2020ApJ...889L..12D


Query : 2020ApJ...889L..12D

2020ApJ...889L..12D - Astrophys. J., 889, L12-L12 (2020/January-3)

Deep Hubble Space Telescope imaging on the extended Lyα emission of a QSO at z=2.19 with a damped Lyman alpha system as a natural coronagraph.

DING J., CAI Z., PROCHASKA J.X., FINLEY H., FAN X., ZHENG Z., FATHIVAVSARI H. and PETITJEAN P.

Abstract (from CDS):

Recent observations suggest that proximate damped Lyα (PDLA) systems can be used to study the host galaxies of quasi-stellar objects (QSOs), because the PDLAs can block the bright point-spread function from central QSOs. Using six orbits of narrowband imaging with Hubble Space Telescope (HST)/WFC3, we present the first high-resolution narrowband image of the Lyα emission in the PDLA trough of the QSO SDSS J115432.67-021537.9. We detect one major component and one minor component in the narrowband imaging. Combining the HST/WFC3 imaging with deep Magellan/MagE spectra, we measure that the Lyα flux FLyα = 1.56±0.10×10–16ergs–1cm–2, which is among the luminous (≃2.7 LLyα^*^) Lyα emitters at z= 2.19. The Lyα-based star formation rate is ∼7 M☉yr–1. These observational results favor that the star formation from the host galaxy could be the main mechanism powering the Lyα emission. This new method sheds light on the study of the kinematic structure and the spatial distribution of the extended Lyα emitting regions around the QSO host.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Quasars - Quasar absorption line spectroscopy - HST photometry

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 SDSS J115432.67-021538.0 QSO 11 54 32.676 -02 15 37.99           ~ 10 0

Query : 2020ApJ...889L..12D

Basic data :
SDSS J115432.67-021538.0 -- Quasar
Other object types:
otypes_help
QSO (2013A&A), Opt (SDSS)
ICRS coord. (ep=J2000) :
11 54 32.676 -02 15 37.99 (Optical) [ 44 40 90 ] C 2012ApJS..203...21A
FK4 coord. (ep=B1950 eq=1950) :
11 51 58.995 -01 58 56.19 [ 44 40 90 ]
Gal coord. (ep=J2000) :
275.685721 +57.570156 [ 44 40 90 ]
Radial velocity / Redshift / cz :
V(km/s) 245836 [~] / z(spectroscopic) 2.180000 [~] / cz 653547.56 [~]
   (Opt) D 2018A&A...613A..51P
Fluxes (5) :
u (AB) 22.3235 [0.1913] D 2020ApJS..250....8L
g (AB) 21.5733 [0.0478] C 2020ApJS..250....8L
r (AB) 21.3859 [0.0631] C 2020ApJS..250....8L
i (AB) 21.0922 [0.0687] C 2020ApJS..250....8L
z (AB) 20.8176 [0.2300] D 2020ApJS..250....8L
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Identifiers (2) :
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SDSS J115432.67-021538.0 SDSS J115432.67-021537.9

References (10 between 1850 and 2026) (Total 10)
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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Velocities : 8   

   


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Data at NED - NASA/IPAC Extragalactic Database : SDSS J115432.67-021538.0

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SDSS J115432.67-021538.0 SDSS J115432.67-021537.9

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