The 2dF-SDSS LRG and QSO Survey: The z<2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85

We have used the 2dF instrument on the AAT to obtain redshifts of a sample of z&lt;3, 18.0<g<21.85 (2000).="" (2004),="" (2qz)="" (2slaq).="" 105.7="" 2df="" 2df-sdss="" 2qz="" 2slaq="" 32%="&quo...

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Glavni autori: Richards, G, Croom, S, Anderson, S, Bland-Hawthorn, J, Boyle, B, Propris, R, Drinkwater, M, Fan, X, Gunn, J, Ivezic, Z, Jester, S, Loveday, J, Meiksin, A, Miller, L, Myers, A, Nichol, R, Outram, P, Pimbblet, K, Roseboom, I, Ross, N, Schneider, D, Shanks, T, Sharp, R, Stoughton, C, Strauss, M
Format: Journal article
Jezik:English
Izdano: 2005
_version_ 1826281210853195776
author Richards, G
Croom, S
Anderson, S
Bland-Hawthorn, J
Boyle, B
Propris, R
Drinkwater, M
Fan, X
Gunn, J
Ivezic, Z
Jester, S
Loveday, J
Meiksin, A
Miller, L
Myers, A
Nichol, R
Outram, P
Pimbblet, K
Roseboom, I
Ross, N
Schneider, D
Shanks, T
Sharp, R
Stoughton, C
Strauss, M
author_facet Richards, G
Croom, S
Anderson, S
Bland-Hawthorn, J
Boyle, B
Propris, R
Drinkwater, M
Fan, X
Gunn, J
Ivezic, Z
Jester, S
Loveday, J
Meiksin, A
Miller, L
Myers, A
Nichol, R
Outram, P
Pimbblet, K
Roseboom, I
Ross, N
Schneider, D
Shanks, T
Sharp, R
Stoughton, C
Strauss, M
author_sort Richards, G
collection OXFORD
description We have used the 2dF instrument on the AAT to obtain redshifts of a sample of z&lt;3, 18.0<g<21.85 (2000).="" (2004),="" (2qz)="" (2slaq).="" 105.7="" 2df="" 2df-sdss="" 2qz="" 2slaq="" 32%="" 5645="" a="" adopted="" agree="" al.="" algorithm="" all="" allow="" analysis,="" and="" are="" at="" beta="-1.45+/-0.03" boyle="" bright="" but="" consistent="" counts="" croom="" data="" deg^2.="" describe="" determinations="" end="" et="" faint="" final="" find="" fit="" for="" form="" from="" function="" functional="" g="" g\sim20.2.="" however,="" if="" imaging.="" in="" inconsistent="" is="" joint="" larger="" likelihood="" lrg="" luminosity="" maximum="" more="" normalization="" not="" number="" of="" only="" other="" our="" parameterization,="" parameters="" part="" preliminary="" present="" programme:="" qso="" quasar="" quasars="" redshift="" resulting="" results="" sdss="" selected="" selection="" slope="" steeper="" survey="" than="" the="" these="" to="" using="" vary="" vary.="" we="" well="" with="" yields="">21 deep surveys. The 2SLAQ data exhibit no well defined ``break'' but do clearly flatten with increasing magnitude. The shape of the quasar luminosity function derived from 2SLAQ is in good agreement with that derived from type I quasars found in hard X-ray surveys. [Abridged]</g<21.85>
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spelling oxford-uuid:7df806a3-bda8-4038-9971-cd7b3bbe3b6c2022-03-26T21:07:13ZThe 2dF-SDSS LRG and QSO Survey: The z&lt;2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:7df806a3-bda8-4038-9971-cd7b3bbe3b6cEnglishSymplectic Elements at Oxford2005Richards, GCroom, SAnderson, SBland-Hawthorn, JBoyle, BPropris, RDrinkwater, MFan, XGunn, JIvezic, ZJester, SLoveday, JMeiksin, AMiller, LMyers, ANichol, ROutram, PPimbblet, KRoseboom, IRoss, NSchneider, DShanks, TSharp, RStoughton, CStrauss, MWe have used the 2dF instrument on the AAT to obtain redshifts of a sample of z&lt;3, 18.0<g<21.85 (2000).="" (2004),="" (2qz)="" (2slaq).="" 105.7="" 2df="" 2df-sdss="" 2qz="" 2slaq="" 32%="" 5645="" a="" adopted="" agree="" al.="" algorithm="" all="" allow="" analysis,="" and="" are="" at="" beta="-1.45+/-0.03" boyle="" bright="" but="" consistent="" counts="" croom="" data="" deg^2.="" describe="" determinations="" end="" et="" faint="" final="" find="" fit="" for="" form="" from="" function="" functional="" g="" g\sim20.2.="" however,="" if="" imaging.="" in="" inconsistent="" is="" joint="" larger="" likelihood="" lrg="" luminosity="" maximum="" more="" normalization="" not="" number="" of="" only="" other="" our="" parameterization,="" parameters="" part="" preliminary="" present="" programme:="" qso="" quasar="" quasars="" redshift="" resulting="" results="" sdss="" selected="" selection="" slope="" steeper="" survey="" than="" the="" these="" to="" using="" vary="" vary.="" we="" well="" with="" yields="">21 deep surveys. The 2SLAQ data exhibit no well defined ``break'' but do clearly flatten with increasing magnitude. The shape of the quasar luminosity function derived from 2SLAQ is in good agreement with that derived from type I quasars found in hard X-ray surveys. [Abridged]</g<21.85>
spellingShingle Richards, G
Croom, S
Anderson, S
Bland-Hawthorn, J
Boyle, B
Propris, R
Drinkwater, M
Fan, X
Gunn, J
Ivezic, Z
Jester, S
Loveday, J
Meiksin, A
Miller, L
Myers, A
Nichol, R
Outram, P
Pimbblet, K
Roseboom, I
Ross, N
Schneider, D
Shanks, T
Sharp, R
Stoughton, C
Strauss, M
The 2dF-SDSS LRG and QSO Survey: The z&lt;2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85
title The 2dF-SDSS LRG and QSO Survey: The z&lt;2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85
title_full The 2dF-SDSS LRG and QSO Survey: The z&lt;2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85
title_fullStr The 2dF-SDSS LRG and QSO Survey: The z&lt;2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85
title_full_unstemmed The 2dF-SDSS LRG and QSO Survey: The z&lt;2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85
title_short The 2dF-SDSS LRG and QSO Survey: The z&lt;2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85
title_sort 2df sdss lrg and qso survey the z lt 2 1 quasar luminosity function from 5645 quasars to g 21 85
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