Table 2
Chandra observation log.
No. | Galaxy | Obs ID | Date | Mode | Exp. Time | 0.4–7 keVa | NH,Galb |
(ks) | (cts) | (1020 cm-2) | |||||
|
|||||||
Cycle 8 targets | |||||||
1 | F01364–1042 | 7801 | 2007 Sep. 10 | VFAINT | 14.57 | 46.0 ± 7.3 | 2.0 |
2 | ESO 203-IG1 | 7802 | 2008 Jan. 17 | VFAINT | 14.85 | 0 (<3) | 1.4 |
3 | VII Zw 31 | 7887 | 2007 May 27 | VFAINT | 14.98 | 173.8 ± 13.3 | 7.4 |
5 | ESO 255-IG7 | 7803 | 2007 May 27 | VFAINT | 14.57 | 341.8 ± 18.8 | 3.8 |
6 | 07251–0248 | 7804 | 2006 Dec. 01 | VFAINT | 15.43 | 12.7 ± 3.6 | 14.6 |
7 | ESO 60-IG16 | 7888 | 2007 May 31 | VFAINT | 14.68 | 122.6 ± 11.1 | 5.2 |
9 | 09022–3615 | 7805 | 2007 Sep. 04 | VFAINT | 14.85 | 265.3 ± 16.5 | 26.6 |
10 | F09111–1007 | 7806 | 2007 Mar. 20 | VFAINT | 14.63 | 118.7 ± 11.1 | 4.6 |
13 | ESO 374-IG32 | 7807 | 2007 Mar. 07 | VFAINT | 14.36 | 75.0 ± 9.1 | 8.8 |
14 | F10173+0828 | 7808 | 2008 Jan. 18 | VFAINT | 14.98 | 9.8 ± 3.2 | 2.3 |
19 | 13120–5453 | 7809 | 2006 Dec. 01 | VFAINT | 14.67 | 300.7 ± 17.4 | 21.3 |
20 | VV 250 | 7810 | 2007 Aug. 22 | VFAINT | 14.85 | 391.9 ± 20.1 | 2.0 |
21 | UGC 8387 | 7811 | 2007 Feb. 19 | VFAINT | 14.07 | 251.4 ± 16.0 | 1.0 |
24 | F14378–3651 | 7889 | 2007 Jun. 25 | VFAINT | 13.86 | 45.3 ± 6.8 | 6.3 |
25 | VV 340 | 7812 | 2006 Dec. 17 | VFAINT | 14.86 | 331.4 ± 20.4 | 3.3 |
29 | ESO 69-IG6 | 7813 | 2007 Jun. 21 | VFAINT | 14.54 | 330.1 ± 18.3 | 9.1 |
31 | F17132+5313 | 7814 | 2007 Apr. 03 | VFAINT | 14.85 | 90.8 ± 10.0 | 1.9 |
33 | F18293-3413 | 7815 | 2007 Feb. 25 | VFAINT | 14.04 | 444.6 ± 21.5 | 9.7 |
34 | ESO 593-IG8 | 7816 | 2007 Jun. 09 | VFAINT | 14.97 | 158.1 ± 13.7 | 8.1 |
35 | F19297–0406 | 7980 | 2007 Jun. 18 | VFAINT | 16.42 | 85.8 ± 9.7 | 15.1 |
36 | 19542+1110 | 7817 | 2007 Sep. 10 | VFAINT | 14.98 | 324.3 ± 18.0 | 14.0 |
37 | CGCG 448-020 | 7818 | 2007 Sep. 10 | VFAINT | 14.56 | 301.3 ± 18.2 | 6.9 |
39 | 21101+5810 | 7819 | 2007 Jul. 01 | VFAINT | 14.85 | 21.7 ± 4.8 | 37.2 |
40 | ESO 239-IG2 | 7820 | 2007 Sep. 10 | VFATIN | 14.57 | 151.5 ± 13.1 | 0.9 |
41 | F22491–1808 | 7821 | 2007 Jul. 13 | VFAINT | 14.97 | 50.9 ± 7.3 | 2.3 |
43 | ESO 77-IG14 | 7822 | 2008 Jan. 26 | VFAINT | 14.98 | 84.1 ± 9.3 | 3.3 |
Archival data | |||||||
4 | F05189-2524 | 3432 | 2002 Jan. 03 | FAINT | 14.86 | 2016.9 ± 45.0 | 1.7 |
8 | F08572+3915 | 6862 | 2006 Jan. 26 | FAINT | 14.94 | 9.7 ± 3.2 | 2.0 |
11 | UGC 4881 | 6857 | 2006 Jan. 12 | FAINT | 14.77 | 69.4 ± 8.4 | 1.4 |
12 | UGC 5101 | 2033 | 2001 May 28 | FAINT | 49.32 | 482.9 ± 22.3 | 3.0 |
15 | F10565+2448 | 4552 | 2003 Oct. 23 | FAINT | 28.87 | 335.2 ± 18.8 | 1.1 |
16 | NGC 3690 | 6227 | 2005 Feb. 14 | FAINT | 10.19 | 2526.0 ± 52.1 | 0.9 |
17 | F12112+0305 | 4110 | 2003 Apr. 15 | VFAINT | 9.87 | 42.6 ± 6.6 | 1.8 |
18 | UGC 8058 | 1031c | 2000 Oct 19 | FAINT | 39.25 | 2312.5 ± 66.2 | 1.0 |
18 | UGC 8058 | 4028 | 2003 Feb. 03 | VFAINT | 39.68 | 2205.6 ± 59.7 | 1.0 |
18 | UGC 8058 | 4029 | 2003 Feb. 11 | VFAINT | 38.63 | 2070.5 ± 57.3 | 1.0 |
18 | UGC 8058 | 4030 | 2003 Feb. 20 | VFAINT | 36.01 | 1876.6 ± 52.0 | 1.0 |
22 | UGC 8696 | 809 | 2000 Apr. 19 | VFAINT | 44.19 | 2054.0 ± 45.8 | 0.9 |
23 | F14348-1447 | 6861 | 2006 Mar. 12 | FAINT | 14.72 | 75.9 ± 8.8 | 7.5 |
26 | VV 705 | 6858 | 2006 Sep. 11 | FAINT | 14.47 | 157.8 ± 12.6 | 1.8 |
27 | F15250+3608 | 4112 | 2003 Aug. 27 | VFAINT | 9.84 | 26.6 ± 5.3 | 1.5 |
28 | UGC 9913 | 869 | 2000 Jun. 24 | FAINT | 56.49 | 1555.1 ± 47.1 | 3.9 |
30 | NGC 6240 | 1590 | 2001 Jul. 29 | FAINT | 36.69 | 10010.7 ± 103.5 | 4.9 |
32 | F17207-0014 | 2035 | 2001 Oct. 24 | FAINT | 48.53 | 476.6 ± 23.1 | 9.7 |
38 | ESO 286-IG19 | 2036 | 2001 Oct. 31 | FAINT | 44.87 | 767.8 ± 28.3 | 3.3 |
42 | ESO 148-IG2 | 2037 | 2001 Sep. 30 | FAINT | 49.31 | 1052.2 ± 34.9 | 1.6 |
44 | F23365+3604 | 4115 | 2003 Feb. 03 | VFAINT | 10.10 | 28.8 ± 5.4 | 9.6 |
Notes. The 26 Cycle 8 Chandra observations (PI: D. Sanders) are listed first, followed by archival data for the additional 18 objects with log (Lir/L⊙) > 11.73. All observations were obtained in imaging mode with the ACIS-S, and the targets were placed at the nominal pointing position on the detector.
The source counts are corrected for background and measured in the 0.4–7 keV band. The counts from separate components in a single objects are summed together.
The Galactic absorption column density is taken from the LAB HI map by Kalberla et al. (2005).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.