J/MNRAS/441/2555    ATLAS 1.4GHz Data Release 2              (Hales+, 2014)

ATLAS 1.4GHz Data Release 2. I. Observations of the CDF-S and ELAIS-S1 fields and methods for constructing differential number counts. Hales C.A., Norris R.P., Gaensler B.M., Middelberg E., Chow K.E., Hopkins A.M., Huynh M.T., Lenc E., Mao M.Y. <Mon. Not. R. Astron. Soc., 441, 2555-2592 (2014)> =2014MNRAS.441.2555H 2014MNRAS.441.2555H
ADC_Keywords: Surveys ; Galaxy catalogs ; Radio sources Keywords: polarization - methods: data analysis - techniques: polarimetric - surveys - radio continuum: galaxies Abstract: This is the first of two papers describing the second data release (DR2) of the Australia Telescope Large Area Survey at 1.4GHz, which comprises deep wide-field observations in total intensity, linear polarization, and circular polarization over the Chandra Deep Field-South and European Large Area Infrared Space Observatory Survey-South 1 regions. DR2 improves upon the first data release by maintaining consistent data reductions across the two regions, including polarization analysis, and including differential number counts in total intensity and linear polarization. Typical DR2 sensitivities across the mosaicked multipointing images are 30µJy/beam at approximately 12"x6" resolution over a combined area of 6.4deg2. In this paper we present detailed descriptions of our data reduction and analysis procedures, including corrections for instrumental effects such as positional variations in image sensitivity, bandwidth smearing with a non-circular beam, and polarization leakage, and application of the BLOBCAT source extractor. We present the DR2 images and catalogues of components (discrete regions of radio emission) and sources (groups of physically associated radio components). We describe new analytic methods to account for resolution bias and Eddington bias when constructing differential number counts of radio components. Description: ATLAS observations of the CDF-S and ELAIS-S1 fields were obtained with the ATCA, a synthesis telescope consisting of six 22m alt-az antennas on an east-west baseline. Each antenna is equipped with linearly polarized feeds used to measure all four polarization products (XX, YY, XY, YX), from which all four Stokes parameters (I, Q, U, V) can be derived. Noise diodes in the feed horns of each antenna replace the need to observe a polarization position angle calibrator to derive absolute XY phase. We supplemented our 1.4GHz radio observations with data at infrared and optical wavelengths. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 144 2588 ATLAS 1.4GHz DR2 component catalogue tableb1.dat 355 2221 ATLAS 1.4GHz DR2 source catalogue -------------------------------------------------------------------------------- See also: II/253 : Chandra Deep Field South: multi-colour data (Wolf+, 2008) J/A+A/451/881 : ESIS BVR catalog, ELAIS-S1 (Berta+, 2006) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- ID Component identification number (1) 10- 16 A7 --- --- [ATLAS2_] 17- 36 A20 --- ATLAS2 Full component name (JHHMMSS.ss+DDMMSS.sA) (2) 38- 46 F9.6 deg RAdeg Right ascension (J2000) 48- 57 F10.6 deg DEdeg Declination (J2000) 59- 62 F4.2 arcsec e_RAdeg Error in right ascension 64- 67 F4.2 arcsec e_DEdeg Error in declination 69- 75 F7.2 --- SNR [5/9500] Signal to noise ratio of raw detection 77- 81 F5.3 mJy rms [0.01/0.1] Local rms noise value (in mJy/beam) 83- 86 F4.2 --- bws [0.8/1] Local bandwidth smearing value 88- 94 F7.3 mJy Speak [0.1/964] Peak 1.4GHz surface brightness corrected for bandwidth smearing (in mJy/beam) 96-101 F6.3 mJy e_Speak [0.01/50] Error in peak surface brightness (in mJy/beam) 103-110 F8.3 mJy Sint [0.08/1068] Integrated surface brightness 112-117 F6.3 mJy e_Sint Error in integrated surface brightness 119-123 F5.3 --- Varea [0/1] Visibility area 125 A1 --- l_theta Limit flag on theta (upper bound) 126-130 F5.2 arcsec theta [0/50] Deconvolved angular size or upper bound 132-135 F4.2 arcsec e_theta ?=- Error in deconvolved angular size 137-144 F8.3 mJy SML [0.1/1068] Deboosted flux density -------------------------------------------------------------------------------- Note (1): This gives the internal designation of the source used within our data processing. The form, FDbbbbCj, is a composite of three descriptors plus an optional fourth: * The first (F) is a single character that represents the ATLAS field: "C" for CDF-S, or "E" for ELAIS-S1. * The second descriptor (D) is a single character that represents the nature of detection: "T" for total intensity, or "L" for linear polarization. * The third descriptor (bbbb) is an integer (1 to 4 digits) that gives the blob identification number assigned by bolbcat. * The fourth descriptor (Cj) is only suffixed for those components that were obtained through refitting all or part of the original blob, using either IMFIT (denoted by Cj), or bolbca (denoted by Fj), for the jth extracted component from a given blob. Note (2): The form is ATLAS2_JHHMMSS.ss+DDMMSS.sT where ATLAS2 is the survey acronym, J specifies the J2000.0 coordinate equinox, HHMMSS.ss are the hours, minutes and truncated (not rounded) seconds of right ascension, + or - is the sign of declination, DDMMSS.s are the degrees, minutes and truncated seconds of declination, and the single final character specifier indicates the nature of detection as T (total) or L (Linear polarization). -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- ID Source identification number (1) 7- 13 A7 --- --- [ATLAS2_] 14- 33 A20 --- ATLAS2 Full component name (JHHMMSS.ss+DDMMSS.s) 34- 41 A8 --- I1 ?=0 ID of total intensity component 1 (2) 43- 50 A8 --- I2 ?=0 ID of total intensity component 2 (2) 52- 59 A8 --- I3 ?=0 ID of total intensity component 3 (2) 61- 68 A8 --- I4 ?=0 ID of total intensity component 4 (2) 70- 77 A8 --- I5 ?=0 ID of total intensity component 5 (2) 79- 86 A8 --- I6 ?=0 ID of total intensity component 6 (2) 88- 95 A8 --- L1 ?=0 ID of inear polarisation component 1 (2) 97-104 A8 --- L2 ?=0 ID of inear polarisation component 2 (2) 106-113 A8 --- L3 ?=0 ID of inear polarisation component 3 (2) 115-123 I9 --- Gr.A ?=999999999 Group A classifications (3) 125-133 I9 --- Gr.B ?=999999999 Group B classifications (3) 135-143 I9 --- Gr.C ?=999999999 Group C classifications (3) 145-152 F8.3 mJy AI ?=0 Group A total intensity flux density 154-159 F6.3 mJy e_AI ?=0 Group A error in total intensity flux density 161-166 F6.3 mJy AL ?=0 Group A linearly polarised flux density 168-172 F5.3 mJy e_AL ?=0 Group A error in linearly polarised flux density 174-181 F8.3 mJy BI ?=0 Group B total intensity flux density 183-188 F6.3 mJy e_BI ?=0 Group B error in total intensity flux density 190-195 F6.3 mJy BL ?=0 Group B linearly polarised flux density 197-201 F5.3 mJy e_BL ?=0 Group B error in linearly polarised flux density 203-209 F7.3 mJy CI ?=0 Group C total intensity flux density 211-216 F6.3 mJy e_CI ?=0 Group C error in total intensity flux density 218-223 F6.3 mJy CL ?=0 Group C linearly polarised flux density 225-229 F5.3 mJy e_CL ?=0 Group C error in linearly polarised flux density 231-237 A7 --- --- [SWIRE3_] 238-256 A19 --- SWIRE3 SWIRE-DR3 cross-matched source (JHHMMSS.ss+DDMMSS.s) 258-266 F9.6 deg RAdeg Right ascension (J2000) 268-277 F10.6 deg DEdeg Declination (J2000) 279-286 F8.3 mJy I [0.1/1355] Total intensity 1.4GHz flux density of source 288-293 F6.3 mJy e_I Error in total intensity flux density of source 295 A1 --- l_L Limit flag on L (upper bound) 296-301 F6.3 mJy L [0.1/59] Linearly polarised flux density of source or upper bound 303-307 F5.3 mJy e_L ?=- Error in linearly polarised flux density of source 309-316 F8.2 uJy S3.6 ?=0 SWIRE 3.6µm flux density 318-325 F8.2 uJy S4.5 ?=0 SWIRE 4.5µm flux density 327-334 F8.2 uJy S5.8 ?=0 SWIRE 5.8µm flux density 336-343 F8.2 uJy S8.0 ?=0 SWIRE 8.0µm flux density 345-353 F9.2 uJy S24 ?=0 SWIRE 24.0µm flux density 355 I1 --- Cl [0/9] Source classification: 0=AGN, 1=SFG (Star-Forming Galaxy), 2=star, 9=unknown -------------------------------------------------------------------------------- Note (1): This gives the internal designation of the source used within our data processing. The form Fnnnn is a composite of two descriptors: * The first (F) is a single character that represents the ATLAS field: "C" for CDF-S or "E" for ELAIS-S1. * The second descriptor (nnnn) is an integer (1 to 4 digits) that reflects the ordering of sources within each field. Note (2): Component identification number, ID, of tablea1.dat. Note (3): Component groupings and their type classifications according to the linear polarization-total intensity association scheme presented in Sect. 6.2. Up to 3 groups may be provided, labelled A, B, and C. Each group is specified by a 9-digit string, where from left to right each digit corresponds to the respective components given in columns I1-L3. If a component is not included in a particular group, then its respective digit is set to 9. All components belonging to a given group have their respective digit set to the type classification for that group. Group A always represents the collection of all components comprising the source. Groups B and C represent subsets of components. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 09-Feb-2015
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