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Home > GRB products > GRB 190129B

TILED_GRB00076

NEWGRB

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GRB 190129B: Swift observation summary

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 14 fields have been scheduled for observations. Data are available and processed for 14 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.

• 20852 — 463 s of cleaned data taken between 2019-01-29 22:31:06 and 2019-01-30 00:22:58
• 20853 — 461 s of cleaned data taken between 2019-01-29 22:37:34 and 2019-01-30 00:18:49
• 20854 — 461 s of cleaned data taken between 2019-01-29 22:43:56 and 2019-01-30 00:20:53
• 20855 — 463 s of cleaned data taken between 2019-01-29 22:50:22 and 2019-01-30 00:16:41
• 20856 — 463 s of cleaned data taken between 2019-01-29 22:56:39 and 2019-01-30 00:14:26
• 20857 — 463 s of cleaned data taken between 2019-01-29 23:02:51 and 2019-01-30 00:09:24
• 20858 — 441 s of cleaned data taken between 2019-01-29 23:08:53 and 2019-01-30 00:12:05
• 20860 — 463 s of cleaned data taken between 2019-01-30 00:43:17 and 2019-01-30 05:03:15
• 20861 — 443 s of cleaned data taken between 2019-01-30 00:44:23 and 2019-01-30 05:02:07
• 20862 — 446 s of cleaned data taken between 2019-01-30 00:45:28 and 2019-01-30 05:00:56
• 20863 — 358 s of cleaned data taken between 2019-01-30 00:46:34 and 2019-01-30 04:59:40
• 20864 — 426 s of cleaned data taken between 2019-01-30 00:47:39 and 2019-01-30 03:38:33
• 20865 — 473 s of cleaned data taken between 2019-01-30 00:48:45 and 2019-01-30 05:04:20
• 20866 — 466 s of cleaned data taken between 2019-01-30 01:43:07 and 2019-01-30 04:57:25

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.

Probable afterglow details

A source was found which matches the afterglow criteria.

#	RA (J2000)	Dec (J2000)	Err901	Detection Flag2	Dist from IPN pos	Exposure	Notes	Vizier
1 [details]	07h 49m 50.76s117.46152°	+00° 56′ 04.9″0.93470°	2.2′′	Good	22.0′	443 s	The source is 4.7-σ above the RASS limit.
Mean XRT rate: 0.44 (±0.04) ct s-1 Peak XRT rate: 0.69 (±0.14) ct s-1 RASS PSPC 3-σ upper limit: 0.04 ct s-1 (XRT equiv count-rate) Mean XRT flux: 1.97 (±0.18) ×10-11 erg cm-1s-1 Peak XRT flux: 3.1 (±0.6) ×10-11 erg cm-1s-1 Products: Light curve | Spectrum | Enhanced position Expected serendipitous sources: ~3.77×10-3 [What is this?] Note: this is extragalactic sources only, whereas the GRB trigger is at b=13.40°

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 2 sources have been found in the XRT data. 1 sources match catalogued sources.

#	RA (J2000)	Dec (J2000)	Err901	Detection Flag2	Dist from IPN pos	Exposure	Notes	Vizier
1 [details]	07h 49m 50.76s117.46152°	+00° 56′ 04.9″0.93470°	2.2′′	Good	22.0′	443 s	The source is 4.7-σ above the RASS limit.
Mean XRT rate: 0.44 (±0.04) ct s-1 Peak XRT rate: 0.69 (±0.14) ct s-1 RASS PSPC 3-σ upper limit: 0.04 ct s-1 (XRT equiv count-rate) Mean XRT flux: 1.97 (±0.18) ×10-11 erg cm-1s-1 Peak XRT flux: 3.1 (±0.6) ×10-11 erg cm-1s-1 Products: Light curve | Spectrum | Enhanced position Expected serendipitous sources: ~3.77×10-3 [What is this?] Note: this is extragalactic sources only, whereas the GRB trigger is at b=13.40°
2 [details]	07h 48m 58.68s117.24452°	+00° 40′ 39.7″0.67768°	6.6′′	Good	34.8′	697 s	Matches known X-ray source: 1SXPS J074858.7+004038 (from 1SXPS), 1.9″ away. Matches SIMBAD source: TYC 180-1818-1, 1.4″ away.
Mean XRT rate: 1.7 (+0.7, -0.6) ×10-2 ct s-1 Peak XRT rate: 1.7 (+0.7, -0.6) ×10-2 ct s-1 RASS PSPC 3-σ upper limit: 0.15 ct s-1 (XRT equiv count-rate) Products: Light curve Expected serendipitous sources: ~0.7 [What is this?] Note: this is extragalactic sources only, whereas the GRB trigger is at b=13.40°

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.

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Exposure map

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FITS exposure map.