Presumed name: GRB 190219A
BAT | 12h 39m 01.68s, +76° 36′ 50.4″ |
---|---|
position: | (189.757, 76.614 ± 180″) |
XRT | 12h 38m 30.31s, +76° 36′ 45.7″ |
position: | (189.6263, 76.6127 ± 2.1″) |
UVOT | No position available. |
Galactic NHI: | 3.12×100 cm-2 |
Galactic E(B-V): | 0.040 mag |
Best RA: | 12h 38m 30.31s | = 189.6263 d |
---|---|---|
Best Dec: | +76° 36′ 45.7″ | = 76.6127 d |
Gal Lat: | 40.49 | |
Gal Long: | 123.92 | |
Sun angle: | 111.78°, 9.5 hr West |
1Sper #7 auto processing.
Observability of this burst for Swift.
No UVOT images are currently available.
SPER results page for this trigger.
There are 9 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 |
---|---|---|---|---|---|---|
0.4′′ | 189.62640 | 76.61280 | GCN #23903 | GRB 190219A: Prompt enhanced Swift-XRT position | ![]() | |
0.4′′ | 189.62654 | 76.61261 | GCN #23907 | GRB 190219A: Enhanced Swift-XRT position | ![]() | |
0.5′′ | 189.62637 | 76.61283 | GCN #23905 | GRB190219A: MASTER Global Robotic Net optical observation | ![]() | |
0.9′′ | 189.62633 | 76.61295 | GCN #23911 | GRB 190219A: NOT optical afterglow candidate | ![]() | |
3.4′′ | 189.62442 | 76.61186 | GCN #23902 | GRB 190219A: Swift detection of a burst | ![]() | |
55.3′′ | 189.68600 | 76.60600 | GCN #23913 | GRB 190219A: 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 | ||
---|---|---|---|---|---|
79.6 | 189.5521 | 76.6266 | 2MASX J12381241+7637358 | G=18.0321, H=12.679, J=13.340, K=12.312 | ![]() |
* 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 | 189.6323 | 76.6123 | B=21.8, R=19.6 | APM-N | ![]() | |
26.2 | 189.6168 | 76.6058 | B1=20.9, B2=21.0, R2=19.8 | USNO-B1 | ![]() | |
30.1 | 189.5925 | 76.6158 | NED | ![]() | ||
31.1 | 189.6396 | 76.6046 | B=21.8, R=19.7 | APM-N | ![]() | |
35.4 | 189.6245 | 76.6029 | B=21.5, R=20.0 | APM-N | ![]() | |
47.2 | 189.6824 | 76.6110 | R1=18.9, R2=20.1 | USNO-B1 | ![]() | |
58.1 | 189.5891 | 76.5990 | B=21.5, R=17.9 | APM-N | ![]() | |
58.9 | 189.6032 | 76.6282 | B=21.8, R=19.5 | APM-N | ![]() | |
59.8 | 189.6980 | 76.6126 | B2=20.9, I=18.7, R2=19.1 | USNO-B1 | ![]() | |
65.2 | 189.5720 | 76.6257 | B=21.8, R=20.0 | APM-N | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 78 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 | ||
---|---|---|---|---|---|
2.4 | 189.6291 | 76.6128 | B2=21.3, R1=20.2 | USNO-B1 | ![]() |
23.8 | 189.6002 | 76.6100 | B2=20.7, I=18.7, R1=19.7, R2=19.9 | USNO-B1 | ![]() |
24.0 | 189.6005 | 76.6098 | B2=21.3, I=18.9 | USNO-B1 | ![]() |
25.6 | 189.6177 | 76.6059 | B2=20.8, R1=20.2, R2=19.9 | USNO-B1 | ![]() |
30.6 | 189.5918 | 76.6156 | h=14.3, j=14.6, k=14.2 | 2MASS | ![]() |
30.9 | 189.5915 | 76.6156 | B1=16.2, B2=15.8, I=15.5, R1=15.0, R2=15.2 | USNO-B1 | ![]() |
57.5 | 189.5899 | 76.5992 | B2=20.3, I=17.9, R1=18.2, R2=18.0 | USNO-B1 | ![]() |
60.4 | 189.6987 | 76.6128 | B2=21.1, I=18.6, R1=19.0, R2=19.2 | USNO-B1 | ![]() |
64.2 | 189.6222 | 76.5949 | B2=21.7, I=18.4, R1=19.7, R2=19.7 | USNO-B1 | ![]() |
68.1 | 189.5951 | 76.6302 | B1=19.1, B2=19.0, I=18.1, R1=18.5, R2=18.5 | USNO-B1 | ![]() |
There are 52 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.