Presumed name: GRB 100316D
BAT | 07h 10m 27.60s, -56° 16′ 40.8″ |
---|---|
position: | (107.615, -56.278 ± 180″) |
XRT | 07h 10m 30.98s, -56° 15′ 24.1″ |
position: | (107.6291, -56.2567 ± 5.0″) |
UVOT | No position available. |
Galactic NHI: | 0.00×100 cm-2 |
Galactic E(B-V): | 0.116 mag |
Best RA: | 07h 10m 30.98s | = 107.6291 d |
---|---|---|
Best Dec: | -56° 15′ 24.1″ | = -56.2567 d |
Gal Lat: | ||
Gal Long: | ||
Sun angle: | not found |
Observability of this burst for Swift.
Blink images with DSS (link via GSFC)
SPER results page for this trigger.
No SPER data received yet. Refresh this page to check again.
Click on the offset to view the transient announcement.
Offset (′′) | RA | Dec | Date reported | Source | Misc | Query |
---|---|---|---|---|---|---|
0.0′′ | 107.62910 | -56.25670 | GCN #10496 | GRB 100316D: Swift detection of a burst | ||
3.9′′ | 107.62821 | -56.25575 | GCN #10512 | GRB 100316D: VLT/X-shooter observations | ||
3.9′′ | 107.62821 | -56.25575 | GCN #10513 | GRB 100316D: Gemini/GMOS and VLT/X-shooter observations | ||
5.3′′ | 107.62762 | -56.25547 | GCN #10519 | GRB 100316D: Swift XRT enhanced position and further refined analysis | ||
5.5′′ | 107.62725 | -56.25556 | GCN #10523 | GRB 100316D: Further Gemini observations | ||
7.8′′ | 107.63250 | -56.25561 | GCN #10543 | Emerging Supernova in the Afterglow of GRB 100316D | ||
88.2′′ | 107.59917 | -56.27469 | GCN #10511 | GRB 100316D: Swift-BAT refined analysis |
There are 13 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 | ||
---|---|---|---|---|---|
5.3 | 107.6276 | -56.2555 | GRB 100316D | ||
6.1 | 107.6290 | -56.2550 | Anon J071031-5615 | ||
7.9 | 107.6325 | -56.2556 | SN 2010bh |
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 |
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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 | ||
---|---|---|---|---|---|---|
6.5 | 107.6261 | -56.2560 | B=18.1, R2=18.6, i=17.9 | SSS | ||
7.9 | 107.6325 | -56.2556 | NED | |||
7.9 | 107.6325 | -56.2556 | 0.059000 | NED | ||
9.2 | 107.6257 | -56.2584 | B=19.5, R2=18.1, i=17.6 | SSS | ||
15.7 | 107.6279 | -56.2524 | B=21.6 | SSS | ||
27.0 | 107.6253 | -56.2495 | B2=18.2, I=16.8, R1=17.0, R2=16.9 | USNO-B1 | ||
44.1 | 107.6433 | -56.2661 | B2=18.2, I=16.6, R1=16.9, R2=16.9 | USNO-B1 | ||
44.9 | 107.6321 | -56.2443 | I=18.3, R1=19.6, R2=19.9 | USNO-B1 | ||
50.3 | 107.6176 | -56.2691 | B=20.1, R2=17.9, i=17.0 | SSS | ||
55.5 | 107.6035 | -56.2508 | B=20.1, R2=18.5, i=17.9 | SSS |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 39 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 | ||
---|---|---|---|---|---|
6.7 | 107.6260 | -56.2560 | B2=16.6, I=16.7, R1=16.0, R2=16.1 | USNO-B1 | |
8.3 | 107.6250 | -56.2562 | I=17.1, R1=16.7, R2=16.5 | USNO-B1 | |
9.1 | 107.6258 | -56.2584 | B2=19.1, I=17.7, R1=18.0, R2=18.2 | USNO-B1 | |
23.7 | 107.6227 | -56.2622 | B2=21.7, I=18.9, R1=19.5, R2=19.6 | USNO-B1 | |
25.4 | 107.6298 | -56.2637 | h=13.4, j=13.8, k=13.3 | 2MASS | |
25.7 | 107.6299 | -56.2638 | B2=15.7, I=14.1, R1=15.0, R2=15.0 | USNO-B1 | |
26.9 | 107.6253 | -56.2495 | h=15.5, j=16.0, k=15.5 | 2MASS | |
38.1 | 107.6299 | -56.2461 | B2=16.5, I=14.6, R1=15.4, R2=15.3 | USNO-B1 | |
38.3 | 107.6298 | -56.2461 | h=13.4, j=13.9, k=13.3 | 2MASS | |
41.3 | 107.6341 | -56.2678 | I=18.6, R1=20.1, R2=19.8 | USNO-B1 |
There are 242 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.