Swift Observations of GRB 200826A

A. D'Ai (INAF-IASFPA) for the Swift team

1. Introduction

Hurley et al. (GCN Circ. 28291) reported the GRB detection. Table 1 contains the best reported positions from Swift.

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 D'Ai et al. (GCN Circ. 28300). Source 3 is fading with 3-sigma significance, and is therefore likely the GRB afterglow.

The light curve (Figure 2) can be modelled with a power-law decay with a decay index of α=1.3 (+0.7, -0.5).

A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 1.8 (+0.6, -0.5). The best-fitting absorption column is 2.2 (+2.5, -1.6) x 1021 cm-2, consistent with the Galactic value of 6.0 x 1020 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 (4.6 x 10-11) erg cm-2 count-1.

4. UVOT Observations and Analysis

UVOT results are not available.

Figure 1. The BAT light curve is not available.

RA (J2000) Dec (J2000) Error Note Reference
00h27m08.32s +34°01'36.1" 3.3" XRT D'Ai et al. GCN Circ. 28300

Table 1. Positions from the Swift instruments.

Band Authors GCN Circ. Subject Observatory Notes
Optical Lipunov et al. 28285 Fermi GRB 200826A: Global MASTER-Net
observations report
MASTER
Optical Ahumada et al. 28295 Zwicky Transient Facility Identifies
Optical Afterglow Candidate of a Fermi
Short GRB (Trigger 620108997)
detection
Optical Belkin et al. 28306 Kitab optical observations
Optical Rossi et al. 28949 TNG and LBT constraints on a supernova
bump
LBT detection
Radio Alexander et al. 28302 VLA Detection at 6 GHz VLA detection
Radio Chandra et al. 28410 uGMRT radio upper limit at 1.25 GHz GMRT upper limits
Gamma-ray Fermi 28284 Fermi GBM Final Real-time Localization Fermi GBM
Gamma-ray Kunzweiler et al. 28286 BALROG localization (Fermi Trigger
620108997 / GRB 200826187)
BALROG
Gamma-ray Mangan et al. 28287 Fermi GBM observation Fermi GBM Epeak=89.8±3.7 keV
T90=1.14 seconds
Fluence=4.8±0.1x10-6erg cm-2
(97 percentile for short GRBs)
Gamma-ray Gupta et al. 28288 AstroSat CZTI detection CZTI
Gamma-ray Pittori et al. 28289 AGILE detection AGILE
Gamma-ray Hurley et al. 28291 IPN triangulation of GRB 200826A
(short/bright)
IPN
Gamma-ray Ridnaia et al. 28294 Konus-Wind detection Konus-Wind Epeak=67 (-17,+31) keV
Duration=~1.6 seconds
Fluence=3.30(-0.42,+0.47)x10-6erg cm-2
Gamma-ray Svinkin et al. 28301 further analysis of the Konus-Wind data
and classification
Konus-Wind
Other Carracedo et al. 28293 Zwicky Transient Facility Follow-Up of
a Fermi Short GRB (Trigger 620108997)
Other Dichiara et al. 28312 Lowell Discovery Telescope observations
of ZTF20abwysqy
Other Rothberg et al. 28319
Other Ahumada et al. 28727 GMOS-N detection of a supernova bump
Other Ahumada et al. 29029 GMOS-N detected source magnitude
(Correction)
detection

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

December 12, 2020