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

Simon P. Driver; Aaron S. G. Robotham; Lee S. Kelvin; Mehmet Alpaslan; Ivan K. Baldry; Steven P. Bamford; Sarah Brough; M. L. Brown; Andrew M. Hopkins; Jochen Liske; Jon Loveday; Peder Norberg; John A. Peacock; Ellen Andrae; Joss Bland-Hawthorn; N. Bourne; Ewan Cameron; Matthew Colless; Christopher J. Conselice; Scott M. Croom; L. Dunne; Carlos S. Frenk; Alister W. Graham; M. Gunawardhana; David T. Hill; David Heath Jones; Konrad Kuijken; Barry F. Madore; Robert C. Nichol; Hannah R. Parkinson; Kevin A. Pimbblet; Steven Phillipps; Cristina C. Popescu; Matthew Prescott; Mark Seibert; Robert G. Sharp; Will J. Sutherland; Edward N. Taylor; Daniel Thomas; Richard J. Tuffs; Eelco Van Kampen; D. B. Wijesinghe; S. Wilkins

doi:10.1111/j.1365-2966.2012.22036.x

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

Simon P. Driver, Aaron S. G. Robotham, Lee S. Kelvin, Mehmet Alpaslan, Ivan K. Baldry, Steven P. Bamford, Sarah Brough, M. L. Brown, Andrew M. Hopkins, Jochen Liske, Jon Loveday, Peder Norberg, John A. Peacock, Ellen Andrae, Joss Bland-Hawthorn, N. Bourne, Ewan Cameron, Matthew Colless, Christopher J. Conselice, Scott M. CroomL. Dunne, Carlos S. Frenk, Alister W. Graham, M. Gunawardhana, David T. Hill, David Heath Jones, Konrad Kuijken, Barry F. Madore, Robert C. Nichol, Hannah R. Parkinson, Kevin A. Pimbblet, Steven Phillipps, Cristina C. Popescu, Matthew Prescott, Mark Seibert, Robert G. Sharp, Will J. Sutherland, Edward N. Taylor, Daniel Thomas, Richard J. Tuffs, Eelco Van Kampen, D. B. Wijesinghe, S. Wilkins

Institute of Cosmology & Gravitation

Research output: Contribution to journal › Article › peer-review

Abstract

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 × 10⁵(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 μm 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) × 1035 h W Mpc⁻³ of which (1.2 ± 0.1) × 10³⁵ h W Mpc⁻³ is directly released into the inter-galactic medium and (0.6 ± 0.1) × 10³⁵ 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 μm 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.

Original language	English
Pages (from-to)	3244-3264
Journal	Monthly Notices of the Royal Astronomical Society
Volume	427
Issue number	4
DOIs	https://doi.org/10.1111/j.1365-2966.2012.22036.x
Publication status	Published - 2012

Keywords

surveys
galaxies: fundamental parameters
galaxies: general
galaxies: luminosity function, mass function
cosmology: observations
infrared: galaxies

Access to Document

10.1111/j.1365-2966.2012.22036.x

Cite this

Driver, S. P., Robotham, A. S. G., Kelvin, L. S., Alpaslan, M., Baldry, I. K., Bamford, S. P., Brough, S., Brown, M. L., Hopkins, A. M., Liske, J., Loveday, J., Norberg, P., Peacock, J. A., Andrae, E., Bland-Hawthorn, J., Bourne, N., Cameron, E., Colless, M., Conselice, C. J., ... Wilkins, S. (2012). Galaxy And Mass Assembly (GAMA): the 0.013 <z <0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm. Monthly Notices of the Royal Astronomical Society, 427(4), 3244-3264. https://doi.org/10.1111/j.1365-2966.2012.22036.x

@article{28bb4fc39df24e37b0c2ba3f665450a9,

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

abstract = "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 × 105 (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 μm 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) × 1035 h W Mpc−3 of which (1.2 ± 0.1) × 1035 h W Mpc−3 is directly released into the inter-galactic medium and (0.6 ± 0.1) × 1035 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 μm 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. ",

keywords = "surveys, galaxies: fundamental parameters, galaxies: general, galaxies: luminosity function, mass function, cosmology: observations, infrared: galaxies",

author = "Driver, {Simon P.} and Robotham, {Aaron S. G.} and Kelvin, {Lee S.} and Mehmet Alpaslan and Baldry, {Ivan K.} and Bamford, {Steven P.} and Sarah Brough and Brown, {M. L.} and Hopkins, {Andrew M.} and Jochen Liske and Jon Loveday and Peder Norberg and Peacock, {John A.} and Ellen Andrae and Joss Bland-Hawthorn and N. Bourne and Ewan Cameron and Matthew Colless and Conselice, {Christopher J.} and Croom, {Scott M.} and L. Dunne and Frenk, {Carlos S.} and Graham, {Alister W.} and M. Gunawardhana and Hill, {David T.} and Jones, {David Heath} and Konrad Kuijken and Madore, {Barry F.} and Nichol, {Robert C.} and Parkinson, {Hannah R.} and Pimbblet, {Kevin A.} and Steven Phillipps and Popescu, {Cristina C.} and Matthew Prescott and Mark Seibert and Sharp, {Robert G.} and Sutherland, {Will J.} and Taylor, {Edward N.} and Daniel Thomas and Tuffs, {Richard J.} and {Van Kampen}, Eelco and Wijesinghe, {D. B.} and S. Wilkins",

year = "2012",

doi = "10.1111/j.1365-2966.2012.22036.x",

language = "English",

volume = "427",

pages = "3244--3264",

journal = "MNRAS",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "4",

}

Driver, SP, Robotham, ASG, Kelvin, LS, Alpaslan, M, Baldry, IK, Bamford, SP, Brough, S, Brown, ML, Hopkins, AM, Liske, J, Loveday, J, Norberg, P, Peacock, JA, Andrae, E, Bland-Hawthorn, J, Bourne, N, Cameron, E, Colless, M, Conselice, CJ, Croom, SM, Dunne, L, Frenk, CS, Graham, AW, Gunawardhana, M, Hill, DT, Jones, DH, Kuijken, K, Madore, BF, Nichol, RC, Parkinson, HR, Pimbblet, KA, Phillipps, S, Popescu, CC, Prescott, M, Seibert, M, Sharp, RG, Sutherland, WJ, Taylor, EN, Thomas, D, Tuffs, RJ, Van Kampen, E, Wijesinghe, DB & Wilkins, S 2012, 'Galaxy And Mass Assembly (GAMA): the 0.013 <z <0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm', Monthly Notices of the Royal Astronomical Society, vol. 427, no. 4, pp. 3244-3264. https://doi.org/10.1111/j.1365-2966.2012.22036.x

TY - JOUR

T1 - Galaxy And Mass Assembly (GAMA)

T2 - the 0.013 <z <0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm

AU - Driver, Simon P.

AU - Robotham, Aaron S. G.

AU - Kelvin, Lee S.

AU - Alpaslan, Mehmet

AU - Baldry, Ivan K.

AU - Bamford, Steven P.

AU - Brough, Sarah

AU - Brown, M. L.

AU - Hopkins, Andrew M.

AU - Liske, Jochen

AU - Loveday, Jon

AU - Norberg, Peder

AU - Peacock, John A.

AU - Andrae, Ellen

AU - Bland-Hawthorn, Joss

AU - Bourne, N.

AU - Cameron, Ewan

AU - Colless, Matthew

AU - Conselice, Christopher J.

AU - Croom, Scott M.

AU - Dunne, L.

AU - Frenk, Carlos S.

AU - Graham, Alister W.

AU - Gunawardhana, M.

AU - Hill, David T.

AU - Jones, David Heath

AU - Kuijken, Konrad

AU - Madore, Barry F.

AU - Nichol, Robert C.

AU - Parkinson, Hannah R.

AU - Pimbblet, Kevin A.

AU - Phillipps, Steven

AU - Popescu, Cristina C.

AU - Prescott, Matthew

AU - Seibert, Mark

AU - Sharp, Robert G.

AU - Sutherland, Will J.

AU - Taylor, Edward N.

AU - Thomas, Daniel

AU - Tuffs, Richard J.

AU - Van Kampen, Eelco

AU - Wijesinghe, D. B.

AU - Wilkins, S.

PY - 2012

Y1 - 2012

N2 - 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 × 105 (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 μm 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) × 1035 h W Mpc−3 of which (1.2 ± 0.1) × 1035 h W Mpc−3 is directly released into the inter-galactic medium and (0.6 ± 0.1) × 1035 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 μm 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.

AB - 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 × 105 (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 μm 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) × 1035 h W Mpc−3 of which (1.2 ± 0.1) × 1035 h W Mpc−3 is directly released into the inter-galactic medium and (0.6 ± 0.1) × 1035 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 μm 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.

KW - surveys

KW - galaxies: fundamental parameters

KW - galaxies: general

KW - galaxies: luminosity function, mass function

KW - cosmology: observations

KW - infrared: galaxies

U2 - 10.1111/j.1365-2966.2012.22036.x

DO - 10.1111/j.1365-2966.2012.22036.x

M3 - Article

VL - 427

SP - 3244

EP - 3264

JO - MNRAS

JF - MNRAS

SN - 0035-8711

IS - 4

ER -

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

Abstract

Keywords

Access to Document

Fingerprint

Cite this