TILED_GRB00060
NEWGRB
60
/xrt_products
Mission: | Fermi/LAT |
---|---|
GRB RA: | 157.854° |
GRB Dec: | +61.821° |
GRB Err: | 22.2 arcmin |
T0: | 2016-11-09 06:18:26 UT |
Galactic: | 146.94° +48.26° |
Galactic NH: | 8.22× 1019 cm-2 |
Galactic E(B-V): | 0.008954587 |
Sun distance: | 94.64° |
---|---|
Sun angle: | 4.46 [hr](West of Sun) |
Moon distance: | 127.47° |
Visibility of this field. | |
First slew: | 2016-11-09 17:33:05 UT |
First observation: | 2016-11-09 17:31:07 UT |
First analysis: | UT |
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.
So far 6 sources have been found in the XRT data. 3 sources match catalogued sources.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Dist from LAT pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|
1 [details] |
10h 34m 27.41s | +61° 48′ 22.1″ | 2.7′′ | Good | 21.6′ | 997 s | Matches known X-ray source: XMMSL1 J103425.3+614830 (from XMM-NEWTON/XMMSLEWCLN), 17.3″ away. Matches SIMBAD source: 2MASX J10342739+6148201, 4.8″ away. |
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2 [details] |
10h 31m 37.24s | +61° 53′ 04.4″ | 3.7′′ | Good | 4.1′ | 2.2 ks | ![]() |
|
3 [details] |
10h 29m 50.83s | +61° 46′ 45.8″ | 2.9′′ | Good | 11.4′ | 1.0 ks | Matches known X-ray source: XMMSL1 J102951.3+614632 (from XMM-NEWTON/XMMSLEWCLN), 14.4″ away. Matches SIMBAD source: 2MASS J10295099+6146428, 3.2″ away. |
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4 [details] |
10h 30m 02.79s | +61° 48′ 49.2″ | 4.9′′ | Good | 9.7′ | 1.0 ks | Matches known X-ray source: 1RXH J103003.0+614845 (from ROSAT/ROSHRI), 8.1″ away. | ![]() |
5 [details] |
10h 31m 53.43s | +61° 56′ 21.6″ | 6.4′′ | Reasonable | 7.9′ | 2.2 ks | ![]() |
|
6 [details] |
10h 32m 15.66s | +61° 40′ 31.5″ | 6.9′′ | Good | 10.6′ | 1.9 ks | ![]() |
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.