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J/ApJ/707/89            Variation of mid-IR extinction              (Gao+, 2009)

Mid-infrared extinction and its variation with galactic longitude. Gao J., Jiang B.W., Li A. <Astrophys. J., 707, 89-102 (2009)> =2009ApJ...707...89G
ADC_Keywords: Extinction ; Galactic plane ; Interstellar medium ; Stars, giant ; Photometry, infrared ; Surveys Keywords: dust, extinction - Galaxy: bulge - Galaxy: structure - infrared: ISM - infrared: stars Abstract: Based on the data obtained from the Spitzer/Galactic Legacy Infrared Midplane Survey Extraordinaire (GLIPMSE) Legacy Program and the Two Micron All Sky Survey (2MASS) project, we derive the extinction in the four IRAC bands, [3.6], [4.5], [5.8], and [8.0]um, relative to the 2MASS Ks band (at 2.16um) for 131 GLIPMSE fields along the Galactic plane within |l|≤65°, using red giants and red clump giants as tracers. As a whole, the mean extinction in the IRAC bands (normalized to the 2MASS Ks band), A[3.6]/AKs∼0.63±0.01, A[4.5]/AKs∼0.57±0.03, A[5.8]/AKs_∼0.49±0.03, A[8.0]/AKs∼0.55±0.03, exhibits little variation with wavelength (i.e., the extinction is somewhat flat or gray). As far as individual sightline is concerned, however, the wavelength dependence of the mid-infrared interstellar extinction Aλ/AKs varies from one sightline to another, suggesting that there may not exist a "universal" IR extinction law. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 126 131 Extinction ratios A(λ)/A(Ks) of the 131 GLIMPSE fields
See also: II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) J/ApJ/658/1264 : IR-excess sources in GLIMPSE and MSX (Uzpen+, 2007) J/A+A/446/551 : Extinctions at 7um + 15um from ISOGAL survey (Jiang+, 2006) J/MNRAS/338/253 : K extinction near the Galactic Centre (Dutra+, 2003) J/A+A/349/L69 : Interstellar extinction (Schultheis+, 1999) http://www.astro.wisc.edu/sirtf/glimpsedata.html : GLIMPSE data home page Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 11 A11 --- FName Field name (1) 13- 17 F5.1 deg GLONl Lower Galactic longitude degree 19- 23 F5.1 deg GLONu Upper Galactic longitude degree 25- 28 F4.1 deg GLATl Lower Galactic latitude degree 30- 33 F4.1 deg GLATu Upper Galactic latitude degree 35- 39 F5.3 --- GA3.6 IRAC [3.6] band to Ks band extinction ratio from Red Giants (2) 41- 45 F5.3 --- e_GA3.6 Uncertainty in GA3.6 47- 51 F5.3 --- GA4.5 IRAC [4.5] band to Ks band extinction ratio from Red Giants (2) 53- 57 F5.3 --- e_GA4.5 Uncertainty in GA4.5 59- 63 F5.3 --- GA5.8 IRAC [5.8] band to Ks band extinction ratio from Red Giants (2) 65- 69 F5.3 --- e_GA5.8 Uncertainty in GA5.8 71- 75 F5.3 --- GA8.0 IRAC [8.0] band to Ks band extinction ratio from Red Giants (2) 77- 81 F5.3 --- e_GA8.0 Uncertainty in GA8.0 83- 86 F4.2 --- CA3.6 IRAC [3.6] band to Ks band extinction ratio from Red Clump Giants (2) 88- 91 F4.2 --- e_CA3.6 Uncertainty in CA3.6 93- 96 F4.2 --- CA4.5 IRAC [4.5] band to Ks band extinction ratio from Red Clump Giants (2) 98-101 F4.2 --- e_CA4.5 Uncertainty in CA4.5 103-106 F4.2 --- CA5.8 IRAC [5.8] band to Ks band extinction ratio from Red Clump Giants (2) 108-111 F4.2 --- e_CA5.8 Uncertainty in CA5.8 113-116 F4.2 --- CA8.0 IRAC [8.0] band to Ks band extinction ratio from Red Clump Giants (2) 118-121 F4.2 --- e_CA8.0 Uncertainty in CA8.0 123-126 F4.1 mag Ksmax Maximum Ks band magnitude for Red Clump Giants
Note (1): GLMXC_l009, GLMXC_l350, GLMIC_l064 and GLMIC_l295 are the combined fields (see Section 2 in the paper). Note (2): The effective wavelengths of the four Spitzer/IRAC bands [3.6], [4.5], [5.8] and [8.0] are actually 3.545, 4.442, 5.675 and 7.760 microns, respectively.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 29-Dec-2011
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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