2022ApJ...938...17E


Query : 2022ApJ...938...17E

2022ApJ...938...17E - Astrophys. J., 938, 17 (2022/October-2)

A Generative Model for Quasar Spectra.

EILERS A.-C., HOGG D.W., SCHOLKOPF B., FOREMAN-MACKEY D., DAVIES F.B. and SCHINDLER J.-T.

Abstract (from CDS):

We build a multi-output generative model for quasar spectra and the properties of their black hole engines, based on a Gaussian process latent-variable model. This model treats every quasar as a vector of latent properties such that the spectrum and all physical properties of the quasar are associated with non-linear functions of those latent parameters; the Gaussian process kernel functions define priors on the function space. Our generative model is trained with a justifiable likelihood function that allows us to treat heteroscedastic noise and missing data correctly, which is crucial for all astrophysical applications. It can simultaneously predict unobserved spectral regions and the physical properties of quasars in held-out test data. We apply the model to rest-frame ultraviolet and optical quasar spectra for which precise black hole masses (based on reverberation-mapping measurements) are available. Unlike reverberation-mapping studies that require multi-epoch data, our model predicts black hole masses from single-epoch spectra-even with limited spectral coverage. We demonstrate the capabilities of the model by predicting black hole masses and unobserved spectral regions. We find that we predict black hole masses at close to the best possible accuracy.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Gaussian Processes regression - Nonparametric inference - Quasars - Astrostatistics techniques - Spectroscopy - Supermassive black holes

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 2C 1590 BLL 18 45 37.622 +09 53 44.74           ~ 82 1

Query : 2022ApJ...938...17E

Basic data :
2C 1590 -- BL Lac
Other object types:
otypes_help
Rad (2C,BWE,...), BLL (2014ApJS), MIR (WISEA,WISE), QSO (QSO), X (SWIFT)
ICRS coord. (ep=J2000) :
18 45 37.622 +09 53 44.74 (Radio) [ 2000 2000 90 ] D 1996AJ....111.1945D
FK4 coord. (ep=B1950 eq=1950) :
18 43 15.246 +09 50 31.60 [ 2000 2000 90 ]
Gal coord. (ep=J2000) :
041.111932 +05.773202 [ 2000 2000 90 ]
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Identifiers (24) :
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2C 1590 DA 463 NVSS J184537+095344 VLSSr J184537.7+095344
BWE 1843+0950 GB6 B1843+0950 QSO B1843+098 WB 1843+0950
3C 390.0 87GB 184315.2+095026 SWIFT J184537.6+095349 WISEA J184537.60+095345.0
3C 390 MRC 1843+098 TGSSADR J184537.6+095344 WISE J184537.57+095346.0
4C 09.62 MSH 18+0-08 TXS 1843+098 [HC69] 8
3CR 390 NRAO 578 UT 1843+098 [JAP2011] J281.43+09.97

References (82 between 1850 and 2026) (Total 82)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : 2C 1590

Link by name to the catalogue in VizieR :

BWE 1843+0950 3C 390.0 3C 390 4C 09.62 3CR 390
NVSS J184537+095344 WISEA J184537.60+095345.0 WISE J184537.57+095346.0

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