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Home > GRB products > GRB 180703A
TILED_GRB00070
NEWGRB
70
/xrt_products
GRB 180703A: Swift observation summary
Mission: | Fermi/LAT |
GRB RA: | 6.541° |
GRB Dec: | -67.090° |
GRB Err: | 18.2 arcmin |
T0: | 2018-07-03 21:01:35 UT |
Galactic: | 306.74° -49.85° |
Galactic NH: | 2.55× 1020 cm-2 |
Galactic E(B-V): | 0.01923181 |
Sun distance: | 113.47° |
Sun angle: | 6.42 [hr](West of Sun) |
Moon distance: | 59.32° |
Visibility of this field. |
First slew: | 2018-07-04 01:50:57 UT |
First observation: | 2018-07-04 01:39:30 UT |
First analysis: | UT |
Source 1 has been manually confirmed as the GRB afterglow; data for this object are now available through the main GRB results area for this GRB.
About tiled field analysis.
So far 4 fields have been scheduled for observations.
Data are available and processed for 5 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.
- 20797 — 531 s of cleaned data taken between 2018-07-04 01:42:07 and 2018-07-04 05:00:13
- 20798 — 468 s of cleaned data taken between 2018-07-04 01:45:25 and 2018-07-04 04:57:10
- 20799 — 539 s of cleaned data taken between 2018-07-04 01:48:43 and 2018-07-04 05:03:11
- 20800 — 428 s of cleaned data taken between 2018-07-04 01:51:53 and 2018-07-04 05:05:22
- 20801 — 4.6 ks of cleaned data taken between 2018-07-06 06:13:40 and 2018-07-06 22:15:36
Find an upper limit.
Sources found so far
So far 5 sources have been found in the XRT data. 1 sources match catalogued sources.
# |
RA (J2000) |
Dec (J2000) |
Err901 |
Detection Flag2 |
Dist from LAT pos |
Exposure |
Notes |
Vizier |
1 [details] |
00h 25m 52.79s6.46995° |
-67° 10′ 48.7″-67.18021° |
4.8′′ |
Good |
5.7′ |
5.6 ks |
|
|
- Mean XRT rate: 4.6 (±1.2) ×10-3 ct s-1
- Peak XRT rate: 4.6 (±1.2) ×10-3 ct s-1
- RASS PSPC 3-σ upper limit: 0.05 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 2.7 (±0.7) ×10-13 erg cm-1s-1
- Peak XRT flux: 2.7 (±0.7) ×10-13 erg cm-1s-1
- Products: Light curve | Spectrum
- Expected serendipitous sources: ~0.7 [What is this?]
|
2 [details] |
00h 23m 22.34s5.84306° |
-67° 11′ 11.1″-67.18641° |
6.2′′ |
Good |
17.3′ |
428 s |
Matches known X-ray source: 1RXS J002324.3-671101 (from ROSAT/RASSFSC), 15.2″ away. |
|
- Mean XRT rate: 2.46 (+1.10, -0.85) ×10-2 ct s-1
- Peak XRT rate: 2.46 (+1.10, -0.85) ×10-2 ct s-1
- RASS PSPC 3-σ upper limit: 0.10 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 6.3 (+2.8, -2.2) ×10-13 erg cm-1s-1
- Peak XRT flux: 6.3 (+2.8, -2.2) ×10-13 erg cm-1s-1
- Products: Light curve | Spectrum
- Expected serendipitous sources: ~0.1 [What is this?]
|
3 [details] |
00h 26m 20.38s6.58492° |
-67° 19′ 00.7″-67.31687° |
6.3′′ |
Good |
13.7′ |
5.2 ks |
|
|
- Mean XRT rate: 1.6 (+0.8, -0.6) ×10-3 ct s-1
- Peak XRT rate: 1.6 (+0.8, -0.6) ×10-3 ct s-1
- RASS PSPC 3-σ upper limit: 0.06 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 3.1 (+1.6, -1.2) ×10-14 erg cm-1s-1
- Peak XRT flux: 3.1 (+1.6, -1.2) ×10-14 erg cm-1s-1
- Products: Light curve | Spectrum
- Expected serendipitous sources: ~2.7 [What is this?]
|
4 [details] |
00h 24m 27.81s6.11587° |
-67° 18′ 22.1″-67.30614° |
5.0′′ |
Good |
16.3′ |
4.6 ks |
|
|
- Mean XRT rate: 8.1 (±1.9) ×10-3 ct s-1
- Peak XRT rate: 8.1 (±1.9) ×10-3 ct s-1
- RASS PSPC 3-σ upper limit: 0.09 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 1.8 (±0.4) ×10-13 erg cm-1s-1
- Peak XRT flux: 1.8 (±0.4) ×10-13 erg cm-1s-1
- Products: Light curve | Spectrum
- Expected serendipitous sources: ~0.3 [What is this?]
|
5 [details] |
00h 26m 43.72s6.68218° |
-67° 07′ 30.9″-67.12526° |
11.9′′ |
Reasonable |
3.9′ |
5.6 ks |
|
|
- Mean XRT rate: 1.6 (+0.8, -0.6) ×10-3 ct s-1
- Peak XRT rate: 1.6 (+0.8, -0.6) ×10-3 ct s-1
- RASS PSPC 3-σ upper limit: 0.06 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 5.3 (+2.5, -2.0) ×10-14 erg cm-1s-1
- Peak XRT flux: 5.3 (+2.5, -2.0) ×10-14 erg cm-1s-1
- Products: Light curve | Spectrum
- Expected serendipitous sources: ~2.7 [What is this?]
|
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.