SVOM_FIELD00040
SVOM
40
/SVOM
Mission: | SVOM/ECLAIRs |
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SVOM RA: | 311.321° |
SVOM Dec: | -31.412° |
SVOM Err: | 8.1 arcmin |
T0: | 2025-10-10 03:47:53 UT |
Galactic: | 12.58° -36.84° |
Galactic NH: | 6.10× 1020 cm-2 |
Sun distance: | 108.09° |
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Sun angle: | 7.73 [hr] (East of Sun) |
Moon distance: | 113.94° |
Visibility of this field. | |
First slew: | 2025-10-10 04:06:25 UT |
First observation: | 2025-10-10 04:05:54 UT |
First analysis: | 2025-10-10 06:46:16 UT |
So far 1 fields have been scheduled for observations. Data are available and processed for 1 of these.
4 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] |
20h 45m 10.19s | -31° 20′ 37.7″ | 2.5′′ * | Good | 2 (O) | 4.3′ | 325 s | This source may be affected by optical loading
This source may be affected by optical loading Matches SIMBAD source: NAME AU Mic e, 11.2″ away. Matches known X-ray source: LSXPS J204509.8-312033 (from LSXPS), 5.3″ away. |
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2 [details] |
20h 45m 03.88s | -31° 21′ 16.6″ | 4.0′′ * | Good | 1 (T) | 4.4′ | 2.1 ks | The source is fading with 3.4-σ significance. The source is 3.9-σ above the RASS limit. This source is extended or caused by diffuse emission. |
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3 [details] |
20h 45m 07.62s | -31° 20′ 33.4″ | 3.8′′ * | Reasonable | 2 (O) | 4.6′ | 325 s | This source may be affected by optical loading
This source is extended or caused by diffuse emission. Matches known X-ray source: 1AXG J204508-3119 (from ASCA/ASCAGIS), 31.581010478147″ away. |
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4 [details] |
20h 45m 14.41s | -31° 20′ 01.5″ | 7.9′′ | Reasonable | 1 (T) | 4.7′ | 2.1 ks | The source is fading with 5.0-σ significance. The source is 5.3-σ above the RASS limit. This source is extended or caused by diffuse emission. |
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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 7 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] |
20h 45m 10.19s | -31° 20′ 37.7″ | 2.5′′ * | Good | 2 (O) | 4.3′ | 325 s | This source may be affected by optical loading
This source may be affected by optical loading Matches SIMBAD source: NAME AU Mic e, 11.2″ away. Matches known X-ray source: LSXPS J204509.8-312033 (from LSXPS), 5.3″ away. |
![]() |
2 [details] |
20h 45m 03.88s | -31° 21′ 16.6″ | 4.0′′ * | Good | 1 (T) | 4.4′ | 2.1 ks | The source is fading with 3.4-σ significance. The source is 3.9-σ above the RASS limit. This source is extended or caused by diffuse emission. |
![]() |
3 [details] |
20h 45m 07.62s | -31° 20′ 33.4″ | 3.8′′ * | Reasonable | 2 (O) | 4.6′ | 325 s | This source may be affected by optical loading
This source is extended or caused by diffuse emission. Matches known X-ray source: 1AXG J204508-3119 (from ASCA/ASCAGIS), 31.581010478147″ away. |
![]() |
4 [details] |
20h 45m 14.41s | -31° 20′ 01.5″ | 7.9′′ | Reasonable | 1 (T) | 4.7′ | 2.1 ks | The source is fading with 5.0-σ significance. The source is 5.3-σ above the RASS limit. This source is extended or caused by diffuse emission. |
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5 [details] |
20h 45m 42.55s | -31° 16′ 44.0″ | 5.7′′ | Poor | 4 (K) | 9.7′ | 2.1 ks | Matches SIMBAD source: 2XMM J204542.1-311652, 8.8″ away. Matches known X-ray source: LSXPS J204542.2-311652 (from LSXPS), 9.4″ away. |
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6 [details] |
20h 45m 04.81s | -31° 21′ 50.1″ | 4.1′′ * | Poor | 3 (U) | 3.9′ | 2.1 ks | This source is extended or caused by diffuse emission. | ![]() |
7 [details] |
20h 45m 00.91s | -31° 32′ 59.1″ | 6.8′′ | Poor | 3 (U) | 9.0′ | 2.1 ks | ![]() |
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.