EP_FIELD00037
EP
37
/EP
Mission: | Einstein Probe/WXT |
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Einstein Probe RA: | 299.150° |
Einstein Probe Dec: | +3.460° |
Einstein Probe Err: | 3.1 arcmin |
T0: | 2025-05-06 21:07:59 UT |
Galactic: | 43.65° -12.81° |
Galactic NH: | 9.55× 1020 cm-2 |
Sun distance: | 102.94° |
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Sun angle: | 6.98 [hr] (West of Sun) |
Moon distance: | 133.38° |
Visibility of this field. | |
First slew: | 2025-05-06 21:54:47 UT |
First observation: | 2025-05-06 21:54:15 UT |
First analysis: | 2025-05-07 00:47:13 UT |
So far 1 fields have been scheduled for observations. Data are available and processed for 1 of these.
1 fields were processed but not included in the analysis. This is because, after standard processing and the removal of times contaminated by light reflected off the bright Earth, there was too little data (<100 s) for source detection to be performed.
1 sources were found which matches the afterglow criteria.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Rank3 | Exposure | Notes | Vizier | |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
19h 56m 39.02s | +03° 26′ 43.8″ | 2.5′′ * | Good | 2 (O) | 1.2′ | 1.1 ks | Matches SIMBAD source: IGR J19566+0326, 1.2″ away. Matches known X-ray source: LSXPS J195639.1+032642 (from LSXPS), 2.4″ away. |
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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 6 sources have been found in the XRT data. 2 sources match catalogued sources. There are also 2 sources marked as spurious.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Rank3 | Dist from Einstein Probe/WXT pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
19h 56m 39.02s | +03° 26′ 43.8″ | 2.5′′ * | Good | 2 (O) | 1.2′ | 1.1 ks | Matches SIMBAD source: IGR J19566+0326, 1.2″ away. Matches known X-ray source: LSXPS J195639.1+032642 (from LSXPS), 2.4″ away. |
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2 [details] |
19h 56m 30.87s | +03° 39′ 09.2″ | 6.6′′ * | Good | 4 (K) | 11.6′ | 1.1 ks | Matches known X-ray source: LSXPS J195631.0+033908 (from LSXPS), 2.2″ away. | ![]() |
3 [details] |
19h 56m 38.95s | +03° 27′ 09.1″ | 4.0′′ * | Reasonable | 4 (K) | 0.9′ | 930 s | The source is 4.9-σ above the LSPXS limit. This source is extended or caused by diffuse emission. |
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4 [details] |
19h 56m 34.18s | +03° 26′ 11.6″ | 5.9′′ * | Poor | 4 (K) | 1.5′ | 1.1 ks | The source is 5.6-σ above the LSPXS limit. This source is extended or caused by diffuse emission. |
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5 [details] |
19h 56m 39.27s | +03° 27′ 49.8″ | 4.6′′ * | Poor | 3 (U) | 0.8′ | 1.1 ks | The source is 5.0-σ above the LSPXS limit. This source may be affected by optical loading |
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6 [details] |
19h 56m 30.41s | +03° 27′ 18.9″ | 6.3′′ * | Poor | 3 (U) | 1.4′ | 1.1 ks | ![]() |
|
7 [details] |
19h 56m 37.78s | +03° 27′ 28.2″ | 6.6′′ * | Poor | 3 (U) | 0.5′ | 1.1 ks | The source is fading with 4.0-σ significance. The source is 4.4-σ above the LSPXS limit. This source may be affected by optical loading This source may be affected by optical loading |
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8 [details] |
19h 56m 42.18s | +03° 27′ 53.0″ | 6.1′′ | Poor | 3 (U) | 1.6′ | 1.1 ks | The source is 4.4-σ above the LSPXS limit. This source may be affected by optical loading |
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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.
Select image style: Draggable PNG | JS9.