Simulations of the OzDES AGN reverberation mapping project

As part of the Australian spectroscopic dark energy survey (OzDES) we are carrying out a large-scale reverberation mapping study of ≥500 quasars over five years in the 30 deg2 area of the Dark Energy Survey (DES) supernova fields. These quasars have redshifts ranging up to 4 and have apparent AB mag...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2015-10, Vol.453 (2), p.1701-1726
Hauptverfasser: King, Anthea L., Martini, Paul, Davis, Tamara M., Denney, K. D., Kochanek, C. S., Peterson, Bradley M., Skielboe, Andreas, Vestergaard, Marianne, Huff, Eric, Watson, Darach, Banerji, Manda, McMahon, Richard, Sharp, Rob, Lidman, C.
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container_issue 2
container_start_page 1701
container_title Monthly notices of the Royal Astronomical Society
container_volume 453
creator King, Anthea L.
Martini, Paul
Davis, Tamara M.
Denney, K. D.
Kochanek, C. S.
Peterson, Bradley M.
Skielboe, Andreas
Vestergaard, Marianne
Huff, Eric
Watson, Darach
Banerji, Manda
McMahon, Richard
Sharp, Rob
Lidman, C.
description As part of the Australian spectroscopic dark energy survey (OzDES) we are carrying out a large-scale reverberation mapping study of ≥500 quasars over five years in the 30 deg2 area of the Dark Energy Survey (DES) supernova fields. These quasars have redshifts ranging up to 4 and have apparent AB magnitudes between 16.8 mag < r 
doi_str_mv 10.1093/mnras/stv1718
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D. ; Kochanek, C. S. ; Peterson, Bradley M. ; Skielboe, Andreas ; Vestergaard, Marianne ; Huff, Eric ; Watson, Darach ; Banerji, Manda ; McMahon, Richard ; Sharp, Rob ; Lidman, C.</creator><creatorcontrib>King, Anthea L. ; Martini, Paul ; Davis, Tamara M. ; Denney, K. D. ; Kochanek, C. S. ; Peterson, Bradley M. ; Skielboe, Andreas ; Vestergaard, Marianne ; Huff, Eric ; Watson, Darach ; Banerji, Manda ; McMahon, Richard ; Sharp, Rob ; Lidman, C. ; Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><description>As part of the Australian spectroscopic dark energy survey (OzDES) we are carrying out a large-scale reverberation mapping study of ≥500 quasars over five years in the 30 deg2 area of the Dark Energy Survey (DES) supernova fields. These quasars have redshifts ranging up to 4 and have apparent AB magnitudes between 16.8 mag &lt; r &lt; 22.5 mag. The aim of the survey is to measure time lags between fluctuations in the quasar continuum and broad emission-line fluxes of individual objects in order to measure black hole masses for a broad range of active galactic nuclei (AGN) and constrain the radius–luminosity (R–L) relationship. Here we investigate the expected efficiency of the OzDES reverberation mapping campaign and its possible extensions. We expect to recover lags for ∼35–45 per cent of the quasars. AGN with shorter lags and greater variability are more likely to yield a lag measurement, and objects with lags ≲6 months or ∼1 yr are expected to be recovered the most accurately. The baseline OzDES reverberation mapping campaign is predicted to produce an unbiased measurement of the R–L relationship parameters for H β, Mg ii λ2798, and C iv λ1549. 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ispartof Monthly notices of the Royal Astronomical Society, 2015-10, Vol.453 (2), p.1701-1726
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subjects Active galactic nuclei
Astronomy
ASTRONOMY AND ASTROPHYSICS
Dark energy
Fluxes
Luminosity
Mapping
Quasars
quasars: general
quasars: supermassive black holes
Simulation
Sky surveys (astronomy)
Spectroscopic analysis
Spectroscopy
Spectrum analysis
title Simulations of the OzDES AGN reverberation mapping project
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