2014A&A...568L...2S


Query : 2014A&A...568L...2S

2014A&A...568L...2S - Astronomy and Astrophysics, volume 568L2-2 (2014/8-1)

Can one determine cosmological parameters from multi-plane strong lens systems ?

SCHNEIDER P.

Abstract (from CDS):

Strong gravitational lensing of sources with different redshifts has been used to determine cosmological distance ratios, which in turn depend on the expansion history. Hence, such systems are viewed as potential tools for constraining cosmological parameters. Here we show that in lens systems with two distinct source redshifts, of which the nearest one contributes to the light deflection toward the more distant one, there exists an invariance transformation that leaves all strong-lensing observables unchanged (except for the product of time delay and Hubble constant), generalizing the well-known mass-sheet transformation in single-plane lens systems. The transformation preserves the relative location of mass and light. All time delays (from sources on both planes) scale with the same factor - time-delay ratios are therefore invariant under the mass-sheet transformation. Changing cosmological parameters, and thus distance ratios, is essentially equivalent to such a mass-sheet transformation. As an example, we discuss the double-source plane system SDSSJ0946+1006, which has recently been studied by Collett and Auger, and show that variations of cosmological parameters within reasonable ranges lead to only a weak mass-sheet transformation in both lens planes. Hence, the ability to extract cosmological information from such systems depends heavily on the ability to break the mass-sheet degeneracy.

Abstract Copyright: ∼

Journal keyword(s): gravitational lensing: strong - cosmological parameters

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 NVSS J094656+100649 rG 09 46 56.6809160266 +10 06 52.903093208     17.78   17.09 ~ 41 0

Query : 2014A&A...568L...2S

Basic data :
NVSS J094656+100649 -- Radio Galaxy
Other object types:
otypes_help
rG (), G (2008ApJS,SLACS), gLe (2008ApJ,[GTK2008]), Rad (NVSS,FIRST), * (Gaia), NIR (2MASS), MIR (WISE), Opt (SDSS)
ICRS coord. (ep=J2000) :
09 46 56.6809160266 +10 06 52.903093208 (Optical) [ 23.6792 17.0010 90 ] C 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
09 44 16.2650012576 +10 20 47.637402199 [ 23.6792 17.0010 90 ]
Gal coord. (ep=J2000) :
225.2404804064599 +43.4207698358608 [ 23.6792 17.0010 90 ]
Radial velocity / Redshift / cz :
V(km/s) 59296 [18] / z(spectroscopic) 0.22193 [0.00006] / cz 66532.9 [18.0]
   (Opt) C 2020ApJS..249....3A
Morphological type:
E D 2009ApJ...705.1099A
Fluxes (11) :
V 17.78 [~] D 2009ApJ...705.1099A
G 21.700422 [0.041170] C 2022yCat.1355....0G
I 17.09 [~] D 2008ApJ...682..964B
J 16.176 [0.129] C 2003yCat.2246....0C
H 15.657 [0.166] D 2003yCat.2246....0C
K 15.072 [0.193] D 2003yCat.2246....0C
u (AB) 20.946 [0.185] D 2020ApJS..249....3A
g (AB) 19.064 [0.016] C 2020ApJS..249....3A
r (AB) 17.700 [0.008] B 2020ApJS..249....3A
i (AB) 17.170 [0.007] B 2020ApJS..249....3A
z (AB) 16.862 [0.020] C 2020ApJS..249....3A
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Hierarchy : number of linked objects
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: 1 : 1 Display criteria :

Identifiers (8) :
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NVSS J094656+100649 2MASS J09465667+1006527 SLACS SDSS J0946+1006 lens [GTK2008] Lens 1
FIRST J094656.6+100652 SDSS J094656.68+100652.8 WISE J094656.69+100652.7 Gaia DR3 612534732378414464

References (41 between 1850 and 2026) (Total 41)
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 : 1   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : NVSS J094656+100649

Link by name to the catalogue in VizieR :

NVSS J094656+100649 FIRST J094656.6+100652 2MASS J09465667+1006527 SDSS J094656.68+100652.8 WISE J094656.69+100652.7
Gaia DR3 612534732378414464

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