79 datasets found

Keywords: photographic photometry

Filter Results
  • 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,...
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