SVOM_FIELD00026
SVOM
26
/SVOM
This is a confirmed GRB (GRB 250806A), the afterglow is source 1 -- please see the GRB results at https://www.swift.ac.uk/xrt_products/00019983 for updated analysis
.Mission: | SVOM/ECLAIRs |
---|---|
SVOM RA: | 348.307° |
SVOM Dec: | +1.357° |
SVOM Err: | 8.5 arcmin |
T0: | 2025-08-06 07:57:54 UT |
Galactic: | 79.30° -52.99° |
Galactic NH: | 4.61× 1020 cm-2 |
Sun distance: | 143.57° |
---|---|
Sun angle: | 9.86 [hr] (West of Sun) |
Moon distance: | 73.03° |
Visibility of this field. |
So far 1 fields have been scheduled for observations. Data are available and processed for 1 of these.
1 sources were found which matches the afterglow criteria.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Rank3 | Dist from SVOM/ECLAIRs pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
23h 13m 43.16s | +01° 21′ 18.1″ | 3.7′′ | Good | 2 (O) | 7.4′ | 972 s | The source is fading with 3.7-σ significance. The source is 4.1-σ above the RASS limit. |
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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.
So far 1 sources have been found in the XRT data. 0 sources match catalogued sources.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Rank3 | Dist from SVOM/ECLAIRs pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
23h 13m 43.16s | +01° 21′ 18.1″ | 3.7′′ | Good | 2 (O) | 7.4′ | 972 s | The source is fading with 3.7-σ significance. The source is 4.1-σ above the RASS limit. |
![]() |
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.
Select image style: Draggable PNG | JS9.