2005ApJ...619..733M

Query : 2005ApJ...619..733M

2005ApJ...619..733M - Astrophys. J., 619, 733-740 (2005/February-1)

Probing galaxy density profiles with future supernova surveys.

MORTSELL E., DAHLE H. and HANNESTAD S.

Abstract (from CDS):

In this paper we discuss the possibility of measuring the Hubble parameter and the slope of galaxy density profiles using future supernova data. With future supernova surveys such as the Supernova/Acceleration Probe (SNAP), large numbers of core-collapse supernovae will be discovered, a small fraction of which will be multiply imaged. Measurements of the image separation, flux ratio, time delay, and properties of the lens galaxy for these systems will provide tight constraints on the slope of galactic halos as well as providing complementary and independent information to other cosmological tests with respect to the Hubble parameter.

Abstract Copyright: ∼

Journal keyword(s): Cosmology: Dark Matter - Cosmology: Distance Scale - Galaxies: Halos - Cosmology: Gravitational Lensing - Stars: Supernovae: General

CDS comments: In the introduction QSO 0957+651 is a misprint for QSO 0957+561

Simbad objects: 5

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Number of rows : 5
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 6C 021803+354230 BLL 02 21 05.4920852208 +35 56 13.848581904   20.0 20.0 19.60   ~ 603 3
2 8C 0958+561 QSO 10 01 20.6918953728 +55 53 55.593949272   17.16 16.95     ~ 757 3
3 YGKOW G1 G 10 01 20.86 +55 53 50.7           ~ 51 1
4 QSO J2240+0321 QSO 22 40 30.234 +03 21 30.63           ~ 705 1
5 Z 378-15 AGN 22 40 30.23447 +03 21 30.6290           ~ 636 0

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