NEUTRINO_FIELD00007
NEUTRINO
7
/neutrino
Mission: | IceCube |
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Neutrino RA: | 77.285° |
Neutrino Dec: | +5.752° |
Neutrino Err: | 0.8 deg |
T0: | 2017-09-22 20:54:25 UT |
Galactic: | 195.31° -19.67° |
Galactic NH: | 1.08× 1021 cm-2 |
Sun distance: | 102.69° |
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Sun angle: | 6.85 [hr](West of Sun) |
Moon distance: | 134.23° |
Visibility of this field. | |
First slew: | 2017-09-23 00:15:54 UT |
First observation: | 2017-09-23 00:08:11 UT |
First analysis: | 2023-03-22 12:06:07 UT |
So far 21 fields have been scheduled for observations. Data are available and processed for 19 of these.
2 sources were found which matches the afterglow criteria.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Rank3 | Exposure | Notes | Vizier | |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
05h 09m 26.34s | +05° 41′ 34.2″ | 2.0′′ * | Good | 2 (O) | 5.7′ | 85.0 ks | Matches SIMBAD source: QSO J0509+0541, 0.3″ away. Matches known X-ray source: 2SXPS J050925.9+054135 (from 2SXPS), 0.5″ away. |
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2 [details] |
05h 09m 42.92s | +05° 46′ 57.4″ | 2.6′′ * | Good | 2 (O) | 8.8′ | 85.0 ks | Matches SIMBAD source: HD 33326, 2.4″ away. Matches known X-ray source: 2SXPS J050942.4+054656 (from 2SXPS), 2.4″ away. |
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1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the LSXPS documentation.
3 T=Transient Source, O=Outbursting known source, U=Uncatalogued X-ray source, K=Known X-ray source.
* The position was enhanced using astrometry derived from the Swift UVOT.So far 11 sources have been found in the XRT data. 10 sources match catalogued sources.
# | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2 |
Rank3 | Dist from IceCube pos |
Exposure | Notes | Vizier |
---|---|---|---|---|---|---|---|---|---|
1 [details] |
05h 09m 26.34s | +05° 41′ 34.2″ | 2.0′′ * | Good | 2 (O) | 5.7′ | 85.0 ks | Matches SIMBAD source: QSO J0509+0541, 0.3″ away. Matches known X-ray source: 2SXPS J050925.9+054135 (from 2SXPS), 0.5″ away. |
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2 [details] |
05h 09m 42.92s | +05° 46′ 57.4″ | 2.6′′ * | Good | 2 (O) | 8.8′ | 85.0 ks | Matches SIMBAD source: HD 33326, 2.4″ away. Matches known X-ray source: 2SXPS J050942.4+054656 (from 2SXPS), 2.4″ away. |
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3 [details] |
05h 06m 53.58s | +06° 06′ 55.9″ | 4.5′′ | Good | 4 (K) | 40.0′ | 679 s | Matches SIMBAD source: TYC 110-755-1, 1.1″ away. Matches known X-ray source: 2SXPS J050653.5+060654 (from 2SXPS), 1.1″ away. |
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4 [details] |
05h 08m 58.03s | +06° 26′ 29.4″ | 5.7′′ | Good | 4 (K) | 41.4′ | 689 s | Matches known X-ray source: 2SXPS J050857.9+062627 (from 2SXPS), 2.2″ away. | ![]() |
5 [details] |
05h 10m 24.90s | +06° 13′ 42.0″ | 5.8′′ | Reasonable | 3 (U) | 34.3′ | 762 s | Matches SIMBAD source: TYC 111-1516-1, 4.9″ away. | ![]() |
6 [details] |
05h 10m 39.07s | +05° 54′ 30.5″ | 5.4′′ | Good | 4 (K) | 24.4′ | 1.6 ks | Matches SIMBAD source: 1RXS J051038.6+055432, 4.3″ away. Matches known X-ray source: 2SXPS J051038.9+055427 (from 2SXPS), 2.9″ away. |
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7 [details] |
05h 08m 33.54s | +05° 31′ 10.2″ | 5.4′′ | Good | 4 (K) | 16.4′ | 804 s | Matches SIMBAD source: 3HSP J050833.4+053109, 3.9″ away. Matches known X-ray source: 2SXPS J050833.4+053110 (from 2SXPS), 1.2″ away. |
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8 [details] |
05h 08m 37.07s | +05° 12′ 15.7″ | 5.8′′ | Good | 4 (K) | 33.8′ | 814 s | This source may be affected by optical loading
Matches known X-ray source: XMMSL2 J050836.8+051224 (from XMM-NEWTON/XMMSLEWCLN), 8.90806790366183″ away. |
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9 [details] |
05h 09m 45.03s | +05° 21′ 53.0″ | 5.9′′ | Good | 4 (K) | 25.0′ | 804 s | Matches known X-ray source: 2SXPS J050944.9+052149 (from 2SXPS), 3.6″ away. | ![]() |
10 [details] |
05h 11m 28.53s | +05° 38′ 34.8″ | 3.4′′ * | Good | 4 (K) | 35.5′ | 6.4 ks | Matches SIMBAD source: PMN J0511+0538, 8.5″ away. Matches known X-ray source: 2SXPS J051127.9+053834 (from 2SXPS), 5.6″ away. |
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11 [details] |
05h 11m 05.47s | +05° 19′ 43.4″ | 8.5′′ | Poor | 3 (U) | 38.6′ | 754 s | ![]() |
1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the LSXPS documentation.
3 T=Transient Source, O=Outbursting known source, U=Uncatalogued X-ray source, K=Known X-ray source.
* The position was enhanced using astrometry derived from the Swift UVOT.Select image style: Draggable PNG | JS9.