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GRB 200325A

Time: n/a
Trigger Number: Ground Analysis
Burst Advocate: n/a

BAT Data:

RA: a 31.7203
02:06:52.9
Dec: a -31.816
-31:48:57.6
90% Error Radius: b 4
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)

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 n/a
Dec: a n/a
90% Error Radius: b n/a
Time to First Observation: c n/a
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

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

a J2000; b arcsec; c seconds

Other Burst Info:

Redshift:
Host Galaxy:
Other Observatory Detections:
Fermi (GMB), AGILE, AstroSat, IPN

Comments:

Detected by Fermi GBM (GCN 27434) which trigger GUANO to look at ground analysis of BAT data.
No XRT or UVOT follow-up will take place due to the source’s proximity to the sun (1.5 hours).

References:

BAT: GCN 27444
XRT:
UVOT:
Radio:
Redshift:
Host:
Other: