2017ApJ...839..124D


Query : 2017ApJ...839..124D

2017ApJ...839..124D - Astrophys. J., 839, 124-124 (2017/April-3)

X-ray temperatures, luminosities, and masses from XMM-Newton follow-up of the first shear-selected galaxy cluster sample.

DESHPANDE A.J., HUGHES J.P. and WITTMAN D.

Abstract (from CDS):

We continue the study of the first sample of shear-selected clusters from the initial 8.6 square degrees of the Deep Lens Survey (DLS); a sample with well-defined selection criteria corresponding to the highest ranked shear peaks in the survey area. We aim to characterize the weak lensing selection by examining the sample's X-ray properties. There are multiple X-ray clusters associated with nearly all the shear peaks: 14 X-ray clusters corresponding to seven DLS shear peaks. An additional three X-ray clusters cannot be definitively associated with shear peaks, mainly due to large positional offsets between the X-ray centroid and the shear peak. Here we report on the XMM-Newton properties of the 17 X-ray clusters. The X-ray clusters display a wide range of luminosities and temperatures; the LX-TX relation we determine for the shear-associated X-ray clusters is consistent with X-ray cluster samples selected without regard to dynamical state, while it is inconsistent with self-similarity. For a subset of the sample, we measure X-ray masses using temperature as a proxy, and compare to weak lensing masses determined by the DLS team. The resulting mass comparison is consistent with equality. The X-ray and weak lensing masses show considerable intrinsic scatter (∼48%), which is consistent with X-ray selected samples when their X-ray and weak lensing masses are independently determined.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): X-rays: galaxies: clusters - X-rays: galaxies: clusters

CDS comments: Table 2: XMMU sources are not in SIMBAD due to incomplete format.

Simbad objects: 26

goto Full paper

goto View the references in ADS

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 CXOU J052147.6-482124 X 05 21 47.6 -48 21 24           ~ 3 0
2 CXOU J052159.6-481606 C?G 05 21 59.6 -48 16 06           ~ 4 0
3 CXOU J052215.6-481817 X 05 22 15.6 -48 18 17           ~ 3 0
4 ACO 3338 ClG 05 22 16.041 -48 18 16.09           ~ 28 0
5 [WDH2006] DLSCL J0522.2-4820 D ClG 05 22 46.6 -48 18 04           ~ 4 0
6 CXOU J091551.8+293637 X 09 15 51.8 +29 36 37           ~ 5 0
7 CXOU J091554.4+293316 X 09 15 54.4 +29 33 16           ~ 7 0
8 DLSCL J0916.0+2931 ClG 09 16 00 +29 31.6           ~ 8 0
9 CXOU J091601.1+292750 X 09 16 01.1 +29 27 50           ~ 5 0
10 DLSCL J0916.3+3025 ClG 09 16.3 +30 25           ~ 1 0
11 SHELS J0919.6+3032 ClG 09 19 35.0414 +30 31 56.346           ~ 15 0
12 CXOU J092011.1+302955 ClG 09 20 11.1 +30 29 55           ~ 6 0
13 ACO 781 ClG 09 20 25.4 +30 30 07           ~ 167 0
14 CXOU J092026.4+302938 ClG 09 20 26.4 +30 29 39           ~ 11 0
15 CXOU J092053.0+302800 ClG 09 20 52.5 +30 27 40           ~ 28 0
16 CXOU J092110.3+302751 ClG 09 21 10.3 +30 27 52           ~ 19 0
17 DLSCL J0921.4+3013 ClG 09 21 18.6 +30 12 13           ~ 3 0
18 DLSCL J1048.5-0411 ClG 10 48.5 -04 11           ~ 1 0
19 DLSCL J1049.6-0417 ClG 10 49 41 -04 17.7           ~ 4 0
20 DLSCL J1054.1-0549 ClG 10 54 08 -05 49.7           ~ 4 0
21 CXOU J105414.8-054849 ClG 10 54 14.8 -05 48 50           ~ 5 0
22 CXOU J105510.1-050414 X 10 55 10.1 -05 04 14           ~ 3 0
23 ClG J1055-0504 ClG 10 55 11.6 -05 04 16           ~ 11 0
24 CXOU J105535.6-045930 ClG 10 55 35.6 -04 59 31           ~ 8 0
25 DLSCL J1402.0-1019 ClG 14 02 03 -10 19.7           ~ 4 0
26 DLSCL J1402.2-1028 ClG 14 02 12 -10 28.2           ~ 3 0

To bookmark this query, right click on this link: simbad:objects in 2017ApJ...839..124D and select 'bookmark this link' or equivalent in the popup menu