J/ApJ/655/212       S3MC IRAC and MIPS photometry               (Bolatto+, 2007)

The Spitzer Survey of the Small Magellanic Cloud: S3MC imaging and photometry in the mid- and far-infrared wave bands. Bolatto A.D., Simon J.D., Stanimirovic S., van Loon J.T., Shah R.Y., Venn K., Leroy A.K., Sandstrom K., Jackson J.M., Israel F.P., Li A., Staveley-Smith L., Bot C., Boulanger F., Rubio M. <Astrophys. J., 655, 212-232 (2007)> =2007ApJ...655..212B 2007ApJ...655..212B
ADC_Keywords: Magellanic Clouds ; YSOs ; Photometry, infrared Keywords: dust, extinction - galaxies: dwarf - galaxies: stellar content - infrared: ISM - infrared: stars - Magellanic Clouds Abstract: We present the initial results from the Spitzer Survey of the Small Magellanic Cloud (S3MC), which imaged the star-forming body of the SMC in all seven MIPS and IRAC wave bands. We find that the F8/F24 ratio (an estimate of PAH abundance) has large spatial variations and takes a wide range of values that are unrelated to metallicity but anticorrelated with 24um brightness and F24/F70 ratio. This suggests that photodestruction is primarily responsible for the low abundance of PAHs observed in star-forming low-metallicity galaxies. We use the S3MC images to compile a photometric catalog of 400000 mid- and far-infrared point sources in the SMC. Description: We obtained Spitzer images of the SMC in all of the bands of the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer and Spectrometer (MIPS) as part of the Cycle I General Observer project 3316, "The Small Magellanic Cloud: A Template for the Primitive Interstellar Medium." The MIPS data were acquired in 2004 November, using five large AORs each lasting over 3hr and two smaller AORs slightly over 1hr long each. The IRAC data were obtained during 2005 May using eight large 4hr long and two small 2hr long AORs with a frame time of 12s and a three-point cycling dithering pattern. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 154 282 S3MC Young Stellar Object Catalog -------------------------------------------------------------------------------- See also: J/AJ/123/855 : Magellanic Clouds Photometric Survey: the SMC (Zaritsky+, 2002) J/A+A/401/873 : The SMC in the Far Infrared (Wilke+, 2003) Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- [BSS2007] Running source identification number 5- 9 A5 --- --- [S3MC_] 10- 29 A20 --- S3MC Source name (JHHMMSS.ss+DDMMSS.ss) 31- 37 F7.4 deg RAdeg Right Ascension in decimal degrees (J2000) 39- 46 F8.4 deg DEdeg Declination in decimal degrees (J2000) 48- 53 F6.1 uJy FB ? The B band flux density 55- 60 F6.1 uJy FV ? The V band flux density 62- 67 F6.1 uJy FI ? The I band flux density 69- 74 F6.1 uJy FJ ? The J band flux density 76- 82 F7.1 uJy FH ? The H band flux density 84- 90 F7.1 uJy FK ? The K band flux density 92- 96 I5 uJy F3.6 ? Spitzer/IRAC 3.6 µm flux density 98-100 I3 uJy e_F3.6 ? Error in 3.6 102-106 I5 uJy F4.5 ? Spitzer/IRAC 4.5 µm flux density 108 I1 uJy e_F4.5 ? Error in 4.5 110-114 I5 uJy F5.8 Spitzer/IRAC 5.8 µm flux density 116-118 I3 uJy e_F5.8 Error in 5.8 120-124 I5 uJy F8.0 Spitzer/IRAC 8.0 µm flux density 126-128 I3 uJy e_F8.0 Error in 8.0 130-136 I7 uJy F24 ? Spitzer/MIPS 24 µm flux density 138-140 I3 uJy e_F24 ? Error in 24 142-148 I7 uJy F70 ? Spitzer/MIPS 70 µm flux density 150-154 I5 uJy e_F70 ? Error in 70 -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 08-Dec-2008
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