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GRB 260204A: Swift observation summary

Mission:SVOM/ECLAIRs
SVOM RA:205.119°
SVOM Dec:+2.020°
SVOM Err:7.4 arcmin
T0:2026-02-04 14:48:28 UT
Galactic:330.07° +62.28°
Galactic NH:1.75× 1020 cm-2
Sun distance:112.42°
Sun angle:7.52 [hr](West of Sun)
Moon distance:35.16°
Visibility of this field.
First slew:2026-02-04 21:25:39 UT
First observation:2026-02-04 21:17:03 UT
First analysis:2026-02-04 23:37:01 UT
Data analysed so far:
  • ObsID: 03000405001 with 1.7 ks exposure.

About tiled field analysis.

So far 1 fields have been scheduled for observations. Data are available and processed for 1 of these.

Find an upper limit.

Sources found so far

So far 4 sources have been found in the XRT data. 3 sources match catalogued sources.

:

# RA (J2000) Dec (J2000) Err901 Detection
Flag2
Rank3 Dist from
SVOM/ECLAIRs pos
Exposure Notes Vizier
1
[details]
13h 40m 25.50s +01° 55′ 50.7″ 4.4′′ * Good 3 (U) 5.4′ 1.7 ks This source may be affected by optical loading Vizier logo
2
[details]
13h 40m 26.94s +02° 09′ 02.7″ 4.4′′ * Good 3 (U) 7.9′ 1.7 ks Matches SIMBAD source: HD 118981, 0.7″ away. Vizier logo
3
[details]
13h 40m 23.65s +01° 56′ 10.5″ 5.9′′ * Good 4 (K) 5.2′ 1.7 ks This source may be affected by optical loading
Matches known X-ray source: XMMSL3 J134023.8+015613 (from XMM-NEWTON/XMMSLEWCLN), 1.5517922236173″ away.
Vizier logo
4
[details]
13h 40m 43.07s +02° 03′ 08.7″ 6.1′′ * Good 3 (U) 4.1′ 1.7 ks Matches SIMBAD source: [VV2006] J134042.9+020307, 4.5″ away. Vizier logo

1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the LSXPS documentation.
3 T=Transient Source, O=Outbursting known source, U=Uncatalogued X-ray source, K=Known X-ray source.
* 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.

FITS image.

Image of all observations processed so far

Exposure map

FITS exposure map.

Exposure map of all observations processed so far