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GRB 250416C (EP250416a): Swift observation summary

This is a confirmed GRB (GRB 250416C), the afterglow is source 1 -- please see the GRB results at https://www.swift.ac.uk/xrt_products/00019721 for updated analysis

.
Mission:Einstein Probe/WXT
Einstein Probe RA:256.402°
Einstein Probe Dec:+25.768°
Einstein Probe Err:3.1 arcmin
T0:2025-04-16 17:53:59 UT
Galactic:47.13° +33.73°
Galactic NH:3.78× 1020 cm-2
Sun distance:118.15°
Sun angle:8.56 [hr] (West of Sun)
Moon distance:53.37°
Visibility of this field.
Data analysed so far:
  • ObsID: 00019721001 with 2.0 ks exposure.
  • ObsID: 00019721002 with 1.9 ks exposure.

About tiled field analysis.

So far 1 fields have been scheduled for observations. Data are available and processed for 1 of these.

Details of afterglow candidates

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]
17h 05m 40.92s +25° 46′ 32.3″ 4.0′′ * Good 2 (O) 1.1′ 4.0 ks The source is 3.9-σ above the RASS limit. Vizier logo

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.


Find an upper limit.

Sources found so far

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]
17h 05m 40.92s +25° 46′ 32.3″ 4.0′′ * Good 2 (O) 1.1′ 4.0 ks The source is 3.9-σ above the RASS limit. Vizier logo
2
[details]
17h 06m 20.72s +25° 39′ 11.4″ 7.2′′ Reasonable 3 (U) 12.1′ 2.9 ks Vizier logo
3
[details]
17h 06m 20.88s +25° 54′ 46.3″ 9.9′′ Poor 3 (U) 13.2′ 1.9 ks Vizier logo

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.


Image

Select image style: Draggable PNG | JS9.

FITS image.

Image of all observations processed so far

Exposure map

FITS exposure map.

Exposure map of all observations processed so far