Search catalogue
J/MNRAS/352/131 13+38 XMM-Newton/ROSAT 1.4GHz radio catalog (Seymour+, 2004)
Radio observations of the 13hXMM-Newton/ROSAT Deep X-ray Survey Area. Seymour N., Mchardy I.M., Gunn K.F. <Mon. Not. R. Astron. Soc., 352, 131-141 (2004)> =2004MNRAS.352..131S
ADC_Keywords: Surveys ; Galaxies, radio ; X-ray sources Keywords: surveys - galaxies: active - radio continuum: galaxies Abstract: In order to determine the relationship between the faint X-ray and faint radio source populations, and hence to help understand the X-ray and radio emission mechanisms in those faint source populations, we have made a deep 1.4-GHz Very Large Array radio survey of the 13h+38° XMMNewton/ROSAT X-ray Survey Area. From a combined data set of 10-h, B-configuration data and 14-h, A-configuration data, maps with 3.35-arcsec resolution and a noise limit of 7.5Jy were constructed. A complete sample of 449 sources was detected within a 30-arcmin diameter region above a 4 detection limit of 30Jy, at the map centre, making this one of the deepest radio surveys at this frequency. The differential source count shows a significant upturn at submilliJansky flux densities, similar to that seen in other deep surveys at 1.4GHz (e.g. the Phoenix survey, Cat. J/MNRAS/296/839), but larger than that seen in the Hubble Deep Field (HDF) which may have been selected to be underdense. This upturn is well modelled by the emergence of a population of medium-redshift star-forming galaxies which dominate at faint flux densities. The brighter source counts are well modelled by active galactic nuclei. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 71 449 1.4GHz source catalog in 13+38 XMM field
See also: B/xmm : XMM-Newton Observation Log (XMM-Newton SOC, 2002) VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998) J/A+A/424/371 : 1.4GHz First Look Survey (FLS) (Morganti+, 2004) J/MNRAS/342/802 : Chandra survey of 13-h XMM/ROSAT survey (McHardy+, 2003) J/MNRAS/296/839 : Phoenix Deep Survey: 1.4-GHz source counts (Hopkins+, 1998) Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [SMG2004] Sequential number 5- 6 I2 h RAh Right ascension (J2000.0) 8- 9 I2 min RAm Right ascension (J2000.0) 11- 16 F6.3 s RAs Right ascension (J2000.0) 18 A1 --- DE- Declination sign (J2000.0) 19- 20 I2 deg DEd Declination (J2000.0) 22- 23 I2 arcmin DEm Declination (J2000.0) 25- 29 F5.2 arcsec DEs Declination (J2000.0) 31- 34 F4.1 arcsec Theta Mean angular size 36- 41 F6.1 --- S/N Signal-to-noise ratio 43- 49 F7.1 uJy Speak Peak flux 1.4GHz density 51- 57 F7.1 uJy Sint Integrated flux 1.4GHz density 59- 63 F5.1 uJy e_Sint rms uncertainty on Sint
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 24-Feb-2005
| 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 |
© UDS/CNRS