Presumed name: GRB 121212A
BAT | 11h 51m 21.84s, +78° 02′ 02.4″ |
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position: | (177.841, 78.034 ± 180″) |
XRT | 11h 51m 10.18s, +78° 02′ 14.6″ |
position: | (177.7924, 78.0374 ± 2.0″) |
UVOT | No position available. |
Galactic NHI: | 3.67×1020 cm-2 |
Galactic E(B-V): | NED unavailable |
Best RA: | 11h 51m 10.18s | = 177.7924 d |
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Best Dec: | +78° 02′ 14.6″ | = 78.0374 d |
Gal Lat: | 38.62 | |
Gal Long: | 126.89 | |
Sun angle: | 110.89°, 5.5 hr West |
1Sper #10 auto processing.
Observability of this burst for Swift.
Blink images with DSS (link via GSFC)
SPER results page for this trigger.
There are 10 SPER messages, and 2 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′′ | 177.79258 | 78.03736 | GCN #14082 | GRB121212A: NOT optical imaging | ![]() | |
0.5′′ | 177.79292 | 78.03731 | GCN #14069 | GRB121212A: Swift/UVOT Detection | ![]() | |
0.7′′ | 177.79152 | 78.03739 | GCN #14066 | GRB 121212A: Enhanced Swift-XRT position | ![]() | |
1.0′′ | 177.79333 | 78.03758 | GCN #14071 | GRB 121212A: optical observations in ISON-NM observatory | ![]() | |
1.0′′ | 177.79346 | 78.03758 | GCN #14070 | GRB 121212A: Keck observations | ![]() | |
7.4′′ | 177.78252 | 78.03720 | GCN #14064 | GRB 121212A: Swift detection of a burst | ![]() | |
21.5′′ | 177.77125 | 78.03336 | GCN #14079 | GRB 121212A: Maidanak optical observations | ![]() | |
50.9′′ | 177.78667 | 78.05150 | GCN #14068 | GRB 121212A: Swift-BAT refined analysis | ![]() |
There are 14 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 |
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* RA/Dec in equinox J2000
RA* | Dec* | Source table2 | Observatory | Query |
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Queried the X-ray MASTER catalogue.
* RA/Dec in equinox J2000
1Energy band for count-rate is mission specific.
RA* | Dec* | Redshift | Catalogue | Query | ||
---|---|---|---|---|---|---|
17.5 | 177.8092 | 78.0408 | B1=19.8, R1=19.7 | USNO-B1 | ![]() | |
21.9 | 177.7710 | 78.0332 | B=20.2, R=19.3 | APM-N | ![]() | |
48.4 | 177.8271 | 78.0488 | B=22.0, R=19.4 | APM-N | ![]() | |
60.4 | 177.8618 | 78.0460 | I=18.7, R1=19.7 | USNO-B1 | ![]() | |
75.3 | 177.8918 | 78.0337 | I=18.7, R1=19.7 | USNO-B1 | ![]() | |
84.8 | 177.8008 | 78.0609 | B1=21.0, I=18.3 | USNO-B1 | ![]() | |
94.5 | 177.9151 | 78.0439 | B=19.5, R=18.3 | APM-N | ![]() | |
101.5 | 177.9276 | 78.0342 | B=21.9, R=20.0 | APM-N | ![]() | |
104.1 | 177.8451 | 78.0106 | B=21.4, R=20.0 | APM-N | ![]() | |
106.9 | 177.8020 | 78.0670 | B=20.4, R=18.7 | APM-N | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 52 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 | ||
---|---|---|---|---|---|
14.6 | 177.7840 | 78.0337 | R1=19.4, R2=19.2 | USNO-B1 | ![]() |
15.3 | 177.7841 | 78.0335 | B1=21.0, I=17.7, R1=19.9 | USNO-B1 | ![]() |
15.9 | 177.7837 | 78.0334 | h=15.5, j=16.1, k=15.3 | 2MASS | ![]() |
21.4 | 177.7713 | 78.0334 | B1=20.3, B2=20.6, R1=19.6, R2=19.4 | USNO-B1 | ![]() |
36.2 | 177.7439 | 78.0376 | h=15.4, j=15.6, k=15.3 | 2MASS | ![]() |
36.2 | 177.7439 | 78.0377 | B1=17.8, B2=17.3, I=16.0, R1=16.7, R2=16.7 | USNO-B1 | ![]() |
49.8 | 177.8287 | 78.0490 | B2=21.8, R1=19.9 | USNO-B1 | ![]() |
59.0 | 177.8610 | 78.0455 | h=15.8, j=16.6, k=15.5 | 2MASS | ![]() |
93.3 | 177.7923 | 78.0115 | B1=17.9, I=18.2, R1=16.4, R2=20.5 | USNO-B1 | ![]() |
94.3 | 177.9149 | 78.0439 | B1=19.5, B2=20.3, R1=18.9, R2=19.6 | USNO-B1 | ![]() |
There are 59 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.