ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:1410.004] UVOTPY: Swift UVOT grism data reduction

The two Swift UVOT grisms provide uv (170.0-500.0 nm) and visible (285.0-660.0 nm) spectra with a resolution of R~100 and 75. To reduce the grism data, UVOTPY extracts a spectrum given source sky position, and outputs a flux calibrated spectrum. UVOTPY is a replacement for the UVOTIMGRISM FTOOL (ascl:9912.002) in the HEADAS Swift package. Its extraction uses a curved aperture for the uv spectra, accounts the coincidence losses in the detector, provides more accurate anchor positions for the wavelength scale, and is valid for the whole detector.

Code site:
https://github.com/PaulKuin/uvotpy
Used in:
https://ui.adsabs.harvard.edu/abs/2014ApJ...780...21M https://ui.adsabs.harvard.edu/abs/2014ApJ...787...29B
Described in:
https://ui.adsabs.harvard.edu/abs/2015MNRAS.449.2514K
Bibcode:
2014ascl.soft10004K

Views: 4463

ascl:1410.004
Add this shield to your page
Copy the above HTML to add this shield to your code's website.