00021752
NEWTOO
21752
/ToO_GRBs
Mission: | SVOM/ECLAIRs |
---|---|
GRB RA: | 22.083° |
GRB Dec: | -5.096° |
GRB Err: | 4.6 arcmin |
T0: | 2025-01-03 09:56:34 UT |
Galactic: | 146.31° -66.28° |
Galactic NH: | 3.97× 1020 cm-2 |
Galactic E(B-V): | 0.04008137 |
Sun distance: | 95.39° |
---|---|
Sun angle: | 6.53 [hr](East of Sun) |
Moon distance: | 52.37° |
Visibility of this field. |
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.
A source was found which matches the afterglow criteria.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Dist from SVOM/ECLAIRs pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|
1 [details] |
01h 28m 15.40s | -05° 03′ 06.4″ | 2.5′′ | Good | 2.9′ | 7.1 ks | The source is fading with 4.1-σ significance. | ![]() |
1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the 2SXPS 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.
So far 4 sources have been found in the XRT data. 2 sources match catalogued sources.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Dist from SVOM/ECLAIRs pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|
1 [details] |
01h 28m 15.40s | -05° 03′ 06.4″ | 2.5′′ | Good | 2.9′ | 7.1 ks | The source is fading with 4.1-σ significance. | ![]() |
2 [details] |
01h 28m 33.26s | -05° 06′ 47.2″ | 6.4′′ | Poor | 3.5′ | 7.1 ks | ![]() |
|
3 [details] |
01h 28m 39.72s | -05° 01′ 24.6″ | 6.7′′ | Poor | 6.6′ | 7.1 ks | Matches known X-ray source: 1WGA J0128.6-0501 (from ROSAT/WGACAT), 19.3″ away. Matches SIMBAD source: PB 8865, 5.7″ away. |
![]() |
4 [details] |
01h 27m 48.73s | -05° 07′ 30.2″ | 6.4′′ | Poor | 8.0′ | 7.1 ks | Matches SIMBAD source: SDSS J012748.60-050725.4, 5″ away. | ![]() |
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.
Select image style: Draggable PNG | JS9.