Complete unchanged bins (NPZ)

Histogram of this display product is unavailable.

Events · technical review

Searched · technical review pending

2 unresolved technical review items · 16 Gaia IDs searched · 2640 tested windows. Windows are not independent events.

No confirmed transit. Short artifact clusters and time-correlated errors can pass this screening. Real periodic search: insufficient coverage; no globally calibrated false-alarm probability is available.

Saved event evidenceTest windows, supporting exposures and limitations

Gaia 369193980014906752 · 15.02 % relative depth · 15 min · cause unresolved.

Gaia 369222193658888320 · 9.72 % relative depth · 15 min · cause unresolved.

Photometry precision and sampling · experimental

Photometry & transit readiness

Individual native exposures, independent of the final display/HDR image. Conditional measurement errors include the comparison ensemble; shared systematics remain outside that model.

M31 — Andromeda Galaxy · RGB · 180 s · 88 frames

measured diagnostics · 88 timed frames; 0 timing exclusions.

Separate segment 56de51e2: 2.41 h span · 183.3 s median cadence · 89.2% exposure duty · 2 large gap(s); 0 overlapping recorded intervals (bins unavailable when present).

Separate segment 54571c9d: 2.55 h span · 183.5 s median cadence · 88.2% exposure duty · 3 large gap(s); 0 overlapping recorded intervals (bins unavailable when present).

1.0251.5652.1062.646Robust scatter (%)13.013.3Gaia G magnitude (catalogue)

Brightness comparison is observational: sources share sky and calibration; points are not independent trials.

Gaia 369284419145014528 · G 12.95

43/43 valid epochs · robust scatter 1.64% · median conditional error 1.12%. single-event diagnostics only.

0.9540.9911.0291.066Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.89% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.39% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.29% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 2.01% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 381169005969155584 · G 13.07

43/43 valid epochs · robust scatter 1.87% · median conditional error 1.45%. single-event diagnostics only.

0.8880.9481.0071.067Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.20% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.14% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.43% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 1.16% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 381191580317044992 · G 13.13

43/43 valid epochs · robust scatter 1.44% · median conditional error 1.02%. single-event diagnostics only.

0.9610.9881.0151.042Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.20% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.57% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.72% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.97% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 381183333980030336 · G 13.14

43/43 valid epochs · robust scatter 1.82% · median conditional error 1.58%. single-event diagnostics only.

0.9340.9791.0241.069Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.34% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.83% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.21% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.60% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 369222193658888320 · G 13.16

43/43 valid epochs · robust scatter 1.53% · median conditional error 1.16%. single-event diagnostics only.

0.9630.9951.0271.059Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.57% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.57% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.02% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.33% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 369152439091358592 · G 13.17

43/43 valid epochs · robust scatter 1.45% · median conditional error 1.17%. single-event diagnostics only.

0.9440.9841.0231.062Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.93% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.20% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.86% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.76% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 387312802066050432 · G 13.19

43/43 valid epochs · robust scatter 1.14% · median conditional error 1.20%. single-event diagnostics only.

0.9600.9881.0151.042Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.33% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.23% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.97% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.62% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 375287340314289664 · G 13.23

43/43 valid epochs · robust scatter 1.28% · median conditional error 1.12%. single-event diagnostics only.

0.9540.9871.0201.053Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.95% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.58% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.63% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.72% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 369291256732926336 · G 13.25

43/43 valid epochs · robust scatter 1.53% · median conditional error 1.34%. single-event diagnostics only.

0.9520.9881.0251.061Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.29% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.85% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.98% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.16% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 375237037657363456 · G 13.27

43/43 valid epochs · robust scatter 1.54% · median conditional error 1.13%. single-event diagnostics only.

0.9560.9871.0171.048Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 0.84% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.00% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.17% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.53% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 381173472735157120 · G 13.28

43/43 valid epochs · robust scatter 1.32% · median conditional error 1.36%. single-event diagnostics only.

0.9510.9851.0191.053Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.25% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.47% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.90% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.30% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 369252739466052352 · G 13.30

43/43 valid epochs · robust scatter 1.78% · median conditional error 1.52%. single-event diagnostics only.

0.9460.9861.0271.067Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.93% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.90% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.16% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.15% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 381278201223285120 · G 13.30

43/43 valid epochs · robust scatter 2.20% · median conditional error 1.29%. single-event diagnostics only.

0.9260.9691.0121.055Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.72% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.13% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.45% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.38% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 375224187115252736 · G 13.31

43/43 valid epochs · robust scatter 1.60% · median conditional error 1.19%. single-event diagnostics only.

0.9500.9861.0231.060Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.36% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.50% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.38% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 1.29% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 369193980014906752 · G 13.32

43/43 valid epochs · robust scatter 1.65% · median conditional error 1.15%. single-event diagnostics only.

0.7350.8430.9511.058Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.79% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.23% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.83% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 0.39% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 381224084629507328 · G 13.32

43/43 valid epochs · robust scatter 2.09% · median conditional error 1.46%. single-event diagnostics only.

0.9260.9711.0161.061Raw / own medianReference ensembleDifferential1.5143.1Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.14% · 18 usable bins · 25 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 2.82% · 13 usable bins · 12 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.17% · 8 usable bins · 8 native points outside this binned view · descriptive only; 2–4 exposures/bin, 360–720 s integrated, 40–80% coverage.
  • 30 min: 1.22% · 5 usable bins · 3 native points outside this binned view · descriptive only; 6–9 exposures/bin, 1080–1620 s integrated, 60–90% coverage.
Gaia 369284419145014528 · G 12.95

45/45 valid epochs · robust scatter 1.91% · median conditional error 1.10%. single-event diagnostics only.

0.9440.9841.0231.062Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.09% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.58% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.70% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.85% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 381169005969155584 · G 13.07

45/45 valid epochs · robust scatter 2.53% · median conditional error 1.38%. single-event diagnostics only.

0.9250.9701.0161.061Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.71% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 2.14% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.93% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.32% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 381191580317044992 · G 13.13

45/45 valid epochs · robust scatter 1.35% · median conditional error 0.98%. single-event diagnostics only.

0.9380.9801.0231.066Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.32% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.40% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.49% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.93% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 381183333980030336 · G 13.14

45/45 valid epochs · robust scatter 2.14% · median conditional error 1.52%. single-event diagnostics only.

0.9360.9841.0311.078Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.95% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.10% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.30% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.60% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 369222193658888320 · G 13.16

45/45 valid epochs · robust scatter 1.89% · median conditional error 1.10%. single-event diagnostics only.

0.8030.8990.9951.091Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.59% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 2.31% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 2.38% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.69% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 369152439091358592 · G 13.17

45/45 valid epochs · robust scatter 1.81% · median conditional error 1.13%. single-event diagnostics only.

0.9430.9811.0191.057Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.55% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.60% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.57% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 1.28% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 387312802066050432 · G 13.19

45/45 valid epochs · robust scatter 2.12% · median conditional error 1.16%. single-event diagnostics only.

0.9460.9841.0231.061Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.58% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.53% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.72% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 1.02% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 375287340314289664 · G 13.23

45/45 valid epochs · robust scatter 2.09% · median conditional error 1.08%. single-event diagnostics only.

0.9390.9781.0171.056Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 3.02% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.33% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 2.17% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.55% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 369291256732926336 · G 13.25

45/45 valid epochs · robust scatter 1.58% · median conditional error 1.31%. single-event diagnostics only.

0.9450.9871.0281.070Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.67% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.81% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.50% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 1.14% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 375237037657363456 · G 13.27

45/45 valid epochs · robust scatter 1.73% · median conditional error 1.10%. single-event diagnostics only.

0.9440.9781.0131.047Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.49% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.70% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.61% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.35% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 381173472735157120 · G 13.28

45/45 valid epochs · robust scatter 1.89% · median conditional error 1.31%. single-event diagnostics only.

0.9280.9741.0191.065Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.46% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.50% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.08% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.97% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 369252739466052352 · G 13.30

45/45 valid epochs · robust scatter 1.98% · median conditional error 1.45%. single-event diagnostics only.

0.9330.9771.0201.064Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.56% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 0.80% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.65% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.25% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 381278201223285120 · G 13.30

45/45 valid epochs · robust scatter 2.32% · median conditional error 1.25%. single-event diagnostics only.

0.9460.9921.0391.085Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.57% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 2.51% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.59% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.77% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 375224187115252736 · G 13.31

45/45 valid epochs · robust scatter 1.43% · median conditional error 1.16%. single-event diagnostics only.

0.9490.9841.0181.053Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 1.34% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.16% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 0.82% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.73% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 369193980014906752 · G 13.32

45/45 valid epochs · robust scatter 1.32% · median conditional error 1.11%. single-event diagnostics only.

0.9070.9671.0281.088Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.40% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.04% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.48% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 0.07% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.
Gaia 381224084629507328 · G 13.32

45/45 valid epochs · robust scatter 2.44% · median conditional error 1.40%. single-event diagnostics only.

0.9220.9711.0201.069Raw / own medianReference ensembleDifferential164.2314.3Minutes from recorded relative session origin
Precision at common wall-clock intervals

1.4826 × median absolute deviation divided by median. Nonoverlapping bins never split an exposure; boundary crossings remain in the native curve. Sparse bins do not establish a precision improvement.

  • 5 min: 2.20% · 19 usable bins · 26 native points outside this binned view · descriptive only; 1–1 exposures/bin, 180–180 s integrated, 60–60% coverage. Single-frame bins do not demonstrate averaging.
  • 10 min: 1.90% · 12 usable bins · 14 native points outside this binned view · conditional block interval; 1–3 exposures/bin, 180–540 s integrated, 30–90% coverage.
  • 15 min: 1.75% · 10 usable bins · 8 native points outside this binned view · descriptive only; 1–4 exposures/bin, 180–720 s integrated, 20–80% coverage.
  • 30 min: 1.19% · 5 usable bins · 4 native points outside this binned view · descriptive only; 1–9 exposures/bin, 180–1620 s integrated, 10–90% coverage.

Recommended next acquisition: characterize unsaturated stars with matched short-exposure Darks and same-session Flats, then keep one exposure/filter configuration through a dedicated known-host event and its before/after baseline. There is no real 60/120 s improvement demonstrated here.

Timing, uncertainty and applicability
  • Not calibrated standard magnitudes. Native G1+G2 response/Flat/pixel-phase and shared errors remain unbounded.
  • Recorded header start times support relative intervals; TIMESYS and clock accuracy are not established. No BJD_TDB.
  • References exclude each target but share sky/calibration systematics. Conditional errors hold median normalizations fixed.
  • No new search is run here. Existing event evidence and eligibility are retained; review scores are not calibrated false-alarm probabilities.
  • No new aperture is promoted. Mixed exposures, passbands, nights and calibration/angle segments stay separate.
Exact native-photometry diagnosticsConditional errors, rates, source/reference IDs and precision support
Comparison-star evidence · experimental

Comparison-star robustness check

Could a more robust reference ensemble improve these light curves? This controlled experiment reuses the original native fluxes. Your published scientific curves and event results remain unchanged.

RGB · 180.0 s · 0 supported source/segment tests

Insufficient contiguous data or independent references for the blocked comparison.

4 contiguous blocks are too short; no test is forced across the gap.

3 contiguous blocks are too short; no test is forced across the gap.

Scientific baseline retained. No promotion from scatter alone; independent control observations and a calibrated uncertainty model are still required.

Validation design and limits

Four contiguous held-out folds per sufficiently long uninterrupted block, with one purged epoch on each side. Reference medians are learned only from training epochs; each target is excluded from its references. Fixed Huber cutoff 1.5, at least six references. No hyperparameter search or target-based refitting.

  • Blocked epoch checks within existing calibration/orientation segments, not independent new-night validation.
  • Stars share references and are not independent trials; no p-values or discovery probability are inferred.
  • Lower scatter may remove reference contamination but does not prove better physical accuracy.
  • Existing shared-master, flat, centroid, sampling and clock uncertainties remain unresolved.
  • Artificial dimming checks algebraic signal transfer only, not transit detection or recovery efficiency.
  • No re-fitting, smoothing or interpolation of target flux; gaps and unavailable measurements remain gaps.
Reference comparison evidenceHeld-out folds, reference membership, unchanged baseline and signal-transfer checks

Example measured light curve

2026-10-16 · RGB · Gaia 369152439091358592. First available session and source ID; not selected for apparent variability.

Relative brightness1.0420.96420.03 — 2.39 hours since the first recorded header start · exposure midpoints
Native G1+G2 measurements · separate calibration segments · no connecting lines.
All saved stellar light curves
Appendix · measurement methods & observing conditions
Observing nights and Moon

RGB

2026-10-16 21:24:51 CEST (UTC+0200) → 2026-10-17 02:40:38 CEST (UTC+0200)

33.8% Moon illumination · saved calculation

Altitude -25.7°Target separation —

Mitte des Aufnahmezeitraums

Original saved observation note

Time assumption: DATE-OBS interpreted as UTC because TIMESYS is missing. Astronomical context is provisional.

Original saved observation note

Moon altitude is approximate; local Earth-orientation data may be incomplete.

Original saved observation note

Geometric Moon altitude, without terrain or refraction; site elevation assumed to be 0 m.

Saved time assumptions are unchanged. Site and weather are shown on the session pages.

Explain this comparison

Comparison with your current archive: each physical observing session has equal weight. Valid per-exposure values are first averaged within each session, then the session means are averaged. Later sessions and the exposures shown here may be included. This is neither an independent test nor a formal quality grade.

Selected data use the exact input IDs of this product. RGB and DNB, methods, units, sampling and recorded acquisition settings remain separate. Unknown setup metadata do not establish physical compatibility. A few sessions form only a small descriptive reference. Missing values do not count as zero.

FWHM and star shape are saved medians of the stellar fits in each exposure; the display averages these per-exposure values. Stellar SNR is the saved median of model estimates from at least five stars per exposure. Model: source Poisson noise, background variance and uncertainty in the mean local sky. Circular aperture radius 3, sky annulus 5–7 sampling pixels, 3σ clipping. EGAIN in electrons/ADU is required. Different star selections remain a limitation even within the same field.

Background and scatter are raw green-grid ADU under compatible acquisition conditions. Field emission, gradients and stellar populations limit comparison. These are not measurements of pure seeing, nebular SNR or transit sensitivity. The previous grading rule requiring eight other nights has not changed.

RGB · Star width (FWHM): 88/88 valid selected exposures; archive 89/89 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Background: 88/88 valid selected exposures; archive 89/89 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Background scatter: 88/88 valid selected exposures; archive 89/89 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Stellar SNR: 88/88 valid selected exposures; archive 89/89 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

RGB · Star shape: 88/88 valid selected exposures; archive 89/89 frames, 1 Sessions. Unknown properties: device_id, readout_mode, optical_configuration, filter, execution_method_version.

Archive version ab3717b4ec376ea87d5261c94fe6dbbd42a97237e09422490b5844921d286006. This export is a frozen snapshot; it does not update without a new export.

All measurements and frozen archive comparison

Individual-frame quality review · advisory

Image-quality assistant

28 selected frames worth reviewing · 88/88 inputs have enough same-session support. All frames remain selected exactly as before.

Separate raw measurements, compared with the median of the same session and recorded setup. No overall score, automatic rejection or diagnosis.

Review suggestions · 28 frames
Saved header time / input IDMeasurementThis frameSession medianWhy review?
2026-10-16T19:24:51.569094
6d575c5dce22
Background level791 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:27:54.910793
ed759b7c94ab
Background level789 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:30:58.151772
1bcc75be3625
Background level785 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:34:12.811621
b4421177a849
Background level783 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:37:16.108012
41e7f9ed2fa6
Background level784 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:40:19.597674
90c318d3a916
Background level783 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:43:35.924242
11b73402eb5e
Background level778 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:46:39.490364
c6671d655b53
Background level776 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:49:42.651940
a3bc149246a5
Background level774 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:52:57.243567
4d415a689a14
Background level773 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:56:00.577528
cc0793050803
Background level771 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T19:59:03.962973
42179a23a342
Background level768 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:02:21.353856
dd3af413dd23
Background level768 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:05:24.781723
8375a230fe75
Background level768 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:08:28.067488
cf8603b79e2b
Background level768 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:11:43.462177
bcdfa079cbaf
Background level765 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:14:46.814531
98155d9e9d16
Background level764 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:17:50.143669
9d18cd1735ec
Background level763 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:21:07.551168
afec7aaeb2df
Background level763 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:24:10.765988
255be81da067
Background level760 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:31:10.198867
5b8159683592
Background level757 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:34:26.948833
af411a4ecba7
Background level753 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:37:30.227225
7e980ad54890
Background level751 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:40:33.410830
e8920380feec
Background level749 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:43:49.545064
dfc64e26e300
Background level748 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:46:52.716434
46990502b882
Background level746 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:49:55.978477
83c5d82db7ac
Background level745 ADU717Different background level; sky, gradients and real field emission can all contribute.
2026-10-16T20:53:16.588717
5a56f6ed0df5
Background level743 ADU717Different background level; sky, gradients and real field emission can all contribute.
Method, coverage and limitations

Review distance = (value − session median) / (1.4826 × MAD). The threshold 3.5 is an advisory rule, not statistical significance. At least 12 valid frames and 75% coverage are required; zero MAD is unavailable. SNR requires the existing gain and star-count checks. Background changes are flagged in either direction.

Shared tracking/focus problems can affect an entire night without producing an outlier. No independent validation labels exist yet. Raw-green sampling and changing star populations limit interpretation. RGB/DNB, exposure, method and recorded orientation remain separate; unknown metadata do not establish compatibility.

RGB · 180.0 s · session acq_6c03bd1f: Background level 89/89; Background scatter 89/89; Detected sources 0/89: too few valid session frames; Star eccentricity 89/89; Star width (FWHM) 89/89; Stellar SNR estimate 89/89. Unknown: device_id, filter, optical_configuration, readout_mode, recorded_orientation_deg.

Method session-quality-assistant-1. Saved measurements and existing archive comparisons are unchanged.