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.