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J/AJ/141/1          Spitzer observations of GOODS fields     (Teplitz+, 2011)

Spitzer infrared spectrometer 16µm observations of the GOODS fields. Teplitz H.I., Chary R., Elbaz D., Dickinson M., Bridge C., Colbert J., Le Floc'h E., Frayer D.T., Howell J.H., Koo D.C., Papovich C., Phillips A., Scarlata C., Siana B., Spinrad H., Stern D. <Astron. J., 141, 1 (2011)> =2011AJ....141....1T
ADC_Keywords: Galaxies, optical ; Galaxies, IR ; Photometry, infrared ; X-ray sources Keywords: cosmology: observations - galaxies: evolution - galaxies: high-redshift - infrared: galaxies Abstract: We present Spitzer 16um imaging of the Great Observatories Origins Deep Survey (GOODS) fields. We survey 150 arcmin2 in each of the two GOODS fields (North and South), to an average 3σ depth of 40 and 65uJy, respectively. We detect ∼1300 sources in both fields combined. We validate the photometry using the 3-24um spectral energy distribution of stars in the fields compared to Spitzer spectroscopic templates. Comparison with ISOCAM and AKARI observations in the same fields shows reasonable agreement, though the uncertainties are large. We provide a catalog of photometry, with sources cross-correlated with available Spitzer, Chandra, and Hubble Space Telescope data. Galaxy number counts show good agreement with previous results from ISOCAM and AKARI with improved uncertainties. Description: Data were taken in two general observer Spitzer programs: GO-3661, observing GOODS-South in Cycle 1, and GO-20599, observing GOODS-North in Cycle 2. The 16µm fluxes were detected with the Spitzer peak-up imaging (PUI) capability offered by the the Infrared Spectrometer (IRS). The Si:As detector was similar to that used in the 24µm channel of the MIPS instrument; in 10 minutes of observation, the PUI achieved 5σ depths of ∼45µJy. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table12.dat 231 840 GOODS-N, Spitzer and ancillary data (tables 1 and 2 of the paper) table34.dat 231 476 GOODS-S, Spitzer and ancillary data (tables 3 and 4 of the paper)
See also: II/261 : GOODS initial results (Giavalisco+, 2004) J/AJ/126/539 : The Chandra Deep Fields North and South (Alexander+, 2003) J/ApJS/179/19 : CDFS survey: 2 Ms source catalogs (Luo+, 2008) Byte-by-byte Description of file: table*.dat
Bytes Format Units Label Explanations
1- 4 I4 --- ID [0/839] Index number 6- 15 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 17- 26 F10.6 deg DEdeg Declination in decimal degrees (J2000) 28- 29 I2 --- Cov Coverage in number of exposures (1) 31- 38 F8.2 uJy S3.6 Spitzer/IRAC 3.6 micron band flux density 40- 46 F7.2 uJy e_S3.6 The 1σ error in S3.6 48- 54 F7.2 uJy S4.5 Spitzer/IRAC 4.5 micron band flux density 56- 61 F6.2 uJy e_S4.5 The 1σ error in S4.5 63- 70 F8.2 uJy S5.8 Spitzer/IRAC 5.8 micron band flux density 72- 77 F6.2 uJy e_S5.8 The 1σ error in S5.8 79- 85 F7.2 uJy S8 Spitzer/IRAC 8.0 micron band flux density 87- 92 F6.2 uJy e_S8 The 1σ error in S8 94- 99 F6.1 uJy S16 Spitzer/IRS 16 micron band flux density 101-105 F5.1 uJy e_S16 The 1σ error in S16 107-112 F6.1 uJy S24 Spitzer/MIPS 24 micron band flux density 114-119 F6.2 uJy e_S24 The 1σ error in S24 121-128 F8.4 --- zsp ?=-99.0000 Spectroscopic redshift 130-131 I2 --- r_zsp Reference for zsp (2) 133 I1 --- X? [0/1] X-ray detected? 1=detected, 0=not detected 135-139 F5.2 aW/m2 FXs Soft X-ray band flux of Chandra detection (3) 140 A1 --- --- [0] 142-146 F5.2 aW/m2 FXh Hard X-ray band flux of Chandra detection (3) 147 A1 --- --- [0] 149 I1 --- S/G [0/2] Star flag: 1=star, 0=galaxy 2=confusion star and neighboring galaxy 151-155 F5.2 --- conc ? 16mum concentration index (4) 157 I1 --- N8 Number of 8µm sources within 4" radius 159 I1 --- N16 Number of 16µm sources within 5.4" radius 161-162 I2 --- Q [1/31] Quality flag (5) 164 I1 --- E [0/1] Extended flag (1=extended, 0=not extended) 166-172 F7.2 mag Bmag ?=-999.00 Giavalisco et al. 2004, Cat. II/261 B band magnitude 174-180 F7.2 mag Vmag ?=-999.00 Giavalisco et al. 2004, Cat. II/261 V band magnitude 182-188 F7.2 mag Imag ?=-999.00 Giavalisco et al. 2004, Cat. II/261 I band magnitude 190-196 F7.2 mag zmag ?=-999.00 Giavalisco et al. 2004, Cat. II/261 z band magnitude 198-204 F7.2 mag e_Bmag ?=-999.00 The 1σ error in Bmag 206-212 F7.2 mag e_Vmag ?=-999.00 The 1σ error in Vmag 214-220 F7.2 mag e_Imag ?=-999.00 The 1σ error in Imag 222-228 F7.2 mag e_zmag ?=-999.00 The 1σ error in zmag 230-231 I2 --- NI Number of I band sources with 1" radius
Note (1): 30 seconds integration per exposure for GOODS-N (table12), 60 seconds integration per exposure for GOODS-S (table34). Note (2): Reference for zspec as follows: -1 = no redshift; 1 = LeFevre et al. (2004, Cat. J/A+A/428/1043) 2 = Szokoly et al. (2004, Cat. J/ApJS/155/271) 3 = Croom et al. (2001, Cat. J/MNRAS/328/150) 9 = K20 Survey, Mignoli et al. (2005, Cat. J/A+A/437/883) 10 = Cohen et al. (2000, Cat. J/ApJ/538/29), Cohen (2001, Cat. J/AJ/121/2895) 11 = Strolger et al. (2004, Cat. J/ApJ/613/200) 12 = Dawson et al. (2001, Cat. J/AJ/122/598) 21 = Wirth et al. (2004, Cat. J/AJ/127/3121) 30 = Vanzella et al. (2008, Cat. J/A+A/434/53) 41 = Popesso et al. (2009A&A...494..443P), Balestra et al. (2010, Cat. J/A+A/512/A12) 42 = Chapman et al. (2005, Cat. J/ApJ/622/772), Swinbank et al. (2004ApJ...617...64S) 45 = Pope et al. (2008ApJ...675.1171P), Murphy et al. (2009ApJ...698.1380M), Spitzer IRS redshifts 51 = Treu et al. (2005, Cat. J/ApJ/633/174) 61 = Reddy et al. (2006, Cat. J/ApJ/653/1004) 62 = Doherty et al. (2005, Cat. J/MNRAS/361/525) 70 = Ravikumar et al. (2007, Cat. J/A+A/465/1099) 72 = Stern et al. (in prep) 73 = Daddi et al. (2008ApJ...673L..21D) 81 = Barger et al. (2008, cat. J/ApJ/689/687) 82 = Kriek et al. (2008ApJ...677..219K) Note (3): From Alexander et al. 2003, Cat. J/AJ/126/539 for table12, from Luo et al. 2003, Cat. J/ApJS/179/19 for table34. Note (4): Ratio of aperture flux in 6:2 pixel radii. Blanks indicate NaN values. Objects which are point sources should fall in the range of 2-3. Note (5): Quality Flag is assigned Bitwise (Q=Σ2b), where b means: 0 = included in catalog 1 = more than one 16 micron source within 5.4 arcsec; possible confusion 2 = source concentration differs from that expected for point source 3 = S/N ratio <5, but coverage indicates it should be higher 4 = sources with coverage of two exposures instead of three For example, an object with a flag value of 19 would indicate that Bits 0, 1, and 4 had been set because: (Bit 0) the object was included in the catalog; (Bit 1) the measurement of the object may suffer from confusion due to a close 16um neighbor; and (Bit 4) the object had a coverage of only two exposures.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 18-Jul-2012
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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