2018MNRAS.479.4153Y


Query : 2018MNRAS.479.4153Y

2018MNRAS.479.4153Y - Mon. Not. R. Astron. Soc., 479, 4153-4171 (2018/September-3)

Using the Properties of Broad Absorption Line Quasars to Illuminate Quasar Structure.

YONG S.Y., KING A.L., WEBSTER R.L., BATE N.F., O'DOWD M.J. and LABRIE K.

Abstract (from CDS):

A key to understanding quasar unification paradigms is the emission properties of broad absorption line quasars (BALQs). The fact that only a small fraction of quasar spectra exhibit deep absorption troughs blueward of the broad permitted emission lines provides a crucial clue to the structure of quasar emitting regions. To learn whether it is possible to discriminate between the BALQ and non-BALQ populations given the observed spectral properties of a quasar, we employ two approaches: one based on statistical methods and the other supervised machine learning classification, applied to quasar samples from the Sloan Digital Sky Survey. The features explored include continuum and emission line properties, in particular the absolute magnitude, redshift, spectral index, line width, asymmetry, strength, and relative velocity offsets of high-ionization C IV λ1549 and low-ionization Mg II λ2798 lines.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: data analysis - methods: statistical - galaxies: active - quasars: absorption lines - quasars: emission lines

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 LEDA 87392 Sy1 00 39 15.8339634552 -51 17 01.481641692   15.77 15.28 15.66   ~ 134 0

Query : 2018MNRAS.479.4153Y

Basic data :
LEDA 87392 -- Seyfert 1 Galaxy
Other object types:
otypes_help
AGN ([VV2000c],[VV2003c],...), G (2016A&A,LEDA,...), X (RBS,RX,...), MIR (WISEA,WISE), Sy1 (2010A&A), EmG (WPVS), * (Gaia), NIR (2MASS)
ICRS coord. (ep=J2000) :
00 39 15.8339634552 -51 17 01.481641692 (Optical) [ 0.0219 0.0248 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
00 36 55.9319351705 -51 33 30.199975759 [ 0.0219 0.0248 90 ]
Gal coord. (ep=J2000) :
307.5668793683320 -65.7348085261623 [ 0.0219 0.0248 90 ]
Proper motions mas/yr :
0.093 -0.124 [0.027 0.032 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 8454 [45] / z(~) 0.02861 [0.00015] / cz 8577.0 [45.0]
   (Opt) C 2009MNRAS.399..683J
Angular size (arcmin):
0.200 0.156 75 (NIR) C 2006AJ....131.1163S
Fluxes (7) :
B 15.77 [~] D 2010A&A...518A..10V
V 15.28 [~] D 2010A&A...518A..10V
R 15.66 [~] D 2009MNRAS.399..683J
G 15.652827 [0.005789] C 2020yCat.1350....0G
J 13.344 [0.064] C 2006AJ....131.1163S
H 12.744 [0.090] C 2006AJ....131.1163S
K 11.934 [0.065] C 2006AJ....131.1163S
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Identifiers (21) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

LEDA 87392 RX J0039.2-5117 WPVS 7 [VV98c] J003916.0-511659
6dFGS gJ003915.9-511702 1RXS J003916.6-511701 3XMM J003915.8-511701 Gaia DR2 4926008222120153088
HE 0036-5133 1RXS J003915.6-511701 [VV2000c] J003916.0-511659 Gaia DR3 4926008222120153088
2MASS J00391583-5117014 TIC 156070422 [VV2003c] J003916.0-511659
2MASX J00391586-5117013 WISEA J003915.83-511701.4 [VV2006c] J003916.0-511659
RBS 88 WISE J003915.82-511701.4 [VV2010c] J003916.0-511659

References (134 between 1850 and 2026) (Total 134)
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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Collections of Measurements Description of Measurements

Velocities : 4    PM : 2   

   

Observing logs
IUE : 2   

   


External archives :

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

Data at NED - NASA/IPAC Extragalactic Database : LEDA 87392

Link by name to the catalogue in VizieR :

2MASS J00391583-5117014 2MASX J00391586-5117013 1RXS J003916.6-511701 1RXS J003915.6-511701 WISEA J003915.83-511701.4
WISE J003915.82-511701.4 Gaia DR2 4926008222120153088 Gaia DR3 4926008222120153088

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