Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm

被引：90

作者：

Driver, S. P. ^{[1
,2
]}

Robotham, A. S. G. ^{[1
,2
]}

Kelvin, L. ^{[1
,2
]}

Alpaslan, M. ^{[1
,2
]}

Baldry, I. K. ^{[3
]}

Bamford, S. P. ^{[4
]}

Brough, S. ^{[5
]}

Brown, M. ^{[6
]}

Hopkins, A. M. ^{[5
]}

Liske, J. ^{[7
]}

Loveday, J. ^{[8
]}

Norberg, P. ^{[9
]}

Peacock, J. A. ^{[10
]}

Andrae, E. ^{[11
]}

Bland-Hawthorn, J. ^{[12
]}

Bourne, N. ^{[4
]}

Cameron, E. ^{[13
]}

Colless, M. ^{[5
]}

Conselice, C. J. ^{[4
]}

Croom, S. M.

Dunne, L. ^{[14
]}

Frenk, C. S. ^{[9
]}

Graham, Alister W. ^{[15
]}

Gunawardhana, M. ^{[12
]}

Hill, D. T. ^{[2
]}

Jones, D. H. ^{[6
]}

Kuijken, K. ^{[16
]}

Madore, B. ^{[17
]}

Nichol, R. C. ^{[18
]}

Parkinson, H. R. ^{[10
]}

Pimbblet, K. A. ^{[6
]}

Phillipps, S. ^{[19
]}

Popescu, C. C. ^{[20
]}

Prescott, M. ^{[3
]}

Seibert, M. ^{[17
]}

Sharp, R. G. ^{[21
]}

Sutherland, W. J. ^{[22
]}

Taylor, E. N. ^{[12
]}

Thomas, D. ^{[18
]}

Tuffs, R. J. ^{[11
]}

van Kampen, E. ^{[7
]}

Wijesinghe, D. ^{[12
]}

Wilkins, S. ^{[23
]}

机构：

[1] Univ Western Australia, ICRAR, Crawley, WA 6009, Australia

[2] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland

[3] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England

[4] Univ Nottingham, Ctr Astron & Particle Theory, Nottingham NG7 2RD, England

[5] Australian Astron Observ, Epping, NSW 1710, Australia

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

[7] European So Observ, D-85748 Garching, Germany

[8] Univ Sussex, Ctr Astron, Brighton BN1 9QH, E Sussex, England

[9] Univ Durham, Inst Computat Cosmol, Dept Phys, Durham DH1 3LE, England

[10] Univ Edinburgh, Inst Astron, Royal Observ, SUPA, Edinburgh EH9 3HJ, Midlothian, Scotland

[11] Max Planck Inst Nucl Phys MPIK, D-69117 Heidelberg, Germany

[12] Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia

[13] Queensland Univ Technol, Sch Math Sci, Brisbane, Qld 4001, Australia

[14] Univ Canterbury, Dept Phys & Astron, Christchurch 8140, New Zealand

[15] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

[16] Leiden Univ, NL-2300 RA Leiden, Netherlands

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

[18] Univ Portsmouth, Inst Cosmol & Gravitat ICG, Portsmouth PO1 3FX, Hants, England

[19] Univ Bristol, HH Wills Phys Lab, Bristol BS8 1TL, Avon, England

[20] Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England

[21] Mt Stromlo & Siding Spring Observ, Res Sch Astron & Astrophys, Western Creek, ACT 2611, Australia

[22] Queen Mary Univ London, Astron Unit, London E1 4NS, England

[23] Univ Oxford, Sch Phys & Astron, Oxford OX1 3RH, England

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2012年 / 427卷 / 04期

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

surveys; galaxies: fundamental parameters; galaxies: general; galaxies: luminosity function; mass function; cosmology: observations; infrared: galaxies; DIGITAL-SKY-SURVEY; EXTRAGALACTIC BACKGROUND LIGHT; LUMINOSITY FUNCTION; REDSHIFT SURVEY; STAR-FORMATION; HERSCHEL-ATLAS/GAMA; PHOTOMETRIC SYSTEM; CATALOG; CALIBRATION; EVOLUTION;

D O I：

10.1111/j.1365-2966.2012.22036.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugriz and YJHK bands from within a single well-constrained volume of 3.4 x 10(5) (Mpc h(-1))(3). The derived luminosity distributions are normalized to the SDSS data release 7 (DR7) main survey to reduce the estimated cosmic variance to the 5 per cent level. The data are used to construct the cosmic spectral energy distribution (CSED) from 0.1 to 2.1 mu m free from any wavelength-dependent cosmic variance for both the elliptical and non-elliptical populations. The two populations exhibit dramatically different CSEDs as expected for a predominantly old and young population, respectively. Using the Driver et al. prescription for the azimuthally averaged photon escape fraction, the non-ellipticals are corrected for the impact of dust attenuation and the combined CSED constructed. The final results show that the Universe is currently generating (1.8 +/- 0.3) x 10(35) h W Mpc(-3) of which (1.2 +/- 0.1) x 10(35) h W Mpc-3 is directly released into the inter-galactic medium and (0.6 +/- 0.1) x 10(35) h W Mpc(-3) is reprocessed and reradiated by dust in the far-IR. Using the GAMA data and our dust model we predict the mid- and far-IR emission which agrees remarkably well with available data. We therefore provide a robust description of the pre- and post-dust attenuated energy output of the nearby Universe from 0.1 mu m to 0.6 mm. The largest uncertainty in this measurement lies in the mid- and far-IR bands stemming from the dust attenuation correction and its currently poorly constrained dependence on environment, stellar mass and morphology.

引用

页码：3244 / 3264

页数：21

共 80 条

[1] The Millennium Galaxy Catalogue: bulge-disc decomposition of 10 095 nearby galaxies [J].

Allen, Paul D. ;

Driver, Simon P. ;

Graham, Alister W. ;

Cameron, Ewan ;

Liske, Jochen ;

De Propris, Roberto .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 371 (01) :2-18

[2] Luminosity functions for galaxies and quasars in the Spitzer wide-area infrared extragalactic legacy survey [J].

Babbedge, T. S. R. ;

Rowan-Robinson, M. ;

Vaccari, M. ;

Surace, J. A. ;

Lonsdale, C. J. ;

Clements, D. L. ;

Fang, F. ;

Farrah, D. ;

Franceschini, A. ;

Gonzalez-Solares, E. ;

Hatziminaoglou, E. ;

Lacey, C. G. ;

Oliver, S. ;

Onyett, N. ;

Perez-Fournon, I. ;

Polletta, M. ;

Pozzi, F. ;

Rodighiero, G. ;

Shupe, D. L. ;

Siana, B. ;

Smith, H. E. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 370 (03) :1159-1180

[3] Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06 [J].

Baldry, I. K. ;

Driver, S. P. ;

Loveday, J. ;

Taylor, E. N. ;

Kelvin, L. S. ;

Liske, J. ;

Norberg, P. ;

Robotham, A. S. G. ;

Brough, S. ;

Hopkins, A. M. ;

Bamford, S. P. ;

Peacock, J. A. ;

Bland-Hawthorn, J. ;

Conselice, C. J. ;

Croom, S. M. ;

Jones, D. H. ;

Parkinson, H. R. ;

Popescu, C. C. ;

Prescott, M. ;

Sharp, R. G. ;

Tuffs, R. J. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 421 (01) :621-634

[4] Galaxy And Mass Assembly (GAMA): the input catalogue and star-galaxy separation [J].

Baldry, I. K. ;

Robotham, A. S. G. ;

Hill, D. T. ;

Driver, S. P. ;

Liske, J. ;

Norberg, P. ;

Bamford, S. P. ;

Hopkins, A. M. ;

Loveday, J. ;

Peacock, J. A. ;

Cameron, E. ;

Croom, S. M. ;

Cross, N. J. G. ;

Doyle, I. F. ;

Dye, S. ;

Frenk, C. S. ;

Jones, D. H. ;

van Kampen, E. ;

Kelvin, L. S. ;

Nichol, R. C. ;

Parkinson, H. R. ;

Popescu, C. C. ;

Prescott, M. ;

Sharp, R. G. ;

Sutherland, W. J. ;

Thomas, D. ;

Tuffs, R. J. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 404 (01) :86-100

[5] The sloan digital sky survey u-band galaxy survey:: luminosity functions and evolution [J].

Baldry, IK ;

Glazebrook, K ;

Budavári, T ;

Eisenstein, DJ ;

Annis, J ;

Bahcall, NA ;

Blanton, MR ;

Brinkmann, J ;

Csabai, I ;

Heckman, TM ;

Lin, H ;

Loveday, J ;

Nichol, RC ;

Schneider, DP .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2005, 358 (02) :441-456

[6] Constraints on a universal stellar initial mass function from ultraviolet to near-infrared galaxy luminosity densities [J].

Baldry, IK ;

Glazebrook, K .

ASTROPHYSICAL JOURNAL, 2003, 593 (01) :258-271

[7] The optical and near-infrared properties of galaxies. I. Luminosity and stellar mass functions [J].

Bell, EF ;

McIntosh, DH ;

Katz, N ;

Weinberg, MD .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2003, 149 (02) :289-312

[8] SExtractor: Software for source extraction [J].

Bertin, E ;

Arnouts, S .

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1996, 117 (02) :393-404

[9] K-corrections and filter transformations in the ultraviolet, optical, and near-infrared [J].

Blanton, Michael R. ;

Roweis, Sam .

ASTRONOMICAL JOURNAL, 2007, 133 (02) :734-754

[10] The galaxy luminosity function and luminosity density at redshift z=0.1 [J].

Blanton, MR ;

Hogg, D ;

Bahcall, NA ;

Brinkmann, J ;

Britton, M ;

Connolly, AJ ;

Csabai, I ;

Fukugita, M ;

Loveday, J ;

Meiksin, A ;

Munn, JA ;

Nichol, RC ;

Okamura, S ;

Quinn, T ;

Schneider, DP ;

Shimasaku, K ;

Strauss, MA ;

Tegmark, M ;

Vogeley, MS ;

Weinberg, DH .

ASTROPHYSICAL JOURNAL, 2003, 592 (02) :819-838

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Galaxy And Mass Assembly (GAMA): the 0.013 &lt; z &lt; 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm

Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm