EP_FIELD00085
EP
85
/EP
| Mission: | Einstein Probe/WXT |
|---|---|
| Einstein Probe RA: | 101.041° |
| Einstein Probe Dec: | +27.394° |
| Einstein Probe Err: | 3.1 arcmin |
| T0: | 2025-11-30 11:07:49 UT |
| Galactic: | 187.48° +10.65° |
| Galactic NH: | 1.30× 1021 cm-2 |
| Sun distance: | 148.05° |
|---|---|
| Sun angle: | 9.69 [hr](West of Sun) |
| Moon distance: | 94.19° |
| Visibility of this field. | |
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] |
06h 44m 04.96s | +27° 23′ 02.8″ | 3.1′′ * | Good | 1 (T) | 1.2′ | 2.0 ks | The source is 3.5-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 3 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] |
06h 44m 04.96s | +27° 23′ 02.8″ | 3.1′′ * | Good | 1 (T) | 1.2′ | 2.0 ks | The source is 3.5-σ above the RASS limit. | ![]() |
| 2 [details] |
06h 43m 39.45s | +27° 23′ 25.5″ | 9.0′′ * | Good | 3 (U) | 6.7′ | 2.0 ks | ![]() |
|
| 3 [details] |
06h 43m 43.88s | +27° 29′ 14.3″ | 7.2′′ | Good | 3 (U) | 8.0′ | 2.0 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.