Gernot Maier
Gernot Maier
What should we do if there are only de-absorbed spectra given in a paper? (example is a MAGIC/VERITAS Mrk 501 paper) I can certainly add a comment (including the EBL...
LC data from Fig 2 and 3 of 1FGL J1018.6–5856 (binary) is missing (and paper is marked as complete, which is not correct)
I am trying to access all published data of a certain object, but I am not entirely sure how to do this. This is what I've started with: ``` import...
Would like to ask for the possibility to add asymmetric errors bars for light curve data: flux_errn and flux_errp (similar to the sed format).
Is it possible for a pl2 spectral model (or for any model) to give an upper/limit systematic error? In the VERITAS paper on B2 1215+30 (2017), the systematic error is...
Is there a possibility to add spectra of the following form? dN/dE = F x (E/E_0) ^ ( -alpha - beta x log(E/E_0) ) Usually called log-parabolic form.
Is there a way to add an energy dependent morphology description? e.g. a gaussian extension which decreases with energy?
I am trying to understand the axes order in the [Edisp IRF](https://github.com/open-gamma-ray-astro/gamma-astro-data-formats/blob/master/source/irfs/full_enclosure/edisp/index.rst) compared to all other IRFs with similar axes For Edisp, we have: - ENERG_LO, ENERG_HI - MIGRA_LO, MIGRA_HI...
Proposal to clarify the meaning of the axes in the PSF histograms (see also issue #174)
The documentation of the PSF tables is not entirely clear and could be clarified by better wording or using other expressions. There is jargon used, which makes it hard to...