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GRB 220730A
The Swift Burst Analyser — GRB 220730A
Last updated using ObsID 01118357000, version 7;
Data were analysed using HEASOFT version 6.32
Related pages:
Position
| Spectrum
| Image
| XRT Catalogue entry
| Download obs data
| BAT analysis
| GCN Notices
| GCN Circulars
From 2016 January, the light curve plots support interactive zooming and exploring. See the jsPlot
documentation for details.
Also, from the same date, the first plot on this page is the observed flux
in the native band of each instrument (including UVOT where available).
Index of bursts .
About these products .
Caveats
If the answer to any of the following is "yes," you should investigate further before
accepting the light curves. See the documentation for details.
Is Γ discontinuous between BAT and XRT?
Is the BAT spectral fit a cut-off power law?
Are the Γ values extreme?
Are the errors on Γ/CF large?
Do all the BAT or XRT bins have identically Γ/CF bins?
Close .
Jump to:
Observed flux | BAT | BAT no evolution .
Downloads:
BAT spectral evolution data | All files for this object: [tar ][tar.gz ][zip ].
Observed BAT flux
Reliability checks .
BAT binning:
SNR 4 SNR 5 SNR 6 SNR 7 64 ms bins 1 s bins 10 s bins
Subplot:
no photon index counts to flux conversion factor
Show 'bad' BAT points? Explain
■ BAT
■ white
■ v
■ b
■ u
■ uvw1
■ uvw2
■ uvm2
BAT unabsorbed flux light curves
Reliability checks .
Show BAT hardness ratio .
BAT binning:
SNR 4 SNR 5 SNR 6 SNR 7 64 ms bins 1 s bins 10 s bins
Subplot:
no photon index counts to flux conversion factor
Display which bands?
Flux density at 10 keV
0.3—10 keV flux
15—50 keV flux
Show 'bad' BAT points? Explain
The fit to the T90 spectrum was used to create the plots in this section. The spectral fit used was a power-law with photon index:
Count-rate light curves are available from GCN .
BAT unabsorbed flux light curves, no spectral evolution
BAT binning:
SNR 4 SNR 5 SNR 6 SNR 7 64 ms bins 1 s bins 10 s bins
Display which bands?
Flux density at 10 keV
0.3—10 keV flux
15—50 keV flux
Show 'bad' BAT points? Explain