Presumed name: GRB 150811A
BAT | 19h 25m 29.04s, -15° 26′ 16.8″ |
---|---|
position: | (291.371, -15.438 ± 180″) |
XRT | 19h 25m 21.40s, -15° 25′ 31.3″ |
position: | (291.33917, -15.42535 ± 3.7″) |
UVOT | No position available. |
Galactic NHI: | 9.61×100 cm-2 |
Galactic E(B-V): | 0.177 mag |
Best RA: | 19h 25m 21.40s | = 291.33917 d |
---|---|---|
Best Dec: | -15° 25′ 31.3″ | = -15.42535 d |
Gal Lat: | -14.35 | |
Gal Long: | 22.71 | |
Sun angle: | 152.02°, -10.1 hr East of Sun |
1Sper #2 auto processing.
Observability of this burst for Swift.
Blink images with DSS (link via GSFC)
SPER results page for this trigger.
There are 2 SPER messages, and 1 objects have been found
See the SPER page for details of how this position was produced.
Click on the offset to view the transient announcement.
Offset (′′) | RA | Dec | Date reported | Source | Misc | Query |
---|---|---|---|---|---|---|
0.0′′ | 291.33917 | -15.42535 | GCN #18119 | GRB 150811A: Swift detection of a burst | ||
0.2′′ | 291.33917 | -15.42531 | GCN #18122 | GRB 150811A: Swift/UVOT Detection | ||
0.3′′ | 291.33913 | -15.42528 | GCN #18134 | GRB 150811A: VLA Detection | ||
0.3′′ | 291.33917 | -15.42527 | GCN #18121 | GRB 150811A: KAIT optical candidate | ||
0.4′′ | 291.33913 | -15.42544 | GCN #18124 | GRB 150811A: Enhanced Swift-XRT position | ||
1.1′′ | 291.33917 | -15.42506 | GCN #18120 | GRB 150811A: RATIR Optical Afterglow Detection | ||
40.3′′ | 291.34708 | -15.43356 | GCN #18129 | GRB 150811A: Swift-BAT refined analysis |
There are 12 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 | ||
---|---|---|---|---|---|
185.4 | 291.3282 | -15.4758 | BD-15 5343 | B=11.28, H=7.035, J=7.707, K=6.872, V=10.04 |
* 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 | ||
---|---|---|---|---|---|---|
5.8 | 291.3401 | -15.4267 | B=19.6, R2=18.3, i=17.8 | SSS | ||
7.7 | 291.3408 | -15.4268 | B=20.2, R2=18.8, i=18.8 | SSS | ||
11.1 | 291.3374 | -15.4279 | I=18.2, R2=19.1 | USNO-B1 | ||
12.7 | 291.3416 | -15.4280 | I=18.5, R1=19.2, R2=19.1 | USNO-B1 | ||
13.1 | 291.3417 | -15.4280 | B=21.3, R2=19.1, i=18.8 | SSS | ||
27.1 | 291.3344 | -15.4313 | B1=19.9, B2=19.3, I=17.1, R1=18.1, R2=17.6 | USNO-B1 | ||
27.4 | 291.3460 | -15.4214 | B2=20.9, I=18.1, R2=18.8 | USNO-B1 | ||
27.6 | 291.3460 | -15.4215 | B=20.8, R2=19.0, i=18.4 | SSS | ||
31.1 | 291.3416 | -15.4170 | B=21.8 | SSS | ||
32.9 | 291.3474 | -15.4299 | B=21.8 | SSS |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 216 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 | ||
---|---|---|---|---|---|
4.9 | 291.3383 | -15.4243 | h=15.1, j=15.5, k=14.8 | 2MASS | |
5.1 | 291.3382 | -15.4243 | B1=18.6, B2=18.5, I=16.2, R1=17.2, R2=17.0 | USNO-B1 | |
5.5 | 291.3401 | -15.4266 | B1=20.2, B2=18.6, I=17.1, R1=18.1, R2=17.1 | USNO-B1 | |
8.0 | 291.3408 | -15.4269 | B1=18.9, B2=18.8, I=17.7, R1=17.3, R2=17.4 | USNO-B1 | |
16.3 | 291.3384 | -15.4209 | B1=19.8, B2=19.2, I=17.4, R1=17.9, R2=18.1 | USNO-B1 | |
22.3 | 291.3367 | -15.4196 | B1=20.5, B2=20.2, R1=18.7, R2=19.0 | USNO-B1 | |
24.7 | 291.3438 | -15.4202 | h=15.5, j=15.8, k=15.3 | 2MASS | |
24.8 | 291.3438 | -15.4201 | B1=18.9, B2=18.5, I=16.7, R1=17.1, R2=17.1 | USNO-B1 | |
26.4 | 291.3456 | -15.4293 | B1=19.9, B2=19.6, I=18.0, R1=18.3, R2=18.3 | USNO-B1 | |
27.1 | 291.3345 | -15.4314 | h=15.8, j=16.1, k=15.3 | 2MASS |
There are 654 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.