Swift Observations of GRB 140723A

V. D'Elia (ASDC) for the Swift team

1. Introduction

Bissaldi et al. (GCN Circ. 16623) reported the GRB detection. At UT 01:36:30.73 on July 23rd, 2014, Fermi-LAT detected high-energy emission from GRB 140723A, which was also detected by Fermi-GBM (trigger427772193 / 140723067). 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

XRT results are not available.

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

Table 1. Positions from the Swift instruments.

Band	Authors	GCN Circ.	Subject	Observatory	Notes
Optical	Guidorzi et al.	16627	LCO-Sutherland optical candidate	LCO	detection
Optical	Gorbovskoy et al.	16629	MASTER optical observation	MASTER
Optical	Guidorzi et al.	16630	LCO-Sutherland optical candidate retraction	LCO	retraction
Gamma-ray	Bissaldi et al.	16623	Fermi-LAT detection	Fermi LAT	Emax=1.8 GeV
Gamma-ray	Hurley et al.	16625	IPN Triangulation	IPN
Gamma-ray	Burns	16626	Fermi GBM detection	Fermi GBM	Epeak=968±231 keV T90=56 seconds Fluence=1.46±0.04x10-5erg cm-2 (82nd percentile for long GRBs)
Gamma-ray	Golenetskii et al.	16628	Konus-Wind observation	Konus-Wind	Epeak=1142 (-452,+1005) keV Fluence=2.3(-0.5,+0.8)x10-5erg cm-2

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

Table 3. Found no UVOT observations.

July 26, 2014