J/ApJ/796/60 ECDFS galaxies photometric redshifts & counterparts (Hsu+, 2014) ================================================================================ CANDELS/GOODS-S, CDFS, and ECDFS: photometric redshifts for normal and X-ray-detected galaxies. Hsu L.-T., Salvato M., Nandra K., Brusa M., Bender R., Buchner J., Donley J.L., Kocevski D.D., Guo Y., Hathi N.P., Rangel C., Willner S.P., Brightman M., Georgakakis A., Budavari T., Szalay A.S., Ashby M.L.N., Barro G., Dahlen T., Faber S.M., Ferguson H.C., Galametz A., Grazian A., Grogin N.A., Huang K.-H., Koekemoer A.M., Lucas R.A., Mcgrath E., Mobasher B., Peth M., Rosario D.J., Trump J.R. =2014ApJ...796...60H (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Cross identifications ; X-ray sources ; Photometry, UBVRI ; Photometry, infrared ; Ultraviolet ; Redshifts ; Surveys Keywords: galaxies: active; galaxies: distances and redshifts; galaxies: photometry; X-rays: galaxies Abstract: We present photometric redshifts and associated probability distributions for all detected sources in the Extended Chandra Deep Field South (ECDFS). This work makes use of the most up-to-date data from the Cosmic Assembly Near-IR Deep Legacy Survey (CANDELS) and the Taiwan ECDFS Near-Infrared Survey (TENIS) in addition to other data. We also revisit multi-wavelength counterparts for published X-ray sources from the 4Ms CDFS and 250ks ECDFS surveys, finding reliable counterparts for 1207 out of 1259 sources (~96%). Data used for photometric redshifts include intermediate-band photometry deblended using the TFIT method, which is used for the first time in this work. Photometric redshifts for X-ray source counterparts are based on a new library of active galactic nuclei/galaxy hybrid templates appropriate for the faint X-ray population in the CDFS. Photometric redshift accuracy for normal galaxies is 0.010 and for X-ray sources is 0.014 and outlier fractions are 4% and 5.2%, respectively. The results within the CANDELS coverage area are even better, as demonstrated both by spectroscopic comparison and by galaxy-pair statistics. Intermediate-band photometry, even if shallow, is valuable when combined with deep broadband photometry. For best accuracy, templates must include emission lines. Description: The main product of this work is photometric redshifts for all sources detected in the CANDELS/GOODS-S, CDFS, and ECDFS area, a total of 105150 sources. This work has improved upon prior catalogs by Guo+ (2013, J/ApJS/207/24), Cardamone+ (2010, J/ApJS/189/270), and Hsieh+ (2012ApJS..203...23H) by using the most up-to-date photometry and SED template libraries including separate libraries for X-ray sources of different characteristics. Probabilities of association between X-ray sources and optical/NIR/MIR sources are also provided. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table8.dat 256 105176 *Cross ID catalog for all the sources in ECDFS area table9.dat 132 1259 X-ray source list in ECDFS region table10.dat 860 1502 Photometry of the Optical/NIR/MIR sources associated to the X-ray detections in ECDFS table11a.dat 132 1207 Redshift catalog for the optical/NIR/MIR to X-ray counterparts with the maximum posterior table11b.dat 132 590 Redshift catalog for the X-ray sources with multiple optical/NIR/MIR counterparts -------------------------------------------------------------------------------- Note on table8.dat: The sources with possible X-ray associations are flagged. -------------------------------------------------------------------------------- See also: II/261 : GOODS initial results (Giavalisco+, 2004) J/A+A/421/41 : FORS Deep Field UV to blue photometry (Gabasch+, 2004) J/A+A/418/885 : The FORS Deep Field Spectroscopic Survey (Noll+, 2004) J/ApJS/155/73 : Photometric redshifts of X-ray sources in CDF-S (Zheng+, 2004) J/ApJS/161/21 : Extended Chandra Deep Field-South survey (Lehmer+, 2005) J/A+A/449/951 : GOODS-MUSIC sample: multicolour catalog (Grazian+, 2006) J/AJ/131/2373 : Extended Chandra Deep Field-South survey (Virani+, 2006) J/ApJ/663/81 : SED of hard X-ray selected AGN in XMDS (Polletta+, 2007) J/ApJ/682/985 : FIREWORKS photometry of GOODS CDF-S (Wuyts+, 2008) J/A+A/497/635 : XMM wide-field survey in COSMOS field (Cappelluti+, 2009) J/ApJS/184/158 : Chandra COSMOS survey I. (Elvis+, 2009) J/ApJS/180/102 : AEGIS-X: Chandra deep survey (Laird+, 2009) J/ApJS/189/270 : MUSYC optical imaging in ECDF-S (Cardamone+, 2010) J/ApJS/187/560 : Photometric redshifts of the 2Ms CDF-S (Luo+, 2010) J/ApJ/727/1 : IRAC/MUSYC SIMPLE survey (Damen+, 2011) J/ApJ/742/61 : Photo. redshift of AGNs from XMM- and C-COSMOS (Salvato+ 2011) J/ApJS/195/10 : The CDF-S survey: 4Ms source catalogs (Xue+, 2011) J/ApJS/201/30 : The Chandra COSMOS survey. III. (Civano+, 2012) J/ApJS/198/1 : Photometry catalogs for the Lockman Hole (Fotopoulou+, 2012) J/ApJ/769/80 : Spitzer/IRAC observations of five deep fields (Ashby+, 2013) J/ApJS/207/24 : GOODS-S CANDELS multiwavelength catalog (Guo+, 2013) J/ApJS/209/30 : MYStIX project: Bayesian matching (Naylor+, 2013) J/MNRAS/428/3089 : X-ray properties of BzK-selected galaxies (Rangel+, 2013) http://www.mpe.mpg.de/XraySurveys/CDFS/ : X-ray surveys at MPE, CDFS main page Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- [HSN2014] [1/105176] Running sequence number 8- 12 I5 --- CANDELS [1/34930]?=-99 ID from the CANDELS catalog (G1) 14- 23 F10.6 deg RACdeg [/53.3]?=-99 CANDELS right ascension (J2000) 25- 34 F10.6 deg DECdeg [/-27.6]?=-99 CANDELS declination (J2000) 36- 40 I5 --- MUSYC [0/84401]?=-99 ID from the MUSYC catalog (G1) 42- 51 F10.6 deg RAMdeg [/53.5]?=-99 MUSYC right ascension (J2000) 53- 62 F10.6 deg DEMdeg [/-27.5]?=-99 MUSYC declination (J2000) 64- 68 I5 --- TENIS [6/62326]?=-99 ID from the TENIS catalog (G1) 70- 79 F10.6 deg RATdeg [/53.5]?=-99 TENIS right ascension (J2000) 81- 90 F10.6 deg DETdeg [/-27.5]?=-99 TENIS declination (J2000) 92- 96 I5 --- SIMPLE [4985/54262]?=-99 ID from the SIMPLE catalog (G1) 98-107 F10.6 deg RASdeg [/53.5]?=-99 TENIS right ascension (J2000) 109-118 F10.6 deg DESdeg [/-27.5]?=-99 TENIS declination (J2000) 120-122 I3 --- R13 [1/570]?=-99 ID from R13 4Ms-CDFS catalog (G1) 124-133 F10.6 deg RARdeg [/53.4]?=-99 R13 right ascension (J2000) 135-144 F10.6 deg DERdeg [/-27.6]?=-99 R13 declination (J2000) 146-151 F6.2 --- errR13 [0.1/1.4]?=-99 Positional error from R13 153-155 I3 --- X11 [2/740]?=-99 ID from X11 4Ms-CDFS catalog (G1) 157-166 F10.6 deg RAXdeg [/53.4]?=-99 X11 right ascension (J2000) 168-177 F10.6 deg DEXdeg [/-27.6]?=-99 X11 declination (J2000) 179-183 F5.1 --- errX11 [0.1/1.5]?=-99 Positional error from X11 185-187 I3 --- L05 [2/762]?=-99 ID from L05 250ks-ECDFS catalog (G1) 189-197 F9.5 deg RALdeg [/53.5]?=-99 L05 right ascension (J2000) 199-207 F9.5 deg DELdeg [/-27.5]?=-99 L05 declination (J2000) 209-213 F5.1 --- errL05 [0.6/2.2]?=-99 Positional error from L05 215-217 I3 --- V06 [2/651]?=-99 ID from V06 250ks-ECDFS catalog (G1) 219-227 F9.5 deg RAVdeg [/53.5]?=-99 V06 right ascension (J2000) 229-237 F9.5 deg DEVdeg [/-27.5]?=-99 V06 declination (J2000) 239-244 F6.2 --- errV06 [0.1/3]?=-99 Positional error from V06 246-248 I3 --- Flag [-99/7] Flag on counterpart (G2) 250-256 F7.3 --- Prob [-99/1] Posterior value (p) (G3) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- R13 [1/571]?=-99 ID from R13 4Ms-CDFS catalog (G1) 5- 7 I3 --- X11 [1/740]?=-99 ID from X11 4Ms-CDFS catalog (G1) 9- 11 I3 --- L05 [1/762]?=-99 ID from L05 250ks-ECDFS (G1) 13- 15 I3 --- V06 [1/651]?=-99 ID from V06 250ks-ECDFS (G1) 17- 25 F9.6 deg RAdeg [52.7/53.5] Right ascension of the X-ray source (J2000) (1) 27- 36 F10.6 deg DEdeg [-28.2/-27.5] Declination of the X-ray source (J2000) (1) 38- 46 E9.3 10-3W/m2 F0.5-2 Soft band X-ray flux (0.5-2keV; in unit of erg/cm^2^/s) (1) 48- 56 E9.3 10-3W/m2 F2-8 Hard band X-ray flux (2-8keV; in unit of erg/cm^2^/s) (1) 58- 66 E9.3 10-3W/m2 F0.5-8 Full band X-ray flux (0.5-8keV; in unit of erg/cm^2^/s) (1) 68- 74 F7.3 10-7W L0.5-2 [35.3/45]?=-99 Soft band X-ray luminosity (0.5-2keV; in unit of erg/s) (2) 76- 82 F7.3 10-7W L2-8 [38.8/45.2]?=-99 Hard band X-ray luminosity (2-8keV; in unit of erg/s) (2) 84- 90 F7.3 10-7W L0.5-8 [35.6/45.4]?=-99 Full band X-ray luminosity (0.5-8keV; in unit of erg/s) (2) 92- 98 F7.3 10-7W L2-10 [38.9/45.3]?=-99 2-10keV hard band X-ray luminosity (2) 100-107 F8.4 --- zbest [0/6.9]?=-99 Redshift used to calculate Lx (3) 109-116 F8.4 --- zspec [0.001/4.8]?=-99 Spectroscopic redshift (N. Hathi, private communication) 118-125 F8.4 --- zphot [0/6.9]?=-99 Photometric redshift (4) 127-132 I6 --- [HSN2014] [125/105176]?=-99 ID of the Optical/NIR/MIR counterpart to the X-ray sources as listed in Hsu+ 2014 (this paper) -------------------------------------------------------------------------------- Note (1): We chose the original X-ray data from, in order of priority, R13, X11, L05 and V06. Note (2): The X-ray luminosity is the rest-frame luminosity uncorrected for absorption. Lx=4*pi*luminosityDistance^2*fx*(1+zbest)^(gamma-2), where gamma=1.4 Note (3): We used reliable spec-z if available, otherwise photo-z as in Hsu+ 2014 (this work). Note (4): Check the detail information in the photo-z catalog (table 11). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- [HSN2014] [72/105150] Sequential number adopted in this work 8- 10 I3 --- R13 [1/570]?=-99 ID from R13 4Ms-CDFS catalog (G1) 12- 14 I3 --- X11 [1/740]?=-99 ID from X11 4Ms-CDFS catalog (G1) 16- 18 I3 --- L05 [2/756]?=-99 ID from L05 250ks-ECDFS (G1) 20- 22 I3 --- V06 [2/651]?=-99 ID from V06 250ks-ECDFS (G1) 24 I1 --- Flag [1/7] Flag on counterpart (G2) 26- 32 F7.3 --- Prob [0.6/1] Posterior value (p) (G3) 34- 45 F12.9 deg RAdeg [52.8/53.5] Opt/NIR/MIR right ascension (J2000) (1) 47- 59 F13.9 deg DEdeg [-28.1/-27.5] Opt/NIR/MIR declination (J2000) (1) 61- 67 F7.3 mag FUVmag [19.8/26]?=-99 GALEX FUV AB magnitude (2) 69- 75 F7.3 mag e_FUVmag [/0.5]?=-99 FUVmag uncertainty 77- 83 F7.3 mag NUVmag [15/27]?=-99 GALEX NUV AB magnitude (2) 85- 91 F7.3 mag e_NUVmag [/0.7]?=-99 NUVmag uncertainty 93- 99 F7.3 mag UCTIO [17.5/32]?=-99 Blanco/Mosaic-II U-band AB magnitude (2) 101-107 F7.3 mag e_UCTIO [0/17]?=-99 UCTIO uncertainty 109-115 F7.3 mag UVIMOS [17.7/35.4]?=-99 VLT/VIMOS U-band AB magnitude (2) 117-123 F7.3 mag e_UVIMOS [/35]?=-99 UVIMOS uncertainty 125-131 F7.3 mag F435W [17.5/35]?=-99 HST/ACS F435W AB magnitude (2) 133-139 F7.3 mag e_F435W [/263]?=-99 F435W uncertainty 141-147 F7.3 mag F606W [16/31]?=-99 HST/ACS F606W AB magnitude (2) 149-155 F7.3 mag e_F606W [0/5]?=-99 F606W uncertainty 157-163 F7.3 mag F775W [15.9/32]?=-99 HST/ACS F775W AB magnitude (2) 165-171 F7.3 mag e_F775W [0/24]?=-99 F775W uncertainty 173-179 F7.3 mag F814W [15.6/32]?=-99 HST/ACS F814W AB magnitude (2) 181-187 F7.3 mag e_F814W [0/41]?=-99 F814W uncertainty 189-195 F7.3 mag F850LP [15.5/30]?=-99 HST/ACS F850LP AB magnitude (2) 197-203 F7.3 mag e_F850LP [0/5]?=-99 F850LP uncertainty 205-211 F7.3 mag F098M [16/30]?=-99 HST/WFC3 F098M AB magnitude (2) 213-219 F7.3 mag e_F098M [0/6]?=-99 F098M uncertainty 221-227 F7.3 mag F105W [15/29]?=-99 HST/WFC3 F105W AB magnitude (2) 229-235 F7.3 mag e_F105W [0/4]?=-99 F105W uncertainty 237-243 F7.3 mag F125W [15/32]?=-99 HST/WFC3 F125W AB magnitude (2) 245-251 F7.3 mag e_F125W [0/6]?=-99 F125W uncertainty 253-259 F7.3 mag F140W [14/29]?=-99 HST/WFC3 F140W AB magnitude (2) 261-267 F7.3 mag e_F140W [0/3]?=-99 F140W uncertainty 269-275 F7.3 mag F160W [14.8/27.5]?=-99 HST/WFC3 F160W AB magnitude (2) 277-283 F7.3 mag e_F160W [0/0.4]?=-99 F160W uncertainty 285-291 F7.3 mag KsISAAC [14.8/29]?=-99 VLT/ISAAC Ks-band AB magnitude (2) 293-299 F7.3 mag e_KsISAAC [0/9]?=-99 KsISAAC uncertainty 301-307 F7.3 mag KsHAWKI [15.9/30]?=-99 VLT/HAWK-I Ks-band AB magnitude (2) 309-315 F7.3 mag e_KsHAWKI [0/5]?=-99 KsHAWKI uncertainty 317-323 F7.3 mag IA427 [12.7/32]?=-99 Subaru IA427 AB magnitude (2) 325-331 F7.3 mag e_IA427 [0/42]?=-99 IA427 uncertainty 333-339 F7.3 mag IA445 [14.8/33]?=-99 Subaru IA445 AB magnitude (2) 341-347 F7.3 mag e_IA445 [0/88]?=-99 IA445 uncertainty 349-355 F7.3 mag IA464 [13/32]?=-99 Subaru IA464 AB magnitude (2) 357-363 F7.3 mag e_IA464 [0/98]?=-99 IA464 uncertainty 365-371 F7.3 mag IA484 [16.5/34]?=-99 Subaru IA484 AB magnitude (2) 373-379 F7.3 mag e_IA484 [0/135]?=-99 IA484 uncertainty 381-387 F7.3 mag IA505 [13/31]?=-99 Subaru IA505 AB magnitude (2) 389-395 F7.3 mag e_IA505 [0/16]?=-99 IA505 uncertainty 397-403 F7.3 mag IA527 [16/32]?=-99 Subaru IA527 AB magnitude (2) 405-411 F7.3 mag e_IA527 [0/18]?=-99 IA527 uncertainty 413-419 F7.3 mag IA550 [14.8/31]?=-99 Subaru IA550 AB magnitude (2) 421-427 F7.3 mag e_IA550 [0/12]?=-99 IA550 uncertainty 429-435 F7.3 mag IA574 [13.8/34]?=-99 Subaru IA574 AB magnitude (2) 437-443 F7.3 mag e_IA574 [0/255]?=-99 IA574 uncertainty 445-451 F7.3 mag IA598 [14.6/32]?=-99 Subaru IA598 AB magnitude (2) 453-459 F7.3 mag e_IA598 [0/11]?=-99 IA598 uncertainty 461-467 F7.3 mag IA624 [14/35]?=-99 Subaru IA624 AB magnitude (2) 469-475 F7.3 mag e_IA624 [0/265]?=-99 IA624 uncertainty 477-483 F7.3 mag IA651 [14.7/32]?=-99 Subaru IA651 AB magnitude (2) 485-491 F7.3 mag e_IA651 [0/11]?=-99 IA651 uncertainty 493-499 F7.3 mag IA679 [15/32]?=-99 Subaru IA679 AB magnitude (2) 501-507 F7.3 mag e_IA679 [0/23]?=-99 IA679 uncertainty 509-515 F7.3 mag IA709 [14.5/32]?=-99 Subaru IA709 AB magnitude (2) 517-523 F7.3 mag e_IA709 [0/135]?=-99 IA709 uncertainty 525-531 F7.3 mag IA738 [14.7/31]?=-99 Subaru IA738 AB magnitude (2) 533-539 F7.3 mag e_IA738 [0/6]?=-99 IA738 uncertainty 541-547 F7.3 mag IA767 [14.9/31]?=-99 Subaru IA767 AB magnitude (2) 549-555 F7.3 mag e_IA767 [0/15]?=-99 IA767 uncertainty 557-563 F7.3 mag IA797 [15/33]?=-99 Subaru IA797 AB magnitude (2) 565-571 F7.3 mag e_IA797 [0/136]?=-99 IA797 uncertainty 573-579 F7.3 mag IA827 [15/33]?=-99 Subaru IA827 AB magnitude (2) 581-587 F7.3 mag e_IA827 [0/411]?=-99 IA827 uncertainty 589-595 F7.3 mag IA856 [14.7/32]?=-99 Subaru IA856 AB magnitude (2) 597-603 F7.3 mag e_IA856 [0/89]?=-99 IA856 uncertainty 605-611 F7.3 mag U38mag [13.9/31]?=-99 WFI/ESO MPG U38 AB magnitude (2) 613-619 F7.3 mag e_U38mag [0/11]?=-99 U38mag uncertainty 621-627 F7.3 mag Umag [14/31]?=-99 ESO MPG/WFI U-band AB magnitude (2) 629-635 F7.3 mag e_Umag [0/6]?=-99 Umag uncertainty 637-643 F7.3 mag Bmag [14.5/30]?=-99 ESO MPG/WFI B-band AB magnitude (2) 645-651 F7.3 mag e_Bmag [0/2]?=-99 Bmag uncertainty 653-659 F7.3 mag Vmag [14/30]?=-99 ESO MPG/WFI V-band AB magnitude (2) 661-667 F7.3 mag e_Vmag [0/2]?=-99 Vmag uncertainty 669-675 F7.3 mag Rmag [14/27]?=-99 ESO MPG/WFI R-band AB magnitude (2) 677-683 F7.3 mag e_Rmag [0/2]?=-99 Rmag uncertainty 685-691 F7.3 mag Imag [14/27]?=-99 ESO MPG/WFI I-band AB magnitude (2) 693-699 F7.3 mag e_Imag [0/2]?=-99 Imag uncertainty 701-707 F7.3 mag zmag [12/28]?=-99 Blanco/Mosaic-II z-band AB magnitude (2) 709-715 F7.3 mag e_zmag [0/5]?=-99 zmag uncertainty 717-723 F7.3 mag Jmag [10.8/31]?=-99 Blanco/ISPI J-band AB magnitude (2) 725-731 F7.3 mag e_Jmag [0/228]?=-99 Jmag uncertainty 733-739 F7.3 mag Hmag [5.9/32]?=-99 ESO NTT/SofI H-band AB magnitude (2) 741-747 F7.3 mag e_Hmag [0/319]?=-99 Hmag uncertainty 749-755 F7.3 mag Kmag [9.6/32]?=-99 Blanco/ISPI K-band AB magnitude (2) 757-763 F7.3 mag e_Kmag [0/560]?=-99 Kmag uncertainty 765-771 F7.3 mag JTENIS [13/28]?=-99 CFHT/WIRCam J-band AB magnitude (2) 773-779 F7.3 mag e_JTENIS [0/5]?=-99 JTENIS uncertainty 781-787 F7.3 mag KsTENIS [13/26]?=-99 CFHT/WIRCam Ks-band AB magnitude (2) 789-795 F7.3 mag e_KsTENIS [0/1]?=-99 KsTENIS uncertainty 797-803 F7.3 mag 3.6mag [12/32]?=-99 Spitzer/IRAC 3.6um SEDS AB magnitude (2) 805-811 F7.3 mag e_3.6mag [0/61]?=-99 3.6mag uncertainty 813-819 F7.3 mag 4.5mag [12.5/28]?=-99 Spitzer/IRAC 4.5um SEDS AB magnitude (2) 821-827 F7.3 mag e_4.5mag [0/3]?=-99 4.5mag uncertainty 829-835 F7.3 mag 5.8mag [12/34]?=-99 Spitzer/IRAC 5.8um GOODS AB magnitude (2) 837-844 F8.3 mag e_5.8mag [0/1911]?=-99 5.8mag uncertainty 846-852 F7.3 mag 8.0mag [13/30]?=-99 Spitzer/IRAC 8.0um GOODS AB magnitude (2) 854-860 F7.3 mag e_8.0mag [0/89]?=-99 8.0mag uncertainty -------------------------------------------------------------------------------- Note (1): R.A. (J2000) and Dec. (J2000) of the optical/NIR/MIR source associated to the X-ray detection. Note (2): Photometric data (table 1): ------------------------------------------------------------------------- Filter |lam |FWHM |5sigma Limiting |Instrument |Area | eff | | Depth | Telescope | |{AA} |{AA} | (AB mag) | | ------------------------------------------------------------------------- U-CTIO^a | 3734| 387|26.63 |Blanco/Mosaic-II|1 U-VIMOS^a | 3722| 297|27.97 |VLT/VIMOS |1 F435W^a | 4317| 920|28.95/30.55^b |HST/ACS |1 F606W^a | 5918| 2324|29.35/31.05^b |HST/ACS |1 F775W^a | 7693| 1511|28.55/30.85^b |HST/ACS |1 F814W^a | 8047| 1826|28.84 |HST/ACS |1 F850LP^a | 9055| 1236|28.55/30.25^b |HST/ACS |1 F098M^a | 9851| 1696|28.77 |HST/WFC3 |1 F105W^a |10550| 2916|27.45/28.45/29.45^c|HST/WFC3 |1 F125W^a |12486| 3005|27.66/28.34/29.78^c|HST/WFC3 |1 F140W^a |13635| 3947|26.89/29.84^d |HST/WFC3 |1 F160W^a |15370| 2874|27.36/28.16/29.74^c|HST/WFC3 |1 Ks-ISAAC^a |21605| 2746|25.09 |VLT/ISAAC |1 Ks-HAWKI^a |21463| 3250|26.45 |VLT/HAWK-I |1 3.6 mum-SEDS^a |35508| 7432|26.52 |Spitzer/IRAC |1 4.5 mum-SEDS^a |44960|10097|26.25 |Spitzer/IRAC |1 5.8 mum-GOODS^a |57245|13912|23.75 |Spitzer/IRAC |1 8.0 mum-GOODS^a |78840|28312|23.72 |Spitzer/IRAC |1 3.6 mum-SIMPLE^e|35508| 7432|23.89 |Spitzer/IRAC |2, 3 4.5 mum-SIMPLE^e|44960|10097|23.75 |Spitzer/IRAC |2, 3 5.8 mum-SIMPLE^e|57245|13912|22.42 |Spitzer/IRAC |2, 3 8.0 mum-SIMPLE^e|78840|28312|22.50 |Spitzer/IRAC |2, 3 U38^e | 3706| 357|25.33 |WFI/ESO MPG |2, 3 U^e | 3528| 625|25.86 |ESO MPG/WFI |2, 3 B^e | 4554| 915|26.45 |ESO MPG/WFI |2, 3 V^e | 5343| 900|26.27 |ESO MPG/WFI |2, 3 R^e | 6411| 1602|26.37 |ESO MPG/WFI |2, 3 I^e | 8554| 1504|24.30 |ESO MPG/WF |2, 3 z^e | 8989| 1285|23.69 |Blanco/Mosaic-II|2, 3 J^e |12395| 1620|22.44 |Blanco/ISPI |2, 3 H^e |16154| 2950|22.46 |ESO NTT/SofI |2, 3 K^e |21142| 3312|21.98 |Blanco/ISPI |2, 3 J^f |12481| 1588|24.50 |CFHT/WIRCam |2, 3 Ks^f |21338| 3270|23.90 |CFHT/WIRCam |2, 3 FUV^g | 1543| 228|25.69 |GALEX |1, 2, 3 NUV^g | 2278| 796|25.99 |GALEX |1, 2, 3 IA427^e,h | 4253| 210|25.01 |Subaru |1, 2, 3 IA445^e,h | 4445| 204|25.18 |Subaru |1, 2, 3 IA464^e,h | 4631| 216|24.38 |Subaru |1, 2, 3 IA484^e,h | 4843| 230|26.22 |Subaru |1, 2, 3 IA505^e,h | 5059| 234|25.29 |Subaru |1, 2, 3 IA527^e,h | 5256| 243|26.18 |Subaru |1, 2, 3 IA550^e,h | 5492| 276|25.45 |Subaru |1, 2, 3 IA574^e,h | 5760| 276|25.16 |Subaru |1, 2, 3 IA598^e,h | 6003| 297|26.05 |Subaru |1, 2, 3 IA624^e,h | 6227| 300|25.91 |Subaru |1, 2, 3 IA651^e,h | 6491| 324|26.14 |Subaru |1, 2, 3 IA679^e,h | 6778| 339|26.02 |Subaru |1, 2, 3 IA709^e,h | 7070| 321|24.52 |Subaru |1, 2, 3 IA738^e,h | 7356| 324|25.93 |Subaru |1, 2, 3 IA768^e,h | 7676| 366|24.92 |Subaru |1, 2, 3 IA797^e,h | 7962| 354|24.69 |Subaru |1, 2, 3 IA827^e,h | 8243| 339|23.60 |Subaru |1, 2, 3 IA856^e,h | 8562| 324|24.41 |Subaru |1, 2, 3 ------------------------------------------------------------------------- Notes: a = CANDELS-TFIT catalog (Guo+ 2013, J/ApJS/207/24). b = Measurements from two regions: GOODS-S and HUDF09. See the details in Guo+ (2013, J/ApJS/207/24). c = Measurements from three regions: CANDELS wide, CANDELS deep, and HUDF09. See Guo+ (2013, J/ApJS/207/24) for details. d = Measurements from two regions: 3D-HST and HUDF12. This is an updated version of Guo+ (2013, J/ApJS/207/24). e = MUSYC catalog (Cardamone+ 2010, J/ApJS/189/270). f = TENIS catalog (Hsieh+ 2012ApJS..203...23H). g = GALEX DR6/7. h = IB-TFIT catalog (J. L. Donley et al. 2014, in preparation). ------------------------------------------------------------------------- -------------------------------------------------------------------------------- Byte-by-byte Description of file: table11[ab].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- [HSN2014] [72/105176] Sequential number adopted in this work 8- 10 I3 --- R13 [1/570]?=-99 ID from R13 4Ms-CDFS catalog (G1) 12- 14 I3 --- X11 [1/740]?=-99 ID from X11 4Ms-CDFS catalog (G1) 16- 18 I3 --- L05 [2/762]?=-99 ID from L05 250ks-ECDFS (G1) 20- 22 I3 --- V06 [2/651]?=-99 ID from V06 250ks-ECDFS (G1) 24 I1 --- Flag [1/7] Flag on counterpart (G2) 26- 30 F5.3 --- Prob [0.6/1] Posterior value (p) (G3) 32- 40 F9.6 deg RAdeg [52.8/53.5] Right ascension of the optical/NIR/MIR counterpart (J2000) 42- 51 F10.6 deg DEdeg [-28.2/-27.5] Declination of the optical/NIR/MIR counterpart (J2000) 53- 60 F8.4 --- zspec [0.001/4.8]?=-99 Spectroscopic redshift (when available) 62- 64 I3 --- q_zspec [-99/3]? Quality of the spectroscopic redshift (0=High) (1) 66- 73 F8.4 --- zphot [0/6.7]?=-99 The photo-z value (zp) as defined by the minimum of chi^2^ 75- 80 F6.2 --- e_zphot [0/6]?=-99 Lower 1-sigma value of zp 82- 87 F6.2 --- E_zphot [0/7]?=-99 Upper 1-sigma value of zp 89- 94 F6.2 --- e_zphot3 [0/6]?=-99 Lower 3-sigma value of zp 96-101 F6.2 --- E_zphot3 [0/7]?=-99 Upper 3-sigma value of zp 103-109 F7.3 --- Area [0/100]?=-99 Normalized area under the curve P(z), computed between zp+-0.1(1+zp) 111-113 I3 --- Num [1/230]?=-99 Template number (2) 115-120 F6.2 --- zp2 [0/7]?=-99 Second solution in the photo-z (zp2) when the P(zp2) is above 5 122-128 F7.3 --- Area2 [0/82]?=-99 Normalized area under the curve P(z), computed between zp2+-0.1(1+zp2) 130-132 I3 --- Num2 [1/226]?=-99 Template number used for SED fitting for zp2 (as in col. Num) -------------------------------------------------------------------------------- Note (1): Quality of the spectroscopic redshift as follows: 0 = High, 1 = Good, 2 = Intermediate, 3 = Poor. -99 = Unavailable. Note (2): Template number used for SED fitting for the best photo-z solution listed in col zphot. 1- 48 are the templates from Lib-EXT; 101-130 are the templates from Lib-PT; 201-230 are the templates from S09; -------------------------------------------------------------------------------- Global notes: Note (G1): Reference of the publications: CANDELS = Guo et al. 2013, J/ApJS/207/24; <[GFG2013b] NNNNN> in Simbad. MUSYC = Cardamone et al., 2010, J/ApJS/189/270; <[CVU2010] NNNNN> in Simbad. TENIS = Hsieh et al. 2012ApJS..203...23H SIMPLE = Damen et al. 2011, J/ApJ/727/1; in Simbad. R13 = Rangel et al. 2013, J/MNRAS/428/3089; <[RNL2013] cdfs4Ms NNN> in Simbad. X11 = Xue et al. 2011, J/ApJS/195/10; <[XLB2011] NNN> in Simbad. L05 = Lehmer et al. 2005, J/ApJS/161/21; <[LBA2005] NNN> in Simbad. V06 = Virani et al. 2006, J/AJ/131/2373; <[VTU2006] NNN> in Simbad. Note (G2): Flag as below: 1 = the source is the only possible counterpart to an X-ray source n = (2 or more) indicates that the source is one of the n possible counterparts to a X-ray source -99 = the source is not associated to any Xray source. Note (G3): Posterior probability p value which indicates the reliability of the optical/NIR/MIR association to a X-ray source. We do not consider the association with p<0.7 to be reliable. See section 3.2 for further explanations. -------------------------------------------------------------------------------- History: Downloaded from http://www.mpe.mpg.de/XraySurveys/CDFS/ ================================================================================ (End) Emmanuelle Perret [CDS] 05-Apr-2017