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J-PLUS DR1 Catalogue (July, 2018)
J-PLUS DR1 Catalogue (July, 2018) is based on scientific images in 12 filters collected from November 2015 to January 2018 covering a total area of ~1020 square degrees. The... -
J-PLUS DR2 Catalogue (July, 2020)
J-PLUS DR2 Catalogue (July, 2020) is based on scientific images in 12 filters collected from November 2015 to February 2020 covering a total area of ~2000 square degrees. The... -
J-PLUS DR3 Catalogue (July, 2022)
J-PLUS DR3 Catalogue (July, 2022) is based on scientific images in 12 filters collected from November 2015 to February 2022 covering a total area of ~3000 square degrees. The... -
MINIJ-PAS PDR201912 Catalogue (December, 2019)
MINIJ-PAS PDR201912 Catalogue (December, 2019) is based on scientific images in 60 filters covering a total area of ~1 square degree. MiniJ-PAS is a 60-band photometric optical... -
J-NEP PDR202107 Catalogue (July, 2024)
J-NEP PDR202107 Catalogue (July, 2024) is based on scientific images in 60 filters. J-NEP is a 60-band photometric optical survey based on images collected by the JST250... -
J-PAS EDR Catalogue (November, 2024)
J-PAS EDR Catalogue (November, 2024) is based on scientific images in 54 narrow-band filters, 2 intermediate-band filters collected from May 2023 to May 2024 covering an... -
J-PLUS DR4 Catalogue (November, 2025)
J-PLUS DR4 Catalogue (November, 2025) is based on scientific images in 12 filters collected from November 2015 to February 2025 covering a total area of ~5000 square degrees.... -
Gaia DR3. Cross-match with known variable objects
In current astronomical surveys with ever-increasing data volumes, automated methods are essential. Objects of known classes from the literature are necessary to train... -
Gaia Focused Product Release (Gaia FPR)
The Gaia Focused Product Release builds partly on the data period that went into Gaia's Data Release 3 but in case of the Solar System objects extends the stretch of time that... -
Gaia DR3 Part 1. Main source
Gaia Data Release 3 (Gaia DR3) will be released on 13 June 2022. The Gaia DR3 catalogue builds upon the Early Data Release 3 (released on 3 December 2020) and combines, for the... -
Gaia EDR3
Gaia DR3 data (both Gaia EDR3 and the full Gaia DR3) are based on data collected between 25 July 2014 (10:30 UTC) and 28 May 2017 (08:44 UTC), spanning a period of 34 months. As... -
Gaia DR2
Gaia Data Release 2. Summary of the contents and survey properties: We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities,... -
Variability of FBS blue stellar objects
A new method for combined calculations of magnitudes based on accurate measurements of POSS1 and POSS2 epoch plates is given. The photometric accuracy of various surveys and... -
FIRST-APM-SDSS survey for high-z radio QSOs
We selected from the VLA FIRST survey a sample of 94 objects with star-like counterparts in the Sloan Digital Sky Survey (SDSS), and with APM POSS-I colour O-E>=2, i.e.... -
Proper motions of IC 2391 possible members
Large-scale astrometric and photometric data bases have been used to search for and confirm stellar membership of the open cluster IC 2391. 125 stars were found that satisfied... -
Multicolour photometry of Sersic 129-01
(no description available) Cone search capability for table J/MNRAS/240/785/appendix (ubri photometry) -
Photographic study of A2197 and A2199
Radii, b26 magnitudes, (b-r) colors, position angles, and ellipticities have been measured on the plates of Palomar 48-inch Schmidt telescope taken in May 1976, for 6925... -
Melotte 66
Photoelectric and photographic photometry of the open cluster Melotte 66 is presented. The CM diagram shows most of the characteristics of an old cluster. The giant branch is... -
Optical Monitoring of Quasar 3C345
Results of long-term monitoring of the quasar 3C345 from 1984 to 1991 are presented. Observations has been conducted on the Byurakanskii station of the St. Petersburg... -
Variable stars in M92
The distance modulus of M92 is determined from the bright stars and the mean magnitude of 12 cluster-type variables. From the former, m-M=14.93; and from the latter,...
