EP_FIELD00017
EP
17
/EP
Mission: | Einstein Probe/WXT |
---|---|
Einstein Probe RA: | 356.911° |
Einstein Probe Dec: | +27.008° |
Einstein Probe Err: | 3.1 arcmin |
T0: | 2025-02-07 15:51:17 UT |
Galactic: | 105.81° -33.73° |
Galactic NH: | 4.48× 1020 cm-2 |
Sun distance: | 54.61° |
---|---|
Sun angle: | 2.38 [hr] (East of Sun) |
Moon distance: | 69.80° |
Visibility of this field. | |
First slew: | 2025-02-07 17:56:54 UT |
First observation: | 2025-02-07 17:56:18 UT |
First analysis: | 2025-02-07 22:57:00 UT |
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 Einstein Probe/WXT pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
23h 47m 37.47s | +27° 02′ 07.3″ | 2.7′′ * | Good | 2 (O) | 1.7′ | 1.7 ks | The source is 4.2-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.
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 Einstein Probe/WXT pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
23h 47m 37.47s | +27° 02′ 07.3″ | 2.7′′ * | Good | 2 (O) | 1.7′ | 1.7 ks | The source is 4.2-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.