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J/MNRAS/426/2342  ATLAS 5.5GHz survey of Chandra Deep Field South (Huynh+, 2012)

The ATLAS 5.5 GHz survey of the extended Chandra Deep Field South: catalogue, source counts and spectral indices. Huynh M.T., Hopkins A.M., Lenc E., Mao M.Y., Middelberg E., Norris R.P., Randall K.E. <Mon. Not. R. Astron. Soc., 426, 2342-2358 (2012)> =2012MNRAS.426.2342H
ADC_Keywords: Surveys ; Galaxy catalogs ; Radio sources ; Morphology Keywords: galaxies: evolution - radio continuum: galaxies Abstract: Star-forming galaxies are thought to dominate the sub-mJy radio population, but recent work has shown that low-luminosity active galactic nuclei (AGNs) can still make a significant contribution to the faint radio source population. Spectral indices are an important tool for understanding the emission mechanism of the faint radio sources. We have observed the extended Chandra Deep Field South at 5.5GHz using a mosaic of 42 pointings with the Australia Telescope Compact Array. Our image reaches an almost uniform sensitivity of ∼12Jy rms over 0.25deg2 with a restoring beam of 4.9"x2.0", making ATLAS 5.5GHz survey one of the deepest 6cm surveys to date. We present the 5.5GHz catalogue and source counts from this field. We take advantage of the large amount of ancillary data in this field to study the 1.4 to 5.5GHz spectral indices of the sub-mJy population. Description: We observed the eCDFS at 6 cm in two runs using the new Compact Array Broadband Backend (CABB; Wilson et al. 2011MNRAS.416..832W) with the full CABB 2048MHz bandwidth centred at 5.5GHz. The first run in 2009 August consisted of an initial set of 12 and 8h observations. A further 144h was allocated in 2010 January. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 101 142 The ATLAS 5.5 GHz catalogue
See also: J/AJ/131/2373 : Extended Chandra Deep Field-South survey (Virani+, 2006) J/ApJS/161/21 : Extended Chandra Deep Field-South survey (Lehmer+, 2005) J/ApJS/179/114 : VLA 1.4GHz survey of E-CDF-S (Miller+, 2008) J/ApJS/205/13 : VLA 1.4GHz survey of ECDF-S (DR2) (Miller+, 2013) J/ApJ/693/1713 : Spectroscopy of X-ray sources in ECDF-S (Treister+, 2009) J/MNRAS/411/505 : Sub-mm observations in Extended Chandra DFS (Chapin+, 2011) J/MNRAS/420/2190 : ECDFS sources with radio counterparts (Vattakunnel+, 2012) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq Sequential number 4 A1 --- m_Seq [abcd] indicates a component of a multiple source 7- 13 A7 --- --- [ATCDFS5] 15- 33 A19 --- Name ATCDFS5 IAU name, 35 I1 h RAh Right ascension (J2000) 37- 38 I2 min RAm Right ascension (J2000) 40- 44 F5.2 s RAs Right ascension (J2000) 46 A1 --- DE- Declination sign (J2000) 47- 48 I2 deg DEd Declination (J2000) 50- 51 I2 arcmin DEm Declination (J2000) 53- 56 F4.1 arcsec DEs Declination (J2000) 58- 64 F7.1 uJy Speak Peak source flux density at 5.5GHz 66- 70 F5.1 uJy e_Speak Uncertainty in peak source flux density 72- 78 F7.1 uJy Sint ?=0 Integrated flux density at 5.5GHz (1) 80 I1 --- Flag [0/1] Resolved flag (2) 82- 85 F4.2 arcsec Bmaj ?=0 Deconvolved major axis (2) 87- 90 F4.2 arcsec Bmin ?=0 Deconvolved minor axis (2) 92- 96 F5.1 deg PA [-90/90]? Deconvolved position angle, measured from north through east (2) 98-101 F4.1 uJy rms Local noise level
Note (1): Zero indicates that the source is not successfully deconvolved and hence no integrated flux density is given. Note (2): Zero indicates that the source is not successfully deconvolved.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 16-Apr-2013
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

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