J.A. Kennea (PSU) and F.E. Marshall (NASA/GSFC) for the Swift team
Ohno et al. (GCN Circ. 27931) reported the GRB detection. On June 13, 2020, Fermi-LAT detected high-energy emission from GRB 200613A, which was also detected by Fermi-GBM at T0 = 05:30:08 UT (GCN Circ. 27926, Bissaldi et al. GCN Circ. 27930). Table 1 contains the best reported positions from Swift.
Pozanenko et al. (GCN Circ. 27937) reported the position from Abastumani Astro. Obs. for the optical afterglow of this GRB. Marshall (GCN Circ. 27944) reported the detection with UVOT of an optical afterglow. de Ugarte Postigo et al. (GCN Circ. 29320) determined a redshift of 1.2280 from GTC. Table 2 is a summary of GCN Circulars about this GRB from observatories other than Swift.
BAT did not observe this burst.
Analysis of the initial XRT data was reported by Kennea et al. (GCN Circ. 27936).
The light curve (Figure 2) can be modelled with a power-law decay with a decay index of α=1.6 ± 0.5.
A spectrum formed from the PC mode data can be fitted with an absorbed
power-law with a photon spectral index of 1.89 (+0.14, -0.13). The
best-fitting absorption column is 2.3 ± 0.5 x 1
Analysis of the UVOT data was reported by Marshall (GCN Circ. 27944).
Table 3 gives preliminary
magnitudes using the UVOT photometric system
(Breeveld et al. 2011, AIP Conf. Proc., 1358, 373).
No correction has been made for the expected extinction in the Milky Way
corresponding to a reddening of
Figure 1. The BAT light curve is not available.
Figure 2. The XRT light curve.
Any data from a crosshatched region are not included in the fit.
RA (J2000) | Dec (J2000) | Error | Note | Reference |
---|---|---|---|---|
1 |
+45°45'14.1" | 0.46" | UVOT-refined | Marshall GCN Circ. 27944 |
1 |
+45°45'14.7" | 1.4" | XRT | Kennea et al. GCN Circ. 27936 |
Band | Authors | GCN Circ. | Subject | Observatory | Notes |
---|---|---|---|---|---|
Optical | Lipunov et al. | 27933 | Fermi GRB 200613A: Global MASTER-Net observations report |
MASTER | |
Optical | Kann et al. | 27935 | Candidate afterglow from OAJ | Obs. Astro. de Javalambre | detection |
Optical | Pozanenko et al. | 27937 | Kitab and AbAO optical afterglow observations, host galaxy candidate |
Abastumani Astro. Obs. | |
Optical | Kann | 27938 | OAJ Afterglow: Error in Coordinates | Obs. Astro. de Javalambre | |
Optical | Kitab and AbAO | 27939 | Liverpool Telescope observations | Liverpool Telescope | detection |
Optical | Zhu et al. | 27943 | Xinglong-2.16m optical observations | Xinglong | detection |
Optical | Liu et al. | 27949 | Continued Xinglong-2.16m optical observations |
Xinglong | |
Optical | Belkin et al. | 27958 | continued AbAO optical afterglow observations |
Abastumani Astro. Obs. | detection |
Optical | Murata et al. | 27962 | MITSuME Akeno optical upper limits | MITSuME Akeno | upper limits |
Optical | Fu et al. | 27971 | Jet-break from Xinglong-2.16m optical observations |
Xinglong | |
Optical | Belkin et al. | 27978 | Mondy optical observations | Mondy | detection |
Optical | Moskvitin | 27982 | SAO RAS optical observations | SAO RAS | |
Optical | Belkin et al. | 27983 | continued Kitab optical observations | detection | |
Optical | Izzo | 27998 | Further Liverpool Telescope observations | Liverpool Telescope | |
Optical | Dutta et al. | 27999 | R-band observations from HCT | Himalayan Chandra Telescope | |
Optical | Belkin et al. | 28000 | CrAO optical observations | CrAO | detection |
Optical | Belkin et al. | 28003 | Continued CrAO optical observations | CrAO | detection |
Optical | de Ugarte Postigo et al. | 29320 | Host galaxy redshift from OSIRIS/GTC | GTC | redshift |
Gamma-ray | Fermi | 27926 | Fermi GBM Final Real-time Localization | Fermi GBM | |
Gamma-ray | Kunzweiler et al. | 27927 | BALROG localization (Fermi Trigger 613719013 / GRB 200613229) |
BALROG | |
Gamma-ray | Bissaldi and Lesage | 27930 | Fermi GBM observation | Fermi GBM | Fluence=4.10±0.05x1 (9 |
Gamma-ray | Ohno et al. | 27931 | Fermi-LAT detection | Fermi LAT | |
Gamma-ray | Yamaoka et al. | 27964 | CALET Gamma-Ray Burst Monitor detection | CALET |
Filter | Exp(s) | Mag | ||
---|---|---|---|---|
white | 44416 | 45204 | 775 | 19.65 ± 0.07 |
v | 45211 | 45427 | 213 | >18.6 |
u | 43621 | 44409 | 775 | 19.02 ± 0.12 |
Table 3. UVOT observations reported by Marshall (GCN Circ. 27944). The start and stop times of the exposures are given in seconds since the BAT trigger. The preliminary detections and 3-σ upper limits are given. No correction has been made for extinction in the Milky Way.
January 19, 2021