2006ApJ...640...47K


Query : 2006ApJ...640...47K

2006ApJ...640...47K - Astrophys. J., 640, 47-61 (2006/March-3)

The time delays of gravitational lens HE 0435-1223: an early-type galaxy with a rising rotation curve.

KOCHANEK C.S., MORGAN N.D., FALCO E.E., McLEOD B.A., WINN J.N., DEMBICKY J. and KETZEBACK B.

Abstract (from CDS):

We present Hubble Space Telescope images and 2 years of optical photometry of the quadruple quasar HE 0435-1223. The time delays between the intrinsic quasar variations are ΔtAD=-14.37+0.75–0.85, ΔtAB=-8.00+0.73–0.82, and ΔtAC=-2.10+0.78–0.71days. We also observed nonintrinsic variations of ∼0.1 mag/yr that we attribute to microlensing. Instead of the traditional approach of assuming a rotation curve for the lens galaxy and then deriving the Hubble constant (H0), we assume H0=(72±7) km/s/Mpc and derive constraints on the rotation curve. On the scale over which the lensed images occur (1".2=5 h–1 kpc≃1.5Re), the lens galaxy must have a rising rotation curve, and it cannot have a constant mass-to-light ratio. These results add to the evidence that the structures of early-type galaxies are heterogeneous.

Abstract Copyright: ∼

Journal keyword(s): Cosmology: Cosmological Parameters - Cosmology: Dark Matter - Galaxies: Kinematics and Dynamics - Cosmology: Gravitational Lensing - quasars: individual (HE 0435-1223)

Nomenclature: Table 3: [KMF2006] SN (Nos S1-S5). Fig.6: [MKP2005] GNN (No. G25) added.

CDS comments: In introd. : Q0957+564 is a misprint for QSO 0957+561. Table 2: Objects are [WSB2002] 0435-1223 A (Nos A-D, G) and object H = QSO HE 0435-1223.

Simbad objects: 26

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Number of rows : 26
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 [MKP2005] G13 G 04 38 12.89 -12 17 02.9     22.486   21.980 ~ 6 0
2 [MKP2005] G19 G 04 38 13.06 -12 16 56.5     21.517   21.230 ~ 4 0
3 [MKP2005] G18 G 04 38 13.56 -12 16 44.7     22.147   21.829 ~ 5 0
4 [MKP2005] G25 G 04 38 13.723 -12 17 32.06     22.134   21.910 ~ 4 0
5 [MKP2005] G12 G 04 38 14.34 -12 17 10.6     21.182   21.158 ~ 10 0
6 [MKP2005] G21 G 04 38 14.43 -12 17 07.7     22.564   21.819 ~ 8 0
7 [MKP2005] G20 G 04 38 14.518 -12 17 00.49     23.946   22.776 ~ 4 0
8 [MKP2005] G23 G 04 38 14.594 -12 17 23.53     24.409   22.850 ~ 6 0
9 [MKP2005] G22 G 04 38 14.724 -12 17 18.20     22.253   21.260 ~ 16 1
10 [WSB2002] 0435-1223 C LeQ 04 38 14.73 -12 17 15.0     19.149   19.631 ~ 39 0
11 [WSB2002] 0435-1223 B LeQ 04 38 14.80 -12 17 13.8     19.082   19.623 ~ 43 0
12 [WSB2002] 0435-1223 D LeQ 04 38 14.84 -12 17 16.0     19.196   19.824 ~ 42 0
13 [WSB2002] 0435-1223 G G 04 38 14.88 -12 17 14.6     20.80   19.83 ~ 25 0
14 [VV2006] J043814.8-122314 QSO 04 38 14.88 -12 17 14.6     17.15     ~ 245 2
15 [WSB2002] 0435-1223 A LeQ 04 38 14.90 -12 17 14.4     18.545   19.106 ~ 41 0
16 [MKP2005] G24 G 04 38 15.046 -12 17 22.56     23.946   22.501 ~ 7 0
17 8C 0958+561 QSO 10 01 20.6918953728 +55 53 55.593949272   17.16 16.95     ~ 757 3
18 QSO B1104-181 QSO 11 06 33.3845199936 -18 21 23.829049296   15.8 15.9 15.7   ~ 338 1
19 [WZA2016] pg1115 6 169.57063+07.76630 G 11 18 16.95 +07 45 58.7           ~ 47 1
20 QSO B1115+080A QSO 11 18 16.951 +07 45 58.23   16.61 16.44     ~ 703 2
21 QSO B1520+530 QSO 15 21 44.8 +52 54 49   18.2       ~ 123 2
22 QSO B1600+4344 QSO 16 01 40.4818 +43 16 47.394   22.12 21.92     ~ 188 1
23 QSO B2149-2745 QSO 21 52 07.4534 -27 31 49.718   18.70 18.39     ~ 108 2
24 QSO J2240+0321 QSO 22 40 30.234 +03 21 30.63           ~ 705 1
25 Z 378-15 AGN 22 40 30.23447 +03 21 30.6290           ~ 636 0

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