Presumed name: GRB 081008
BAT | 18h 39m 56.88s, -57° 27′ 50.4″ |
---|---|
position: | (279.987, -57.464 ± 180″) |
XRT | 18h 39m 49.92s, -57° 25′ 54.8″ |
position: | (279.95800, -57.43189 ± 1.9″) |
UVOT | No position available. |
Galactic NHI: | 0.00×100 cm-2 |
Galactic E(B-V): | 0.095 mag |
Best RA: | 18h 39m 49.92s | = 279.95800 d |
---|---|---|
Best Dec: | -57° 25′ 54.8″ | = -57.43189 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 |
---|---|---|---|---|---|---|
0.5′′ | 279.95776 | -57.43188 | GCN #8347 | GRB 081008: Enhanced Swift-XRT position | ![]() | |
2.0′′ | 279.95782 | -57.43135 | GCN #8348 | GRB081008: Swift/UVOT observations | ![]() | |
2.7′′ | 279.95683 | -57.43150 | GCN #8372 | GRB 081008: Galaxy associated with z=1.967 absorber | ![]() | |
2.8′′ | 279.95867 | -57.43119 | GCN #8344 | GRB 081008: Swift detection of a burst with optical afterglow | ![]() | |
2.9′′ | 279.95833 | -57.43111 | GCN #8367 | GRB 081008 optical upper limit | ![]() | |
2.9′′ | 279.95833 | -57.43111 | GCN #8343 | GRB 081008: ROTSE-III Detection of Optical Counterpart | ![]() | |
19.8′′ | 279.96800 | -57.43300 | GCN #8351 | GRB 081008� Swift-BAT refined analysis | ![]() |
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 | ||
---|---|---|---|---|---|
20.4 | 279.9683 | -57.4330 | GRB 081008 | ![]() |
* 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 | ||
---|---|---|---|---|---|---|
2.9 | 279.9588 | -57.4311 | NED | ![]() | ||
13.2 | 279.9629 | -57.4293 | I=15.2, R1=15.9 | USNO-B1 | ![]() | |
14.4 | 279.9631 | -57.4290 | I=14.3, R1=14.8 | USNO-B1 | ![]() | |
36.6 | 279.9698 | -57.4398 | B2=19.9, I=17.1, R1=16.3, R2=17.6 | USNO-B1 | ![]() | |
37.8 | 279.9640 | -57.4419 | I=12.0, R1=13.5 | USNO-B1 | ![]() | |
43.5 | 279.9753 | -57.4396 | B2=19.7, I=17.8, R1=19.0, R2=19.1 | USNO-B1 | ![]() | |
43.8 | 279.9536 | -57.4438 | B2=18.3, I=16.7, R1=16.4, R2=17.0 | USNO-B1 | ![]() | |
52.3 | 279.9824 | -57.4381 | B2=19.8, I=18.1, R1=18.4, R2=19.1 | USNO-B1 | ![]() | |
61.5 | 279.9737 | -57.4171 | B2=21.1, R2=20.0 | USNO-B1 | ![]() | |
64.4 | 279.9255 | -57.4281 | B=22.3 | SSS | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 200 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 | ||
---|---|---|---|---|---|
10.7 | 279.9540 | -57.4340 | B2=19.5, I=16.8, R1=17.3, R2=17.7 | USNO-B1 | ![]() |
10.9 | 279.9540 | -57.4340 | h=15.2, j=15.8, k=15.1 | 2MASS | ![]() |
11.5 | 279.9525 | -57.4307 | B2=18.1, I=16.6, R1=16.5, R2=16.9 | USNO-B1 | ![]() |
11.8 | 279.9625 | -57.4297 | h=14.5, j=15.1, k=14.3 | 2MASS | ![]() |
12.0 | 279.9522 | -57.4307 | h=15.6, j=15.9, k=15.8 | 2MASS | ![]() |
12.6 | 279.9616 | -57.4348 | B2=18.6, I=16.9, R1=16.9, R2=17.2 | USNO-B1 | ![]() |
12.9 | 279.9613 | -57.4350 | h=16.0, j=16.6, k=15.8 | 2MASS | ![]() |
15.8 | 279.9634 | -57.4286 | B2=16.8, I=14.9, R1=15.6, R2=15.3 | USNO-B1 | ![]() |
16.7 | 279.9636 | -57.4284 | h=15.1, j=15.4, k=15.1 | 2MASS | ![]() |
28.1 | 279.9587 | -57.4397 | B2=20.7, I=18.3, R1=19.0, R2=19.2 | USNO-B1 | ![]() |
There are 406 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.