Lens models of Herschel-selected galaxies from high-resolution near-IR observations

We present Keck-Adaptive Optics and Hubble Space Telescope high resolution near-infrared (IR) imaging for 500 μm bright candidate lensing systems identified by the Herschel Multi-tiered Extragalactic Survey and Herschel Astrophysical Terahertz Large Area Survey. Out of 87 candidates with near-IR ima...

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Main Authors: Calanog, J.A., Fu, Hai, Cooray, A., Wardlow, J., Ma, B., Amber, S., Baker, A.J., Baes, M., Bock, J., Bourne, N., Bussmann, R.S., Casey, C.M., Chapman, S.C., Clements, D.L., Conley, A., Dannerbauer, H., De Zotti, G., Dunne, L., Dye, S., Eales, S., Farrah, D., Furlanetto, C., Harris, A.I., Ivison, R.J., Kim, S., Maddox, S.J., Magdis, G., Messias, H., Michałowski, M.J., Negrello, M., Nightingale, J., O'Bryan, J.M., Oliver, S.J., Riechers, D., Scott, D., Serjeant, S., Simpson, J., Smith, M., Timmons, N., Thacker, C., Valiante, E., Vieira, J.D.
Format: Article
Published: American Astronomical Society 2014
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Online Access:https://eprints.nottingham.ac.uk/42373/
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author Calanog, J.A.
Fu, Hai
Cooray, A.
Wardlow, J.
Ma, B.
Amber, S.
Baker, A.J.
Baes, M.
Bock, J.
Bourne, N.
Bussmann, R.S.
Casey, C.M.
Chapman, S.C.
Clements, D.L.
Conley, A.
Dannerbauer, H.
De Zotti, G.
Dunne, L.
Dye, S.
Eales, S.
Farrah, D.
Furlanetto, C.
Harris, A.I.
Ivison, R.J.
Kim, S.
Maddox, S.J.
Magdis, G.
Messias, H.
Michałowski, M.J.
Negrello, M.
Nightingale, J.
O'Bryan, J.M.
Oliver, S.J.
Riechers, D.
Scott, D.
Serjeant, S.
Simpson, J.
Smith, M.
Timmons, N.
Thacker, C.
Valiante, E.
Vieira, J.D.
author_facet Calanog, J.A.
Fu, Hai
Cooray, A.
Wardlow, J.
Ma, B.
Amber, S.
Baker, A.J.
Baes, M.
Bock, J.
Bourne, N.
Bussmann, R.S.
Casey, C.M.
Chapman, S.C.
Clements, D.L.
Conley, A.
Dannerbauer, H.
De Zotti, G.
Dunne, L.
Dye, S.
Eales, S.
Farrah, D.
Furlanetto, C.
Harris, A.I.
Ivison, R.J.
Kim, S.
Maddox, S.J.
Magdis, G.
Messias, H.
Michałowski, M.J.
Negrello, M.
Nightingale, J.
O'Bryan, J.M.
Oliver, S.J.
Riechers, D.
Scott, D.
Serjeant, S.
Simpson, J.
Smith, M.
Timmons, N.
Thacker, C.
Valiante, E.
Vieira, J.D.
author_sort Calanog, J.A.
building Nottingham Research Data Repository
collection Online Access
description We present Keck-Adaptive Optics and Hubble Space Telescope high resolution near-infrared (IR) imaging for 500 μm bright candidate lensing systems identified by the Herschel Multi-tiered Extragalactic Survey and Herschel Astrophysical Terahertz Large Area Survey. Out of 87 candidates with near-IR imaging, 15 (~17%) display clear near-IR lensing morphologies. We present near-IR lens models to reconstruct and recover basic rest-frame optical morphological properties of the background galaxies from 12 new systems. Sources with the largest near-IR magnification factors also tend to be the most compact, consistent with the size bias predicted from simulations and previous lensing models for submillimeter galaxies (SMGs). For four new sources that also have high-resolution submillimeter maps, we test for differential lensing between the stellar and dust components and find that the 880 μm magnification factor (μ880) is ~1.5 times higher than the near-IR magnification factor (μNIR), on average. We also find that the stellar emission is ~2 times more extended in size than dust. The rest-frame optical properties of our sample of Herschel-selected lensed SMGs are consistent with those of unlensed SMGs, which suggests that the two populations are similar.
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institution University of Nottingham Malaysia Campus
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last_indexed 2025-11-14T19:48:33Z
publishDate 2014
publisher American Astronomical Society
recordtype eprints
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spelling nottingham-423732020-05-04T16:59:01Z https://eprints.nottingham.ac.uk/42373/ Lens models of Herschel-selected galaxies from high-resolution near-IR observations Calanog, J.A. Fu, Hai Cooray, A. Wardlow, J. Ma, B. Amber, S. Baker, A.J. Baes, M. Bock, J. Bourne, N. Bussmann, R.S. Casey, C.M. Chapman, S.C. Clements, D.L. Conley, A. Dannerbauer, H. De Zotti, G. Dunne, L. Dye, S. Eales, S. Farrah, D. Furlanetto, C. Harris, A.I. Ivison, R.J. Kim, S. Maddox, S.J. Magdis, G. Messias, H. Michałowski, M.J. Negrello, M. Nightingale, J. O'Bryan, J.M. Oliver, S.J. Riechers, D. Scott, D. Serjeant, S. Simpson, J. Smith, M. Timmons, N. Thacker, C. Valiante, E. Vieira, J.D. We present Keck-Adaptive Optics and Hubble Space Telescope high resolution near-infrared (IR) imaging for 500 μm bright candidate lensing systems identified by the Herschel Multi-tiered Extragalactic Survey and Herschel Astrophysical Terahertz Large Area Survey. Out of 87 candidates with near-IR imaging, 15 (~17%) display clear near-IR lensing morphologies. We present near-IR lens models to reconstruct and recover basic rest-frame optical morphological properties of the background galaxies from 12 new systems. Sources with the largest near-IR magnification factors also tend to be the most compact, consistent with the size bias predicted from simulations and previous lensing models for submillimeter galaxies (SMGs). For four new sources that also have high-resolution submillimeter maps, we test for differential lensing between the stellar and dust components and find that the 880 μm magnification factor (μ880) is ~1.5 times higher than the near-IR magnification factor (μNIR), on average. We also find that the stellar emission is ~2 times more extended in size than dust. The rest-frame optical properties of our sample of Herschel-selected lensed SMGs are consistent with those of unlensed SMGs, which suggests that the two populations are similar. American Astronomical Society 2014-12-08 Article PeerReviewed Calanog, J.A., Fu, Hai, Cooray, A., Wardlow, J., Ma, B., Amber, S., Baker, A.J., Baes, M., Bock, J., Bourne, N., Bussmann, R.S., Casey, C.M., Chapman, S.C., Clements, D.L., Conley, A., Dannerbauer, H., De Zotti, G., Dunne, L., Dye, S., Eales, S., Farrah, D., Furlanetto, C., Harris, A.I., Ivison, R.J., Kim, S., Maddox, S.J., Magdis, G., Messias, H., Michałowski, M.J., Negrello, M., Nightingale, J., O'Bryan, J.M., Oliver, S.J., Riechers, D., Scott, D., Serjeant, S., Simpson, J., Smith, M., Timmons, N., Thacker, C., Valiante, E. and Vieira, J.D. (2014) Lens models of Herschel-selected galaxies from high-resolution near-IR observations. Astrophysical Journal, 797 (2). p. 138. ISSN 1538-4357 galaxies: star formation; gravitational lensing: strong; submillimeter: galaxies http://iopscience.iop.org/article/10.1088/0004-637X/797/2/138/meta doi:10.1088/0004-637X/797/2/138 doi:10.1088/0004-637X/797/2/138
spellingShingle galaxies: star formation; gravitational lensing: strong; submillimeter: galaxies
Calanog, J.A.
Fu, Hai
Cooray, A.
Wardlow, J.
Ma, B.
Amber, S.
Baker, A.J.
Baes, M.
Bock, J.
Bourne, N.
Bussmann, R.S.
Casey, C.M.
Chapman, S.C.
Clements, D.L.
Conley, A.
Dannerbauer, H.
De Zotti, G.
Dunne, L.
Dye, S.
Eales, S.
Farrah, D.
Furlanetto, C.
Harris, A.I.
Ivison, R.J.
Kim, S.
Maddox, S.J.
Magdis, G.
Messias, H.
Michałowski, M.J.
Negrello, M.
Nightingale, J.
O'Bryan, J.M.
Oliver, S.J.
Riechers, D.
Scott, D.
Serjeant, S.
Simpson, J.
Smith, M.
Timmons, N.
Thacker, C.
Valiante, E.
Vieira, J.D.
Lens models of Herschel-selected galaxies from high-resolution near-IR observations
title Lens models of Herschel-selected galaxies from high-resolution near-IR observations
title_full Lens models of Herschel-selected galaxies from high-resolution near-IR observations
title_fullStr Lens models of Herschel-selected galaxies from high-resolution near-IR observations
title_full_unstemmed Lens models of Herschel-selected galaxies from high-resolution near-IR observations
title_short Lens models of Herschel-selected galaxies from high-resolution near-IR observations
title_sort lens models of herschel-selected galaxies from high-resolution near-ir observations
topic galaxies: star formation; gravitational lensing: strong; submillimeter: galaxies
url https://eprints.nottingham.ac.uk/42373/
https://eprints.nottingham.ac.uk/42373/
https://eprints.nottingham.ac.uk/42373/