Presumed name: GRB 200509A
BAT | 07h 45m 48.00s, -04° 38′ 27.6″ |
---|---|
position: | (116.450, -4.641 ± 180″) |
XRT | 07h 45m 41.57s, -04° 37′ 52.0″ |
position: | (116.42322, -4.63112 ± 3.5″) |
UVOT | 07h 45m 41.18s, -04° 37′ 49.1″ |
position: | (116.4216, -4.6303 ± 1.1″) |
Galactic NHI: | 1.09×100 cm-2 |
Galactic E(B-V): | 0.130 mag |
Best RA: | 07h 45m 41.18s | = 116.4216 d |
---|---|---|
Best Dec: | -04° 37′ 49.1″ | = -4.6303 d |
Gal Lat: | 9.86 | |
Gal Long: | 223.37 | |
Sun angle: | 72.55°, -4.7 hr East of Sun |
1Sper #3 auto processing.
Observability of this burst for Swift.
No UVOT images are currently available.
SPER results page for this trigger.
There are 7 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′′ | 116.42167 | -4.63039 | GCN #27701 | GRB 200509A: Swift detection of a burst with a possible optical counterpart | ![]() | |
1.5′′ | 116.42200 | -4.63036 | GCN #27709 | GRB 200509A: Swift/UVOT Detection | ![]() | |
2.8′′ | 116.42238 | -4.63042 | GCN #27703 | GRB 200509A: Enhanced Swift-XRT position | ![]() | |
2.8′′ | 116.42238 | -4.63042 | GCN #27710 | GRB 200509A: GROWTH-India r band upper limits | ![]() | |
27.2′′ | 116.41500 | -4.63400 | GCN #27713 | GRB 200509A: Swift-BAT refined analysis | ![]() |
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 | ||
---|---|---|---|---|---|
147.9 | 116.4084 | -4.6695 | TYC 4840-1797-1 | B=12.31, G=11.8906, H=11.232, J=11.303, K=11.152, V=11.83 | ![]() |
168.6 | 116.3921 | -4.5960 | TYC 4840-1906-1 | B=10.22, G=9.9564, H=9.495, J=9.555, K=9.386, V=9.90 | ![]() |
* 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 | ||
---|---|---|---|---|---|---|
9.8 | 116.4237 | -4.6317 | NED | ![]() | ||
22.5 | 116.4233 | -4.6244 | NED | ![]() | ||
32.0 | 116.4137 | -4.6258 | NED | ![]() | ||
32.2 | 116.4248 | -4.6399 | B=20.2, R2=19.3, i=18.6 | SSS | ![]() | |
32.7 | 116.4188 | -4.6232 | B1=18.8, B2=17.7, I=15.8, R1=17.0 | USNO-B1 | ![]() | |
33.6 | 116.4179 | -4.6217 | NED | ![]() | ||
34.2 | 116.4121 | -4.6325 | NED | ![]() | ||
34.2 | 116.4316 | -4.6267 | B=21.9 | SSS | ![]() | |
35.7 | 116.4117 | -4.6325 | NED | ![]() | ||
37.3 | 116.4242 | -4.6203 | NED | ![]() |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 240 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 | ||
---|---|---|---|---|---|
3.3 | 116.4240 | -4.6316 | h=15.8, j=16.2, k=16.9 | 2MASS | ![]() |
3.5 | 116.4240 | -4.6317 | B1=18.5, B2=18.0, I=16.7, R1=17.6, R2=17.4 | USNO-B1 | ![]() |
24.5 | 116.4235 | -4.6243 | B2=19.2, I=17.8, R2=19.2 | USNO-B1 | ![]() |
31.9 | 116.4248 | -4.6399 | B2=19.6, I=17.8, R1=19.1, R2=19.0 | USNO-B1 | ![]() |
36.2 | 116.4273 | -4.6403 | B1=18.6, B2=17.7, I=16.2, R1=16.8, R2=17.2 | USNO-B1 | ![]() |
36.2 | 116.4273 | -4.6403 | h=15.5, j=15.9, k=15.3 | 2MASS | ![]() |
37.7 | 116.4191 | -4.6407 | I=17.9, R2=19.5 | USNO-B1 | ![]() |
38.4 | 116.4179 | -4.6218 | B1=16.3, B2=15.4, I=13.1, R1=14.1, R2=14.4 | USNO-B1 | ![]() |
38.8 | 116.4179 | -4.6217 | h=12.2, j=12.7, k=12.0 | 2MASS | ![]() |
39.1 | 116.4242 | -4.6203 | B1=18.4, B2=17.9, I=16.3, R1=17.3, R2=17.2 | USNO-B1 | ![]() |
There are 341 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.