| site map
- Home
- About
The Swift Mission UK involvement Instruments
GRBs before Swift GRBs in the Swift era Non-GRB science with Swift GRB research at Leicester
Spacecraft status Swift in the press Swift Videos
- Support
Helpdesk TOO requests Guest Investigator program Target visibility checker Search transient database
- Data Access
Overview Quick Look GCN Notices Download obs data Search obs catalogue The 2SXPS catalogue The LSXPS catalogue
- Data Analysis
Data analysis overview Swift software
Build XRT products
BAT data analysis guide XRT data analysis guide XRT digest UVOT data analysis guide
- GRB Products
Full dataset Swift XRT products for GRBs XRT positions XRT light curves XRT spectra XRT GRB catalogue XRT GRB images Burst analyser Prompt dataset GRB field info XRT prompt analysis
- Publications
Publication index Published papers Submitted papers XRT instrument papers ATels GCNs Conferences
- Links
Databases NED Simbad GCN circulars archive GRB data table Software & Tools Swift Software (HEASoft) Xanadu WebPIMMS Institutional Swift Sites GSFC PSU OAB SSDC MSSL University of Leicester
Home > GRB products > Burst Analyser > GRB 180709A
GRB 180709A
Last updated using ObsID 00846868000, version 5;
Data were analysed using HEASOFT version 6.32
Related pages: Enhanced position | Light curve | 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.
Jump to: Observed flux | BAT+XRT | BAT | XRT | BAT no evolution.
Downloads: BAT spectral evolution data | XRT spectral evolution data | All files for this object: [tar][tar.gz][zip].
All data uses absorption NH=7.976 × 1022 cm-2 at z=0.
(Source: the late-time spectrum from the XRT spectrum repository).
Observed BAT+XRT+UVOT flux
Reliability checks.
Show Observed Flux hardness ratio.
■ BAT
■ XRT (all modes)
Observed flux density, with photon index sub plot. BAT binning: SNR 5.
Show full observed flux Observed flux density plot controls.
Generate postscript plot | Data file.
BAT-XRT unabsorbed flux light curves
Reliability checks.
Show BAT-XRT hardness ratio.
Flux density at 10 keV, with photon index sub plot. BAT binning: SNR 5.
Show full BAT-XRT Flux density at 10 keV plot controls.
Generate postscript plot | Data file.
BAT unabsorbed flux light curves
Reliability checks.
Show BAT hardness ratio.
Flux density at 10 keV, with photon index sub plot. BAT binning: SNR 5.
Show full BAT Flux density at 10 keV plot controls.
Generate postscript plot | Data file.
XRT unabsorbed flux light curves
Reliability checks.
Show XRT hardness ratio.
Flux density at 10 keV, with photon index sub plot. BAT binning: SNR 5.
Show full XRT Flux density at 10 keV plot controls.
Generate postscript plot | Data file.
The fit to the T90 spectrum was used to create the plots in this section.
T90 was 194.8, from 2.7 to 197.5
The spectral fit used was a power-law with photon index: 1.45
Count-rate light curves are available from GCN.
BAT unabsorbed flux light curves, no spectral evolution
Flux density at 10 keV. BAT binning: SNR 5.
Show full BAT, no spectral evolution Flux density at 10 keV plot controls.
Generate postscript plot | Data file.
UK Swift Science Data Centre
Last updated 0000 null 00 at 00:00:00
Web page maintained by Phil Evans
E-mail: swift help
Please read our privacy notice.
