UV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST LEGACY FIELDS

The remarkable Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the evolution of the rest-frame UV luminosity function (LF) from z ~ 10 to z ~ 4. We develop new color criteria that more optimally utilize the full wavelengt...

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Vydáno v:	The Astrophysical journal Ročník 803; číslo 1; s. 34 - 49
Hlavní autoři:	Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Trenti, M., Labbé, I., Bradley, L., Carollo, M., van Dokkum, P. G., Gonzalez, V., Holwerda, B., Franx, M., Spitler, L., Smit, R., Magee, D.
Médium:	Journal Article
Jazyk:	angličtina
Vydáno:	United Kingdom 10.04.2015
Témata:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Evolution GALACTIC EVOLUTION GALAXIES Halos LUMINOSITY MASS RED SHIFT Searching SPACE TELESCOPES
ISSN:	1538-4357, 0004-637X, 1538-4357
On-line přístup:	Získat plný text
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Abstract	The remarkable Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the evolution of the rest-frame UV luminosity function (LF) from z ~ 10 to z ~ 4. We develop new color criteria that more optimally utilize the full wavelength coverage from the optical, near-IR, and mid-IR observations over our search fields, while simultaneously minimizing the incompleteness and eliminating redshift gaps. We have identified 5859, 3001, 857, 481, 217, and 6 galaxy candidates at z ~ 4, z ~ 5, z ~ 6, z ~ 7, z ~ 7, and z ~ 10, respectively, from the ~1000 arcmin super(2) area covered by these data sets. This sample of >10,000 galaxy candidates at z [> or =, slanted] 4 is by far the largest assembled to date with HST. The selection of z ~ 4-8 candidates over the five CANDELS fields allows us to assess the cosmic variance; the largest variations are at z [> or =, slanted] 7. Our new LF determinations at z ~ 4 and z ~ 5 span a 6 mag baseline and reach to -16 AB mag. These determinations agree well with previous estimates, but the larger samples and volumes probed here result in a more reliable sampling of >L* galaxies and allow us to reassess the form of the UV LFs. Our new LF results strengthen our earlier findings to 3.4[sigma] significance for a steeper faint-end slope of the UV LF at z > 4, with alpha evolving from alpha = -1.64 + or - 0.04 at z ~ 4 to alpha = -2.06 + or - 0.13 at z ~ 7 (and alpha = -2.02 + or - 0.23 at z ~ 8), consistent with that expected from the evolution of the halo mass function. We find less evolution in the characteristic magnitude M* from z ~ 7 to z ~ 4; the observed evolution in the LF is now largely represented by changes in [phi]*. No evidence for a non-Schechter-like form to the z ~ 4-8 LFs is found. A simple conditional LF model based on halo growth and evolution in the M/L ratio ([is proportional to](1 + z) super(-1.5)) of halos provides a good representation of the observed evolution.
AbstractList	The remarkable Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the evolution of the rest-frame UV luminosity function (LF) from z ~ 10 to z ~ 4. We develop new color criteria that more optimally utilize the full wavelength coverage from the optical, near-IR, and mid-IR observations over our search fields, while simultaneously minimizing the incompleteness and eliminating redshift gaps. We have identified 5859, 3001, 857, 481, 217, and 6 galaxy candidates at z ~ 4, z ~ 5, z ~ 6, z ~ 7, z ~ 7, and z ~ 10, respectively, from the ~1000 arcmin super(2) area covered by these data sets. This sample of >10,000 galaxy candidates at z [> or =, slanted] 4 is by far the largest assembled to date with HST. The selection of z ~ 4-8 candidates over the five CANDELS fields allows us to assess the cosmic variance; the largest variations are at z [> or =, slanted] 7. Our new LF determinations at z ~ 4 and z ~ 5 span a 6 mag baseline and reach to -16 AB mag. These determinations agree well with previous estimates, but the larger samples and volumes probed here result in a more reliable sampling of >L* galaxies and allow us to reassess the form of the UV LFs. Our new LF results strengthen our earlier findings to 3.4[sigma] significance for a steeper faint-end slope of the UV LF at z > 4, with alpha evolving from alpha = -1.64 + or - 0.04 at z ~ 4 to alpha = -2.06 + or - 0.13 at z ~ 7 (and alpha = -2.02 + or - 0.23 at z ~ 8), consistent with that expected from the evolution of the halo mass function. We find less evolution in the characteristic magnitude M* from z ~ 7 to z ~ 4; the observed evolution in the LF is now largely represented by changes in [phi]. No evidence for a non-Schechter-like form to the z ~ 4-8 LFs is found. A simple conditional LF model based on halo growth and evolution in the M/L ratio ([is proportional to](1 + z) super(-1.5)) of halos provides a good representation of the observed evolution. The remarkable Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the evolution of the rest-frame UV luminosity function (LF) from z∼10 to z∼4. We develop new color criteria that more optimally utilize the full wavelength coverage from the optical, near-IR, and mid-IR observations over our search fields, while simultaneously minimizing the incompleteness and eliminating redshift gaps. We have identified 5859, 3001, 857, 481, 217, and 6 galaxy candidates at z∼4, z∼5, z∼6, z∼7, z∼8, and z∼10, respectively, from the ∼1000 arcmin{sup 2} area covered by these data sets. This sample of >10,000 galaxy candidates at z⩾4 is by far the largest assembled to date with HST. The selection of z ∼ 4–8 candidates over the five CANDELS fields allows us to assess the cosmic variance; the largest variations are at z⩾7. Our new LF determinations at z∼4 and z∼5 span a 6 mag baseline and reach to –16 AB mag. These determinations agree well with previous estimates, but the larger samples and volumes probed here result in a more reliable sampling of >L{sup ∗} galaxies and allow us to reassess the form of the UV LFs. Our new LF results strengthen our earlier findings to 3.4σ significance for a steeper faint-end slope of the UV LF at z>4, with α evolving from α=−1.64±0.04 at z∼4 to α=−2.06±0.13 at z∼7 (and α=−2.02±0.23 at z∼8), consistent with that expected from the evolution of the halo mass function. We find less evolution in the characteristic magnitude M{sup } from z∼7 to z∼4; the observed evolution in the LF is now largely represented by changes in ϕ{sup ∗}. No evidence for a non-Schechter-like form to the z ∼ 4–8 LFs is found. A simple conditional LF model based on halo growth and evolution in the M/L ratio (∝(1+z){sup −1.5}) of halos provides a good representation of the observed evolution.
Author	Holwerda, B. Labbé, I. Bradley, L. Franx, M. Carollo, M. Spitler, L. Gonzalez, V. Illingworth, G. D. Trenti, M. Bouwens, R. J. van Dokkum, P. G. Magee, D. Smit, R. Oesch, P. A.
Author_xml	– sequence: 1 givenname: R. J. surname: Bouwens fullname: Bouwens, R. J. – sequence: 2 givenname: G. D. surname: Illingworth fullname: Illingworth, G. D. – sequence: 3 givenname: P. A. surname: Oesch fullname: Oesch, P. A. – sequence: 4 givenname: M. orcidid: 0000-0001-9391-305X surname: Trenti fullname: Trenti, M. – sequence: 5 givenname: I. surname: Labbé fullname: Labbé, I. – sequence: 6 givenname: L. orcidid: 0000-0002-7908-9284 surname: Bradley fullname: Bradley, L. – sequence: 7 givenname: M. surname: Carollo fullname: Carollo, M. – sequence: 8 givenname: P. G. orcidid: 0000-0002-8282-9888 surname: van Dokkum fullname: van Dokkum, P. G. – sequence: 9 givenname: V. surname: Gonzalez fullname: Gonzalez, V. – sequence: 10 givenname: B. surname: Holwerda fullname: Holwerda, B. – sequence: 11 givenname: M. orcidid: 0000-0002-8871-3026 surname: Franx fullname: Franx, M. – sequence: 12 givenname: L. surname: Spitler fullname: Spitler, L. – sequence: 13 givenname: R. orcidid: 0000-0001-8034-7802 surname: Smit fullname: Smit, R. – sequence: 14 givenname: D. surname: Magee fullname: Magee, D.
BackLink	https://www.osti.gov/biblio/22882576$$D View this record in Osti.gov
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Snippet	The remarkable Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the evolution of... The remarkable Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the evolution of...
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SubjectTerms	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Evolution GALACTIC EVOLUTION GALAXIES Halos LUMINOSITY MASS RED SHIFT Searching SPACE TELESCOPES
Title	UV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST LEGACY FIELDS
URI	https://www.proquest.com/docview/1765945505 https://www.proquest.com/docview/1786219040 https://www.osti.gov/biblio/22882576
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