Presumed name: GRB 220305A
BAT | 07h 10m 20.16s, -37° 42′ 28.8″ |
---|---|
position: | (107.584, -37.708 ± 180″) |
XRT | 07h 10m 23.62s, -37° 40′ 48.6″ |
position: | (107.59841, -37.68016 ± 3.8″) |
UVOT | No position available. |
Galactic NHI: | 1.50×1021 cm-2 |
Galactic E(B-V): | 0.305 mag |
Best RA: | 07h 10m 23.62s | = 107.59841 d |
---|---|---|
Best Dec: | -37° 40′ 48.6″ | = -37.68016 d |
Gal Lat: | -12.74 | |
Gal Long: | 248.97 | |
Sun angle: | 110.40°, -8.1 hr East of Sun |
Observability of this burst for Swift.
No UVOT images are currently available.
SPER results page for this trigger.
There are 12 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′′ | 107.59841 | -37.68016 | GCN #31685 | GRB 220305A: Swift-XRT observations | ![]() | |
0.7′′ | 107.59853 | -37.68033 | GCN #31688 | GRB 220305A: Enhanced Swift-XRT position | ![]() | |
87.1′′ | 107.61000 | -37.70256 | GCN #31698 | GRB 220305A: Swift-BAT refined analysis | ![]() | |
108.3′′ | 107.58400 | -37.70800 | GCN #31684 | GRB 220305A: Swift detection of a burst | ![]() |
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 | ||
---|---|---|---|---|---|
74.8 | 107.6181 | -37.6665 | TYC 7630-863-1 | B=13.38, G=12.166514, H=10.946, J=11.136, K=10.869, V=12.26 | ![]() |
141.6 | 107.6271 | -37.6481 | TYC 7630-874-1 | B=12.83, G=11.991081, H=10.148, J=10.615, K=10.071, V=12.25 | ![]() |
147.5 | 107.6186 | -37.6424 | TYC 7630-877-1 | B=12.32, G=12.069963, H=11.194, J=11.288, K=11.138, V=12.11 | ![]() |
There are 3 SIMBAD objects within the position error. The full list is here.
* 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 | ||
---|---|---|---|---|---|---|
5.2 | 107.5988 | -37.6817 | NED | ![]() | ||
10.6 | 107.5955 | -37.6784 | B2=18.1, I=17.2, R1=16.7, R2=17.8 | USNO-B1 | ![]() | |
10.7 | 107.5954 | -37.6784 | B=19.0, R2=17.9, i=17.2 | SSS | ![]() | |
10.8 | 107.5954 | -37.6783 | NED | ![]() | ||
13.5 | 107.6029 | -37.6806 | NED | ![]() | ||
13.9 | 107.6033 | -37.6808 | NED | ![]() | ||
20.3 | 107.5934 | -37.6762 | B=19.6, R2=18.4, i=17.8 | SSS | ![]() | |
20.7 | 107.6050 | -37.6825 | NED | ![]() | ||
21.1 | 107.6050 | -37.6825 | NED | ![]() | ||
21.7 | 107.5929 | -37.6758 | NED | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 303 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 | ||
---|---|---|---|---|---|
5.0 | 107.5988 | -37.6815 | B2=19.6, I=18.0, R1=17.9, R2=18.6 | USNO-B1 | ![]() |
10.8 | 107.5952 | -37.6785 | B2=19.3, I=17.2, R1=17.6, R2=17.2 | USNO-B1 | ![]() |
13.5 | 107.6031 | -37.6806 | h=14.7, j=15.4, k=14.5 | 2MASS | ![]() |
13.5 | 107.6031 | -37.6806 | B2=19.4, I=16.8, R1=17.3, R2=17.7 | USNO-B1 | ![]() |
19.6 | 107.6007 | -37.6750 | B2=19.9, I=18.3, R1=18.5, R2=19.1 | USNO-B1 | ![]() |
20.9 | 107.5932 | -37.6760 | B2=18.2, I=16.6, R1=16.9, R2=17.3 | USNO-B1 | ![]() |
21.1 | 107.6052 | -37.6826 | h=15.1, j=15.9, k=14.8 | 2MASS | ![]() |
21.2 | 107.6052 | -37.6825 | B2=19.6, I=17.3, R1=18.1, R2=18.2 | USNO-B1 | ![]() |
21.9 | 107.5930 | -37.6758 | B2=18.6, I=16.8, R1=16.9, R2=17.4 | USNO-B1 | ![]() |
23.2 | 107.6053 | -37.6767 | B2=20.7, I=18.6, R1=19.5, R2=18.7 | USNO-B1 | ![]() |
There are 315 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.