%++++++++++++++++ %.IDENTIFICATION II/286/.Summary (original name!) %.LANGUAGE LaTeX %.AUTHOR CDS %.ENVIRONMENT %.KEYWORDS CDS Catalogues %.VERSION 1.0 03-Oct-2008 %.VERSION 1.1 18-Jan-2009: -- Reformatted %.PURPOSE Description of catalogue for edition in CDS Bulletin %.COMMENTS %---------------- \hmm{.} % Catalogue Identification \cTitle{ The VIRMOS deep imaging survey. \ UBVRIJK photometry of 0226-04 (F02) deep field } \cUsualName{ VVDS-DEEP } % Short Designation \cUsualName{ VVDS-DP } \cUsualName{ VVDS } \cDic{morph,icat}{VVDS @{VVDS}} % Link for VizieR-S %\cObjectType{ } % Type of Objects (see Simbad) \cRecords{ 253588} % Total number of records \cId{ II/286/ } \cCenters{ f } % ftp vizier Bejing India LaPlata Moscow NASA Tokyo zero_data \cSimbad{0} % Simbad Status 0=Not 1=Ids_only 2=Fully_accessible % References \cAuthors{ McCracken H.J. et al.} \cReference{ Astron. Astrophys., {\bf 410}, 17 } \sReference{2003A+A...410...17M} \cAuthors{ Radovich M. et al.} \cReference{ Astron. Astrophys., {\bf 417}, 51 } \sReference{2004A+A...417...51R} \cAuthors{ Iovino A. et al.} \cReference{ Astron. Astrophys., {\bf 442}, 423 } \sReference{2005A+A...442..423I} \cAuthors{ Temporin S. et al.} \cReference{ Astron. Astrophys., {\bf 482}, 81 } \sReference{2008A+A...482...81T} % Availability \cAdded{ 19-Dec-2008 } % Electronic version \cBulletin{ --- } % Bulletin number where catalogue announced %\cRemoved{ --- } % Date when catalogue removed % Contents of the Catalogue \cContents{ {\em Id.}: VIRMOS } \cContents{ $\alpha$, $\delta$ (J2000) } \cContents{ $UBVRIJK$ photometry } % Notes %\cRemarks{ by exchange from NASA-Goddard} %\cRemarks{ by exchange from the Moscow Data Center } %\cRemarks{ by exchange from Beijing } %\cRemarks{ by exchange from NAO-Japan} % %%%%%%%% % VIZIER Definitions %%%%%%%% \cType{ OC } %\vizKeyword{Category}{KeyName} %\vizCatrole{Keyword=value} % from 0 (fundamental) to 255 (bof!) \vizDB{ * }{ * vizA@SYBASE -norecno } %\vizQbox{ boxes } % List of boxes containing stars %\vizIgnoreTables{ tables_to_ignore } %\vizMerge{ tables }{ new_name }{ Explanation of the union } %\vizPaste{ tables }{ new_name }{ Explanation of the larger table } %\vizComment{ tables }{Cols}{ Comment text } \vizExplain{ * }{ VVDS }{+ \linkRole{morphological and photometric data \ data about this source}} %\vizOrder{ file }{ column }{ +/-col } %\vizPosition{ file }{}{*vizSim c= scale= x= y= PA= Eq= Ep= x0= y0=}{ Explain } \vizAddColumn{ morph }{ n_VVDS }{ S}{}{ -VVDS }{\ucd{DATA_LINK}{\bf S} \ indicates the objects having spectroscopic results in Le F\`evre et al. \ 2005A&A...439..845L, Cat. III/250 } %\vizAddFKflag{ file }{ name }{*}{}{ +/-col }{\use{vMore}indicates that} \vizIgnoreColumns{ morph }{ * ePA? eXY* PAi *[XY][XY2]w Flag } \vizIgnoreColumns{ *cat }{ * *mag[12]* thr backg Fmax F* e_F* } \vizDisplayColumns{ morph }{ n_VVDS VVDS RAdeg DEdeg Aw e_Aw Bw e_Bw PAw S/G Sp} \vizDisplayColumns{ *cat }{ VVDS mauto e_mauto misoc mbest e_mbest \ Sflg Krad isoA } %\vizUCD{ morph }{ * Xpos* }{ =POS_CCD_X } %\vizUCD{ morph }{ * Ypos* }{ =POS_CCD_Y } \vizUCD{ * }{ VVDS }{ =ID_MAIN } \vizUCD{ morph }{ * X2* Y2* }{ =STAT_VAR } \vizUCD{ morph }{ * XY* eXY* }{ =STAT_COVAR } \vizUCD{ morph }{ * ePA* }{ =POS_POS-ANG } \vizUCD{ morph }{ * A[iw] }{ =EXTENSION_DIAM } \vizUCD{ morph }{ * B[iw] }{ = EXTENSION_SMIN } \vizUCD{ morph }{ * eTheta* eXYpos* }{ =ERROR } \vizUCD{ ucat }{ * m* }{ U notspecific magnitude } \vizUCD{ ucat }{ * Fiso* Fauto* Fbest* F*ap }{ U flux ultra-violet U } \vizUCD{ bcat }{ * m* }{ B JHN Johsnon B blue JHN Johsnon magnitude } \vizUCD{ bcat }{ * Fiso* Fauto* Fbest* F*ap }{ B flux blue B } \vizUCD{ vcat }{ * m* }{ V JHN Johsnon V visible JHN Johsnon magnitude } \vizUCD{ vcat }{ * Fiso* Fauto* Fbest* F*ap }{ V flux visible V } \vizUCD{ rcat }{ * m* }{ R COUS Cousins R magnitude } \vizUCD{ rcat }{ * Fiso* Fauto* Fbest* F*ap }{ R flux red R } \vizUCD{ icat }{ * m* }{ I Cous cousins I magnitude } \vizUCD{ icat }{ * Fiso* Fauto* Fbest* F*ap }{ I flux infra-red I } \vizUCD{ jcat }{ * m* }{ J JHN Johsnon J magnitude } \vizUCD{ jcat }{ * Fiso* Fauto* Fbest* F*ap }{ J flux infra-red J-band } \vizUCD{ kcat }{ * m* }{ K JHN Johsnon K magnitude } \vizUCD{ kcat }{ * Fiso* Fauto* Fbest* F*ap }{ K flux infra-red K-band } %\vizUCD{ *cat }{ * IsoAreaI* }{ =INST_AREA } \vizUCD{ *cat }{ isoA }{ =EXTENSION_AREA } \vizUCD{ *cat }{ F1rad F2rad F3rad }{ Angular radius effective } \vizUCD{ *cat }{ thr }{ =OBS_DETECT-SIGNIF } \vizUCD{ *cat }{ backg }{ =INST_BACKGROUND } \vizUCD{ * }{ Sflg }{ !n=f_Sex } %\vizUCD{ *cat }{ * Flux* }{ =SPECT_FLUX_VALUE } \vizUCD{ *cat }{ * mu* }{ =PHOT_SB_GENERAL } \vizSet{ *cat }{ isoA }{ dbtype=i2 } \vizSet{ *cat }{ mautoc miso misoc mbest e_mauto e_miso e_misoc e_mbest }\ { dbtype=i2t } \vizMore{ * }{ }{\vMORE{-source=@{@cat}/*\&@{=*}}{@{}}} \vizMore{ morph }{ n_VVDS }{ \vMORE{-source=3250\&ID=@{*VVDS}}{@{}}} \vizMore{ morph }{ VVDS }{ \vMore{-source=@{@cat}/*\&@{=*VVDS}}{@{}}} \vizMore{ *cat }{ Sflg }{\ifnum{@{}}>0\showFlag{Sextractor}{@{}}\else{@{}}\fi} %\vizNote{ file }{ (1) }{+\end{noteasatable}} %\vizLinkToNote{ file }{ field } \vizIndex{ * }{ VVDS } \vizPK{ * }{ VVDS } %\vizFK{ file }{ field : table } %\vizPFK{ file }{field(s) both PK and FK } %\vizPKlink{ file }{ column }{ link explanation } %\vizFKlink{ file }{ column }{ link explanation } %\vizCatK{file }{field(s) for Catalog Connection} %\vizSimK{file }{field(s) for SIMBAD Connection} %\vizLEDA{file }{ Generation } %\vizNED{file }{ Generation } %\vizSimbad{file }{ Generation } %\vizSimbadName{ file } { +/-col file_or_script } %\vizVizier{ file }{ Generation, e.g. IRAS ${IRAS} } %%% Peut-on juste afficher les magnitudes ???? %\vizLink{ morph *cat }{ Phot }{ Phot }\ % {\vMore{-source=@{@cat}/*cat\&@{=*VVDS}\&-out=\ % Krad,mbest,e_mbest,mauto,mautoc,miso,misoc }{@{}}}\ % {Display UBVRIJK Kron radius, auto, iso and best magnitudes in {\em UBVRIJK}} %\vizLink{ *cat }{Morph}{Morph}{\vMORE{-source=@{@cat}/morph\&@{=*VVDS}}{@{}}} % {Display the morphology of this source (from I filter)} \vizLink{ morph }{Sp}{Sp}{\vizContent{spectrum}\ \ifmatch{S}{@{n_VVDS}}\glutag{CENCOS.vvds,w 0@{VVDS}|@{}}\else{@{}}\fi} {Get the plot of the spectrum if exists} %\vizLink{ morph }{FITS}{FITS}{\vizContent{spectrum/fits}\ % \glutag{CENCOS.fits @{VVDS}|@{}}} % {Download the spectrum in FITS format from CENCOS center if exists} %\vizObj{ Link from METAobj } %\vizSQL{ ucat }{ } %\vizSQL{ morph }{ } %\vizTeX{ file }{ fields } %\vizSoft{ file }{ fields } %\vizHTML{ file }{ fields } %\vizCSV{ file }{ fields } \vizSQL{ morph }{\ set n_VVDS='' where VVDS not in (select @{:III/250/vvds_dp:ID} \ from @{.III/250/vvds_dp}); \ DUMP TRANSACTION vizA with truncate_only; } \vizSQL{ *cat }{ set isoA=0 where isoA<0; \ DUMP TRANSACTION vizA with truncate_only; \ set mauto =null where mauto >=32000; \ set mautoc=null where mautoc>=32000; \ set miso =null where miso >=32000; \ set misoc =null where misoc >=32000; \ set mbest =null where mbest >=32000; \ set e_mauto =null where e_mauto >=32000; \ set e_miso =null where e_miso >=32000; \ DUMP TRANSACTION vizA with truncate_only; \ set Krad=null where Krad=0 and isoA=0; \ DUMP TRANSACTION vizA with truncate_only; \ set muthr=null where muthr=0 and isoA=0; \ DUMP TRANSACTION vizA with truncate_only; \ set muMax=null where muMax=0 and isoA=0; \ } %\vizConvert{ file }{shell conversions} % Keywords \cKey{ Photometric data } \ADSartdoi{10.1051/0004-6361:20031081}