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Results (31)
- Action #2868 (Closed): Add radial CTA Gaussian background model with energy dependence of sigma
- The analysis of the H.E.S.S. observations of ... </spectrum> </source> </code></pre>
- Change request #2659 (Closed): Do not require ... model template for On/Off fitting with wstat
- On/Off fitting with @wstat@ does not need to ... round template as with @use_irf_bkg = false@.
- Action #2654 (Closed): Correct handling of H.E.S.S. 3D energy dispersion IRFs
- Andreas Specovius reported some issues with t ... ms to be an issue with the renormalization.
- Bug #2458 (Closed): Extended model fits better than diffuse map
- Michele Fiori reported a problem where simula ... y sampled at the centre of the spatial bins).
- Action #2422 (Closed): Add energy integration methods to GCTAEdisp
- Energy integration methods <pre> double pro ... @ to speed up the computations of @csphagen@.
- Action #2403 (Closed): Check if the energy dispersion integration can be optimised
- Try to see whether we can reduce the integrat ... t in @GResponse::convolve@ (constant @iter@).
- Action #2342 (Closed): Handle noisy CTA energy dispersion
- The energy dispersion histogram for CTA data ... um near 2 TeV !specres_3D2_nosmooth.png!
- Change request #2120 (Closed): Improve access time of keyword values in GFitsHeader
- While looking into the simulated data challen ... sion of its entries and uses a binary search algorithm to lookup items. After talking with ... amatically improve the time issue I'm seeing.
- Action #1855 (Closed): Add GSkyDir::moon() method
- A @moon(const GTime& time)@ method should be ... a corresponding method for the Sun position).
- Change request #1817 (New): GLog should regularly update log file
- I stumbled upon this when sending @ct...@-job ... tool after certain tasks have been performed.