J/MNRAS/393/1275 STAGES master catalog (Gray+, 2009)
STAGES: the Space Telescope A901/2 Galaxy Evolution Survey.
Gray M.E., Wolf C., Barden M., Peng C.Y., Haussler B., Bell E.F.,
Mcintosh D.H., Guo Y., Caldwell J.A.R., Bacon D., Balogh M., Barazza F.D.,
Bohm A., Heymans C., Jahnke K., Jogee S., Van Kampen E., Lane K.,
Meisenheimer K., Sanchez S.F., Taylor A., Wisotzki L., Zheng X.,
Green D.A., Beswick R.J., Saikia D.J., Gilmour R., Johnson B.D.,
Papovich C.
<Mon. Not. R. Astron. Soc., 393, 1275-1301 (2009)>
=2009MNRAS.393.1275G 2009MNRAS.393.1275G
ADC_Keywords: Surveys ; Galaxy catalogs ; Galaxies, photometry ; Morphology
Keywords: surveys - galaxies: clusters: general - galaxies: evolution
Abstract:
We present an overview of the Space Telescope A901/2 Galaxy Evolution
Survey (STAGES). STAGES is a multiwavelength project designed to probe
physical drivers of galaxy evolution across a wide range of
environments and luminosity. A complex multicluster system at z∼0.165
has been the subject of an 80-orbit F606W Hubble Space Telescope
(HST)/Advanced Camera for Surveys (ACS) mosaic covering the full
0.5x0.5deg2 (∼5x5Mpc2) span of the supercluster. Extensive
multiwavelength observations with XMM-Newton, GALEX, Spitzer, 2dF,
Giant Metrewave Radio Telescope and the 17-band COMBO-17 photometric
redshift survey complement the HST imaging. Our survey goals include
simultaneously linking galaxy morphology with other observables such
as age, star formation rate, nuclear activity and stellar mass. In
addition, with the multiwavelength data set and new high-resolution
mass maps from gravitational lensing, we are able to disentangle the
large-scale structure of the system. By examining all aspects of an
environment we will be able to evaluate the relative importance of the
dark matter haloes, the local galaxy density and the hot X-ray gas in
driving galaxy transformation.
Description:
Having created separate catalogues from the STAGES and COMBO-17 data
sets, we create a combined, master catalogue.
In summary, the combined catalogue contains 88 879 sources. Of these,
∼6577 objects with a COMBO-17 ID are not within the region covered by
the STAGES HST mosaic. Moreover, ∼1271 STAGES detections are outside
the COMBO-17 observation footprint. Inside the region covered by both
surveys, there are ∼81031 sources. For 50701 objects, the method
described above provides a match between COMBO-17 and STAGES . ∼23833
sources detected in STAGES do not have counterparts in COMBO-17; ∼6497
sources from the COMBO-17 catalogue are not matched to STAGES
detections.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
stages.dat 1506 88879 STAGES master catalogue (2008/05/29 version)
table1.dat 53 80 Details of STAGES HST/ACS observations
table4.dat 46 17 COMBO-17 imaging data on the A901/2 field
stages_v1.fit 2880 29810 FITS version of STAGES master catalogue
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See also:
II/253 : Chandra Deep Field South: multi-colour data (Wolf+, 2008)
J/A+A/377/442 : Chandra Deep Field South: R-band photometry (Wolf+, 2001)
Byte-by-byte Description of file: stages.dat
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Bytes Format Units Label Explanations
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2- 3 I2 --- Tile [1/80]? Tile number in STAGES mosaic (G1)
5- 8 I4 --- STAGES [1/1333]? STAGES sequential number
within the tile (G1)
10- 18 F9.4 pix Xpos ? X-position from SExtractor on tile
20- 28 F9.4 pix Ypos ? Y-position from SExtractor on tile
30- 37 F8.5 pix CXX ? Ellipse parameter from SExtractor
39- 46 F8.5 pix CYY ? Ellipse parameter from SExtractor
48- 55 F8.5 pix CXY ? Ellipse parameter from SExtractor
57- 61 F5.1 deg PA [-180/180]? Position angle of ellipse from
SExtractor in image coordinates (right to up)
63- 67 F5.1 deg PAw [-180/180]? Position angle
(world coordinates)
69- 73 F5.3 --- Ell ? Ellipticity from SExtractor
75- 79 F5.2 --- Rad ? Kron radius in units of amaj
81- 87 F7.3 pix amaj ? Semimajor half-axis from SExtractor
89- 95 F7.3 pix bmaj ? Semiminor half-axis from SExtractor
97-105 F9.5 deg RAdeg ? Right ascension, SExtractor (J2000)
107-115 F9.5 deg DEdeg ? Declination from SExtractor (J2000)
117-124 E8.2 ct bckg ? Background value from SExtractor
126-134 E9.3 ct Fbest ? 'Best' flux (V606) from SExtractor
136-144 E9.3 ct e_Fbest ? Error of Fbest
146-151 F6.3 mag F606 ? Best magnitude (V606) from SExtractor
in AB system
153-158 F6.3 mag e_F606 ? Error of F606
160-165 F6.2 pix r0.5 ? Half-light radius from SExtractor
167-173 I7 pix+2 Area ? Isophotal area from SExtractor
175-180 F6.2 pix FWHM ? FWHM from SExtractor
182-183 I2 --- Sf [0,50]? SExtractor quality flags
185-188 F4.2 --- S/G [0,1]? SExtractor stellarity estimator
(0=galaxy, 1=star)
190-205 A16 --- Image ? Postage stamp image file name
207-223 A17 --- GALFIT ? GALFIT output filename containing data
225-231 F7.2 pix XposG ? GALFIT X-position on postage stamp
233-239 F7.2 pix e_XposG ? Error of XposG
241-247 F7.2 pix YposG ? Y-position from GALFIT
249-255 F7.2 pix e_YposG ? Error of YposG
257-262 F6.3 mag VTmag ? Total AB magnitude from GALFIT
264-269 F6.3 mag e_VTmag ? Error of magTot
271-275 F5.1 pix r0.5G ? Half-light radius from GALFIT
277-281 F5.1 pix e_r0.5G ? Error of RadhlG
283-286 F4.2 --- n ? Sersic index from GALFIT
288-291 F4.2 --- e_n ? Error of Sersic
293-296 F4.2 --- b/a ? GALFIT minor-to-major axis ratio
298-301 F4.2 --- e_b/a ? Error of b/a
303-307 F5.1 deg PAG ? GALFIT position angle (up to left)
309-313 F5.1 deg e_PAG ? Error of PAG
315-320 F6.3 --- Sky ? Sky value from GALAPAGOS (profile fit)
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% COMBO-17 general information
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323-327 I5 --- COMBO-17 [1/63775]? COMBO-17 A901/2 field
object number (G1)
329-337 F9.5 deg RA2deg ? COMBO-17 right ascension (J2000)
339-347 F9.5 deg DE2deg ? COMBO-17 declination (J2000)
349-355 F7.2 pix X2pos ? X-position on COMBO-17 R frame
357-363 F7.2 pix Y2pos ? Y-position on COMBO-17 R frame
365-370 F6.3 mag Rmag ? Total R-band magnitude
372-377 F6.3 mag e_Rmag ? 1σ error of total R-band magnitude
379-384 F6.3 mag apRmag ? Aperture R-band magnitude in run E
386-392 F7.3 mag apdRmag ? Difference total to aperture
(point source ∼ 0)
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% Various flags for sample selection
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394-397 I4 --- ph [0/1536]? COMBO-17 photometry flags (1)
399 I1 --- s [0,5]? COMBO-17 sample flag (3)
401 I1 --- S [0,4]? STAGES sample flag (2)
403 I1 --- MIPS [0,3]? MIPS sample flag (4)
405-409 F5.2 --- chi2 ? chi2/Nf of best-fitting template
411-415 F5.2 --- chi2s ? chi2/Nf of best-fitting star template
417-421 F5.2 --- chi2g ? chi2/Nf of best-fitting galaxy template
423-427 F5.2 --- chi2q ? chi2/Nf of best-fitting QSO template
429-433 F5.2 --- chi2wd ? chi2/Nf of best-fitting WD template
435-439 F5.2 --- chi2cl ? chi2/Nf of best-fitting galaxy template
at z= 0.167
441-454 A14 --- MCclass Multicolour class (5)
456-460 F5.3 --- MCz ? Mean redshift in distribution p(z)
462-466 F5.3 --- e_MCz ? Standard deviation (1σ) in
distribution p(z)
468-472 F5.3 --- MCz2 ? Alternative redshift if p(z) bimodal
474-478 F5.3 --- e_MCz2 ? Standard deviation (1σ) at
alternative redshift
480-484 F5.3 --- MCzml ? Peak redshift in distribution p(z)
486-490 F5.3 mag MCE ? Mean E(B-V) in distribution p(z)
492-496 F5.3 mag e_MCE ? Standard deviation (1σ) in
distribution p[E(B-V)]
498-502 F5.3 mag MCEml ? Peak value in distribution p[E(B-V)]
504-507 F4.1 --- MCage [0,59]? Mean template age index (7)
509-512 F4.1 --- e_MCage ? Standard deviation (1σ) of MCage
514-515 I2 --- MCageml ? Peak in template age index distribution
517-524 F8.6 --- MCzcl [0.167207]? Redshift
assuming cluster membership
526-531 F6.3 mag MCEcl ? Mean E(B-V) assuming cluster membership
533-538 F6.3 mag e_MCEcl ? Standard deviation in p(E(B-V))
if cluster member
540-543 F4.1 --- MCagecl ? Mean age index assuming cluster membership
545-548 F4.1 --- e_MCagecl ? Standard deviation in age index
if cluster member
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% Total galaxy rest-frame luminosities
--------------------------------------------------------------------------------
550-556 F7.3 mag U280MAG ? Absolute Magnitude in 280/40nm filter
(0.25≤z≤1.3)
558-564 F7.3 mag e_U280MAG ? 1σ error of U280MAG
566-572 F7.3 mag UMAG ? Absolute Magnitude in Johnson U
(ok at all z)
574-580 F7.3 mag e_UMAG ? 1σ error of UMAG
582-588 F7.3 mag BMAG ? Absolute Magnitude in Johnson B
(0.0≤z≤1.1)
590-596 F7.3 mag e_BMAG ? 1σ error of BMAG
598-604 F7.3 mag VMAG ? Absolute Magnitude in Johnson V
(0.0≤z≤0.7])
606-612 F7.3 mag e_VMAG ? 1σ error of VMAG
614-620 F7.3 mag uMAG ? Absolute Magnitude in SDSS u (ok at all z)
622-628 F7.3 mag e_uMAG ? 1σ error of uMAG
630-636 F7.3 mag gMAG ? Absolute Magnitude in SDSS g (0.0≤z≤1.0)
638-644 F7.3 mag e_gMAG ? 1σ error of gMAG
646-652 F7.3 mag rMAG ? Absolute Magnitude in SDSS r (0.0≤z≤0.5)
654-660 F7.3 mag e_rMAG ? 1σ error of rMAG
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% Rest-frame luminosities at cluster distance
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662-668 F7.3 mag U280Mcl ? Absolute Magnitude in 280/40nm cluster
(if cluster member)
670-676 F7.3 mag e_U280Mcl ? 1σ error of U280Mcl
678-684 F7.3 mag UMcl ? Absolute Magnitude in Johnson U
(if cluster member)
686-692 F7.3 mag e_UMcl ? 1σ error of UMcl
694-700 F7.3 mag BMcl ? Absolute Magnitude in Johnson B
(if cluster member)
702-708 F7.3 mag e_BMcl ? 1σ error of BMcl
710-716 F7.3 mag VMcl ? Absolute Magnitude in Johnson V
(if cluster member)
718-724 F7.3 mag e_VMcl ? 1σ error of BMcl
726-732 F7.3 mag uMcl ? Absolute Magnitude in SDSS u
(if cluster member)
734-740 F7.3 mag e_uMcl ? 1σ error of uMcl
742-748 F7.3 mag gMcl ? Absolute Magnitude in SDSS g
(if cluster member)
750-756 F7.3 mag e_gMcl ? 1σ error of gMcl
758-764 F7.3 mag rMcl ? Absolute Magnitude in SDSS r
(if cluster member)
766-772 F7.3 mag e_rMcl ? 1σ error of rMcl
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% QSO rest-frame luminosities
--------------------------------------------------------------------------------
774-780 F7.3 mag U145MAG ? QSO Absolute Magnitude in 145/10nm
(1.4≤z≤5.2)
782-788 F7.3 mag e_U145MAG ? 1σ error of U145MAG10
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% Observed seeing-adaptive aperture fluxes
--------------------------------------------------------------------------------
790-798 E9.3 ct/m2/s/nm W420f ? Photon flux in filter 420nm
800-807 E8.2 ct/m2/s/nm e_W420f ? 1σ photon flux error in 420nm
809-817 E9.3 ct/m2/s/nm W462f ? Photon flux in filter 462nm
819-826 E8.2 ct/m2/s/nm e_W462f ? 1σ photon flux error in 462nm
828-836 E9.3 ct/m2/s/nm W485f ? Photon flux in filter 485nm
838-845 E8.2 ct/m2/s/nm e_W485f ? 1σ photon flux error in 485nm
847-855 E9.3 ct/m2/s/nm W518f ? Photon flux in filter 518nm
857-864 E8.2 ct/m2/s/nm e_W518f ? 1σ photon flux error in 518nm
866-874 E9.3 ct/m2/s/nm W571f ? Photon flux in filter 571nm
876-883 E8.2 ct/m2/s/nm e_W571f ? 1σ photon flux error in 571nm
885-893 E9.3 ct/m2/s/nm W604f ? Photon flux in filter 604nm
895-902 E8.2 ct/m2/s/nm e_W604f ? 1σ photon flux error in 604nm
904-912 E9.3 ct/m2/s/nm W646f ? Photon flux in filter 646nm
914-921 E8.2 ct/m2/s/nm e_W646f ? 1σ photon flux error in 646nm
923-931 E9.3 ct/m2/s/nm W696f ? Photon flux in filter 696nm
933-940 E8.2 ct/m2/s/nm e_W696f ? 1σ photon flux error in 696nm
942-950 E9.3 ct/m2/s/nm W753f ? Photon flux in filter 753nm
952-959 E8.2 ct/m2/s/nm e_W753f ? 1σ photon flux error in 753nm
961-969 E9.3 ct/m2/s/nm W815f ? Photon flux in filter 815nm
971-978 E8.2 ct/m2/s/nm e_W815f ? 1σ photon flux error in 815nm
980-988 E9.3 ct/m2/s/nm W856f ? Photon flux in filter 856nm
990-997 E8.2 ct/m2/s/nm e_W856f ? 1σ photon flux error in 856nm
999-1007 E9.3 ct/m2/s/nm W914f ? Photon flux in filter 914nm
1009-1016 E8.2 ct/m2/s/nm e_W914f ? 1σ photon flux error in 914nm
1018-1026 E9.3 ct/m2/s/nm Uf ? Photon flux in filter U
1028-1035 E8.2 ct/m2/s/nm e_Uf ? 1σ photon flux error in U
1037-1045 E9.3 ct/m2/s/nm BfA ? Photon flux in filter B in run A
1047-1054 E8.2 ct/m2/s/nm e_BfA ? 1σ photon flux error in B/A
1056-1064 E9.3 ct/m2/s/nm BfG ? Photon flux in filter B in run G
1066-1073 E8.2 ct/m2/s/nm e_BfG ? 1σ photon flux error in B/G
1075-1083 E9.3 ct/m2/s/nm Vf ? Photon flux in filter V
1085-1092 E8.2 ct/m2/s/nm e_Vf ? 1σ photon flux error in V
1094-1102 E9.3 ct/m2/s/nm Rf ? Photon flux in filter R
1104-1111 E8.2 ct/m2/s/nm e_Rf ? 1σ photon flux error in R
1113-1121 E9.3 ct/m2/s/nm If ? Photon flux in filter I
1123-1130 E8.2 ct/m2/s/nm e_If ? 1σ photon flux error in I
--------------------------------------------------------------------------------
% Observed aperture Asinh Vega magnitudes
--------------------------------------------------------------------------------
1132-1137 F6.3 mag W420 ? Magnitude in filter 420nm
1139-1144 F6.3 mag e_W420 ? 1σ magnitude error in 420
1146-1151 F6.3 mag W462 ? Magnitude in filter 462nm
1153-1158 F6.3 mag e_W462 ? 1σ magnitude error in 462
1160-1165 F6.3 mag W485 ? Magnitude in filter 485nm
1167-1172 F6.3 mag e_W485 ? 1σ magnitude error in 485
1174-1179 F6.3 mag W518 ? Magnitude in filter 518nm
1181-1186 F6.3 mag e_W518 ? 1σ magnitude error in 518
1188-1193 F6.3 mag W571 ? Magnitude in filter 571nm
1195-1200 F6.3 mag e_W571 ? 1σ magnitude error in 571
1202-1207 F6.3 mag W604 ? Magnitude in filter 604nm
1209-1214 F6.3 mag e_W604 ? 1σ magnitude error in 604
1216-1221 F6.3 mag W646 ? Magnitude in filter 646nm
1223-1228 F6.3 mag e_W646 ? 1σ magnitude error in 646
1230-1235 F6.3 mag W696 ? Magnitude in filter 696nm
1237-1242 F6.3 mag e_W696 ? 1σ magnitude error in 696
1244-1249 F6.3 mag W753 ? Magnitude in filter 753nm
1251-1256 F6.3 mag e_W753 ? 1σ magnitude error in 753
1258-1263 F6.3 mag W815 ? Magnitude in filter 815nm
1265-1270 F6.3 mag e_W815 ? 1σ magnitude error in 815
1272-1277 F6.3 mag W856 ? Magnitude in filter 856nm
1279-1284 F6.3 mag e_W856 ? 1σ magnitude error in 856
1286-1291 F6.3 mag W914 ? Magnitude in filter 914nm
1293-1298 F6.3 mag e_W914 ? 1σ magnitude error in 914
1300-1305 F6.3 mag U365A ? Magnitude in filter U
1307-1312 F6.3 mag e_U365A ? 1σ magnitude error in U
1314-1319 F6.3 mag B458A ? Magnitude in filter B in run A
1321-1326 F6.3 mag e_B458A ? 1σ magnitude error in run A
1328-1333 F6.3 mag B458G ? Magnitude in filter B in run G
1335-1340 F6.3 mag e_B458G ? 1σ magnitude error in run G
1342-1347 F6.3 mag V538A ? Magnitude in filter V
1349-1354 F6.3 mag e_V538A ? 1σ magnitude error in V
1356-1361 F6.3 mag R648A ? Magnitude in filter R
1363-1368 F6.3 mag e_R648A ? 1σ magnitude error in R
1370-1375 F6.3 mag I857A ? Magnitude in filter I
1377-1382 F6.3 mag e_I857A ? 1σ magnitude error in I
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% Stellar masses and SFRs
--------------------------------------------------------------------------------
1384-1388 F5.2 [solMass] logM ? log10 of stellar mass
1390-1394 F5.2 [solMass] logMcl ? log10 of stellar mass if cluster member
1396-1404 E9.3 uJy F24um ? MIPS 24um flux in microJy
1406-1414 E9.3 solLum LIR ? IR luminosity
1416-1424 E9.3 solLum LUV ? UV luminosity
1426-1434 E9.3 solLum LIRcl ? IR luminosity if cluster member
1436-1444 E9.3 solLum LUVcl ? UV luminosity if cluster member
1446-1454 E9.3 solMass/yr SFRdet ? SFR from UV+IR if IR detected
1456-1464 E9.3 solMass/yr SFRlo ? SFR lower limit from UV alone
(if IR non-detected)
1466-1474 E9.3 solMass/yr SFRHI ? SFR upper limit (if IR non-detected)
1476-1484 E9.3 solMass/yr SFRcl ? SFR if IR detected (if cluster member)
1486-1494 E9.3 solMass/yr SFRcl0 ? SFR lower limit from UV alone
(if no-IR, if cluster member)
1496-1504 E9.3 solMass/yr SFRcl1 ? SFR upper limit from UV alone
(if no-IR, if cluster member)
1506 I1 --- SED [1/3]? SED type (6)
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Note (1): COMBO-17 photometry flags:
* bit 0-7 (corresponding to values 0-128) are original SExtractor flags
* bit 9 (from COMBO-17) indicates only potential problem from bright
neighbours or reflexes from the optics (check images),
* bit 10 (from COMBO-17) indicates uncorrected hot pixels,
* bit 11 (from COMBO-17) is set interactively when photometry is erroneous
Note (2): Stages flags as follows:
0 = Not in STAGES footprint (only in COMBO-17)
1 = In STAGES footprint, but not detected by STAGES (only in COMBO-17)
2 = Detected by STAGES, but not HST extended source
3 = HST-extended source, but GALFIT ran into constraint
4 = HST-extended source, but GALFIT successful
Note (3): COMBO flag as follows:
0 = Not in COMBO-17 footprint (only in STAGES)
1 = In COMBO-17 footprint, but not detected by COMBO-17 (only in STAGES)
2 = Detected by COMBO-17, but neither galaxy, nor cluster, nor WGM05
3 = Galaxy but neither cluster, nor WGM05
4 = Cluster galaxy, but not WGM05
5 = Cluster galaxy in WGM05
Note (4): MIPS flags as follows:
0 = Detected only by STAGES
1 = Detected by COMBO-17, but outside MIPS footprint
2 = Detected by COMBO-17 and inside MIPS footprint,
but not detected by MIPS
3 = Detected by COMBO-17 and detected by MIPS
Note (5): mcclass as follows:
Star = Stars (only point sources)
WDwarf = White dwarf (only point sources)
Galaxy = Galaxies (shape irrelevant)
Galaxy (Star?) = Binary or low-z galaxy
(star SED but extended; ambiguous colour space)
Galaxy (Uncl!) = SED fit undecided (most often galaxy)
QSO = QSOs (only point sources)
QSO (Galaxy?) = Seyfert-1 AGN or interloping galaxy
(AGN SED but extended; ambiguous colour space)
Strange object = Unusual strange spectrum (chi2red>30)
Note (6): SED type takes the following values:
1 = old red
2 = dusty red
3 = blue cloud
Note (7): Ages are encoded in a template number running from 0 (youngest)
to 59 (oldest)
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Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 I2 --- Tile [1/80] Tile number
4- 13 A10 "DD/MM/YYYY" Date Observation date
15- 16 I2 h RAh Right ascension (J2000)
18- 19 I2 min RAm Right ascension (J2000)
21- 24 F4.1 s RAs Right ascension (J2000)
26 A1 --- DE- Declination sign (J2000)
27- 28 I2 deg DEd Declination (J2000)
30- 31 I2 arcmin DEm Declination (J2000)
33- 34 I2 arcsec DEs [0,60] Declination (J2000)
36- 39 I4 s ExpTime Exposure time
41- 44 I4 --- Nhot Number of hot SEXtractor configuration
46- 48 I3 --- Ncold Number of cold SEXtractor configuration
50- 53 I4 --- Ngood Number of good SEXtractor configuration
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Byte-by-byte Description of file: table4.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 nm lamc Central wavelength of filter
4 A1 --- --- [/]
5- 7 I3 nm FWHM Filter width
9 A1 --- Filt [UBVRI] Filter name
12- 16 I5 s ExpTime Exposition time
19- 22 F4.2 arcsec Seeing Seeing
24- 27 F4.1 mag maglim 10σ (Vega) magnitude limits
29- 32 A4 --- Run [AEG, ] Observing run code(s) (1)
35- 39 F5.2 mag Mag Magnitude of Vega (in AB system)
42- 46 F5.3 10+8/m2/nm/s Flux Photon flux of Vega in filter
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Note (1): COMBO-17 observing runs with A901/2 imaging:
A = 1999/02/11-1999/02/22
E = 2000/01/28-2000/02/11
G = 2001/01/19-2001/01/20
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Global notes:
Note (G1): Nomenclature note:
* STAGES sources identified as STAGES FF-NNNN,
* COMBO-17 sources identified as
COMBO JHHMMSSs+DDMMSS = [GWB2009] NNNNN
--------------------------------------------------------------------------------
History:
Copied at http://www.nottingham.ac.uk/astronomy/stages/astro_data.html
* 30-Jan-2010: reformatted (impossible values truncated).
(End) Patricia Vannier [CDS] 20-Oct-2009