J/ApJ/591/640     XMM-LSS low-frequency radio counterparts   (Cohen+, 2003)

The low-frequency radio counterpart of the XMM Large-Scale Structure Survey. Cohen A.S., Rottgering H.J.A., Kassim N.E., Cotton W.D., Perley R.A., Wilman R., Best P., Pierre M., Birkinshaw M., Bremer M., Zanichelli A. <Astrophys. J. 591, 640 (2003)> =2003ApJ...591..640C 2003ApJ...591..640C
ADC_Keywords: Clusters, galaxy ; Radio sources ; Morphology Keywords: cosmology: observations - galaxies: clusters: general - radio continuum: general Abstract: The XMM Large-Scale Structure Survey (XMM-LSS) is a major project to map the large-scale structure of the universe out to cosmological distances. An 8x8 region will be surveyed by XMM with planned optical follow-up to produce a three-dimensional map of many hundreds of clusters out to a redshift of z=1. To explore the relation of the large-scale structure to the location and properties of extragalactic radio sources, the XMM-LSS project also includes a low-frequency radio survey of this region. This combination will provide unprecedented insight into how the radio source formation and evolution are affected by the local environment. Here we present preliminary results from our 325 and 74MHz surveys in this region. At 325MHz, we have a flux limit of 4mJy/beam, a resolution of 6.3", and a total of 256 source detections over 5.6deg2. At 74MHz, we have a flux limit of 275mJy/beam, a resolution of 30", and a total of 211 source detections over 110deg2. We describe these results and explore what they tell us about the population of extragalactic low-frequency radio sources. The 74MHz survey represents the first presentation of a deep, subarcminute resolution survey at such a low frequency. This was made possible by recent advances in both hardware and data reduction algorithms, which we describe in detail. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 107 334 325MHz source list table3.dat 107 241 74MHz source list table4.dat 63 22 Objects with known redshifts refs.dat 123 12 References -------------------------------------------------------------------------------- See also: B/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2002) IX/37 : XMM-Newton Serendipitous Source Catalogue (1XMM) (XMM-SSC, 2003) Byte-by-byte Description of file: table2.dat table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- XMM-LSS Source name (JHHMM.m+DDMM) 13 A1 --- n_XMM-LSS [*] Indicates source detected at 74 and 325MHz 15- 16 I2 h RAh Hour of Right Ascension (J2000) 18- 19 I2 min RAm Minute of Right Ascension (J2000) 21- 25 F5.2 s RAs Second of Right Ascension (J2000) 27- 29 F3.1 arcsec e_RAs Error in Right Ascension 31 A1 --- DE- Sign of the Declination (J2000) 32- 33 I2 deg DEd Degree of Declination (J2000) 35- 36 I2 arcmin DEm Arcminute of Declination (J2000) 38- 41 F4.1 arcsec DEs Arcsecond of Declination (J2000) 43- 45 F3.1 arcsec e_DEs Error in Declination 47- 50 F4.2 deg Dist Distance from pointing center 52 A1 --- Type Source type (1) 54- 60 F7.2 mJy Flux Integrated flux (at 325MHz for table2, 74MHz for table3) 62- 66 F5.2 mJy e_Flux Uncertainty in Flux 68- 69 A2 --- l_MajAxis [≤ ] Indicates a 2σ upper limit for unresolved source on MajAxis 70- 74 F5.1 arcsec MajAxis ? Size of Major Axis (2) 76- 79 F4.1 arcsec e_MajAxis ? Error in MajAxis 81- 82 A2 --- l_MinAxis [≤ ] Indicates a 2σ upper limit for unresolved source on MinAxis 83- 86 F4.1 arcsec MinAxis ? Size of Minor Axis 88- 90 F3.1 arcsec e_MinAxis ? Error in MinAxis 92- 94 I3 deg PA ? Position Angle 96- 97 I2 deg e_PA ? Error in PA 99 A1 --- f_PA [N] Indicates not applicable 101 A1 --- l_alpha Limit flag on alpha 102-106 F5.2 --- alpha Spectral index with respect to NVSS 1.4GHz flux (3) -------------------------------------------------------------------------------- Note (1): Source type: S = Single source; M = Multiple source; C = Component of multiple source. Note (2): MaxAxis is the maximum separation between source components for multiple sources (Type = M). Note (3): alpha = α1400325 in table2, α140074 in table3. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- XMM-LSS Source name (JHHMM.m+DDMM) 14- 15 I2 h RAh Right ascension (J2000.0) 17- 18 I2 min RAm Right ascension (J2000.0) 20- 24 F5.2 s RAs Right ascension (J2000.0) 26 A1 --- DE- Declination sign (J2000.0) 27- 28 I2 deg DEd Declination (J2000.0) 30- 31 I2 arcmin DEm Declination (J2000.0) 33- 36 F4.1 arcsec DEs Declination (J2000.0) 38- 43 A6 --- Type Type (Galaxy or QSO) 46- 52 F7.5 --- z Redshift 54- 60 F7.5 -- e_z ? rms uncertainty on z 62- 63 I2 --- r_z Reference for redshift, in refs.dat file -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref Reference number 4- 22 A19 --- BibCode Bibcode 24- 44 A21 --- Aut Authotr's name 46-122 A77 --- Com Comments -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 22-Sep-2003
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