II/341ivo://CDS.VizieR/II/341CDSDrew J.E.Gonzalez-Solares E.Greimel R.Irwin M.J.Kupcu Yoldas A.,Lewis J.Barentsen G.Eisloffel J.Farnhill H.J.Martin W.E.,Walsh J.R.Walton N.A.Mohr-Smith M.Raddi R.Sale S.E.Wright N.J.,Groot P.Barlow M.J.Corradi R.L.M.Drake J.J.Fabregat J.Frew D.J.,Gansicke B.T.Knigge C.Mampaso A.Morris R.A.H.Naylor T.,Parker Q.A.Phillipps S.Ruhland C.Steeghs D.Unruh Y.C.Vink J.S.,Wesson R.Zijlstra A.A.2024-01-10T07:52:22Z2016-10-05T08:06:27ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frsurveysvisible-astronomymedium-band-photometryh-alpha-photometryThe primary goal of the VST Photometric H{alpha} Survey of the Southern Galactic Plane and Bulge (VPHAS+) is to collect single-epoch ugri broad-band and Ha narrow-band photometry across the southern Galactic Plane within the latitude range -5{deg}<b<+5{deg} down to point source magnitudes of ~21 or better. The VPHAS+ footprint also includes the inner Galactic Bulge, defined as a 20x20 deg^2^ box around the Galactic Centre: this assures optical coverage of the full VVV footprint. For all massive OBA stars this survey is deep enough to explore all but the most heavily obscured locations of the southern Plane, reaching to >4kpc from the Sun. These data will increase the number of known southern emission line stars by up to an order of magnitude, yielding much better statistics on important short-lived types of object. The wide-area uniform photometry obtained will also facilitate stellar population studies, capable of tracing structure over much of the southern Plane. VPHAS+ will trawl the star-formation history of the Galaxy as seen in stellar remnants of all types.2016yCat.2341....0Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/II/341CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/440/2036 : VPHAS+ survey synthetic colours (Drew+, 2014)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=II/341https://vizier.iucaa.in/viz-bin/VizieR-2?-source=II/341http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=II/341https://vizier.cds.unistra.fr/viz-bin/votable?-source=II/341https://vizier.iucaa.in/viz-bin/votable?-source=II/341http://vizieridia.saao.ac.za/viz-bin/votable?-source=II/341GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table II/341/vphasp (VPHAS+ catalog, output (on a total of 319,126,837 sources))https://vizier.cds.unistra.fr/viz-bin/conesearch/II/341/vphasp?https://vizier.iucaa.in/viz-bin/conesearch/II/341/vphasp?http://vizieridia.saao.ac.za/viz-bin/conesearch/II/341/vphasp?GETtext/xml+votable180.050000true111.40454-20.449750.005555555555555556Hips catalogue for table II/341/vphasphttps://hipscat.cds.unistra.fr/HiPSCatService/II/341/vphaspESO3/450 4/1807 1844-1845 1891 2333 2357 2370 2453 2485 2487 2652-2653 5/5205 5376 5378-5379 5381-5382 5384-5385 5387 5390 5409-5411 5413 5416-5417 5420 5422 5509-5511 5517 5519 5523 5526 5528-5530 5541 5543 5552 5554 7216 7218-7219 7222-7225 7227 7266 7272 7274-7275 7278-7279 7290 7365 7553-7556 7558 7561 7577-7582 7601 9307 9309-9311 9341 9343 9432 9436 9438 9460 9462 9467-9468 9470 9473-9476 9478 9504 9506-9507 9610 9809 9811 9817-9820 9822 9841 9843-9844 9846-9847 9849 9851-9852 9854 9937 9939 9945-9947 9969 9972-9973 9975 9980-9981 9983 10114 10152-10154 10366-10367 10396 10399 10407 10412-10414 10418-10422 10424 10439-10440 10442 10449-10454 10456 10541-10543 10551-10553 10590 10593-10595 10597-10600 10621 10624 10753-10756 10758 10760 6/20828-20829 20831 20853 20855 20957 20959 20981 21510 21523 21532-21534 21545 21547 21554-21555 21567 21610 21633-21635 21648 21650 21656 21658-21659 21672-21673 21676-21677 21679 21686 21692 21696 21698 22035 22065 22075 22088 22090-22091 22128-22130 22161 22169 22171 22196-22197 22212 22214 22220 22240 28715 28718-28719 28730-28731 28734 28868 28870-28871 28881-28883 28886 28904-28905 28907 29058-29059 29094-29095 29106-29107 29110 29164 29166-29167 29178-29179 29182 29184-29185 29188-29189 29200-29202 29269 29440-29441 29444-29445 29456-29457 29459 29468-29469 29471 29493 29536-29537 29540-29541 29552-29553 29556-29557 29871 29882-29883 30210-30211 30240-30242 30253 30287 30302-30304 30306-30307 30332 30356-30357 30400-30401 30403 30416 37213-37215 37223 37234-37235 37316-37317 37319 37325 37327 37361 37363 37369 37371 37687 37707-37708 37710-37711 37732-37733 37735-37736 37743 37748 37756 37758-37759 37829 37831 37837 37839 37844-37846 37854 37861-37863 37876 37878 37886-37887 37889-37891 37908 37910 37916 37936 37938 37944 38020 38022-38023 38033-38036 38038 38040-38042 38048-38050 38056 38435-38436 38438 38444 38528 38570 39231 39233 39235 39265 39267 39284 39317 39360-39361 39363 39369 39371 39395 39401 39412-39414 39779 39873 39875 39896-39897 39899 39929 39936 39938 40074 40450 40480-40482 40591 40600 40602-40603 40620-40621 40624-40626 41459 41462-41463 41562-41563 41573 41575 41581 41591-41593 41595 41627 41645-41647 41660-41662 41666-41667 41669-41671 41692 41700-41701 41704 41712 41755 41772 41774 41777 41780-41781 41783 41794-41795 41820-41822 41828-41829 41856-41857 42153-42156 42158-42159 42163 42187 42190-42191 42202-42203 42216-42218 42220-42222 42224-42226 42228-42229 42231 42350-42351 42364 42366-42367 42371 42386-42387 42404-42405 42416-42417 42419-42420 42464-42465 42468-42469 42480-42481 42483 42500 42504 42512-42513 42515-42518 43009-43011 43028 43030-43031 43036-43038 43044-43045 43048 43056-43058https://cdsarc.cds.unistra.fr/viz-bin/moc/II/341?format=asciiOpticaldefaultII/341/vphaspVPHAS+ catalog, output (on a total of 319,126,837 sources)DEJ2000Declination in decimal degrees (J2000) (DEJ2000)degpos.eq.dec;meta.mainindexedVPHASDR2Position-based source name. Not a unique identifier (VPHASDR2 JHHMMSS.s+DDMMSS.s) (name)meta.id;meta.maincharPrimaryIDSourceID of the preferred catalogue entry for this source (primaryID)meta.idcharfPrimary[0/1] Flag =1 if the entry is the preferred observation of a unique source (Primary_source)meta.codeinte_gmagap? Statistical uncertainty for gmagap, not including systematics (aperMagErr_g)magstat.errorfloatnullablesnrg? Ratio of the signal in the aperture relative to the background (snr_g)stat.snrfloatnullablegmaglim? The Vega magnitude a SNR=3 source would have at this position (magLim_g)magphot.magfloatnullablePSFFWHMg? Typical PSF FWHM in the CCD frame (psffwhm_g)arcsecphys.angSizefloatnullableMJDg? Modified Julian Date at the start of the g-band exposure (mjd_g)dtime.epochdoublenullabledetIDgDetection identifier: night-#exposure-#extension-#number (detectionID_g)meta.idcharcleanr2[0/1] =1 if the r2-band detection is significant and the PSF fit good (clean_r2)meta.codeintr2mag? Second r-band VEGA magnitude obtained using PSF fitting (r2)magphot.mag;em.opt.RfloatnullablewarningHaFlags problems encountered while fitting the PSF, if any (warning_ha) (1)meta.codecharHamagap? H-alpha VEGA magnitude obtained using aperture photometry (aperMag_ha)magphot.flux;em.line.Halphafloatnullablee_Hamagap? Statistical uncertainty for Hamagap, not including systematics (aperMagErr_ha)magstat.errorfloatnullablesnrHa? Ratio of the signal in the aperture relative to the background (snr_ha)stat.snrfloatnullableHamaglim? The Vega magnitude a SNR=3 source would have at this position (magLim_ha)magphot.magfloatnullablePSFFWHMHa? Typical PSF FWHM in the CCD frame (psffwhm_ha)arcsecphys.angSizefloatnullableMJDHa? Modified Julian Date at the start of the H-alpha exposure (mjd_ha)dtime.epochdoublenullabledetIDHaDetection identifier: night-#exposure-#extension-#number (detectionID_ha)meta.idcharcleanr[0/1] =1 if the r-band detection is significant and the PSF fit good (clean_r)meta.codeintrmag? Default r-band VEGA magnitude obtained using PSF fitting (r)magphot.mag;em.opt.RfloatnullableindexedrmagAB? Default r-band AB magnitude obtained using PSF fitting (r_AB)magphot.mag;em.opt.RfloatnullablermagapAB? r-band AB magnitude obtained using aperture photometry (aperMag_r_AB)magphot.mag;em.opt.Rfloatnullablee_rmagap? Statistical uncertainty for rmagap, not including systematics (aperMagErr_r)magstat.errorfloatnullablesnrr? Ratio of the signal in the aperture relative to the background (snr_r)stat.snrfloatnullablesourceIDUnique VPHAS source identifier in the format field-extension-number (sourceID)meta.idcharindexedRAJ2000Right Ascension in decimal degrees (J2000) (RAJ2000)degpos.eq.ra;meta.mainindexedNobs[1-6] Number of observations of this source in the survey (nObs)meta.numberintclean[0/1] =1 if cleang, cleanr2, cleanha, cleanr and cleani are true (clean)meta.codeintu-g? (u-g) colour index, formed by subtracting columns u and g (u_g)magphot.color;em.opt.U;em.opt.Bfloatnullableg-r2? (g-r2) colour index, formed by subtracting columns g and r2 (g_r2)magphot.color;em.opt.B;em.opt.Rfloatnullabler-i? (r-i) colour index, formed by subtracting columns r and i (r_i)magphot.color;em.opt.R;em.opt.Ifloatnullabler-ha? (r-Halpha) colour index, formed by subtracting columns r and ha (r_ha)magphot.color;em.opt.R;em.line.Halphafloatnullablecleanu[0/1] =1 if the u-band detection is significant and the PSF fit good (clean_u)meta.codeintumag? Default u-band VEGA magnitude obtained using PSF fitting (u)magphot.mag;em.opt.UfloatnullableindexedumagAB? Default u-band AB magnitude obtained using PSF fitting (u_AB)magphot.mag;em.opt.Ufloatnullablee_umag? Statistical uncertainty for u, not including systematics (err_u)magstat.error;phot.magfloatnullablechiu? Goodness of the PSF fit in u, as determined by DAOPHOT ALLSTAR (chi_u)stat.fit.goodness;instr.det.psffloatnullablewarninguFlags problems encountered while fitting the PSF, if any (warning_u) (1)meta.codecharumagap? u-band VEGA magnitude obtained using aperture photometry (aperMag_u)magphot.mag;em.opt.UfloatnullableumagapAB? u-band AB magnitude obtained using aperture photometry (aperMag_u_AB)magphot.mag;em.opt.Ufloatnullablee_umagap? Statistical uncertainty for umagap, not including systematics (aperMagErr_u)magstat.error;pos.cartesian.xfloatnullablesnru? Ratio of the signal in the aperture relative to the background (snr_u)stat.snrfloatnullableumaglim? The Vega magnitude a SNR=3 source would have at this position (magLim_u)magphot.magfloatnullablePSFFWHMu? Typical PSF FWHM in the CCD frame (psffwhm_u)arcsecphys.angSizefloatnullableMJDu? Modified Julian Date at the start of the u-band exposure (mjd_u)dtime.epochdoublenullableindexeddetIDuDetection identifier: night-#exposure-#extension-#number (detectionID_u)meta.idcharcleang[0/1] =1 if the g-band detection is significant and the PSF fit good (clean_g)meta.codeintgmag? Default g-band VEGA magnitude obtained using PSF fitting (g)magphot.mag;em.opt.BfloatnullableindexedgmagAB? Default g-band AB magnitude obtained using PSF fitting (g_AB)magphot.mag;em.opt.Bfloatnullablee_gmag? Statistical uncertainty for g, not including systematics (err_g)magstat.error;phot.magfloatnullablechig? Goodness of the PSF fit in g, as determined by DAOPHOT ALLSTAR (chi_g)stat.fit.goodness;instr.det.psffloatnullablewarninggFlags problems encountered while fitting the PSF, if any (warning_g) (1)meta.codechargmagap? g-band VEGA magnitude obtained using aperture photometry (aperMag_g)magphot.mag;em.opt.BfloatnullablegmagapAB? g-band AB magnitude obtained using aperture photometry (aperMag_g_AB)magphot.mag;em.opt.Bfloatnullabler2magAB? Second r-band AB magnitude obtained using PSF fitting (r2_AB)magphot.mag;em.opt.Rfloatnullablee_r2mag? Statistical uncertainty for r2, not including systematics (err_r2)magstat.error;phot.magfloatnullablechir2? Goodness of the PSF fit in r2, as determined by DAOPHOT ALLSTAR (chi_r2)stat.fit.goodness;instr.det.psffloatnullablewarningr2Flags problems encountered while fitting the PSF, if any (warning_r2) (1)meta.codecharr2magap? r2-band VEGA magnitude obtained using aperture photometry (aperMag_r2)magphot.mag;em.opt.Rfloatnullabler2magapAB? r2-band AB magnitude obtained using aperture photometry (aperMag_r2_AB)magphot.mag;em.opt.Rfloatnullablee_r2magap? Statistical uncertainty for r2magap, not including systematics (aperMagErr_r2)magstat.errorfloatnullablesnrr2? Ratio of the signal in the aperture relative to the background (snr_r2)stat.snrfloatnullabler2maglim? The Vega magnitude a SNR=3 source would have at this position (magLim_r2)magphot.magfloatnullablePSFFWHMr2? Typical PSF FWHM in the CCD frame (psffwhm_r2)arcsecphys.angSizefloatnullableMJDr2? Modified Julian Date at the start of the r2-band exposure (mjd_r2)dtime.epochdoublenullabledetIDr2Detection identifier: night-#exposure-#extension-#number (detectionID_r2)meta.idcharcleanHa[0/1] =1 if the H-alpha detection is significant and the PSF fit good (clean_ha)meta.codeintHamag? Default H-alpha VEGA magnitude obtained using PSF fitting (ha)magphot.flux;em.line.Halphafloatnullablee_Hamag? Statistical uncertainty for ha, not including systematics (err_ha)magstat.error;phot.magfloatnullablechiHa? Goodness of the PSF fit in H-alpha, as determined by DAOPHOT (chi_ha)stat.fit.goodness;instr.det.psffloatnullablee_rmag? Statistical uncertainty for r, not including systematics (err_r)magstat.error;phot.magfloatnullablechir? Goodness of the PSF fit in r, as determined by DAOPHOT ALLSTAR (chi_r)stat.fit.goodness;instr.det.psffloatnullablewarningrFlags problems encountered while fitting the PSF, if any (warning_r) (1)meta.codecharrmagap? r-band VEGA magnitude obtained using aperture photometry (aperMag_r)magphot.mag;em.opt.Rfloatnullablermaglim? The Vega magnitude a SNR=3 source would have at this position (magLim_r)magphot.magfloatnullablePSFFWHMr? Typical PSF FWHM in the CCD frame (psffwhm_r)arcsecphys.angSizefloatnullableMJDr? Modified Julian Date at the start of the r-band exposure (mjd_r)dtime.epochdoublenullabledetIDrDetection identifier: night-#exposure-#extension-#number (detectionID_r)meta.idcharcleani[0/1] =1 if the i-band detection is significant and the PSF fit good (clean_i)meta.codeintimag? Default i-band VEGA magnitude obtained using PSF fitting (i)magphot.mag;em.opt.IfloatnullableindexedimagAB? Default i-band AB magnitude obtained using PSF fitting (i_AB)magphot.mag;em.opt.Ifloatnullablee_imag? Statistical uncertainty for i, not including systematics (err_i)magstat.error;phot.magfloatnullablechii? Goodness of the PSF fit in i, as determined by DAOPHOT ALLSTAR (chi_i)stat.fit.goodness;instr.det.psffloatnullablewarningiFlags problems encountered while fitting the PSF, if any (warning_i) (1)meta.codecharimagap? i-band VEGA magnitude obtained using aperture photometry (aperMag_i)magphot.mag;em.opt.IfloatnullableimagapAB? i-band AB magnitude obtained using aperture photometry (aperMag_i_AB)magphot.mag;em.opt.Ifloatnullablee_imagap? Statistical uncertainty for imagap, not including systematics (aperMagErr_i)magstat.errorfloatnullablesnri? Ratio of the signal in the aperture relative to the background (snr_i)stat.snrfloatnullableimaglim? The Vega magnitude a SNR=3 source would have at this position (magLim_i)magphot.magfloatnullablePSFFWHMiTypical PSF FWHM in the CCD frame (psffwhm_i)arcsecphys.angSizefloatMJDiModified Julian Date at the start of the i-band exposure (mjd_i)dtime.epochdoubledetIDiDetection identifier: night-#exposure-#extension-#number (detectionID_i)meta.idcharFieldSurvey-specific identifier of the telescope pointing (field)meta.id;instr.telcharExt[1/32] OmegaCAM CCD extension used (ext)phys.angSize;instr.plateintnbDistDistance to the nearest neighbour detected inarcsecpos.angDistancefloat