Swift Observations of GRB 200613A

J.A. Kennea (PSU) and F.E. Marshall (NASA/GSFC) for the Swift team

1. Introduction

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.

2. BAT Observations and Analysis

BAT did not observe this burst.

3. XRT Observations and Analysis

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 1021 cm-2, in excess of the Galactic value of 8.4 x 1019 cm-2 (Willingale et al. 2013). The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 3.5 x 10-11 (4.7 x 10-11) erg cm-2 count-1.

4. UVOT Observations and Analysis

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 EB-V of 0.01 mag. in the direction of the GRB (Schlegel et al. 1998).

Figure 1. The BAT light curve is not available.

XRT light curve

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
10h12m10.03s +45°45'14.1" 0.46" UVOT-refined Marshall GCN Circ. 27944
10h12m10.08s +45°45'14.7" 1.4" XRT Kennea et al. GCN Circ. 27936

Table 1. Positions from the Swift instruments.

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 Epeak=111±3 keV
T90=470 seconds
Fluence=4.10±0.05x10-5erg cm-2
(93rd percentile for long GRBs)
Gamma-ray Ohno et al. 27931 Fermi-LAT detection Fermi LAT Emax=7.6 GeV
Gamma-ray Yamaoka et al. 27964 CALET Gamma-Ray Burst Monitor detection CALET

Table 2. Summary of GCN Circulars from other observatories sorted by band and then circular number.

Filter Tstart(s) Tstop(s) 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