AN ATLAS OF GALAXY SPECTRAL ENERGY DISTRIBUTIONS FROM THE ULTRAVIOLET TO THE MID-INFRARED

被引：207

作者：

Brown, Michael J. I. ^{[1
,2
]}

Moustakas, John ^{[3
]}

Smith, J. -D. T. ^{[4
]}

da Cunha, Elisabete ^{[5
]}

Jarrett, T. H. ^{[6
]}

Imanishi, Masatoshi ^{[7
,8
,9
]}

Armus, Lee ^{[10
]}

Brandl, Bernhard R. ^{[11
]}

Peek, J. E. G. ^{[12
]}

机构：

[1] Monash Univ, Sch Phys, Clayton, Vic 3800, Australia

[2] Monash Univ, Monash Ctr Astrophys, Clayton, Vic 3800, Australia

[3] Siena Coll, Dept Phys & Astron, Loudonville, NY 12211 USA

[4] Univ Toledo, Dept Phys & Astron, Ritter Observ, Toledo, OH 43606 USA

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

[6] Univ Cape Town, Dept Astron, ZA-7701 Rondebosch, South Africa

[7] Subaru Telescope, Hilo, HI 96720 USA

[8] Grad Univ Adv Studies SOKENDAI, Sch Sci, Dept Astron, Mitaka, Tokyo 1818588, Japan

[9] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[10] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA

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

[12] Columbia Univ, Dept Astron, New York, NY 10027 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2014年 / 212卷 / 02期

基金：

澳大利亚研究理事会; 美国国家航空航天局; 美国国家科学基金会;

关键词：

atlases; galaxies: general; galaxies: photometry; techniques: spectroscopic; STAR-FORMING GALAXIES; LUMINOUS INFRARED GALAXIES; SPITZER-SPACE-TELESCOPE; ACTIVE GALACTIC NUCLEI; HIGH-REDSHIFT GALAXIES; WIDE-FIELD SURVEY; SKY LIRG SURVEY; PHOTOMETRIC REDSHIFTS; K-CORRECTIONS; POPULATION SYNTHESIS;

D O I：

10.1088/0067-0049/212/2/18

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength coverage spanning from the ultraviolet to the mid-infrared. Our atlas spans a broad range of galaxy types, including ellipticals, spirals, merging galaxies, blue compact dwarfs, and luminous infrared galaxies. We have combined ground-based optical drift-scan spectrophotometry with infrared spectroscopy from Spitzer and Akari with gaps in spectral coverage being filled using Multi-wavelength Analysis of Galaxy Physical Properties spectral energy distribution models. The spectroscopy and modelswere normalized, constrained, and verified with matched-aperture photometry measured from Swift, Galaxy Evolution Explorer, Sloan Digital Sky Survey, Two Micron All Sky Survey, Spitzer, and Wide-field Infrared Space Explorer images. The availability of 26 photometric bands allowed us to identify and mitigate systematic errors present in the data. Comparison of our spectral energy distributions with other template libraries and the observed colors of galaxies indicates that we have smaller systematic errors than existing atlases, while spanning a broader range of galaxy types. Relative to the prior literature, our atlas will provide improved K-corrections, photometric redshifts, and star-formation rate calibrations.

引用

页数：23

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