C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES)

被引：42

作者：

Hoormann, J. K. ^{[1
]}

Martini, P. ^{[2
,3
]}

Davis, T. M. ^{[1
]}

King, A. ^{[4
]}

Lidman, C. ^{[5
]}

Mudd, D. ^{[6
]}

Sharp, R. ^{[5
]}

Sommer, N. E. ^{[5
]}

Tucker, B. E. ^{[5
]}

Yu, Z. ^{[3
]}

Allam, S. ^{[7
]}

Asorey, J. ^{[8
]}

Avila, S. ^{[9
]}

Banerji, M. ^{[10
,11
]}

Brooks, D. ^{[12
]}

Buckley-Geer, E. ^{[7
]}

Burke, D. L. ^{[13
,14
]}

Calcino, J. ^{[1
]}

Carnero Rosell, A. ^{[15
,16
]}

Carollo, D. ^{[17
]}

Kind, M. Carrasco ^{[18
,19
]}

Carretero, J. ^{[20
]}

Castander, F. J. ^{[21
,22
]}

Childress, M. ^{[23
]}

De Vicente, J. ^{[15
]}

Desai, S. ^{[24
]}

Diehl, H. T. ^{[7
]}

Doel, P. ^{[12
]}

Flaugher, B. ^{[7
]}

Fosalba, P. ^{[21
,22
]}

Frieman, J. ^{[7
,25
]}

Garcia-Bellido, J. ^{[26
]}

Gerdes, D. W. ^{[27
,28
]}

Gruen, D. ^{[13
,14
,29
]}

Gutierrez, G. ^{[7
]}

Hartley, W. G. ^{[12
,30
]}

Hinton, S. R. ^{[1
]}

Hollowood, D. L. ^{[31
]}

Honscheid, K. ^{[2
,32
]}

Hoyle, B. ^{[33
,34
]}

James, D. J. ^{[35
]}

Krause, E. ^{[36
]}

Kuehn, K. ^{[37
]}

Kuropatkin, N. ^{[7
]}

Lewis, G. F. ^{[38
]}

Lima, M. ^{[16
,39
]}

Macaulay, E. ^{[9
]}

Maia, M. A. G. ^{[16
,40
]}

Menanteau, F. ^{[18
,19
]}

Miller, C. J. ^{[27
,28
]}

机构：

[1] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072, Australia

[2] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA

[3] Ohio State Univ, Dept Astron, 174 W 18Th Ave, Columbus, OH 43210 USA

[4] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia

[5] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia

[6] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[7] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[8] Korea Astron & Space Sci Inst, Daejeon 305348, South Korea

[9] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[10] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[11] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

[12] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[13] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[14] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[15] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid, Spain

[16] Lab Interinst & Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[17] INAF, Astrophys Observ Turin, I-10025 Pino Torinese, Italy

[18] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA

[19] Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA

[20] Barcelona Inst Sci & Technol, IFAE, Campus UAB, E-08193 Bellaterra, Barcelona, Spain

[21] IEEC, E-08034 Barcelona, Spain

[22] CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain

[23] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England

[24] IIT Hyderabad, Dept Phys, Kandi 502285, Telangana, India

[25] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[26] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain

[27] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[28] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[29] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA

[30] Swiss Fed Inst Technol, Dept Phys, Wolfgang Pauli Str 16, CH-8093 Zurich, Switzerland

[31] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA

[32] Ohio State Univ, Dept Phys, 174 W 18th Ave, Columbus, OH 43210 USA

[33] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany

[34] Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte, Scheinerstr 1, D-81679 Munich, Germany

[35] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[36] Steward Observ, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA

[37] Macquarie Univ, Australian Astron Opt, N Ryde, NSW 2113, Australia

[38] Univ Sydney, Sydney Inst Astron, Sch Phys, A28, Sydney, NSW 2006, Australia

[39] Univ Sao Paulo, Inst Fis, Dept Fis Matemat, CP 66318, BR-05314970 Sao Paulo, SP, Brazil

[40] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[41] Inst Catalana Recerca & Estudis Avancats, E-08010 Barcelona, Spain

[42] Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA

[43] Univ Sussex, Dept Phys & Astron, Pevensey Bldg, Brighton BN1 9QH, E Sussex, England

[44] Natl Opt Astron Observ, Cerra Tololo Interamer Observ, Casilla 603, La Serena, Chile

[45] Brandeis Univ, Phys Dept, 415 South St, Waltham, MA 02453 USA

[46] Univ Estadual Campinas, Inst Fis Gleb Wataghin, BR-13083859 Campinas, SP, Brazil

[47] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA

[48] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2019年 / 487卷 / 03期

基金：

英国科学技术设施理事会; 美国国家科学基金会; 欧洲研究理事会; 澳大利亚研究理事会;

关键词：

accretion; accretion discs; black hole physics; galaxies: evolution; quasars: emission lines; ACTIVE GALACTIC NUCLEI; BROAD-LINE REGION; QUASARS; SIZE; LUMINOSITY; CONTINUUM; GALAXIES; STEPS;

D O I：

10.1093/mnras/stz1539

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Black hole mass measurements outside the local Universe are critically important to derive the growth of supermassive black holes over cosmic time, and to study the interplay between black hole growth and galaxy evolution. In this paper, we present two measurements of supermassive black hole masses from reverberation mapping (RM) of the broad C IV emission line. These measurements are based on multiyear photometry and spectroscopy from the Dark Energy Survey Supernova Program (DES-SN) and the Australian Dark Energy Survey (OzDES), which together constitute the OzDES RM Program. The observed reverberation lag between the DES continuum photometry and the OzDES emission line fluxes is measured to be 358(-123)(+126) and 343(-84)(+58) d for two quasars at redshifts of 1,905 and 2.593, respectively. The corresponding masses of the two supermassive black holes are 4.4 x 10(9) and 3.3 x 10(9) M-circle dot, which are among the highest redshift and highest mass black holes measured to date with RM studies. We use these new measurements to better determine the C IV radius luminosity relationship for high-luminosity quasars, which is fundamental to many quasar black hole mass estimates and demographic studies,

引用

页码：3650 / 3663

页数：14

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