J/ApJS/203/15     Counterparts to 1.4GHz sources in ECDF-S     (Bonzini+, 2012)

The sub-mJy radio population of the E-CDFS: optical and infrared counterpart identification. Bonzini M., Mainieri V., Padovani P., Kellermann K.I., Miller N., Rosati P., Tozzi P., Vattakunnel S., Balestra I., Brandt W.N., Luo B., Xue Y.Q. <Astrophys. J. Suppl. Ser., 203, 15 (2012)> =2012ApJS..203...15B 2012ApJS..203...15B
ADC_Keywords: Radio sources ; Cross identifications ; X-ray sources ; Redshifts ; Surveys ; Photometry, infrared ; Photometry, RI Keywords: cosmology: observations - galaxies: active - galaxies: starburst - radio continuum: galaxies Abstract: We study a sample of 883 sources detected in a deep Very Large Array survey at 1.4GHz in the Extended Chandra Deep Field South. This paper focuses on the identification of their optical and infrared (IR) counterparts. We use a likelihood-ratio technique that is particularly useful when dealing with deep optical images to minimize the number of spurious associations. We find a reliable counterpart for 95% of our radio sources. Most of the counterparts (74%) are detected at optical wavelengths, but there is a significant fraction (21%) that are only detectable in the IR. Combining newly acquired optical spectra with data from the literature, we are able to assign a redshift to 81% of the identified radio sources (37% spectroscopic). We also investigate the X-ray properties of the radio sources using the Chandra 4Ms and 250ks observations. In particular, we use a stacking technique to derive the average properties of radio objects undetected in the Chandra images. The results of our analysis are collected in a new catalog containing the position of the optical/IR counterpart, the redshift information, and the X-ray fluxes. It is the deepest multi-wavelength catalog of radio sources, which will be used for future study of this galaxy population. Description: The E-CDFS was observed at 1.4GHz with the VLA between 2007 June and September (Miller et al. 2008, Cat. J/ApJS/179/114). The mosaic image covers an area of about 34x34arcmin with near-uniform sensitivity. The second data release (N. Miller et al. 2012, in preparation) provides a new source catalog with a 5σ point-source detection limit, for a total of 883 sources. We assigned a progressive identification number (RID) to the sources ordered by increasing right ascension. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 95 883 Radio information and identification process results table5.dat 123 839 Main characteristics and redshift information of the radio source counterparts -------------------------------------------------------------------------------- See also: II/261 : GOODS initial results (Giavalisco+, 2004) J/ApJS/195/10 : The CDF-S survey: 4Ms source catalogs (Xue+, 2011) J/ApJ/727/1 : IRAC/MUSYC SIMPLE survey (Damen+, 2011) J/ApJS/191/124 : Opt. spectroscopy of ECDF-S X-ray sources (Silverman+, 2010) J/ApJS/189/270 : MUSYC optical imaging in ECDF-S (Cardamone+, 2010) J/A+A/511/A50 : JHks of GOODS-South field (Retzlaff+, 2010) J/ApJ/693/1713 : Spectroscopy of X-ray sources in ECDF-S (Treister+, 2009) J/ApJS/183/295 : A K-selected catalog of the ECDFS from MUSYC (Taylor+, 2009) J/A+A/504/751 : GOODS-MUSIC catalog updated version (Santini+, 2009) J/A+A/478/83 : GOODS-South Field VLT/FORS2 redshifts. III. (Vanzella+, 2008) J/ApJS/179/114 : VLA 1.4GHz survey of E-CDF-S (Miller+, 2008) J/A+A/465/1099 : Redshift catalog of 691 objects in CDFS (Ravikumar+, 2007) J/AJ/132/2409 : Deep ATLAS radio observations of CDFS (Norris+, 2006) J/A+A/456/881 : EIS: infrared deep public survey (Olsen+, 2006) J/ApJS/161/21 : Extended Chandra Deep Field-South survey (Lehmer+, 2005) J/ApJS/155/271 : CDF-S: Optical spectroscopy (Szokoly+, 2004) J/A+A/428/1043 : Redshifts from VIMOS VLT Deep Survey (Le Fevre+, 2004) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- RID Radio source identification number 5 I1 h RAh [3] Radio Hour of Right Ascension (J2000) 7- 8 I2 min RAm [31/33] Radio Minute Right Ascension (J2000) 10- 14 F5.2 s RAs Radio Second of Right Ascension (J2000) 16 A1 --- DE- [-] Sign of the Radio Declination (J2000) 17- 18 I2 deg DEd [27/28] Radio Degree of Declination (J2000) 20- 21 I2 arcmin DEm Radio Arcminute of Declination (J2000) 23- 26 F4.1 arcsec DEs Radio Arcsecond of Declination (J2000) 28- 34 F7.1 uJy Sr [30.2/90450] Radio flux density at 1.4GHz 36- 40 F5.1 uJy e_Sr The 1σ error in Sr 42- 47 F6.1 --- S/N Signal-to-Noise 49 I1 h RACh ?=0 Counterpart Hour of Right Ascension (J2000) 51- 52 I2 min RACm ?=0 Counterpart Minute of Right Ascension (J2000) 54- 58 F5.2 s RACs ?=0 Counterpart Second of Right Ascension (J2000) 60 A1 --- DEC- [-] Sign of the Counterpart Declination (J2000) 61- 62 I2 deg DECd ?=0 Counterpart Degree of Declination (J2000) 64- 65 I2 arcmin DECm ?=0 Counterpart Arcminute of Declination (J2000) 67- 71 F5.2 arcsec DECs ?=0 Counterpart Arcsecond of Declination (J2000) 73- 77 F5.2 --- Rel [0.6/10]?=0 Reliability of the association (1) 79- 82 F4.1 arcsec Sep [0/2.3]?=99 Distance between radio and counterpart 84- 95 A12 --- CCat Counterpart catalog (2) -------------------------------------------------------------------------------- Note (1): After a careful analysis, we decided to consider as reliable only counterparts with reliability greater than 0.6. This threshold ensures that the expected number of spurious associations is below 5% for each auxiliary catalog. 9.00 = revisited association (see Section 3.4). See Sections 3.2 and 3.5 for further explanations. Note (2): Counterpart catalog, as in table 1, as follows: 24um-FIDEL = Spitzer/MIPS; Dickinson & FIDEL Team (2007AAS...211.5216D 2007AAS...211.5216D) IRAC-SIMPLE = Spitzer/IRAC; Damen et al. (2011, Cat. J/ApJ/727/1) Ks-MUSYC = CTIO 4m/ISPI; Taylor et al. (2009, Cat. J/ApJS/183/295; <[TFV2009] ECDFS NNNNN> for Simbad) Ks-ISAAC = ESO VLT/ISAAC; Retzlaff et al. (2010, Cat. J/A+A/511/A50) H-SOFI = ESO NTT/SOFI; Olsen et al. (2006, Cat. J/A+A/456/881) H-GNS = HST/NICMOS; Conselice et al. (2011MNRAS.413...80C 2011MNRAS.413...80C) z-GOODS = HST/ACS; Dickinson et al. (2003mglh.conf..324D) and Giavalisco et al. (2004, Cat. II/261; in Simbad) R-WFI = ESO 2.2m/WFI; Giavalisco et al. (2004, Cat. II/261) v-GEMS = HST/ACS; Rix et al. (2004ApJS..152..163R 2004ApJS..152..163R) and Caldwell et al. (2008ApJS..174..136C 2008ApJS..174..136C) U-VIMOS = ESO VLT/VIMOS; Nonino et al. (2009ApJS..183..244N 2009ApJS..183..244N) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- RID Radio identification number 5- 9 F5.2 mag Rmag [16.23/26.77]?=0 WFI catalog (Cat. II/261) R band AB magnitude 11- 15 F5.2 mag e_Rmag ?=0 Error in Rmag 17- 21 F5.2 mag Kmag [14.73/22.62]?=0 MUSYC catalog (Cat. J/ApJS/183/295) KS band AB magnitude 23- 26 F4.2 mag e_Kmag ?=0 Error in Kmag 28- 32 F5.2 mag [3.6] ?=0 SIMPLE catalog (Cat. J/ApJ/727/1) 3.6 micron band AB magnitude 34- 37 F4.2 mag e_[3.6] ?=0 Error in 3.6mag 39- 43 F5.2 --- z [0/6.99]?=99 Best redshift of counterpart (1) 45- 49 F5.2 --- zph ?=99 Photometric redshift 51- 55 F5.2 --- e_zph ?=99 Lower 68% uncertainty in zphot 57- 61 F5.2 --- E_zph ?=99 Upper 68% uncertainty in zphot 63- 68 A6 --- r_zph Reference for zphot (2) 70- 74 F5.2 mag zsp [0/4.5]?=99 Spectroscopic redshift 76 I1 --- q_zsp ?=0 Quality flag, 3=secure (3) 78- 82 A5 --- r_zsp Reference for zspec (4) 84- 91 E8.2 mW/m2 Soft ? Soft X-ray (0.5-2keV) band flux; erg/s/cm2 93-100 E8.2 mW/m2 e_Soft ? Error in Soft 102-109 E8.2 mW/m2 Hard ? Hard X-ray (2-10keV) band flux; erg/s/cm2 111-118 E8.2 mW/m2 e_Hard ? Error in Hard 120-123 I4 --- XID ? X-ray identifier (5) -------------------------------------------------------------------------------- Note (1): The best redshift is spectroscopic if q_zsp≥2, photometric otherwise. Note (2): Reference as follows: ZEB_pz = Rafferty et al. (2011ApJ...742....3R 2011ApJ...742....3R); C10_pz = Cardamone et al. (2010, cat. J/ApJS/189/270); S09_pz = Santini et al. (2009, Cat. J/A+A/504/751); KM_pz = Taylor et al. (2009, Cat. J/ApJS/183/295). Note (3): Quality flag as follows: 3 = secure redshift; 2 = reasonable redshift; 1 = one line detection or tentative redshift. Note (4): References for spectroscopic redshift, as in table 4, as follows: FORS = FORS2; Vanzella et al. 2008, Cat. J/A+A/478/83 GMASS = FORS2; Kurk et al. (2012arXiv1209.1561K 2012arXiv1209.1561K) K07 = Keck (N=32 zspec adopted); Silverman et al. 2010, Cat. J/ApJS/191/124 K08 = Keck (N=18 zspec adopted); Silverman et al. 2010, Cat. J/ApJS/191/124 N06 = 2dF; Norris et al. (2006, Cat. J/AJ/132/2409) P80 = VIMOS; Silverman et al. 2010, Cat. J/ApJS/191/124 P81 = VIMOS; this work R07 = VIMOS; Ravikumar et al. 2007, Cat. J/A+A/465/1099 S04 = FORS1/FORS2 (N=38 zspec adopted); Szokoly et al. 2004, Cat. J/ApJS/155/271 S04F = FORS1/FORS2 (N=1 zspec adopted); Szokoly et al. 2004, Cat. J/ApJS/155/271 T09 = VIMOS; Treister et al. 2009, Cat. J/ApJ/693/1713 VJB = VIMOS; Silverman et al. 2010, Cat. J/ApJS/191/124 VLR = VIMOS-LR; Balestra et al. 2010, Cat. J/A+A/512/A1 VMR = VIMOS-MR; Balestra et al. 2010, Cat. J/A+A/512/A1 VVDS = VIMOS; Le Fevre et al. 2004, Cat. J/A+A/428/1043 Note (5): Source of XID: * XID<1000: from Xue et al. 2011, Cat. J/ApJS/195/10; <[XLB2011] JHHMMSS.ss+DDMMSS.s> in Simbad. * XID>1000: from Lehmer et al. 2005, Cat. J/ApJS/161/21; <[LBA2005] NNN> in Simbad, where "NNN" is XID-1000. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 04-Dec-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line