Presumed name: GRB 091020
BAT | 11h 42m 51.60s, +50° 58′ 19.2″ |
---|---|
position: | (175.715, +50.972 ± 180″) |
XRT | 11h 42m 55.20s, +50° 58′ 41.9″ |
position: | (175.7300, 50.9783 ± 2.1″) |
UVOT | No position available. |
Galactic NHI: | 0.00×100 cm-2 |
Galactic E(B-V): | 0.017 mag |
Best RA: | 11h 42m 55.20s | = 175.7300 d |
---|---|---|
Best Dec: | +50° 58′ 41.9″ | = 50.9783 d |
Gal Lat: | ||
Gal Long: | ||
Sun angle: | not found |
Observability of this burst for Swift.
Blink images with DSS (link via GSFC)
SPER results page for this trigger.
No SPER data received yet. Refresh this page to check again.
Click on the offset to view the transient announcement.
Offset (′′) | RA | Dec | Date reported | Source | Misc | Query |
---|---|---|---|---|---|---|
0.1′′ | 175.73000 | 50.97833 | GCN #10054 | GRB091020 Swift/UVOT observations | ![]() | |
0.2′′ | 175.72992 | 50.97831 | GCN #10048 | GRB 091020: Swift detection of a burst with an optical afterglow | ![]() | |
0.3′′ | 175.73004 | 50.97839 | GCN #10050 | GRB 091020: Enhanced Swift-XRT position | ![]() | |
0.8′′ | 175.73028 | 50.97816 | GCN #10088 | Radio afterglow detection from GRB 091020 | ![]() | |
8.3′′ | 175.72700 | 50.97700 | GCN #10051 | GRB 091020� Swift-BAT refined analysis | ![]() | |
142.3′′ | 175.70500 | 51.01456 | GCN #10076 | GRB 091020: Early TLS Multicolor detections� red afterglow | ![]() |
There are 13 matches in total. See the full table for details.
Click on the distance to view the full details (not available for sources from the SSS catalogue). Click on the column headers to sort the table on that column (click again to invert sort order).
RA* | Dec* | SIMBAD name | Query | ||
---|---|---|---|---|---|
0.1 | 175.7300 | 50.9783 | GRB 091020 | ![]() | |
172.6 | 175.6590 | 50.9610 | 2MASS J11423814+5057396 | B=19.8, H=13.48, I=15.5, J=14.08, K=13.26, R=18.0 | ![]() |
* RA/Dec in equinox J2000
RA* | Dec* | Source table2 | Observatory | Query |
---|
Queried the X-ray MASTER catalogue.
* RA/Dec in equinox J2000
1Energy band for count-rate is mission specific.
RA* | Dec* | Redshift | Catalogue | Query | ||
---|---|---|---|---|---|---|
0.2 | 175.7300 | 50.9783 | NED | ![]() | ||
11.2 | 175.7337 | 50.9761 | Mag=20.9 | NED | ![]() | |
11.3 | 175.7256 | 50.9797 | B2=18.7, I=19.3 | USNO-B1 | ![]() | |
18.2 | 175.7379 | 50.9783 | Mag=21.9 | NED | ![]() | |
18.3 | 175.7381 | 50.9782 | R=20.6, g=21.8, i=20.1, u=22.3, z=19.9 | SDSS | ![]() | |
23.8 | 175.7237 | 50.9728 | Mag=23.1 | NED | ![]() | |
27.3 | 175.7326 | 50.9709 | R=24.5, g=24.2, i=21.7, u=25.8, z=22.9 | SDSS | ![]() | |
29.0 | 175.7208 | 50.9842 | Mag=23.3 | NED | ![]() | |
31.5 | 175.7163 | 50.9772 | Mag=23.9 | NED | ![]() | |
31.5 | 175.7162 | 50.9773 | R=21.7, g=24.6, i=20.7, u=24.6, z=20.0 | SDSS | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 426 galaxies within the position error. The full list is here.
* RA/Dec in equinox J2000
Magnitudes depend on the catalogue. e.g. For Sloan, R is the Sloan r mag, not the Johnson R from APM, for example
RA* | Dec* | Catalogue | Query | ||
---|---|---|---|---|---|
7.8 | 175.7318 | 50.9801 | I=21.3, R=23.2, g=25.6, u=25.8, z=20.4 | SDSS | ![]() |
10.5 | 175.7334 | 50.9763 | B1=20.6, B2=21.0, R1=20.2, R2=19.9 | USNO-B1 | ![]() |
11.2 | 175.7336 | 50.9762 | I=20.5, R=20.6, g=20.9, u=21.5, z=20.3 | SDSS | ![]() |
18.0 | 175.7379 | 50.9783 | B2=20.4, R2=20.0 | USNO-B1 | ![]() |
23.8 | 175.7240 | 50.9729 | I=21.8, R=22.1, g=23.1, u=23.2, z=21.3 | SDSS | ![]() |
24.4 | 175.7194 | 50.9797 | I=22.4, R=24.8, g=26.2, u=25.8, z=23.1 | SDSS | ![]() |
28.3 | 175.7298 | 50.9862 | I=22.1, R=24.0, g=25.7, u=24.9, z=23.6 | SDSS | ![]() |
29.0 | 175.7211 | 50.9841 | I=21.9, R=22.8, g=23.4, u=25.1, z=21.8 | SDSS | ![]() |
30.1 | 175.7428 | 50.9805 | I=18.3, R1=19.8 | USNO-B1 | ![]() |
35.7 | 175.7410 | 50.9712 | B2=21.0, I=19.2, R1=19.7 | USNO-B1 | ![]() |
There are 166 stars within the position error. The full list is here.
* RA/Dec in equinox J2000
Magnitudes depend on the catalogue. e.g. For Sloan, R is the Sloan r mag, not the Johnson R from APM, for example.