Table 1.
Log of UVIT imaging observations for six galaxy clusters.
| Galaxy cluster | RAJ2000 | DecJ2000 | Channel | Filter | λmean | δλ | Integration time |
|---|---|---|---|---|---|---|---|
| (h:m:s) | (°:′:″) | (Å) | (Å) | (s) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| Abell 1668 | 13:04:06 | +19:17:13 | FUV | F154W | 1541 | 380 | 17 989 |
| Abell 1991 | 14:53:51 | +18:39:05 | FUV | F148W | 1481 | 500 | 12 900 |
| NUV | N242W | 2418 | 785 | 12 516 | |||
| Abell 2626 | 23:36:25 | +21:09:03 | FUV | F148W | 1481 | 500 | 11 539 |
| NUV | N242W | 2418 | 785 | 10 107 | |||
| Abell 3376 | 06:00:48 | −39:55:07 | FUV | F148W | 1481 | 500 | 31 619 |
| Abell 4059 | 23:57:01 | −34:40:50 | FUV | F148W | 1481 | 500 | 37 504 |
| Abell 85 | 00:41:50 | −09:19:37 | FUV | F148W | 1481 | 500 | 15 429 |
| NUV | N242W | 2418 | 785 | 18 326 |
Notes. Key to columns: (1) Cluster name; (2) and (3) UVIT pointing centre coordinates; (4) UVIT channels used; (5) filter for imaging observations; (6) mean wavelength for filter; (7) filter bandwidth; and (8) total integration time. NUV and FUV imaging data exist for three clusters; for three others, only FUV imaging is available. Note that the six clusters were imaged in NUV and FUV to varying depths. The UVIT NUV and FUV filters used in this study are broadly similar to the NUV and FUV filters on GALEX (see Tandon et al. 2017).
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.