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Home > GRB products > ToO GRBs > GRB 150902A
00020549
TOO
GRB 150902A: Swift observation summary
Mission: Fermi/LAT
GRB RA: 214.926°
GRB Dec: -69.361°
GRB Err: 7.6 arcmin
T0: 2015-09-02 17:35:24 UT
Galactic: 310.61° -7.82°
Galactic NH : 2.35× 1021 cm-2
Galactic E(B-V): 0.3964772
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 ToO field analysis .
Probable afterglow details
A source was found which matches the afterglow criteria.
#
RA (J2000)
Dec (J2000)
Err90 1
Detection Flag2
Dist from LAT pos
Exposure
Notes
Vizier
1 [details ]
14h 19m 55.09s 214.97956°
-69° 21′ 13.1″ -69.35365°
4.3′′
Good
1.2′
6.4 ks
Mean XRT rate: 7.9 (±1.3) ×10-3 ct s-1
Peak XRT rate: 9.4 (±1.7) ×10-3 ct s-1
RASS PSPC 3-σ upper limit: 0.04 ct s-1 (PSPC count-rate) Mean XRT rate converted to PSPC: 5.9 (±1.0) ×10-3 ct s-1
Peak XRT rate converted to PSPC: 7.0 (±1.3) ×10-3 ct s-1 Mean XRT flux: 3.6 (±0.6) ×10-13 erg cm-1 s-1
Peak XRT flux: 4.3 (±0.8) ×10-13 erg cm-1 s-1 Products: Light curve | Spectrum | Expected serendipitous sources: ~1.10×10-3 [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.
Find an upper limit .
Sources found so far
So far 5 sources have been found in the XRT data. 0 sources match catalogued sources.
#
RA (J2000)
Dec (J2000)
Err90 1
Detection Flag2
Dist from LAT pos
Exposure
Notes
Vizier
1 [details ]
14h 19m 55.09s 214.97956°
-69° 21′ 13.1″ -69.35365°
4.3′′
Good
1.2′
6.4 ks
Mean XRT rate: 7.9 (±1.3) ×10-3 ct s-1
Peak XRT rate: 9.4 (±1.7) ×10-3 ct s-1
RASS PSPC 3-σ upper limit: 0.04 ct s-1 (PSPC count-rate) Mean XRT rate converted to PSPC: 5.9 (±1.0) ×10-3 ct s-1
Peak XRT rate converted to PSPC: 7.0 (±1.3) ×10-3 ct s-1 Mean XRT flux: 3.6 (±0.6) ×10-13 erg cm-1 s-1
Peak XRT flux: 4.3 (±0.8) ×10-13 erg cm-1 s-1 Products: Light curve | Spectrum | Expected serendipitous sources: ~1.10×10-3 [What is this? ]
2 [details ]
14h 21m 05.04s 215.27099°
-69° 29′ 29.7″ -69.49158°
6.4′′
Poor
10.7′
5.4 ks
Mean XRT rate: 0.00 (±0.00) ×10-1 ct s-1
Peak XRT rate: 0.00 (±0.00) ×10-1 ct s-1
RASS PSPC 3-σ upper limit: 0.03 ct s-1 (PSPC count-rate) Mean XRT rate converted to PSPC: 2.18 (+1.17, -0.92) ×10-3 ct s-1
Peak XRT rate converted to PSPC: 2.18 (+1.17, -0.92) ×10-3 ct s-1 Mean XRT flux: 2.8 (+1.5, -1.2) ×10-14 erg cm-1 s-1
Peak XRT flux: 2.8 (+1.5, -1.2) ×10-14 erg cm-1 s-1 Products: Light curve | Spectrum | Expected serendipitous sources: ~0.03 [What is this? ]
3 [details ]
14h 21m 18.44s 215.32683°
-69° 14′ 13.3″ -69.23702°
6.0′′
Reasonable
11.3′
5.6 ks
Mean XRT rate: 2.0 (±0.7) ×10-3 ct s-1
Peak XRT rate: 2.0 (±0.7) ×10-3 ct s-1
RASS PSPC 3-σ upper limit: 0.04 ct s-1 (PSPC count-rate) Products: Light curve | Spectrum | Expected serendipitous sources: ~1.89×10-2 [What is this? ]
4 [details ]
14h 20m 41.55s 215.17314°
-69° 27′ 01.7″ -69.45046°
7.8′′
Reasonable
7.5′
6.2 ks
Mean XRT rate: 1.1 (±0.5) ×10-3 ct s-1
Peak XRT rate: 1.1 (±0.5) ×10-3 ct s-1
RASS PSPC 3-σ upper limit: 0.02 ct s-1 (PSPC count-rate) Mean XRT rate converted to PSPC: 5.8 (±2.8) ×10-4 ct s-1
Peak XRT rate converted to PSPC: 5.8 (±2.8) ×10-4 ct s-1 Mean XRT flux: 9 (±4) ×10-14 erg cm-1 s-1
Peak XRT flux: 9 (±4) ×10-14 erg cm-1 s-1 Products: Light curve | Spectrum | Expected serendipitous sources: ~1.89×10-2 [What is this? ]
5 [details ]
14h 21m 12.25s 215.30104°
-69° 14′ 55.8″ -69.24885°
5.7′′
Good
10.4′
5.9 ks
Mean XRT rate: 1.2 (±0.6) ×10-3 ct s-1
Peak XRT rate: 1.2 (±0.6) ×10-3 ct s-1
RASS PSPC 3-σ upper limit: 0.05 ct s-1 (PSPC count-rate) Mean XRT rate converted to PSPC: 2.1 (±1.0) ×10-3 ct s-1
Peak XRT rate converted to PSPC: 2.1 (±1.0) ×10-3 ct s-1 Mean XRT flux: 1.7 (±0.8) ×10-14 erg cm-1 s-1
Peak XRT flux: 1.7 (±0.8) ×10-14 erg cm-1 s-1 Products: Light curve | Spectrum | Expected serendipitous sources: ~0.03 [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
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FITS image .
Exposure map
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FITS exposure map .