Presumed name: EXO 1745-248
BAT | 17h 48m 00.00s, -24° 46′ 19.2″ |
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position: | (267.000, -24.772 ± 0″) |
XRT | 17h 48m 04.80s, -24° 46′ 48.4″ |
position: | (267.0200, -24.7801 ± 5.4″) |
UVOT | No position available. |
Galactic NHI: | 6.24×100 cm-2 |
Galactic E(B-V): | 3.523 mag |
Best RA: | 17h 48m 04.80s | = 267.0200 d |
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Best Dec: | -24° 46′ 48.4″ | = -24.7801 d |
Gal Lat: | 1.71 | |
Gal Long: | 3.84 | |
Sun angle: | not found |
1Sper #0 auto processing.
Observability of this burst for Swift.
No UVOT images are currently available.
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′′ | 267.02000 | -24.78010 | GCN #17679 | Swift triggered on a source in Terzan 5 (trigger=637212) | ||
0.8′′ | 267.02012 | -24.78031 | ATEL #3264 | A possible IR counterpart to the transient X-ray pulsar IGR J17480-2446 in Terzan 5 | ||
1.2′′ | 267.02025 | -24.78034 | ATEL #3924 | A Candidate Optical Counterpart of IGR J17480-2446 in Terzan 5 identified with the Hubble Space Telescope | ||
1.5′′ | 267.01988 | -24.78050 | ATEL #2937 | Eclipsing X-ray Burster in Terzan 5: Improved Swift Localization | ||
1.5′′ | 267.01997 | -24.77968 | ATEL #2933 | The Eclipsing X-ray Burster in Terzan 5 is Probably Not the 2000 Transient | ||
4.6′′ | 267.02070 | -24.77900 | ATEL #7242 | Swift/XRT follow up of the X-ray transient in the globular cluster Terzan 5 | ||
4.6′′ | 267.02100 | -24.78100 | ATEL #2920 | Swift-XRT location of the ongoing Terzan 5 outburst | ||
5.5′′ | 267.02167 | -24.78019 | ATEL #3723 | Improved Swift-XRT position of the transient source in Terzan 5 | ||
5.5′′ | 267.02165 | -24.77983 | ATEL #2919 | A hard X-ray transient in the direction of Terzan 5 detected by INTEGRAL | ||
5.7′′ | 267.02175 | -24.78017 | ATEL #8982 | A sub-luminous outburst of a transient in the Galactic globular cluster Terzan 5� possibly due to EXO 1745-248 (aka Terzan 5 X-1) | ||
5.9′′ | 267.02180 | -24.77992 | ATEL #7262 | VLA observations identify the currently active source in Terzan 5 as the neutron star transient EXO 1745-248 |
There are 23 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 | ||
---|---|---|---|---|---|
7.2 | 267.0000 | -24.7700 | [HWC2006] CX 25 | ||
14.9 | 266.9963 | -24.7696 | CXOU J174759.1-244610 | B=18.85, I=13.2, R=14.8 | |
35.4 | 267.0094 | -24.7769 | PSR B1744-24A | ||
39.3 | 267.0108 | -24.7672 | CXOGlb J174802.6-244602 | ||
51.7 | 267.0142 | -24.7783 | Cl* Terzan 5 SAW V5 | ||
56.8 | 267.0147 | -24.7803 | CXOGlb J174803.5-244649 | ||
57.9 | 267.0155 | -24.7797 | [ORF2011] 15 | ||
58.5 | 267.0161 | -24.7791 | [ORF2011] 25 | ||
58.9 | 266.9977 | -24.7882 | Cl* Terzan 5 SAW V2 | H=8.515, J=9.980, K=7.802 | |
59.3 | 267.0169 | -24.7779 | CXOGlb J174804.0-244640 |
There are 120 SIMBAD objects within the position error. The full list is here.
* RA/Dec in equinox J2000
RA* | Dec* | Source table2 | Observatory | Query | ||
---|---|---|---|---|---|---|
20.5 | 267.0063 | -24.7724 | 0.000596749046417 +/- 0.000138091972196 | CHANDRA | ||
20.8 | 267.0063 | -24.7725 | 0.000644564105009 +/- 0.000127679019033 | CHANDRA | ||
27.5 | 266.9997 | -24.7796 | 0.0210874546319 +/- 0.00167977518868 | CHANDRA | ||
27.9 | 266.9985 | -24.7796 | 0.0231084357947 +/- 0.00176521704998 | CHANDRA | ||
28.2 | 267.0014 | -24.7797 | 0.0579143330481 +/- 0.00326485612337 | CHANDRA | ||
29.1 | 266.9969 | -24.7796 | 0.0426198482275 +/- 0.00295684965012 | CHANDRA | ||
29.2 | 267.0026 | -24.7798 | 0.0661832984842 +/- 0.00336406833798 | CHANDRA | ||
29.9 | 266.9962 | -24.7796 | 0.0236317031085 +/- 0.00176521530375 | CHANDRA | ||
30.6 | 267.0037 | -24.7798 | 0.0655973256084 +/- 0.00343538948637 | CHANDRA | ||
30.7 | 266.9956 | -24.7796 | 0.0596007390775 +/- 0.00311571837217 | CHANDRA |
Queried the X-ray MASTER catalogue.
There are 443 X-ray sources within the position error. The full list is here.
* RA/Dec in equinox J2000
1Energy band for count-rate is mission specific.
RA* | Dec* | Redshift | Catalogue | Query | ||
---|---|---|---|---|---|---|
9.7 | 267.0029 | -24.7713 | I=14.5, R1=16.9 | USNO-B1 | ||
15.1 | 266.9963 | -24.7694 | NED | |||
22.3 | 267.0006 | -24.7658 | B2=19.5, I=15.3 | USNO-B1 | ||
25.9 | 267.0008 | -24.7648 | B2=20.5, I=16.7 | USNO-B1 | ||
26.9 | 266.9960 | -24.7785 | B2=19.5, I=13.9, R1=16.5, R2=17.4 | USNO-B1 | ||
27.2 | 267.0031 | -24.7650 | B2=20.4, I=15.9 | USNO-B1 | ||
30.0 | 266.9916 | -24.7686 | I=16.0, R1=16.7 | USNO-B1 | ||
31.9 | 267.0097 | -24.7721 | B2=19.5, I=10.2 | USNO-B1 | ||
32.5 | 266.9903 | -24.7740 | B2=19.5, I=16.9 | USNO-B1 | ||
32.8 | 267.0023 | -24.7809 | I=11.4, R2=16.8 | USNO-B1 |
Queried APM-N, SDSS, PSCz, SSS, NED, 2MASSX, USNO-B1.
There are 428 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 | ||
---|---|---|---|---|---|
1.8 | 267.0005 | -24.7717 | h=12.6, j=14.0, k=12.2 | 2MASS | |
8.6 | 267.0015 | -24.7740 | h=10.2, j=11.8, k=9.6 | 2MASS | |
8.9 | 267.0026 | -24.7714 | h=10.4, j=11.9, k=9.9 | 2MASS | |
9.2 | 266.9979 | -24.7703 | h=13.1, j=14.5, k=12.8 | 2MASS | |
11.6 | 266.9975 | -24.7743 | h=11.5, j=13.0, k=11.0 | 2MASS | |
13.1 | 267.0003 | -24.7756 | h=13.4, j=14.6, k=12.9 | 2MASS | |
14.0 | 267.0026 | -24.7689 | h=12.8, j=14.0, k=12.2 | 2MASS | |
14.8 | 266.9963 | -24.7696 | h=11.1, j=12.0, k=10.8 | 2MASS | |
15.0 | 266.9963 | -24.7695 | B1=19.0, B2=18.7, I=13.2, R1=14.4, R2=15.2 | USNO-B1 | |
15.7 | 267.0003 | -24.7677 | h=13.3, j=14.6, k=12.8 | 2MASS |
There are 1461 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.