TILED_GRB00050
GRB
Mission: | MAXI |
---|---|
GRB RA: | 68.109° |
GRB Dec: | -3.775° |
GRB Err: | 30.0 arcmin |
T0: | 2015-12-12 14:00:11 UT |
Galactic: | 199.17° -32.43° |
Galactic NH: | 3.98× 1020 cm-2 |
Galactic E(B-V): | 0.04778237 |
Sun distance: | 150.99° |
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Sun angle: | 11.25 [hr](East of Sun) |
Moon distance: | 146.09° |
Visibility of this field. | |
First slew: | 2015-12-12 16:12:07 UT |
First observation: | 2015-12-12 16:11:57 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 9 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] |
04h 32m 36.50s | -03° 57′ 41.3″ | 5.2′′ | Good | 11.5′ | 157 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] |
04h 32m 36.50s | -03° 57′ 41.3″ | 5.2′′ | Good | 11.5′ | 157 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.