J/MNRAS/453/4244    Faint radio source population at 15.7GHz (Whittam+, 2015)

The faint radio source population at 15.7 GHz. II. Multi-wavelength properties. Whittam I.H., Riley J.M., Green D.A., Jarvis M.J., Vaccari M. <Mon. Not. R. Astron. Soc., 453, 4244-4263 (2015)> =2015MNRAS.453.4244W 2015MNRAS.453.4244W (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Radio sources ; Photometry ; Redshifts Keywords: catalogues - surveys - galaxies: active - radio continuum: galaxies Abstract: A complete, flux density limited sample of 96 faint (>0.5mJy) radio sources is selected from the 10C survey at 15.7GHz in the Lockman Hole. We have matched this sample to a range of multi-wavelength catalogues, including Spitzer Extragalactic Representative Volume Survey, Spitzer Wide-area Infrared Extragalactic survey, United Kingdom Infrared Telescope Infrared Deep Sky Survey and optical data; multi-wavelength counterparts are found for 80 of the 96 sources and spectroscopic redshifts are available for 24 sources. Photometric redshifts are estimated for the sources with multi-wavelength data available; the median redshift of the sample is 0.91 with an interquartile range of 0.84. Radio-to-optical ratios show that at least 94 per cent of the sample are radio loud, indicating that the 10C sample is dominated by radio galaxies. This is in contrast to samples selected at lower frequencies, where radio-quiet AGN and star-forming galaxies are present in significant numbers at these flux density levels. All six radio-quiet sources have rising radio spectra, suggesting that they are dominated by AGN emission. These results confirm the conclusions of that the faint, flat-spectrum sources which are found to dominate the 10C sample below ∼1mJy are the cores of radio galaxies. The properties of the 10C sample are compared to the Square Kilometre Array Design Studies Simulated Skies; a population of low-redshift star-forming galaxies predicted by the simulation is not found in the observed sample. Description: The work in Paper I (Whittam et al., 2013, Cat. J/MNRAS/429/2080) is based on a sample of sources selected from the 10C survey at 15.7GHz. In this paper we have studied the multi-wavelength properties of a complete sample of 96 sources selected from the 10C survey. This sample was matched to the Data Fusion multi-wavelength catalogue, which contains up to 10 photometric bands in the optical and mid-infrared, and counterparts were identified for 80 out of 96 10C Jsources. Spectroscopic redshifts are available for 24 sources. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 128 96 Multi-wavelength properties of the 96 10C sources studied in this paper tablea2.dat 93 24 References for the spectroscopic redshifts used in this work -------------------------------------------------------------------------------- See also: II/326 : Revised SWIRE photometric redshifts (Rowan-Robinson+, 2013) J/MNRAS/415/2708 : 10C survey of radio sources at 15.7GHz (Davies+, 2011) J/ApJS/198/1 : Photometry catalogs for the Lockman Hole (Fotopoulou+, 2012) J/MNRAS/429/2080 : Lockman Hole 10C sources radio spectral indices (Whittam+ 2013) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- --- [10C] 5- 18 A14 --- 10C 10C designation (JHHMMSS+DDMMSS) 20- 24 F5.2 mag gmag ?=- g magnitude (AB) 26- 30 F5.2 mag imag ?=- i magnitude (AB) 32- 36 F5.2 mag rmag ?=- r magnitude (AB) 38- 42 F5.2 mag zmag ?=- z magnitude (AB) 44- 48 F5.2 mag Jmag ?=- J magnitude (AB) 50- 54 F5.2 mag Kmag ?=- K magnitude (AB) 56- 62 F7.2 uJy FSERVS1 ? SERVS1 (3.6um) flux density 63 A1 --- n_FSERVS1 [*] *: value estimated from the SERVS image 64- 69 F6.2 uJy FSERVS2 ? SERVS2 (4.5um) flux density 71- 77 F7.2 uJy FSWIRE1 ? SWIRE1 (3.6um) flux density 79- 84 F6.2 uJy FSWIRE2 ? SWIRE2 (4.5um) flux density 86- 91 F6.2 uJy FSWIRE3 ?=- SWIRE3 (5.8um) flux density 93- 99 F7.2 uJy FSWIRE4 ?=- SWIRE4 (8.0um) flux density 101 I1 --- Flag [1/7] Optical matching flag (1) 103-106 F4.2 --- z ?=- Le PHARE redshift 108-111 F4.2 --- RR13z ? Redshift from Rowan-Robinson et al., (2013MNRAS.428.1958R 2013MNRAS.428.1958R, Cat. II/326) 113-116 F4.2 --- F12z ? Redshift from Fotopoulou et al. (2012, Cat. J/ApJS/198/1) 118-121 F4.2 --- zsp ? Spectroscopic redshift 123-126 F4.2 --- zBest ?=- Best redshift used in the analysis (2) 128 I1 --- f_z [1/4]? Origin of final redshift value flag (3) -------------------------------------------------------------------------------- Note (1): Optical matching flag as follows: 1 = extended, probable match 2 = extended, possible match 3 = extended, confused 4 = extended, no match 5 = compact, match 6 = compact, no match 7 = 10C position only Note (2): Final redshift value, description is given in Section 4.3. Note (3): Origin of final redshift value as follows: 1 = spectroscopic (see Table A2) 2 = RR13, Rowan-Robinson et al., 2013MNRAS.428.1958R 2013MNRAS.428.1958R, Cat. II/326 3 = F12, Fotopoulou et al. (2012, Cat. J/ApJS/198/1) 4 = LE PHARE -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- --- [10C] 5- 18 A14 --- 10C 10C designation (JHHMMSS+DDMMSS) 20- 23 F4.2 --- zsp Specroscopic redshift 25- 93 A69 --- r_zsp Reference for redshift -------------------------------------------------------------------------------- History: From electronic version of the journal References: Whittam et al., Paper I 2013MNRAS.429.2080W 2013MNRAS.429.2080W, Cat. J/MNRAS/429/2080
(End) Patricia Vannier [CDS] 21-Jun-2016
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