Swift Observations of GRB 150702A

P. D'Avanzo (INAF-OAB) for the Swift team

1. Introduction

Vianello et al. (GCN Circ. 17989) 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

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	Buckley et al.	17992	MASTER-SAAO inspection	Abastumani Astro. Obs.
Gamma-ray	Vianello et al.	17989	Fermi-LAT detection	Fermi LAT
Gamma-ray	Hurley et al.	17993	IPN Triangulation	IPN
Gamma-ray	Jenke	17994	Fermi GBM detection	Fermi GBM	Epeak=987±100 keV T90=45 seconds Fluence=2.1±0.4x10-5erg cm-2 (88th percentile for long GRBs)
Gamma-ray	Golenetskii et al.	17995	Konus-Wind observation	Konus-Wind	Epeak=2059 (-903,+1940) keV Fluence=5.50(-1.45,+1.86)x10-5erg cm-2

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

July 7, 2015