TILED_GRB00090
NEWGRB
90
/xrt_products
Mission: | MAXI |
---|---|
GRB RA: | 17.230° |
GRB Dec: | -50.745° |
GRB Err: | 1.5 deg |
T0: | 2020-05-17 11:26:56 UT |
Galactic: | 296.08° -66.15° |
Galactic NH: | 1.58× 1020 cm-2 |
Galactic E(B-V): | 0.01115602 |
Sun distance: | 77.59° |
---|---|
Sun angle: | 2.50 [hr](West of Sun) |
Moon distance: | 47.52° |
Visibility of this field. |
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.
An additional 1 field has also been used for follow up observations. These data are not searched for sources, but are used to update the light curves etc of any sources already found.
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] |
01h 10m 47.28s | -50° 55′ 24.1″ | 4.1′′ | Good | 20.7′ | 4.4 ks | The source is fading with 4.8-σ significance. The source is 7.3-σ above the RASS limit. |
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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] |
01h 10m 47.28s | -50° 55′ 24.1″ | 4.1′′ | Good | 20.7′ | 4.4 ks | The source is fading with 4.8-σ significance. The source is 7.3-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.