TILED_GRB00088
NEWGRB
88
/xrt_products
Mission: | Fermi/LAT |
---|---|
GRB RA: | 262.690° |
GRB Dec: | +10.420° |
GRB Err: | 15.6 arcmin |
T0: | 2020-02-19 23:56:45 UT |
Galactic: | 33.33° +22.60° |
Galactic NH: | 8.07× 1020 cm-2 |
Galactic E(B-V): | 0.152495 |
Sun distance: | 73.00° |
---|---|
Sun angle: | 4.68 [hr](West of Sun) |
Moon distance: | 43.82° |
Visibility of this field. |
Source 2 has been manually confirmed as the GRB afterglow; data for this object are now available through the main GRB results area for this GRB.
So far 3 fields have been scheduled for observations. Data are available and processed for 4 of these. The list gives the exposure time used in source detection. If any individual sources were selected for follow-up observations, the source detection is not repeated for the follow up observations and the table below is not updated.
A source was found which matches the afterglow criteria.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Dist from LAT pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|
2 [details] |
17h 30m 02.16s | +10° 32′ 21.6″ | 2.1′′ | Good | 12.9′ | 2.4 ks | The source is 9.3-σ above the RASS limit. |
1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the 1SXPS documentation.
* 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 2 sources have been found in the XRT data. 0 sources match catalogued sources.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Dist from LAT pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|
1 [details] |
17h 30m 58.79s | +10° 19′ 38.9″ | 5.6′′ | Poor | 6.4′ | 2.4 ks | ||
2 [details] |
17h 30m 02.16s | +10° 32′ 21.6″ | 2.1′′ | Good | 12.9′ | 2.4 ks | The source is 9.3-σ above the RASS limit. |
1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the 1SXPS documentation.
* 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.