Presumed name: GRB 190324A
BAT | 03h 18m 18.24s, -47° 14′ 20.4″ |
---|---|
position: | (49.576, -47.239 ± 180″) |
XRT | 03h 18m 28.93s, -47° 12′ 44.6″ |
position: | (49.62054, -47.21240 ± 3.7″) |
UVOT | 03h 18m 27.72s, -47° 12′ 52.6″ |
position: | (49.6155, -47.2146 ± 0.8″) |
Galactic NHI: | 1.66×100 cm-2 |
Galactic E(B-V): | 0.017 mag |
Best RA: | 03h 18m 27.72s | = 49.6155 d |
---|---|---|
Best Dec: | -47° 12′ 52.6″ | = -47.2146 d |
Gal Lat: | -54.98 | |
Gal Long: | 257.83 | |
Sun angle: | 63.18°, -3.1 hr East of Sun |
1Sper #5 auto processing.
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 |
---|---|---|---|---|---|---|
0.2′′ | 49.61558 | -47.21461 | GCN #24014 | GRB 190324A: Swift/UVOT Observations | ![]() | |
0.3′′ | 49.61550 | -47.21469 | GCN #23996 | GRB 190324A: Swift/UVOT afterglow candidate | ![]() | |
1.3′′ | 49.61588 | -47.21486 | GCN #24001 | GRB 190324A: Enhanced Swift-XRT position | ![]() | |
14.7′′ | 49.62054 | -47.21240 | GCN #23997 | GRB 190324A: Swift-XRT observations | ![]() | |
31.4′′ | 49.60333 | -47.21178 | GCN #24007 | GRB 190324A: Swift-BAT refined analysis | ![]() | |
130.5′′ | 49.57600 | -47.23900 | GCN #23995 | SWIFT GRB190324.95 Global MASTER-Net observations report | ![]() | |
130.5′′ | 49.57600 | -47.23900 | GCN #23993 | GRB 190324A: Swift detection of a burst | ![]() |
There are 11 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 | ||
---|---|---|---|---|---|
87.6 | 49.6350 | -47.2350 | LEDA 504547 | ![]() |
* 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 | ||
---|---|---|---|---|---|---|
23.6 | 49.6203 | -47.2203 | B=20.0, R2=18.4, i=17.5 | SSS | ![]() | |
23.9 | 49.6206 | -47.2203 | B2=18.6, I=17.5, R1=19.2, R2=18.1 | USNO-B1 | ![]() | |
24.4 | 49.6204 | -47.2206 | Mag=19.94 | NED | ![]() | |
32.6 | 49.6145 | -47.2056 | B=18.6 | SSS | ![]() | |
34.3 | 49.6167 | -47.2242 | Mag=19.3 | NED | ![]() | |
45.1 | 49.6015 | -47.2228 | B=22.5 | SSS | ![]() | |
47.1 | 49.6039 | -47.2042 | B=22.6 | SSS | ![]() | |
47.9 | 49.6037 | -47.2039 | Mag=19.3 | NED | ![]() | |
47.9 | 49.5958 | -47.2139 | Mag=19.3 | NED | ![]() | |
49.7 | 49.6289 | -47.2250 | B2=21.1, I=18.2, R2=22.1 | USNO-B1 | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 95 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 | ||
---|---|---|---|---|---|
47.1 | 49.6039 | -47.2041 | B2=23.5, R2=21.6 | USNO-B1 | ![]() |
48.0 | 49.5959 | -47.2138 | h=14.7, j=15.3, k=14.6 | 2MASS | ![]() |
48.0 | 49.5959 | -47.2138 | B2=18.1, I=16.2, R1=16.4, R2=16.4 | USNO-B1 | ![]() |
49.6 | 49.6284 | -47.2252 | h=16.6, j=17.2, k=15.5 | 2MASS | ![]() |
49.8 | 49.6284 | -47.2253 | B2=21.8, I=18.3, R1=19.5, R2=19.5 | USNO-B1 | ![]() |
50.1 | 49.6092 | -47.2278 | B2=22.8, R1=20.6, R2=21.0 | USNO-B1 | ![]() |
50.8 | 49.6294 | -47.2041 | B2=21.9, R2=23.5 | USNO-B1 | ![]() |
54.9 | 49.6349 | -47.2069 | B2=18.3, I=16.9, R1=17.2, R2=16.5 | USNO-B1 | ![]() |
54.9 | 49.6348 | -47.2068 | h=15.8, j=16.3, k=14.9 | 2MASS | ![]() |
56.2 | 49.6354 | -47.2068 | B2=18.2, R2=17.5 | USNO-B1 | ![]() |
There are 84 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.