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

J. K. Hoormann; P. Martini; T. M. Davis; A. King; C. Lidman; D. Mudd; R. Sharp; N. E. Sommer; B. E. Tucker; Z. Yu; S. Allam; J. Asorey; S. Avila; M. Banerji; D. Brooks; E. Buckley-Geer; D. L. Burke; J. Calcino; A. Carnero Rosell; D. Carollo; M. Carrasco Kind; J. Carretero; F. J. Castander; M. Childress; J. De Vicente; S. Desai; H. T. Diehl; P. Doel; B. Flaugher; P. Fosalba; J. Frieman; J. García-Bellido; D. W. Gerdes; D. Gruen; G. Gutierrez; W. G. Hartley; S. R. Hinton; D. L. Hollowood; K. Honscheid; B. Hoyle; D. J. James; E. Krause; K. Kuehn; N. Kuropatkin; G. F. Lewis; M. Lima; E. Macaulay; M. A.G. Maia; F. Menanteau; C. J. Miller; R. Miquel; A. Möller; A. A. Plazas; A. K. Romer; A. Roodman; E. Sanchez; V. Scarpine; M. Schubnell; S. Serrano; I. Sevilla-Noarbe; M. Smith; R. C. Smith; M. Soares-Santos; F. Sobreira; E. Suchyta; E. Swann; M. E.C. Swanson; G. Tarle; S. A. Uddin

doi:10.1093/mnras/stz1539

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

J. K. Hoormann, P. Martini, T. M. Davis, A. King, C. Lidman, D. Mudd, R. Sharp, N. E. Sommer, B. E. Tucker, Z. Yu, S. Allam, J. Asorey, S. Avila, M. Banerji, D. Brooks, E. Buckley-Geer, D. L. Burke, J. Calcino, A. Carnero Rosell, D. CarolloM. Carrasco Kind, J. Carretero, F. J. Castander, M. Childress, J. De Vicente, S. Desai, H. T. Diehl, P. Doel, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, D. W. Gerdes, D. Gruen, G. Gutierrez, W. G. Hartley, S. R. Hinton, D. L. Hollowood, K. Honscheid, B. Hoyle, D. J. James, E. Krause, K. Kuehn, N. Kuropatkin, G. F. Lewis, M. Lima, E. Macaulay, M. A.G. Maia, F. Menanteau, C. J. Miller, R. Miquel, A. Möller, A. A. Plazas, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, M. Smith, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, E. Swann, M. E.C. Swanson, G. Tarle, S. A. Uddin

Department of Morphological Sciences

Research output: Contribution to journal › Article › Research

9 Citations (Scopus)

Abstract

© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. 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 $358{+126}-{-123}$ and $343{+58}-{-84}$ 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 × 10 and 3.3 × 10 M , 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.

Original language	English
Pages (from-to)	3650-3663
Journal	Monthly Notices of the Royal Astronomical Society
Volume	487
DOIs	https://doi.org/10.1093/mnras/stz1539
Publication status	Published - 1 Jan 2019

Keywords

accretion
accretion discs
black hole physics
galaxies: evolution
quasars: emission lines

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Hoormann, J. K., Martini, P., Davis, T. M., King, A., Lidman, C., Mudd, D., Sharp, R., Sommer, N. E., Tucker, B. E., Yu, Z., Allam, S., Asorey, J., Avila, S., Banerji, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Calcino, J., Carnero Rosell, A., ... Uddin, S. A. (2019). C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES). Monthly Notices of the Royal Astronomical Society, 487, 3650-3663. https://doi.org/10.1093/mnras/stz1539

Hoormann, J. K. ; Martini, P. ; Davis, T. M. ; King, A. ; Lidman, C. ; Mudd, D. ; Sharp, R. ; Sommer, N. E. ; Tucker, B. E. ; Yu, Z. ; Allam, S. ; Asorey, J. ; Avila, S. ; Banerji, M. ; Brooks, D. ; Buckley-Geer, E. ; Burke, D. L. ; Calcino, J. ; Carnero Rosell, A. ; Carollo, D. ; Carrasco Kind, M. ; Carretero, J. ; Castander, F. J. ; Childress, M. ; De Vicente, J. ; Desai, S. ; Diehl, H. T. ; Doel, P. ; Flaugher, B. ; Fosalba, P. ; Frieman, J. ; García-Bellido, J. ; Gerdes, D. W. ; Gruen, D. ; Gutierrez, G. ; Hartley, W. G. ; Hinton, S. R. ; Hollowood, D. L. ; Honscheid, K. ; Hoyle, B. ; James, D. J. ; Krause, E. ; Kuehn, K. ; Kuropatkin, N. ; Lewis, G. F. ; Lima, M. ; Macaulay, E. ; Maia, M. A.G. ; Menanteau, F. ; Miller, C. J. ; Miquel, R. ; Möller, A. ; Plazas, A. A. ; Romer, A. K. ; Roodman, A. ; Sanchez, E. ; Scarpine, V. ; Schubnell, M. ; Serrano, S. ; Sevilla-Noarbe, I. ; Smith, M. ; Smith, R. C. ; Soares-Santos, M. ; Sobreira, F. ; Suchyta, E. ; Swann, E. ; Swanson, M. E.C. ; Tarle, G. ; Uddin, S. A. / C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES). In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 487. pp. 3650-3663.

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title = "C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES)",

abstract = "{\textcopyright} 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. 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 $358{+126}-{-123}$ and $343{+58}-{-84}$ 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 × 10 and 3.3 × 10 M , 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.",

keywords = "accretion, accretion discs, black hole physics, galaxies: evolution, quasars: emission lines",

author = "Hoormann, {J. K.} and P. Martini and Davis, {T. M.} and A. King and C. Lidman and D. Mudd and R. Sharp and Sommer, {N. E.} and Tucker, {B. E.} and Z. Yu and S. Allam and J. Asorey and S. Avila and M. Banerji and D. Brooks and E. Buckley-Geer and Burke, {D. L.} and J. Calcino and {Carnero Rosell}, A. and D. Carollo and {Carrasco Kind}, M. and J. Carretero and Castander, {F. J.} and M. Childress and {De Vicente}, J. and S. Desai and Diehl, {H. T.} and P. Doel and B. Flaugher and P. Fosalba and J. Frieman and J. Garc{\'i}a-Bellido and Gerdes, {D. W.} and D. Gruen and G. Gutierrez and Hartley, {W. G.} and Hinton, {S. R.} and Hollowood, {D. L.} and K. Honscheid and B. Hoyle and James, {D. J.} and E. Krause and K. Kuehn and N. Kuropatkin and Lewis, {G. F.} and M. Lima and E. Macaulay and Maia, {M. A.G.} and F. Menanteau and Miller, {C. J.} and R. Miquel and A. M{\"o}ller and Plazas, {A. A.} and Romer, {A. K.} and A. Roodman and E. Sanchez and V. Scarpine and M. Schubnell and S. Serrano and I. Sevilla-Noarbe and M. Smith and Smith, {R. C.} and M. Soares-Santos and F. Sobreira and E. Suchyta and E. Swann and Swanson, {M. E.C.} and G. Tarle and Uddin, {S. A.}",

year = "2019",

month = jan,

day = "1",

doi = "10.1093/mnras/stz1539",

language = "English",

volume = "487",

pages = "3650--3663",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

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Hoormann, JK, Martini, P, Davis, TM, King, A, Lidman, C, Mudd, D, Sharp, R, Sommer, NE, Tucker, BE, Yu, Z, Allam, S, Asorey, J, Avila, S, Banerji, M, Brooks, D, Buckley-Geer, E, Burke, DL, Calcino, J, Carnero Rosell, A, Carollo, D, Carrasco Kind, M, Carretero, J, Castander, FJ, Childress, M, De Vicente, J, Desai, S, Diehl, HT, Doel, P, Flaugher, B, Fosalba, P, Frieman, J, García-Bellido, J, Gerdes, DW, Gruen, D, Gutierrez, G, Hartley, WG, Hinton, SR, Hollowood, DL, Honscheid, K, Hoyle, B, James, DJ, Krause, E, Kuehn, K, Kuropatkin, N, Lewis, GF, Lima, M, Macaulay, E, Maia, MAG, Menanteau, F, Miller, CJ, Miquel, R, Möller, A, Plazas, AA, Romer, AK, Roodman, A, Sanchez, E, Scarpine, V, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Smith, M, Smith, RC, Soares-Santos, M, Sobreira, F, Suchyta, E, Swann, E, Swanson, MEC, Tarle, G & Uddin, SA 2019, 'C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES)', Monthly Notices of the Royal Astronomical Society, vol. 487, pp. 3650-3663. https://doi.org/10.1093/mnras/stz1539

C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES). / Hoormann, J. K.; Martini, P.; Davis, T. M.; King, A.; Lidman, C.; Mudd, D.; Sharp, R.; Sommer, N. E.; Tucker, B. E.; Yu, Z.; Allam, S.; Asorey, J.; Avila, S.; Banerji, M.; Brooks, D.; Buckley-Geer, E.; Burke, D. L.; Calcino, J.; Carnero Rosell, A.; Carollo, D.; Carrasco Kind, M.; Carretero, J.; Castander, F. J.; Childress, M.; De Vicente, J.; Desai, S.; Diehl, H. T.; Doel, P.; Flaugher, B.; Fosalba, P.; Frieman, J.; García-Bellido, J.; Gerdes, D. W.; Gruen, D.; Gutierrez, G.; Hartley, W. G.; Hinton, S. R.; Hollowood, D. L.; Honscheid, K.; Hoyle, B.; James, D. J.; Krause, E.; Kuehn, K.; Kuropatkin, N.; Lewis, G. F.; Lima, M.; Macaulay, E.; Maia, M. A.G.; Menanteau, F.; Miller, C. J.; Miquel, R.; Möller, A.; Plazas, A. A.; Romer, A. K.; Roodman, A.; Sanchez, E.; Scarpine, V.; Schubnell, M.; Serrano, S.; Sevilla-Noarbe, I.; Smith, M.; Smith, R. C.; Soares-Santos, M.; Sobreira, F.; Suchyta, E.; Swann, E.; Swanson, M. E.C.; Tarle, G.; Uddin, S. A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 487, 01.01.2019, p. 3650-3663.

Research output: Contribution to journal › Article › Research

TY - JOUR

T1 - C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES)

AU - Hoormann, J. K.

AU - Martini, P.

AU - Davis, T. M.

AU - King, A.

AU - Lidman, C.

AU - Mudd, D.

AU - Sharp, R.

AU - Sommer, N. E.

AU - Tucker, B. E.

AU - Yu, Z.

AU - Allam, S.

AU - Asorey, J.

AU - Avila, S.

AU - Banerji, M.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Calcino, J.

AU - Carnero Rosell, A.

AU - Carollo, D.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Castander, F. J.

AU - Childress, M.

AU - De Vicente, J.

AU - Desai, S.

AU - Diehl, H. T.

AU - Doel, P.

AU - Flaugher, B.

AU - Fosalba, P.

AU - Frieman, J.

AU - García-Bellido, J.

AU - Gerdes, D. W.

AU - Gruen, D.

AU - Gutierrez, G.

AU - Hartley, W. G.

AU - Hinton, S. R.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - Hoyle, B.

AU - James, D. J.

AU - Krause, E.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lewis, G. F.

AU - Lima, M.

AU - Macaulay, E.

AU - Maia, M. A.G.

AU - Menanteau, F.

AU - Miller, C. J.

AU - Miquel, R.

AU - Möller, A.

AU - Plazas, A. A.

AU - Romer, A. K.

AU - Roodman, A.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Serrano, S.

AU - Sevilla-Noarbe, I.

AU - Smith, M.

AU - Smith, R. C.

AU - Soares-Santos, M.

AU - Sobreira, F.

AU - Suchyta, E.

AU - Swann, E.

AU - Swanson, M. E.C.

AU - Tarle, G.

AU - Uddin, S. A.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. 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 $358{+126}-{-123}$ and $343{+58}-{-84}$ 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 × 10 and 3.3 × 10 M , 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.

AB - © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. 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 $358{+126}-{-123}$ and $343{+58}-{-84}$ 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 × 10 and 3.3 × 10 M , 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.

KW - accretion

KW - accretion discs

KW - black hole physics

KW - galaxies: evolution

KW - quasars: emission lines

U2 - 10.1093/mnras/stz1539

DO - 10.1093/mnras/stz1539

M3 - Article

VL - 487

SP - 3650

EP - 3663

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

ER -