Visual Magnitude Observations of the Suspected Variable Star Gaia DR3 1822800617416961152
Abstract
This dataset contains visual magnitude estimates of the star Gaia DR3 1822800617416961152, suspected of variability. The brightness estimates were derived from photographic observations obtained with the Seven-Camera Astrograph of the Odessa Astronomical Observatory. Visual magnitudes were estimated using comparison stars identified in Gaia DR3.The data are provided as a time series of Julian Dates (JD) and corresponding stellar magnitudes in the photovisual magnitude system. All Julian Dates are strictly increasing and unique. The numerical precision of the original measurements is fully preserved.A colon “:” following a magnitude denotes an uncertain visual estimate, in accordance with standard variable-star observing practice. Unmarked values represent normal-confidence estimates.The dataset is intended for independent verification of variability and determination of variability parameters. Stellar Coordinates (ICRS, J2000) Suspected variable star:Gaia DR3 1822800617416961152RA 20 09 41.9731Dec +20 16 31.1672Gmag = 9.9947 Comparison star “a”:Gaia DR3 1822753235334715520RA 20 10 49.3698Dec +20 09 41.4737Gmag = 9.5454 Comparison star “b”:Gaia DR3 1822749490123590784RA 20 09 32.1250Dec +20 04 14.5299Gmag = 9.9583 Comparison star “c”:Gaia DR3 1822725060328578560RA 20 09 29.5283Dec +20 01 44.8758Gmag = 10.3906 Magnitude Range: 9.73–10.23, Δm ≈ 0.5 mag Data Summary Number of observations: 152Julian Date range: JD 2436381 – 2440509Observation type: visual estimates from photographic platesInstrument: Seven-Camera Astrograph, Odessa Astronomical ObservatoryPhotometric system on plates: photovisual
Fields of Study & Subjects
Stellar
planetary
and galactic studies
Astronomy and Astrophysical Research
History and Developments in Astronomy
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 16 February 2026
- Language
- EN