Calibration of the total infrared luminosity of nearby galaxies from Spitzer and Herschel bands

被引：115

作者：

Galametz, M. ^{[1
]}

Kennicutt, R. C. ^{[1
]}

Calzetti, D. ^{[2
]}

Aniano, G. ^{[3
,4
]}

Draine, B. T. ^{[3
]}

Boquien, M. ^{[5
]}

Brandl, B. ^{[6
]}

Croxall, K. V. ^{[7
,8
]}

Dale, D. A. ^{[9
]}

Engelbracht, C. W. ^{[10
,11
]}

Gordon, K. D. ^{[12
]}

Groves, B. ^{[13
]}

Hao, C. -N. ^{[14
]}

Helou, G. ^{[15
]}

Hinz, J. L. ^{[10
]}

Hunt, L. K. ^{[16
]}

Johnson, B. D. ^{[17
]}

Li, Y. ^{[2
]}

Murphy, E. ^{[18
]}

Roussel, H. ^{[17
]}

Sandstrom, K. ^{[13
]}

Skibba, R. A. ^{[10
,19
]}

Tabatabaei, F. S. ^{[13
]}

机构：

[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England

[2] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA

[3] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[4] Univ Paris 11, Inst Astrophys Spatiale, CNRS UMR 8617, F-91405 Orsay, France

[5] Univ Aix Marseille, Lab Astrophys Marseille, CNRS UMR 7326, F-13388 Marseille 13, France

[6] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[7] Univ Toledo, Dept Phys & Astron, Toledo, OH 43606 USA

[8] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA

[9] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA

[10] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

[11] Raytheon Co, Tucson, AZ 85756 USA

[12] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[13] Max Planck Inst Astron, D-69117 Heidelberg, Germany

[14] Tianjin Normal Univ, Tianjin Astrophys Ctr, Tianjin 300387, Peoples R China

[15] CALTECH, NASA Herschel Sci Ctr, IPAC, Pasadena, CA 91125 USA

[16] INAF Osservatorio Astrofis Arcetri, I-50125 Florence, Italy

[17] Univ Paris 06, Inst Astrophys Paris, CNRS UMR 7095, F-75014 Paris, France

[18] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA

[19] Univ Calif San Diego, Ctr Astrophys & Space Sci, Dept Phys, San Diego, CA 92093 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2013年 / 431卷 / 02期

基金：

美国国家航空航天局;

关键词：

dust; extinction; galaxies: ISM; submillimetre: galaxies; SPECTRAL ENERGY-DISTRIBUTION; STAR-FORMING GALAXIES; LOW-METALLICITY ENVIRONMENTS; SMALL-MAGELLANIC-CLOUD; DUST EMISSION; SUBMILLIMETER GALAXIES; INTERSTELLAR DUST; FORMATION RATES; DWARF GALAXIES; ISM PROPERTIES;

D O I：

10.1093/mnras/stt313

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

When combined with infrared observations with the Spitzer telescope (3 to 160 mu m), the Herschel Space Observatory now fully samples the thermal dust emission up to 500 mu m and enables us to better estimate the total infrared-submm energy budget (L-TIR) of nearby galaxies. We present new empirical calibrations to estimate resolved and integrated total infrared luminosities from Spitzer and Herschel bands used as monochromatic or combined tracers. We base our calibrations on resolved elements of nearby galaxies (3 to 30 Mpc) observed with Herschel. We perform a resolved spectral energy distribution (SED) modelling of these objects using the Draine & Li dust models and investigate the influence of the addition of Spectral and Photometric Imaging Receiver (SPIRE) measurements in the estimation of L-TIR. We find that using data up to 250 mu m leads to local L-TIR values consistent with those obtained with a complete coverage (up to 500 mu m) within +/- 10 per cent for most of our resolved elements. We then study the distribution of energy in the resolved SEDs of our galaxies. The bulk of energy (30-50 per cent) is contained in the [70-160 mu m] band. The [24-70 mu m] fraction decreases with increasing metallicity. The [160-1100 mu m] submillimetre band can account for up to 25 per cent of the L-TIR in metal-rich galaxies. We investigate the correlation between the total infrared (TIR) surface brightnesses/luminosities and monochromatic Spitzer and Herschel surface brightnesses/luminosities. The three Photodetector Array Camera and Spectrometer (PACS) bands can be used as reliable monochromatic estimators of the L-TIR, the 100 mu m band being the most reliable monochromatic tracer. There is also a strong correlation between the SPIRE 250 mu m and L-TIR, although with more scatter than for the PACS relations. We also study the ability of our monochromatic relations to reproduce integrated L-TIR of nearby galaxies as well as L-TIR of z similar to 1-3 sources. Finally, we provide calibration coefficients that can be used to derive TIR surface brightnesses/luminosities from a combination of Spitzer and Herschel surface brightnesses/fluxes and analyse the associated uncertainties.

引用

页码：1956 / 1986

页数：31

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