GRB 200914A

Time: 12:48:30
Trigger Number: INTEGRAL
Burst Advocate:

BAT Data:

RA: a	256.4 17:05:36.0
Dec: a	-37.6 -37:36:00.0
90% Error Radius: b	n/a
T90: c	n/a
Fluence: d	n/a (n/a)
1s Peak Photon Flux: e	n/a (n/a)
Photon Index: f	n/a (n/a)

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90% error in parentheses,
^a J2000; ^b arcmin; ^c seconds; ^d 10^-7 erg/cm² (15-150 keV); ^e ph/cm²/sec (15-150 keV); ^f PL = simple power-law, CPL = cutoff power-law (15-150 keV)

XRT Data:

RA: a	16:58:4.84
Dec: a	-36:16:41.6
90% Error Radius: b	6.5
Time to First Observation: c	8900
Early Flux: d	n/a
11 Hour Flux: d	n/a
24 Hour Flux: d	n/a
Initial Temporal Index:	n/a
Spectral Index (Gamma):	n/a
Column Density (NH): e	n/a

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Note: Please be aware that only the very basic temporal and spectral quantities are reported here. You are strongly encouraged to see the referenced GCN circulars for full details.
^a J2000; ^b arcsec; ^c seconds; ^d 10^-11 erg/cm²/s (0.3-10 keV); ^e 10²¹ cm^-2

UVOT Data:

RA: a	n/a
Dec: a	n/a
90% Error Radius: b	n/a
Time to First Observation: c	n/a
V Magnitude:	n/a
Other Filter Magnitudes:	n/a

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^a J2000; ^b arcsec; ^c seconds

Comments:

INTEGRAL: GCN 28419
XRT: Although there is moderate evidence for fading, we cannot exclude that the observed X-ray emission is coming from the bright IR source reported in Perri et al. (GCN Circ. 28425), possibly unrelated to GRB 200914A.

References:

BAT:
XRT: GCN 28425; GCN 28466
UVOT:
Radio:
Redshift:
Host:
Other: