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：

美国国家航空航天局; 美国国家科学基金会;

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 22 条

[1] Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1 < z < 0.35
Wethers, Clare F.
Acharya, Nischal
De Propris, Roberto
Kotilainen, Jari
Baldry, Ivan K.
Brough, Sarah
Driver, Simon P.
Graham, Alister W.
Holwerda, Benne W.
Hopkins, Andrew M.
Lopez-Sanchez, Angel R.
Loveday, Jonathan
Phillipps, Steven
Pimbblet, Kevin A.
Taylor, Edward
Wang, Lingyu
Wright, Angus H.
ASTROPHYSICAL JOURNAL, 2022, 928 (02):
[2] Galaxy and Mass Assembly (GAMA): Demonstrating the Power of WISE in the Study of Galaxy Groups to z < 0.1
Cluver, M. E.
Jarrett, T. H.
Taylor, E. N.
Hopkins, A. M.
Brough, S.
Casura, S.
Holwerda, B. W.
Liske, J.
Pimbblet, K. A.
Wright, A. H.
ASTROPHYSICAL JOURNAL, 2020, 898 (01):
[3] Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
Driver, Simon P.
Bellstedt, Sabine
Robotham, Aaron S. G.
Baldry, Ivan K.
Davies, Luke J.
Liske, Jochen
Obreschkow, Danail
Taylor, Edward N.
Wright, Angus H.
Alpaslan, Mehmet
Bamford, Steven P.
Bauer, Amanda E.
Bland-Hawthorn, Joss
Bilicki, Maciej
Bravo, Matias
Brough, Sarah
Casura, Sarah
Cluver, Michelle E.
Colless, Matthew
Conselice, Christopher J.
Croom, Scott M.
de Jong, Jelte
D'Eugenio, Franceso
De Propris, Roberto
Dogruel, Burak
Drinkwater, Michael J.
Dvornik, Andrej
Farrow, Daniel J.
Frenk, Carlos S.
Giblin, Benjamin
Graham, Alister W.
Grootes, Meiert W.
Gunawardhana, Madusha L. P.
Hashemizadeh, Abdolhosein
Haeussler, Boris
Heymans, Catherine
Hildebrandt, Hendrik
Holwerda, Benne W.
Hopkins, Andrew M.
Jarrett, Tom H.
Jones, D. Heath
Kelvin, Lee S.
Koushan, Soheil
Kuijken, Konrad
Lara-Lopez, Maritza A.
Lange, Rebecca
Lopez-Sanchez, Angel R.
Loveday, Jon
Mahajan, Smriti
Meyer, Martin
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 513 (01) : 439 - 467
[4] Galaxy And Mass Assembly (GAMA): The mechanisms for quiescent galaxy formation at z < 1
Rowlands, K.
Wild, V.
Bourne, N.
Bremer, M.
Brough, S.
Driver, S. P.
Hopkins, A. M.
Owers, M. S.
Phillipps, S.
Pimbblet, K.
Sansom, A. E.
Wang, L.
Alpaslan, M.
Bland-Hawthorn, J.
Colless, M.
Holwerda, B. W.
Taylor, E. N.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 473 (01) : 1168 - 1185
[5] Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sersic index, colour and morphology
Lange, Rebecca
Driver, Simon P.
Robotham, Aaron S. G.
Kelvin, Lee S.
Graham, Alister W.
Alpaslan, Mehmet
Andrews, Stephen K.
Baldry, Ivan K.
Bamford, Steven
Bland-Hawthorn, Joss
Brough, Sarah
Cluver, Michelle E.
Conselice, Christopher J.
Davies, Luke J. M.
Haeussler, Boris
Konstantopoulos, Iraklis S.
Loveday, Jon
Moffett, Amanda J.
Norberg, Peder
Phillipps, Steven
Taylor, Edward N.
Lopez-Sanchez, Angel R.
Wilkins, Stephen M.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 447 (03) : 2603 - 2630
[6] Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06
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
[7] Galaxy And Mass Assembly: the evolution of the cosmic spectral energy distribution from z=1 to z=0
Andrews, S. K.
Driver, S. P.
Davies, L. J. M.
Kafle, P. R.
Robotham, A. S. G.
Vinsen, K.
Wright, A. H.
Bland-Hawthorn, J.
Bourne, N.
Bremer, M.
da Cunha, E.
Drinkwater, M.
Holwerda, B.
Hopkins, A. M.
Kelvin, L. S.
Loveday, J.
Phillipps, S.
Wilkins, S.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 470 (02) : 1342 - 1359
[8] The growth of intracluster light in XCS-HSC galaxy clusters from 0.1 < z < 0.5
Furnell, Kate E.
Collins, Chris A.
Kelvin, Lee S.
Baldry, Ivan K.
James, Phil A.
Manolopoulou, Maria
Mann, Robert G.
Giles, Paul A.
Bermeo, Alberto
Hilton, Matthew
Wilkinson, Reese
Romer, A. Kathy
Vergara, Carlos
Bhargava, Sunayana
Stott, John P.
Mayers, Julian
Viana, Pedro
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 502 (02) : 2419 - 2437
[9] Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function to z=0.1 from the r-band selected equatorial regions
Wright, A. H.
Robotham, A. S. G.
Driver, S. P.
Alpaslan, M.
Andrews, S. K.
Baldry, I. K.
Bland-Hawthorn, J.
Brough, S.
Brown, M. J. I.
Colless, M.
da Cunha, E.
Davies, L. J. M.
Graham, Alister W.
Holwerda, B. W.
Hopkins, A. M.
Kafle, P. R.
Kelvin, L. S.
Loveday, J.
Maddox, S. J.
Meyer, M. J.
Moffett, A. J.
Norberg, P.
Phillipps, S.
Rowlands, K.
Taylor, E. N.
Wang, L.
Wilkins, S. M.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 470 (01) : 283 - 302
[10] Galaxy and Mass Assembly (GAMA): Accurate number densities and environments of massive ultra-compact galaxies at 0.02 < z < 0.3
Buitrago, F.
Ferreras, I.
Kelvin, L. S.
Baldry, I. K.
Davies, L.
Angthopo, J.
Khochfar, S.
Hopkins, A. M.
Driver, S. P.
Brough, S.
Sabater, J.
Conselice, C. J.
Liske, J.
Holwerda, B. W.
Bremer, M. N.
Phillipps, S.
Lopez-Sanchez, A. R.
Graham, A. W.
ASTRONOMY & ASTROPHYSICS, 2018, 619

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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