GRB 240513A: Swift observation summary

Mission:	Fermi/LAT
GRB RA:	163.400°
GRB Dec:	-27.500°
GRB Err:	24.0 arcmin
T0:	2024-05-13 07:22:02 UT
Galactic:	273.18° +28.48°
Galactic N_H:	5.56× 10²⁰ cm^-2
Galactic E(B-V):	0.07036541

Sun distance:	118.45°
Sun angle:	7.54 [hr] (East of Sun)
Moon distance:	66.80°
Visibility of this field.
First slew:	2024-05-13 20:10:35 UT
First observation:	2024-05-13 20:10:00 UT
First analysis:	UT

Source 6 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 2 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.

21685 — 782 s of cleaned data taken between 2024-05-14 02:26:26 and 2024-05-14 02:42:24
21686 — 839 s of cleaned data taken between 2024-05-14 05:31:27 and 2024-05-14 05:47:32
21687 — 554 s of cleaned data taken between 2024-05-13 20:10:31 and 2024-05-13 20:22:38
21688 — 734 s of cleaned data taken between 2024-05-13 21:22:27 and 2024-05-13 21:36:23
21689 — 702 s of cleaned data taken between 2024-05-13 21:36:27 and 2024-05-13 21:48:30
21690 — 692 s of cleaned data taken between 2024-05-13 21:48:35 and 2024-05-13 22:00:30
21691 — 814 s of cleaned data taken between 2024-05-13 22:53:41 and 2024-05-13 23:08:58

Find an upper limit.

Sources found so far

So far 6 sources have been found in the XRT data. 3 sources match catalogued sources.

#	RA (J2000)	Dec (J2000)	Err₉₀¹	Detection Flag²	Dist from LAT pos	Exposure	Notes
1 [details]	10h 52m 51.09s163.21288°	-27° 27′ 19.4″-27.45539°	3.5′′	Good	10.3′	8.8 ks	Matches known X-ray source: 1RXS J105251.7-272709 (from ROSAT/RASSBSC), 9.7378579140968″ away. Matches SIMBAD source: HE 1050-2711, 2.1″ away.
Mean XRT rate: 7.6 (±0.4) ×10^-2 ct s^-1 Peak XRT rate: 0.110 (±0.021) ct s^-1 RASS PSPC 3-σ upper limit: 0.0×10⁰ ct s^-1 (XRT equiv count-rate) Mean XRT flux: 1.86 (±0.10) ×10^-12 erg cm^-1s^-1 Peak XRT flux: 2.7 (±0.5) ×10^-12 erg cm^-1s^-1 Products: Light curve \| Spectrum \| Enhanced position
2 [details]	10h 55m 17.69s163.82370°	-27° 37′ 20.9″-27.62248°	9.7′′	Poor	23.7′	814 s
Mean XRT rate: 9 (+5, -4) ×10^-3 ct s^-1 Peak XRT rate: 9 (+5, -4) ×10^-3 ct s^-1 RASS PSPC 3-σ upper limit: 0.02 ct s^-1 (XRT equiv count-rate) Products: Spectrum
3 [details]	10h 52m 01.19s163.00496°	-27° 34′ 21.8″-27.57271°	6.0′′	Good	21.5′	684 s	This source is affected by optical loading. Matches SIMBAD source: HD 94209, 3.1″ away.
Mean XRT rate: 1.4 (+0.7, -0.5) ×10^-2 ct s^-1 Peak XRT rate: 1.4 (+0.7, -0.5) ×10^-2 ct s^-1 RASS PSPC 3-σ upper limit: 0.03 ct s^-1 (XRT equiv count-rate) Mean XRT flux: 5.3 (+2.5, -2.0) ×10^-13 erg cm^-1s^-1 Peak XRT flux: 5.3 (+2.5, -2.0) ×10^-13 erg cm^-1s^-1 Products: Spectrum
4 [details]	10h 55m 44.10s163.93377°	-27° 35′ 36.2″-27.59340°	7.6′′	Poor	28.9′	814 s
Mean XRT rate: 7 (+5, -3) ×10^-3 ct s^-1 Peak XRT rate: 7 (+5, -3) ×10^-3 ct s^-1 RASS PSPC 3-σ upper limit: 0.05 ct s^-1 (XRT equiv count-rate) Products: Spectrum
5 [details]	10h 53m 41.32s163.42216°	-27° 40′ 30.9″-27.67526°	5.9′′	Reasonable	10.6′	1.5 ks	Matches known X-ray source: 1RXS J105338.6-274002 (from ROSAT/RASSFSC), 46.28940458107″ away.
Mean XRT rate: 8.3 (+3.7, -2.8) ×10^-3 ct s^-1 Peak XRT rate: 8.3 (+3.7, -2.8) ×10^-3 ct s^-1 RASS PSPC 3-σ upper limit: 0.0×10⁰ ct s^-1 (XRT equiv count-rate) Mean XRT flux: 1.3 (+0.6, -0.4) ×10^-13 erg cm^-1s^-1 Peak XRT flux: 1.3 (+0.6, -0.4) ×10^-13 erg cm^-1s^-1 Products: Spectrum
6 [details]	10h 53m 49.05s163.45436°	-27° 24′ 41.7″-27.41160°	5.1′′	Good	6.0′	8.1 ks
Mean XRT rate: 9.5 (+1.4, -1.3) ×10^-3 ct s^-1 Peak XRT rate: 2.2 (+0.7, -0.6) ×10^-2 ct s^-1 RASS PSPC 3-σ upper limit: 0.04 ct s^-1 (XRT equiv count-rate) Mean XRT flux: 4.5 (±0.6) ×10^-13 erg cm^-1s^-1 Peak XRT flux: 1.07 (+0.34, -0.28) ×10^-12 erg cm^-1s^-1 Products: Spectrum

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.