TILED_GRB00072
NEWGRB
72
/xrt_products
Mission: | MAXI |
---|---|
GRB RA: | 297.793° |
GRB Dec: | -34.663° |
GRB Err: | 30.0 arcmin |
T0: | 2018-08-09 11:38:03 UT |
Galactic: | 5.67° -26.61° |
Galactic NH: | 7.96× 1020 cm-2 |
Galactic E(B-V): | 0.1530784 |
Sun distance: | 153.01° |
---|---|
Sun angle: | 10.57 [hr] (East of Sun) |
Moon distance: | 164.63° |
Visibility of this field. | |
First slew: | 2018-08-09 15:33:36 UT |
First observation: | 2018-08-09 15:26:01 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 6 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] |
19h 51m 36.71s | -34° 47′ 07.5″ | 2.2′′ | Good | 9.1′ | 892 s | The source is 5.1-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 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] |
19h 51m 36.71s | -34° 47′ 07.5″ | 2.2′′ | Good | 9.1′ | 892 s | The source is 5.1-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.