BGDS time seriesbgds.phot_allivo://org.gavo.dc/bgds/l/phot_allThe GAVO DC teamHackstein, M.Haas, M.Fein, C.Chini, R.2022-01-25T14:30:51ZGAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837surveysgalaxy-planesmilky-way-galaxyvariable-starsbroad-band-photometrytime-domain-astronomy All mean photometry of bgds in one table. It may be simpler to write
queries against the split-band tables phot_band. Measurements in
different fields and bands have not been merged, as that procedure is
too error-prone in crowded milky way regions.http://dc.zah.uni-heidelberg.de/tableinfo/bgds.phot_allSurveyResearchUniversitätssternwarte Bochum near Cerro ArmazonesRobotic Bochum Twin Telescope (RoBoTT)3/336,338,450-451,461,472,591-592,613,615,621,651-652,659,662-663
4/1301,1303,1358,1376-1377,1379-1380,1382,1794,1816,1818-1819,1822-1823,1829,1840-1841,1892,1894,1897,2327,2333,2335,2357-2359,2376,2378,2400,2402,2408,2492-2493,2495,2528,2530,2536,2538,2591,2599,2601-2603,2612-2614,2616,2634-2635,2643,2646-2647,2656-2657,2688-269055450 58106.41.777e-19 6.621e-19OpticalbgdsBGDS time series
From the Bochum Galactic Disk Survey, time series have been obtained in the
r and i bands on an (up to) nightly basis. Depending on the field, the time
series contain up to more than 300 nights over more than 7 years. Each
measurement represents the averaged flux over 10 minutes of observation
(from 9 averaged 10s images).
The Bochum Galactic Disk Survey is an ongoing project to monitor the
stellar content of the Galactic disk in a 6 degree wide stripe centered on
the Galactic plane. The data has been recorded since mid-2010 in Sloan r
and i simultaneously with the Robotic Bochum Twin Telescope (RoBoTT) at the
Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama
desert. It contains measurements of about 2x10^7 stars over more than seven
years. Additionally, intermittent measurements in Johnson UVB and Sloan z
have been recorded as well.
bgds.phot_all All mean photometry of bgds in one table. It may be simpler to write
queries against the split-band tables phot_band. Measurements in
different fields and bands have not been merged, as that procedure is
too error-prone in crowded milky way regions.band_nameThe band the mean photometry is given for.meta.id;instr.filtercharnullableobs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharnullableraICRS right ascension for this object.pos.eq.ra;meta.maindoublenullabledecICRS declination for this object.pos.eq.dec;meta.maindoublenullablemean_magMean magnitude in band given in phot_band.magphot.mag;stat.meanfloatnullableerr_magError in mean magnitude in this bandmagstat.error;phot.magfloatnullableampDifference between brightest and weakest observation.magphot.mag;arith.difffloatnullablefluxMean flux in this band; this is computed from the mean magnitude based on Landolt standard stars.mJyphot.flux;stat.meanfloatnullableerr_fluxError in mean flux in this bandmJystat.error;phot.fluxfloatnullablenobsNumber of observations in this light curvemeta.number;obsshort