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Home > GRB products > ToO GRBs > GRB 230707A
00021587
NEWTOO
21587
/ToO_GRBs
GRB 230707A: Swift observation summary
Mission: | Swift/BAT-GUANO |
GRB RA: | 171.476° |
GRB Dec: | -21.512° |
GRB Err: | 2.0 arcmin |
T0: | 2023-07-07 03:22:51 UT |
Galactic: | 277.75° +37.14° |
Galactic NH: | 3.69× 1020 cm-2 |
Galactic E(B-V): | 0.04468591 |
- Data analysed so far:
- ObsID: 00021587001 with 4.7 ks exposure.
About ToO analysis.
Find an upper limit.
Sources found so far
So far 3 sources have been found in the XRT data. 0 sources match catalogued sources.
# |
RA (J2000) |
Dec (J2000) |
Err901 |
Detection Flag2 |
Dist from Swift/BAT-GUANO pos |
Exposure |
Notes |
Vizier |
1 [details] |
11h 25m 12.17s171.30070° |
-21° 27′ 58.9″-21.46637° |
6.6′′ |
Good |
10.2′ |
4.7 ks |
|
|
- Mean XRT rate: 3.3 (+1.3, -1.0) ×10-3 ct s-1
- Peak XRT rate: 3.3 (+1.3, -1.0) ×10-3 ct s-1
- RASS PSPC 3-σ upper limit: 0.04 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 9.1 (+3.5, -2.8) ×10-14 erg cm-1s-1
- Peak XRT flux: 9.1 (+3.5, -2.8) ×10-14 erg cm-1s-1
- Products: Spectrum |
- Expected serendipitous sources: ~0.00×10+0 [What is this?]
|
2 [details] |
11h 26m 13.81s171.55755° |
-21° 23′ 32.6″-21.39238° |
5.7′′ |
Good |
8.5′ |
4.7 ks |
|
|
- Mean XRT rate: 2.99 (+1.18, -0.94) ×10-3 ct s-1
- Peak XRT rate: 2.99 (+1.18, -0.94) ×10-3 ct s-1
- RASS PSPC 3-σ upper limit: 0.04 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 9.5 (+3.7, -3.0) ×10-14 erg cm-1s-1
- Peak XRT flux: 9.5 (+3.7, -3.0) ×10-14 erg cm-1s-1
- Products: Spectrum |
- Expected serendipitous sources: ~0.00×10+0 [What is this?]
|
3 [details] |
11h 26m 06.91s171.52880° |
-21° 27′ 55.1″-21.46530° |
7.7′′ |
Poor |
4.1′ |
4.7 ks |
|
|
- Mean XRT rate: 1.4 (+0.9, -0.6) ×10-3 ct s-1
- Peak XRT rate: 1.4 (+0.9, -0.6) ×10-3 ct s-1
- RASS PSPC 3-σ upper limit: 0.23 ct s-1 (XRT equiv count-rate)
- Mean XRT flux: 7 (+4, -3) ×10-13 erg cm-1s-1
- Peak XRT flux: 7 (+4, -3) ×10-13 erg cm-1s-1
- Products: Spectrum |
- Expected serendipitous sources: ~0.00×10+0 [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.