The clustering of intermediate-redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey

Martin White, Adam D. Myers, Nicholas P. Ross, David J. Schlegel, Joseph F. Hennawi, Yue Shen, Ian McGreer, Michael A. Strauss, Adam S. Bolton, Jo Bovy, X. Fan, Jordi Miralda-Escude, N. Palanque-Delabrouille, I. Paris, P. Petitjean, D. P. Schneider, M. Viel, David H. Weinberg, Ch Yeche, I. ZehaviK. Pan, S. Snedden, D. Bizyaev, H. Brewington, J. Brinkmann, V. Malanushenko, E. Malanushenko, D. Oravetz, A. Simmons, A. Sheldon, Benjamin A. Weaver

Research output: Contribution to journalArticle

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Abstract

We measure the quasar two-point correlation function over the redshift range 2.2 < z < 2.8 using data from the Baryon Oscillation Spectroscopic Survey. We use a homogeneous subset of the data consisting of 27129 quasars with spectroscopic redshifts - by far the largest such sample used for clustering measurements at these redshifts to date. The sample covers 3600deg 2, corresponding to a comoving volume of 9.7(h -1Gpc) 3 assuming a fiducial Λ cold dark matter cosmology, and it has a median absolute i-band magnitude of -26, k-corrected to z= 2. After accounting for redshift errors we find that the redshift-space correlation function is fitted well by a power law of slope -2 and amplitude s 0= (9.7 ± 0.5)h -1Mpc over the range 3 < s < 25h -1Mpc. The projected correlation function, which integrates out the effects of peculiar velocities and redshift errors, is fitted well by a power law of slope -1 and r 0= (8.4 ± 0.6)h -1Mpc over the range 4 < R < 16h -1Mpc. There is no evidence for strong luminosity or redshift dependence to the clustering amplitude, in part because of the limited dynamic range in our sample. Our results are consistent with, but more precise than, previous measurements at similar redshifts. Our measurement of the quasar clustering amplitude implies a bias factor of b≃ 3.5 for our quasar sample. We compare the data to models to constrain the manner in which quasars occupy dark matter haloes at z∼ 2.4 and infer that such quasars inhabit haloes with a characteristic mass of 〈M〉≃ 10 12h -1M with a duty cycle for the quasar activity of 1 per cent.

Original languageEnglish (US)
Pages (from-to)933-950
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume424
Issue number2
DOIs
StatePublished - Aug 1 2012

Fingerprint

quasars
baryons
oscillation
oscillations
power law
cosmology
halos
dark matter
slopes
set theory
dynamic range
luminosity
cycles
cold
effect

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

White, Martin ; Myers, Adam D. ; Ross, Nicholas P. ; Schlegel, David J. ; Hennawi, Joseph F. ; Shen, Yue ; McGreer, Ian ; Strauss, Michael A. ; Bolton, Adam S. ; Bovy, Jo ; Fan, X. ; Miralda-Escude, Jordi ; Palanque-Delabrouille, N. ; Paris, I. ; Petitjean, P. ; Schneider, D. P. ; Viel, M. ; Weinberg, David H. ; Yeche, Ch ; Zehavi, I. ; Pan, K. ; Snedden, S. ; Bizyaev, D. ; Brewington, H. ; Brinkmann, J. ; Malanushenko, V. ; Malanushenko, E. ; Oravetz, D. ; Simmons, A. ; Sheldon, A. ; Weaver, Benjamin A. / The clustering of intermediate-redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey. In: Monthly Notices of the Royal Astronomical Society. 2012 ; Vol. 424, No. 2. pp. 933-950.
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abstract = "We measure the quasar two-point correlation function over the redshift range 2.2 < z < 2.8 using data from the Baryon Oscillation Spectroscopic Survey. We use a homogeneous subset of the data consisting of 27129 quasars with spectroscopic redshifts - by far the largest such sample used for clustering measurements at these redshifts to date. The sample covers 3600deg 2, corresponding to a comoving volume of 9.7(h -1Gpc) 3 assuming a fiducial Λ cold dark matter cosmology, and it has a median absolute i-band magnitude of -26, k-corrected to z= 2. After accounting for redshift errors we find that the redshift-space correlation function is fitted well by a power law of slope -2 and amplitude s 0= (9.7 ± 0.5)h -1Mpc over the range 3 < s < 25h -1Mpc. The projected correlation function, which integrates out the effects of peculiar velocities and redshift errors, is fitted well by a power law of slope -1 and r 0= (8.4 ± 0.6)h -1Mpc over the range 4 < R < 16h -1Mpc. There is no evidence for strong luminosity or redshift dependence to the clustering amplitude, in part because of the limited dynamic range in our sample. Our results are consistent with, but more precise than, previous measurements at similar redshifts. Our measurement of the quasar clustering amplitude implies a bias factor of b≃ 3.5 for our quasar sample. We compare the data to models to constrain the manner in which quasars occupy dark matter haloes at z∼ 2.4 and infer that such quasars inhabit haloes with a characteristic mass of 〈M〉≃ 10 12h -1M ⊙ with a duty cycle for the quasar activity of 1 per cent.",
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White, M, Myers, AD, Ross, NP, Schlegel, DJ, Hennawi, JF, Shen, Y, McGreer, I, Strauss, MA, Bolton, AS, Bovy, J, Fan, X, Miralda-Escude, J, Palanque-Delabrouille, N, Paris, I, Petitjean, P, Schneider, DP, Viel, M, Weinberg, DH, Yeche, C, Zehavi, I, Pan, K, Snedden, S, Bizyaev, D, Brewington, H, Brinkmann, J, Malanushenko, V, Malanushenko, E, Oravetz, D, Simmons, A, Sheldon, A & Weaver, BA 2012, 'The clustering of intermediate-redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey', Monthly Notices of the Royal Astronomical Society, vol. 424, no. 2, pp. 933-950. https://doi.org/10.1111/j.1365-2966.2012.21251.x

The clustering of intermediate-redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey. / White, Martin; Myers, Adam D.; Ross, Nicholas P.; Schlegel, David J.; Hennawi, Joseph F.; Shen, Yue; McGreer, Ian; Strauss, Michael A.; Bolton, Adam S.; Bovy, Jo; Fan, X.; Miralda-Escude, Jordi; Palanque-Delabrouille, N.; Paris, I.; Petitjean, P.; Schneider, D. P.; Viel, M.; Weinberg, David H.; Yeche, Ch; Zehavi, I.; Pan, K.; Snedden, S.; Bizyaev, D.; Brewington, H.; Brinkmann, J.; Malanushenko, V.; Malanushenko, E.; Oravetz, D.; Simmons, A.; Sheldon, A.; Weaver, Benjamin A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 424, No. 2, 01.08.2012, p. 933-950.

Research output: Contribution to journalArticle

TY - JOUR

T1 - The clustering of intermediate-redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey

AU - White, Martin

AU - Myers, Adam D.

AU - Ross, Nicholas P.

AU - Schlegel, David J.

AU - Hennawi, Joseph F.

AU - Shen, Yue

AU - McGreer, Ian

AU - Strauss, Michael A.

AU - Bolton, Adam S.

AU - Bovy, Jo

AU - Fan, X.

AU - Miralda-Escude, Jordi

AU - Palanque-Delabrouille, N.

AU - Paris, I.

AU - Petitjean, P.

AU - Schneider, D. P.

AU - Viel, M.

AU - Weinberg, David H.

AU - Yeche, Ch

AU - Zehavi, I.

AU - Pan, K.

AU - Snedden, S.

AU - Bizyaev, D.

AU - Brewington, H.

AU - Brinkmann, J.

AU - Malanushenko, V.

AU - Malanushenko, E.

AU - Oravetz, D.

AU - Simmons, A.

AU - Sheldon, A.

AU - Weaver, Benjamin A.

PY - 2012/8/1

Y1 - 2012/8/1

N2 - We measure the quasar two-point correlation function over the redshift range 2.2 < z < 2.8 using data from the Baryon Oscillation Spectroscopic Survey. We use a homogeneous subset of the data consisting of 27129 quasars with spectroscopic redshifts - by far the largest such sample used for clustering measurements at these redshifts to date. The sample covers 3600deg 2, corresponding to a comoving volume of 9.7(h -1Gpc) 3 assuming a fiducial Λ cold dark matter cosmology, and it has a median absolute i-band magnitude of -26, k-corrected to z= 2. After accounting for redshift errors we find that the redshift-space correlation function is fitted well by a power law of slope -2 and amplitude s 0= (9.7 ± 0.5)h -1Mpc over the range 3 < s < 25h -1Mpc. The projected correlation function, which integrates out the effects of peculiar velocities and redshift errors, is fitted well by a power law of slope -1 and r 0= (8.4 ± 0.6)h -1Mpc over the range 4 < R < 16h -1Mpc. There is no evidence for strong luminosity or redshift dependence to the clustering amplitude, in part because of the limited dynamic range in our sample. Our results are consistent with, but more precise than, previous measurements at similar redshifts. Our measurement of the quasar clustering amplitude implies a bias factor of b≃ 3.5 for our quasar sample. We compare the data to models to constrain the manner in which quasars occupy dark matter haloes at z∼ 2.4 and infer that such quasars inhabit haloes with a characteristic mass of 〈M〉≃ 10 12h -1M ⊙ with a duty cycle for the quasar activity of 1 per cent.

AB - We measure the quasar two-point correlation function over the redshift range 2.2 < z < 2.8 using data from the Baryon Oscillation Spectroscopic Survey. We use a homogeneous subset of the data consisting of 27129 quasars with spectroscopic redshifts - by far the largest such sample used for clustering measurements at these redshifts to date. The sample covers 3600deg 2, corresponding to a comoving volume of 9.7(h -1Gpc) 3 assuming a fiducial Λ cold dark matter cosmology, and it has a median absolute i-band magnitude of -26, k-corrected to z= 2. After accounting for redshift errors we find that the redshift-space correlation function is fitted well by a power law of slope -2 and amplitude s 0= (9.7 ± 0.5)h -1Mpc over the range 3 < s < 25h -1Mpc. The projected correlation function, which integrates out the effects of peculiar velocities and redshift errors, is fitted well by a power law of slope -1 and r 0= (8.4 ± 0.6)h -1Mpc over the range 4 < R < 16h -1Mpc. There is no evidence for strong luminosity or redshift dependence to the clustering amplitude, in part because of the limited dynamic range in our sample. Our results are consistent with, but more precise than, previous measurements at similar redshifts. Our measurement of the quasar clustering amplitude implies a bias factor of b≃ 3.5 for our quasar sample. We compare the data to models to constrain the manner in which quasars occupy dark matter haloes at z∼ 2.4 and infer that such quasars inhabit haloes with a characteristic mass of 〈M〉≃ 10 12h -1M ⊙ with a duty cycle for the quasar activity of 1 per cent.

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