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J/AJ/125/2411       SIRTF First-Look Survey                  (Condon+, 2003)

The SIRTF first-look survey. I. VLA image and source catalog. Condon J.J., Cotton W.D., Yin Q.F., Shupe D.L., Storrie-Lombardi L.J., Helou G., Soifer B.T., Werner M.W. <Astron. J. 125, 2411 (2003)> =2003AJ....125.2411C (SIMBAD/NED BibCode)
ADC_Keywords: Radio sources ; Galaxies, radio ; Surveys Mission_Name: Spitzer Keywords: catalogs - galaxies: active - galaxies: starburst - infrared radiation - radio continuum - surveys Abstract: The First-Look Survey (FLS) of the Space Infrared Telescope Facility (SIRTF) will cover about 5deg2 centered on J2000.0 (17:18+59:30) in order to characterize the extragalactic infrared sky 2 orders of magnitude deeper than the IRAS survey. We expect that most of the FLS far-infrared (λ = 160, 70, and 24 µm) sources will be star-forming galaxies obeying the very tight far-infrared/radio correlation and will be continuum radio sources with flux densities S≳100µJy at ν=1.4GHz. Conversely, radio sources stronger than 100µJy are usually powered by star-forming galaxies, plus some active galactic nuclei, and most should be detectable by the SIRTF FLS. Thus, a sensitive radio survey can be used to select and identify most of the SIRTF FLS source population before launch. We used the B configuration of the VLA to make an image of the FLS area at ν=1.4GHz with σ≃23µJy/beam rms fluctuations, θ=5'' resolution, and σα≃σδ≃0.5'' rms uncertainties in right ascension and declination. The resulting radio image and catalog of 3565 radio components with peak flux densities Sp≥5σ=115µJy/beam have been released via the Web to expedite follow-up optical identification and spectroscopy. Mission: SIRTIF mission has been renamed Spitzer. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 105 3565 Component Catalog table2.dat 42 105 Multicomponent Sources Catalog
See also: http://sirtf.caltech.edu/SSC/fls/ : the First Look Survey (FLS) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh Hour of right ascension (J2000) 4- 5 I2 min RAm Minute of right ascension (J2000) 7- 12 F6.3 s RAs Second of right ascension (J2000) 14- 18 F5.3 s e_RAs RMS uncertainty in RAs (J2000) 20 A1 --- DE- Sign of the declination (J2000) 21- 22 I2 deg DEd Degrees of declination (J2000) 24- 25 I2 arcmin DEm Arcminute of declination (J2000) 27- 31 F5.2 arcsec DEs Arcsecond of declination (J2000) 33- 36 F4.2 arcsec e_DEs RMS uncertainty in DEs (J2000) 38- 44 F7.3 mJy Flux Integrated 1.4GHz flux density 46- 50 F5.3 mJy e_Flux RMS uncertainty in Flux 52 A1 --- l_MajAxis Upper limit symbol for MajAxis 54- 57 F4.1 arcsec MajAxis Deconvolved source FWHM major axis 59- 61 F3.1 arcsec e_MajAxis ? RMS uncertainty in MajAxis 64 A1 --- l_MinAxis Upper limit symbol for MinAxis 66- 69 F4.1 arcsec MinAxis Deconvolved source FWHM minor axis 71- 73 F3.1 arcsec e_MinAxis ? RMS uncertainty in MinAxis 75- 79 F5.1 deg PosAng ? Major-axis position angle (east of north) 81- 84 F4.1 deg e_PosAng ? RMS uncertainty in PosAng 86- 92 F7.2 pix Xpix X-axis pixel location of source on image 94-100 F7.2 pix Ypix Y-axis pixel location of source on image 102-105 A4 --- Group Group label for multicomponent sources
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 4 A4 --- Group Component group number 6- 7 I2 --- Ncomp Number of components in group 9- 10 I2 h RAh Hour of right ascension (J2000) 12- 13 I2 min RAm Minute of right ascension (J2000) 15- 19 F5.2 s RAs Second of right ascension (J2000) 21 A1 --- DE- Sign of the declination (J2000) 22- 23 I2 deg DEd Degrees of declination (J2000) 25- 26 I2 arcmin DEm Arcminute of declination (J2000) 28- 31 F4.1 arcsec DEs Arcsecond of declination (J2000) 33- 38 F6.2 mJy Flux Integrated 1.4GHz flux density 40- 42 A3 --- Fig Figure number for contour plot

(End) Greg Schwarz [AAS] 19-Aug-2003
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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