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GRB 180914A: Swift observation summary
| Mission: | Fermi/LAT |
|---|---|
| GRB RA: | 52.740° |
| GRB Dec: | -5.260° |
| GRB Err: | 24.0 arcmin |
| T0: | 2018-09-14 12:31:25 UT |
| Galactic: | 190.25° -46.21° |
| Galactic NH: | 3.83× 1020 cm-2 |
| Galactic E(B-V): | 0.0446915 |
| Sun distance: | 119.75° |
|---|---|
| Sun angle: | 7.97 [hr](West of Sun) |
| Moon distance: | 160.83° |
| Visibility of this field. | |
| First slew: | 2018-09-14 23:47:03 UT |
| First observation: | 2018-09-14 23:43:38 UT |
| First analysis: | UT |
So far 7 fields have been scheduled for observations. Data are available and processed for 7 of these. The list gives the exposure time used in source detection. If any individual sources were selected for follow-up observations, the source detection is not repeated for the follow up observations and the table below is not updated.
- 20830 — 373 s of cleaned data taken between 2018-09-14 23:44:21 and 2018-09-14 23:52:57
- 20832 — 368 s of cleaned data taken between 2018-09-14 23:53:01 and 2018-09-14 23:59:29
- 20833 — 132 s of cleaned data taken between 2018-09-14 23:59:34 and 2018-09-15 00:05:58
- 20834 — 358 s of cleaned data taken between 2018-09-15 00:06:03 and 2018-09-15 00:12:21
- 20835 — 340 s of cleaned data taken between 2018-09-15 00:12:25 and 2018-09-15 00:18:26
- 20836 — 335 s of cleaned data taken between 2018-09-15 00:18:32 and 2018-09-15 00:24:27
- 20837 — 223 s of cleaned data taken between 2018-09-15 00:24:32 and 2018-09-15 00:28:34
An additional 1 field has also been used for follow up observations. These data are not searched for sources, but are used to update the light curves etc of any sources already found.
Sources found so far
So far 1 sources have been found in the XRT data. 0 sources match catalogued sources.
| # | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Dist from LAT pos |
Exposure | Notes | Vizier |
|---|---|---|---|---|---|---|---|---|
| 1 [details] |
03h 32m 19.25s | -05° 37′ 27.5″ | 4.7′′ | Good | 29.8′ | 132 s |  |
1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the 1SXPS documentation.
* The position was enhanced using astrometry derived from the Swift UVOT.
† The position was astrometrically corrected using the XRT sources and the 2MASS catalogue.
Image
Select image style: Draggable PNG | JS9.
