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The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations

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The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations. / Bakx, Tom J. L. C.; Eales, S. A.; Negrello, M. et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 473, No. 2, 11.01.2018, p. 1751-1773.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Bakx, TJLC, Eales, SA, Negrello, M, Smith, MWL, Valiante, E, Holland, WS, Baes, M, Bourne, N, Clements, DL, Dannerbauer, H, De Zotti, G, Dunne, L, Dye, S, Furlanetto, C, Ivison, RJ, Maddox, S, Marchetti, L, Michałowski, MJ, Omont, A, Oteo, I, Wardlow, JL, van der Werf, P & Yang, C 2018, 'The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations', Monthly Notices of the Royal Astronomical Society, vol. 473, no. 2, pp. 1751-1773. https://doi.org/10.1093/mnras/stx2267

APA

Bakx, T. J. L. C., Eales, S. A., Negrello, M., Smith, M. W. L., Valiante, E., Holland, W. S., Baes, M., Bourne, N., Clements, D. L., Dannerbauer, H., De Zotti, G., Dunne, L., Dye, S., Furlanetto, C., Ivison, R. J., Maddox, S., Marchetti, L., Michałowski, M. J., Omont, A., ... Yang, C. (2018). The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations. Monthly Notices of the Royal Astronomical Society, 473(2), 1751-1773. https://doi.org/10.1093/mnras/stx2267

Vancouver

Bakx TJLC, Eales SA, Negrello M, Smith MWL, Valiante E, Holland WS et al. The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations. Monthly Notices of the Royal Astronomical Society. 2018 Jan 11;473(2):1751-1773. Epub 2017 Sept 4. doi: 10.1093/mnras/stx2267

Author

Bakx, Tom J. L. C. ; Eales, S. A. ; Negrello, M. et al. / The Herschel Bright Sources (HerBS) : sample definition and SCUBA-2 observations. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 473, No. 2. pp. 1751-1773.

Bibtex

@article{a9d7371ac87647f3b30dc1df0de41e03,
title = "The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations",
abstract = "We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 deg2 Herschel Astrophysical Terahertz Large Area Survey. The HerBS sample contains 209 galaxies, selected with a 500 μm flux density greater than 80 mJy and an estimated redshift greater than 2. The sample consists of a combination of hyperluminous infrared galaxies and lensed ultraluminous infrared galaxies during the epoch of peak cosmic star formation. In this paper, we present Submillimetre Common-User Bolometer Array 2 (SCUBA-2) observations at 850 μm of 189 galaxies of the HerBS sample, 152 of these sources were detected. We fit a spectral template to the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) and 850 μm SCUBA-2 flux densities of 22 sources with spectroscopically determined redshifts, using a two-component modified blackbody spectrum as a template. We find a cold- and hot-dust temperature of 21.29_{-1.66}^{+1.35} and 45.80_{-3.48}^{+2.88} K, a cold-to-hot dust mass ratio of 26.62_{-6.74}^{+5.61} and a β of 1.83_{-0.28}^{+0.14}. The poor quality of the fit suggests that the sample of galaxies is too diverse to be explained by our simple model. Comparison of our sample to a galaxy evolution model indicates that the fraction of lenses are high. Out of the 152 SCUBA-2 detected galaxies, the model predicts 128.4 ± 2.1 of those galaxies to be lensed (84.5 per cent). The SPIRE 500 μm flux suggests that out of all 209 HerBS sources, we expect 158.1 ± 1.7 lensed sources, giving a total lensing fraction of 76 per cent.",
keywords = "gravitational lensing: strong, galaxies: high-redshift, submillimetre: galaxies",
author = "Bakx, {Tom J. L. C.} and Eales, {S. A.} and M. Negrello and Smith, {M. W. L.} and E. Valiante and Holland, {W. S.} and M. Baes and N. Bourne and Clements, {D. L.} and H. Dannerbauer and {De Zotti}, G. and L. Dunne and S. Dye and C. Furlanetto and Ivison, {R. J.} and S. Maddox and L. Marchetti and Micha{\l}owski, {M. J.} and A. Omont and I. Oteo and Wardlow, {J. L.} and {van der Werf}, P. and C. Yang",
note = "This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society {\textcopyright}: 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.",
year = "2018",
month = jan,
day = "11",
doi = "10.1093/mnras/stx2267",
language = "English",
volume = "473",
pages = "1751--1773",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "2",

}

RIS

TY - JOUR

T1 - The Herschel Bright Sources (HerBS)

T2 - sample definition and SCUBA-2 observations

AU - Bakx, Tom J. L. C.

AU - Eales, S. A.

AU - Negrello, M.

AU - Smith, M. W. L.

AU - Valiante, E.

AU - Holland, W. S.

AU - Baes, M.

AU - Bourne, N.

AU - Clements, D. L.

AU - Dannerbauer, H.

AU - De Zotti, G.

AU - Dunne, L.

AU - Dye, S.

AU - Furlanetto, C.

AU - Ivison, R. J.

AU - Maddox, S.

AU - Marchetti, L.

AU - Michałowski, M. J.

AU - Omont, A.

AU - Oteo, I.

AU - Wardlow, J. L.

AU - van der Werf, P.

AU - Yang, C.

N1 - This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

PY - 2018/1/11

Y1 - 2018/1/11

N2 - We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 deg2 Herschel Astrophysical Terahertz Large Area Survey. The HerBS sample contains 209 galaxies, selected with a 500 μm flux density greater than 80 mJy and an estimated redshift greater than 2. The sample consists of a combination of hyperluminous infrared galaxies and lensed ultraluminous infrared galaxies during the epoch of peak cosmic star formation. In this paper, we present Submillimetre Common-User Bolometer Array 2 (SCUBA-2) observations at 850 μm of 189 galaxies of the HerBS sample, 152 of these sources were detected. We fit a spectral template to the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) and 850 μm SCUBA-2 flux densities of 22 sources with spectroscopically determined redshifts, using a two-component modified blackbody spectrum as a template. We find a cold- and hot-dust temperature of 21.29_{-1.66}^{+1.35} and 45.80_{-3.48}^{+2.88} K, a cold-to-hot dust mass ratio of 26.62_{-6.74}^{+5.61} and a β of 1.83_{-0.28}^{+0.14}. The poor quality of the fit suggests that the sample of galaxies is too diverse to be explained by our simple model. Comparison of our sample to a galaxy evolution model indicates that the fraction of lenses are high. Out of the 152 SCUBA-2 detected galaxies, the model predicts 128.4 ± 2.1 of those galaxies to be lensed (84.5 per cent). The SPIRE 500 μm flux suggests that out of all 209 HerBS sources, we expect 158.1 ± 1.7 lensed sources, giving a total lensing fraction of 76 per cent.

AB - We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 deg2 Herschel Astrophysical Terahertz Large Area Survey. The HerBS sample contains 209 galaxies, selected with a 500 μm flux density greater than 80 mJy and an estimated redshift greater than 2. The sample consists of a combination of hyperluminous infrared galaxies and lensed ultraluminous infrared galaxies during the epoch of peak cosmic star formation. In this paper, we present Submillimetre Common-User Bolometer Array 2 (SCUBA-2) observations at 850 μm of 189 galaxies of the HerBS sample, 152 of these sources were detected. We fit a spectral template to the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) and 850 μm SCUBA-2 flux densities of 22 sources with spectroscopically determined redshifts, using a two-component modified blackbody spectrum as a template. We find a cold- and hot-dust temperature of 21.29_{-1.66}^{+1.35} and 45.80_{-3.48}^{+2.88} K, a cold-to-hot dust mass ratio of 26.62_{-6.74}^{+5.61} and a β of 1.83_{-0.28}^{+0.14}. The poor quality of the fit suggests that the sample of galaxies is too diverse to be explained by our simple model. Comparison of our sample to a galaxy evolution model indicates that the fraction of lenses are high. Out of the 152 SCUBA-2 detected galaxies, the model predicts 128.4 ± 2.1 of those galaxies to be lensed (84.5 per cent). The SPIRE 500 μm flux suggests that out of all 209 HerBS sources, we expect 158.1 ± 1.7 lensed sources, giving a total lensing fraction of 76 per cent.

KW - gravitational lensing: strong

KW - galaxies: high-redshift

KW - submillimetre: galaxies

U2 - 10.1093/mnras/stx2267

DO - 10.1093/mnras/stx2267

M3 - Journal article

VL - 473

SP - 1751

EP - 1773

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -