EP_FIELD00035
EP
35
/EP
Mission: | Einstein Probe/WXT |
---|---|
Einstein Probe RA: | 172.413° |
Einstein Probe Dec: | -24.683° |
Einstein Probe Err: | 3.0 arcmin |
T0: | 2025-04-21 16:16:28 UT |
Galactic: | 280.26° +34.56° |
Galactic NH: | 4.26× 1020 cm-2 |
Sun distance: | 142.90° |
---|---|
Sun angle: | 9.54 [hr] (East of Sun) |
Moon distance: | 119.44° |
Visibility of this field. | |
First slew: | 2025-04-21 17:51:20 UT |
First observation: | 2025-04-21 17:50:49 UT |
First analysis: | 2025-04-21 23:11:45 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] |
11h 29m 40.80s | -24° 40′ 32.4″ | 2.7′′ * | Good | 2 (O) | 0.6′ | 1.8 ks | The source is 4.0-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] |
11h 29m 40.80s | -24° 40′ 32.4″ | 2.7′′ * | Good | 2 (O) | 0.6′ | 1.8 ks | The source is 4.0-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.