Probing star formation in the dense environments of z ∼ 1 lensing haloes aligned with dusty star-forming galaxies detected with the South Pole Telescope

We probe star formation in the environments of massive (∼1013 M⊙) dark matter haloes at redshifts of z ∼ 1. This star formation is linked to a submillimetre clustering signal which we detect in maps of the Planck High Frequency Instrument that are stacked at the positions of a sample of high redshif...

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Published inMonthly notices of the Royal Astronomical Society Vol. 455; no. 2; pp. 1629 - 1646
Main Authors Welikala, N., Béthermin, M., Guery, D., Strandet, M., Aird, K. A., Aravena, M., Ashby, M. L. N., Bothwell, M., Beelen, A., Bleem, L. E., de Breuck, C., Brodwin, M., Carlstrom, J. E., Chapman, S. C., Crawford, T. M., Dole, H., Doré, O., Everett, W., Flores-Cacho, I., Gonzalez, A. H., González-Nuevo, J., Greve, T. R., Gullberg, B., Hezaveh, Y. D., Holder, G. P., Holzapfel, W. L., Keisler, R., Lagache, G., Ma, J., Malkan, M., Marrone, D. P., Mocanu, L. M., Montier, L., Murphy, E. J., Nesvadba, N. P. H., Omont, A., Pointecouteau, E., Puget, J. L., Reichardt, C. L., Rotermund, K. M., Scott, D., Serra, P., Spilker, J. S., Stalder, B., Stark, A. A., Story, K., Vanderlinde, K., Vieira, J. D., Weiß, A.
Format Journal Article
LanguageEnglish
Published London Oxford University Press 11.01.2016
Royal Astronomical Society
Subjects
ASTRONOMY AND ASTROPHYSICS
Clustering
Corona
Dark matter
Flux
Galaxies
Mathematical models
Red shift
South Pole
Space telescopes
Star & galaxy formation
Star formation
Antarctica, South Pole
surveys
galaxies: formation
submillimetre: galaxies
galaxies: statistics
diffuse radiation
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Abstract We probe star formation in the environments of massive (∼1013 M⊙) dark matter haloes at redshifts of z ∼ 1. This star formation is linked to a submillimetre clustering signal which we detect in maps of the Planck High Frequency Instrument that are stacked at the positions of a sample of high redshift (z > 2) strongly lensed dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope (SPT) 2500 deg2 survey. The clustering signal has submillimetre colours which are consistent with the mean redshift of the foreground lensing haloes (z ∼ 1). We report a mean excess of star formation rate (SFR) compared to the field, of (2700 ± 700) M⊙ yr−1 from all galaxies contributing to this clustering signal within a radius of 3.5 arcmin from the SPT DSFGs. The magnitude of the Planck excess is in broad agreement with predictions of a current model of the cosmic infrared background. The model predicts that 80 per cent of the excess emission measured by Planck originates from galaxies lying in the neighbouring haloes of the lensing halo. Using Herschel maps of the same fields, we find a clear excess, relative to the field, of individual sources which contribute to the Planck excess. The mean excess SFR compared to the field is measured to be (370 ± 40) M⊙ yr−1 per resolved, clustered source. Our findings suggest that the environments around these massive z ∼ 1 lensing haloes host intense star formation out to about 2 Mpc. The flux enhancement due to clustering should also be considered when measuring flux densities of galaxies in Planck data.
AbstractList We probe star formation in the environments of massive (...) dark matter haloes at redshifts of z ~ 1. This star formation is linked to a submillimetre clustering signal which we detect in maps of the Planck High Frequency Instrument that are stacked at the positions of a sample of high redshift (z > 2) strongly lensed dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope (SPT) 2500 deg2 survey. The clustering signal has submillimetre colours which are consistent with the mean redshift of the foreground lensing haloes (z ~ 1). We report a mean excess of star formation rate (SFR) compared to the field, of (2700 plus or minus 700) ... from all galaxies contributing to this clustering signal within a radius of 3.5 arcmin from the SPT DSFGs. The magnitude of the Planck excess is in broad agreement with predictions of a current model of the cosmic infrared background. The model predicts that 80 per cent of the excess emission measured by Planck originates from galaxies lying in the neighbouring haloes of the lensing halo. UsingHerschel maps of the same fields, we find a clear excess, relative to the field, of individual sources which contribute to the Planckexcess. The mean excess SFR compared to the field is measured to be (370 plus or minus 40) ... per resolved, clustered source. Our findings suggest that the environments around these massive z ~ 1 lensing haloes host intense star formation out to about 2 Mpc. The flux enhancement due to clustering should also be considered when measuring flux densities of galaxies in Planck data. (ProQuest: ... denotes formulae/symbols omitted.)
We probe star formation in the environments of massive ~1013M⊙ dark matter halos at redshifts of z~1. This star formation is linked to a sub-millimetre clustering signal which we detect in maps of the Planck High Frequency Instrument that are stacked at the positions of a sample of high-redshift (z>2) strongly-lensed dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope (SPT) 2500 deg2 survey. The clustering signal has sub-millimetre colours which are consistent with the mean redshift of the foreground lensing halos (z~1). We report a mean excess of star formation rate (SFR) compared to the field, of (2700±700)M⊙yr-1 from all galaxies contributing to this clustering signal within a radius of 3.5' from the SPT DSFGs. The magnitude of the Planck excess is in broad agreement with predictions of a current model of the cosmic infrared background. The model predicts that 80% of the excess emission measured by Planck originates from galaxies lying in the neighbouring halos of the lensing halo. Using Herschel maps of the same fields, we find a clear excess, relative to the field, of individual sources which contribute to the Planck excess. The mean excess SFR compared to the field is measured to be (370±40)M⊙yr-1 per resolved, clustered source. Our findings suggest that the environments around these massive z~1 lensing halos host intense star formation out to about 2Mpc. The flux enhancement due to clustering should also be considered when measuring flux densities of galaxies in Planck data.
We probe star formation in the environments of massive (∼1013 M⊙) dark matter haloes at redshifts of z ∼ 1. This star formation is linked to a submillimetre clustering signal which we detect in maps of the Planck High Frequency Instrument that are stacked at the positions of a sample of high redshift (z > 2) strongly lensed dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope (SPT) 2500 deg2 survey. The clustering signal has submillimetre colours which are consistent with the mean redshift of the foreground lensing haloes (z ∼ 1). We report a mean excess of star formation rate (SFR) compared to the field, of (2700 ± 700) M⊙ yr−1 from all galaxies contributing to this clustering signal within a radius of 3.5 arcmin from the SPT DSFGs. The magnitude of the Planck excess is in broad agreement with predictions of a current model of the cosmic infrared background. The model predicts that 80 per cent of the excess emission measured by Planck originates from galaxies lying in the neighbouring haloes of the lensing halo. Using Herschel maps of the same fields, we find a clear excess, relative to the field, of individual sources which contribute to the Planck excess. The mean excess SFR compared to the field is measured to be (370 ± 40) M⊙ yr−1 per resolved, clustered source. Our findings suggest that the environments around these massive z ∼ 1 lensing haloes host intense star formation out to about 2 Mpc. The flux enhancement due to clustering should also be considered when measuring flux densities of galaxies in Planck data.
We probe star formation in the environments of massive (...) dark matter haloes at redshifts of z ~ 1. This star formation is linked to a submillimetre clustering signal which we detect in maps of the Planck High Frequency Instrument that are stacked at the positions of a sample of high redshift (z > 2) strongly lensed dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope (SPT) 2500 deg2 survey. The clustering signal has submillimetre colours which are consistent with the mean redshift of the foreground lensing haloes (z ~ 1). We report a mean excess of star formation rate (SFR) compared to the field, of (2700 ± 700) ... from all galaxies contributing to this clustering signal within a radius of 3.5 arcmin from the SPT DSFGs. The magnitude of the Planck excess is in broad agreement with predictions of a current model of the cosmic infrared background. The model predicts that 80 per cent of the excess emission measured by Planck originates from galaxies lying in the neighbouring haloes of the lensing halo. UsingHerschel maps of the same fields, we find a clear excess, relative to the field, of individual sources which contribute to the Planckexcess. The mean excess SFR compared to the field is measured to be (370 ± 40) ... per resolved, clustered source. Our findings suggest that the environments around these massive z ~ 1 lensing haloes host intense star formation out to about 2 Mpc. The flux enhancement due to clustering should also be considered when measuring flux densities of galaxies in Planck data. (ProQuest: ... denotes formulae/symbols omitted.)
Author Guery, D.
Bleem, L. E.
Keisler, R.
Gullberg, B.
Montier, L.
Rotermund, K. M.
Hezaveh, Y. D.
Beelen, A.
Strandet, M.
Ma, J.
Scott, D.
González-Nuevo, J.
Spilker, J. S.
Dole, H.
Reichardt, C. L.
Gonzalez, A. H.
Aravena, M.
Mocanu, L. M.
Béthermin, M.
Stalder, B.
Bothwell, M.
Nesvadba, N. P. H.
Serra, P.
Carlstrom, J. E.
Doré, O.
Omont, A.
Stark, A. A.
Puget, J. L.
Marrone, D. P.
Brodwin, M.
Everett, W.
Flores-Cacho, I.
Vanderlinde, K.
Vieira, J. D.
Chapman, S. C.
Pointecouteau, E.
Story, K.
Aird, K. A.
Crawford, T. M.
Weiß, A.
Holder, G. P.
Murphy, E. J.
Ashby, M. L. N.
Malkan, M.
Lagache, G.
Holzapfel, W. L.
Welikala, N.
de Breuck, C.
Greve, T. R.
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Snippet We probe star formation in the environments of massive (∼1013 M⊙) dark matter haloes at redshifts of z ∼ 1. This star formation is linked to a submillimetre...
We probe star formation in the environments of massive (...) dark matter haloes at redshifts of z ~ 1. This star formation is linked to a submillimetre...
We probe star formation in the environments of massive ~1013M⊙ dark matter halos at redshifts of z~1. This star formation is linked to a sub-millimetre...
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SubjectTerms ASTRONOMY AND ASTROPHYSICS
Clustering
Corona
Dark matter
Flux
Galaxies
Mathematical models
Red shift
South Pole
Space telescopes
Star & galaxy formation
Star formation
Title Probing star formation in the dense environments of z ∼ 1 lensing haloes aligned with dusty star-forming galaxies detected with the South Pole Telescope
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https://search.proquest.com/docview/1762372974
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https://www.osti.gov/biblio/1390826
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