TILED_GRB00051
GRB
| Mission: | MAXI | 
|---|---|
| GRB RA: | 219.733° | 
| GRB Dec: | -13.823° | 
| GRB Err: | 30.0 arcmin | 
| T0: | 2016-01-01 00:43:36 UT | 
| Galactic: | 338.78° +41.45° | 
| Galactic NH: | 6.83× 1020 cm-2 | 
| Galactic E(B-V): | 0.09217398 | 
| Sun distance: | 58.36° | 
|---|---|
| Sun angle: | 4.08 [hr](West of Sun) | 
| Moon distance: | 44.62° | 
| Visibility of this field. | |
| First slew: | 2016-01-01 04:31:42 UT | 
| First observation: | 0000-00-00 00:00:00 UT | 
| First analysis: | UT | 
Source 1 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 8 fields have been scheduled for observations. Data are available and processed for 7 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 MAXI pos | Exposure | Notes | Vizier | 
|---|---|---|---|---|---|---|---|---|
| 1 [details] | 14h 38m 36.14s | -13° 48′ 55.5″ | 3.7′′ | Good | 4.8′ | 168 s | The source is brighter than 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 1 sources have been found in the XRT data. 0 sources match catalogued sources.
| # | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 | Dist from MAXI pos | Exposure | Notes | Vizier | 
|---|---|---|---|---|---|---|---|---|
| 1 [details] | 14h 38m 36.14s | -13° 48′ 55.5″ | 3.7′′ | Good | 4.8′ | 168 s | The source is brighter than 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.
 
