Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel

Rebecca Larson, Shardha Jogee, Nicholas Watson, Marco Viero, Tim Weinzirl, Harold W. Yorke, Steve Finkelstein, Casey Papovich, Caitlin M. Casey, Robin Ciardullo, Caryl Gronwall, Stephanie LaMassa, C. Meg Urry

Research output: Contribution to journalConference article

Abstract

In the next few years, we will embark on an unprecedented study of how a million galaxie grow their stars and dark matter halos over a large comoving volume (0.5 Gpc3) in the cosmi web at the epoch (1:9 < z < 3:5) where cosmic star formation and black hole activity peak, an proto-clusters start to collapse. This study is enabled by the powerful synergy of six photometri and spectroscopic surveys, which are providing Herschel SPIRE, Spitzer IRAC, NEWFIRM Kband DECam ugriz, and XMM X-ray imaging data, along with future optical spectroscopic dat from HETDEX over a very large area (28 deg2) in the Stripe82/HETDEX field. In this work we illustrate the power of these combined datasets and focus on studying dusty, star-formin systems (DSFSs) identified by the Herschel Stripe 82 Survey (HerS). Using the 250, 350, an 500 micron SPIRE data over our 28 deg2 field, we identify a number of possible high redshif (z > 4) DSFSs which will be prime candidates for follow-up observations. We discuss thei properties and possible association with galaxies and quasars detected at X-ray, IR, optical, an UV wavelengths. We discuss broader implications for galaxy growth at early cosmic times.

Original languageEnglish (US)
Article number029
JournalProceedings of Science
Volume18-20-October-2015
StatePublished - Jan 1 2015
Event16th Frank N. Bash Symposium, BASH 2015 - Austin, United States
Duration: Oct 18 2015Oct 20 2015

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galaxies
stars
quasars
halos
dark matter
time measurement
wavelengths
x rays

All Science Journal Classification (ASJC) codes

  • General

Cite this

Larson, R., Jogee, S., Watson, N., Viero, M., Weinzirl, T., Yorke, H. W., ... Urry, C. M. (2015). Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel. Proceedings of Science, 18-20-October-2015, [029].
Larson, Rebecca ; Jogee, Shardha ; Watson, Nicholas ; Viero, Marco ; Weinzirl, Tim ; Yorke, Harold W. ; Finkelstein, Steve ; Papovich, Casey ; Casey, Caitlin M. ; Ciardullo, Robin ; Gronwall, Caryl ; LaMassa, Stephanie ; Urry, C. Meg. / Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel. In: Proceedings of Science. 2015 ; Vol. 18-20-October-2015.
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title = "Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel",
abstract = "In the next few years, we will embark on an unprecedented study of how a million galaxie grow their stars and dark matter halos over a large comoving volume (0.5 Gpc3) in the cosmi web at the epoch (1:9 < z < 3:5) where cosmic star formation and black hole activity peak, an proto-clusters start to collapse. This study is enabled by the powerful synergy of six photometri and spectroscopic surveys, which are providing Herschel SPIRE, Spitzer IRAC, NEWFIRM Kband DECam ugriz, and XMM X-ray imaging data, along with future optical spectroscopic dat from HETDEX over a very large area (28 deg2) in the Stripe82/HETDEX field. In this work we illustrate the power of these combined datasets and focus on studying dusty, star-formin systems (DSFSs) identified by the Herschel Stripe 82 Survey (HerS). Using the 250, 350, an 500 micron SPIRE data over our 28 deg2 field, we identify a number of possible high redshif (z > 4) DSFSs which will be prime candidates for follow-up observations. We discuss thei properties and possible association with galaxies and quasars detected at X-ray, IR, optical, an UV wavelengths. We discuss broader implications for galaxy growth at early cosmic times.",
author = "Rebecca Larson and Shardha Jogee and Nicholas Watson and Marco Viero and Tim Weinzirl and Yorke, {Harold W.} and Steve Finkelstein and Casey Papovich and Casey, {Caitlin M.} and Robin Ciardullo and Caryl Gronwall and Stephanie LaMassa and Urry, {C. Meg}",
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Larson, R, Jogee, S, Watson, N, Viero, M, Weinzirl, T, Yorke, HW, Finkelstein, S, Papovich, C, Casey, CM, Ciardullo, R, Gronwall, C, LaMassa, S & Urry, CM 2015, 'Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel', Proceedings of Science, vol. 18-20-October-2015, 029.

Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel. / Larson, Rebecca; Jogee, Shardha; Watson, Nicholas; Viero, Marco; Weinzirl, Tim; Yorke, Harold W.; Finkelstein, Steve; Papovich, Casey; Casey, Caitlin M.; Ciardullo, Robin; Gronwall, Caryl; LaMassa, Stephanie; Urry, C. Meg.

In: Proceedings of Science, Vol. 18-20-October-2015, 029, 01.01.2015.

Research output: Contribution to journalConference article

TY - JOUR

T1 - Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel

AU - Larson, Rebecca

AU - Jogee, Shardha

AU - Watson, Nicholas

AU - Viero, Marco

AU - Weinzirl, Tim

AU - Yorke, Harold W.

AU - Finkelstein, Steve

AU - Papovich, Casey

AU - Casey, Caitlin M.

AU - Ciardullo, Robin

AU - Gronwall, Caryl

AU - LaMassa, Stephanie

AU - Urry, C. Meg

PY - 2015/1/1

Y1 - 2015/1/1

N2 - In the next few years, we will embark on an unprecedented study of how a million galaxie grow their stars and dark matter halos over a large comoving volume (0.5 Gpc3) in the cosmi web at the epoch (1:9 < z < 3:5) where cosmic star formation and black hole activity peak, an proto-clusters start to collapse. This study is enabled by the powerful synergy of six photometri and spectroscopic surveys, which are providing Herschel SPIRE, Spitzer IRAC, NEWFIRM Kband DECam ugriz, and XMM X-ray imaging data, along with future optical spectroscopic dat from HETDEX over a very large area (28 deg2) in the Stripe82/HETDEX field. In this work we illustrate the power of these combined datasets and focus on studying dusty, star-formin systems (DSFSs) identified by the Herschel Stripe 82 Survey (HerS). Using the 250, 350, an 500 micron SPIRE data over our 28 deg2 field, we identify a number of possible high redshif (z > 4) DSFSs which will be prime candidates for follow-up observations. We discuss thei properties and possible association with galaxies and quasars detected at X-ray, IR, optical, an UV wavelengths. We discuss broader implications for galaxy growth at early cosmic times.

AB - In the next few years, we will embark on an unprecedented study of how a million galaxie grow their stars and dark matter halos over a large comoving volume (0.5 Gpc3) in the cosmi web at the epoch (1:9 < z < 3:5) where cosmic star formation and black hole activity peak, an proto-clusters start to collapse. This study is enabled by the powerful synergy of six photometri and spectroscopic surveys, which are providing Herschel SPIRE, Spitzer IRAC, NEWFIRM Kband DECam ugriz, and XMM X-ray imaging data, along with future optical spectroscopic dat from HETDEX over a very large area (28 deg2) in the Stripe82/HETDEX field. In this work we illustrate the power of these combined datasets and focus on studying dusty, star-formin systems (DSFSs) identified by the Herschel Stripe 82 Survey (HerS). Using the 250, 350, an 500 micron SPIRE data over our 28 deg2 field, we identify a number of possible high redshif (z > 4) DSFSs which will be prime candidates for follow-up observations. We discuss thei properties and possible association with galaxies and quasars detected at X-ray, IR, optical, an UV wavelengths. We discuss broader implications for galaxy growth at early cosmic times.

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JO - Proceedings of Science

JF - Proceedings of Science

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Larson R, Jogee S, Watson N, Viero M, Weinzirl T, Yorke HW et al. Probing galaxy growth and dusty star-forming systems at z > 1.5 across diverse environments in the stripe82/hetdex field with herschel. Proceedings of Science. 2015 Jan 1;18-20-October-2015. 029.