Presumed name: GRB 190123A
BAT | 03h 32m 54.96s, +45° 29′ 02.4″ |
---|---|
position: | (53.229, 45.484 ± 180″) |
XRT | 03h 32m 52.97s, +45° 31′ 27.3″ |
position: | (53.22071, 45.52425 ± 4.0″) |
UVOT | No position available. |
Galactic NHI: | 3.02×100 cm-2 |
Galactic E(B-V): | 0.433 mag |
Best RA: | 03h 32m 52.97s | = 53.22071 d |
---|---|---|
Best Dec: | +45° 31′ 27.3″ | = 45.52425 d |
Gal Lat: | -8.61 | |
Gal Long: | 150.25 | |
Sun angle: | 116.26°, -7.2 hr East of Sun |
1Sper #1 auto processing.
Observability of this burst for Swift.
No UVOT images are currently available.
SPER results page for this trigger.
There are 1 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′′ | 53.22071 | 45.52425 | GCN #23769 | GRB 190123A: Swift detection of a burst | ![]() | |
0.0′′ | 53.22071 | 45.52425 | GCN #23770 | GRB 190123A: MASTER Global Robotic Net optical observation | ![]() | |
3.8′′ | 53.22058 | 45.52531 | GCN #23771 | GRB 190123A: Enhanced Swift-XRT position | ![]() | |
134.5′′ | 53.17500 | 45.50500 | GCN #23780 | GRB 190123A: Swift-BAT refined analysis | ![]() |
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 | ||
---|---|---|---|---|---|
153.4 | 53.2238 | 45.5668 | 2MASS J03325370+4534004 | G=13.5072, H=10.634, J=11.283, K=10.447 | ![]() |
177.8 | 53.1692 | 45.5580 | BD+45 779B | B=11.11, G=10.8331, H=10.318, J=10.355, K=10.259, V=10.84 | ![]() |
* 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 | ||
---|---|---|---|---|---|---|
9.6 | 53.2171 | 45.5251 | B2=20.1, R2=19.6 | USNO-B1 | ![]() | |
12.4 | 53.2165 | 45.5261 | B2=21.0, I=18.6, R1=19.6, R2=19.1 | USNO-B1 | ![]() | |
27.1 | 53.2232 | 45.5169 | B2=21.4, I=18.3, R1=19.4, R2=19.0 | USNO-B1 | ![]() | |
27.5 | 53.2230 | 45.5168 | I=18.1, R1=19.3 | USNO-B1 | ![]() | |
32.2 | 53.2232 | 45.5330 | B1=19.9, B2=20.7, I=18.5, R2=19.7 | USNO-B1 | ![]() | |
32.6 | 53.2332 | 45.5267 | I=18.8, R2=20.3 | USNO-B1 | ![]() | |
45.2 | 53.2100 | 45.5343 | B1=21.0, B2=20.9, I=18.9, R1=19.5, R2=20.0 | USNO-B1 | ![]() | |
48.5 | 53.2093 | 45.5351 | B1=20.4, R1=19.4 | USNO-B1 | ![]() | |
54.2 | 53.2335 | 45.5122 | I=18.3, R2=20.3 | USNO-B1 | ![]() | |
58.7 | 53.2435 | 45.5275 | B1=20.6, I=19.0, R2=19.1 | USNO-B1 | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 84 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 | ||
---|---|---|---|---|---|
7.5 | 53.2178 | 45.5243 | B2=20.2, I=18.3, R1=18.7, R2=19.1 | USNO-B1 | ![]() |
12.0 | 53.2167 | 45.5225 | B1=19.8, B2=19.4, I=17.9, R1=18.4, R2=18.4 | USNO-B1 | ![]() |
14.2 | 53.2263 | 45.5247 | B1=17.9, B2=17.7, I=16.2, R1=16.6, R2=16.7 | USNO-B1 | ![]() |
14.3 | 53.2264 | 45.5246 | h=15.1, j=15.6, k=15.4 | 2MASS | ![]() |
22.8 | 53.2245 | 45.5300 | h=15.4, j=15.8, k=15.3 | 2MASS | ![]() |
23.3 | 53.2118 | 45.5225 | B2=21.1, I=16.5, R1=18.5, R2=18.7 | USNO-B1 | ![]() |
23.3 | 53.2118 | 45.5224 | h=14.4, j=15.0, k=14.1 | 2MASS | ![]() |
23.5 | 53.2243 | 45.5303 | B1=18.4, B2=18.2, I=16.3, R1=16.9, R2=16.6 | USNO-B1 | ![]() |
25.6 | 53.2156 | 45.5181 | B1=20.1, B2=19.4, I=17.7, R1=17.9, R2=17.6 | USNO-B1 | ![]() |
25.9 | 53.2157 | 45.5179 | h=15.7, j=16.4, k=15.8 | 2MASS | ![]() |
There are 409 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.