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dmbounds's Issues

Plotting styles & conventions

Ideas:

  • Colors/style could be related to experiments/target classes.
  • We can also use width in function of the time of publication.
  • For example, MAGIC green, gc=solid, dsph=dashed, clusters=dot-dashed, others=dotted, etc)
  • thermal line from recent reference

VERITAS limits

Arlen, T., Aune, T., Beilicke, M., Benbow, W., Bouvier, A., Buckley, J. H., Bugaev, V., Byrum, K., Cannon, A., Cesarini, A., Ciupik, L., Collins-Hughes, E., Connolly, M. P., Cui, W., Dickherber, R., Dumm, J., Falcone, A., Federici, S., Feng, Q., … Pinzke, A. (2012). Constraints on cosmic rays, magnetic fields, and dark matter from gamma-ray observations of the coma cluster of galaxies with veritas and fermi. Astrophysical Journal, 757(2). https://doi.org/10.1088/0004-637X/757/2/123
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Limits as issues

@moritzhuetten we are using 'issues' to list limits. I propose we instead prepare markdown files to list them. Is that ok with you? I can do that if you want.

Parameter spaces

Hi @moritzhuetten I have an idea which I think can really boost the usefulness and interest of these bounds. Take https://github.com/moritzhuetten/DMbounds/issues/6#issuecomment-1028531196, you see that there is the parameter space below scanned by us back then, rather than only the thermal line. This is something we CAN do. We can assume some parameters and scan parameters spaces (e.g. mSUGRA, pMSSM, etc) and take the envelope. Some of these are published so we do not need to do it. Adding this on our plots would be great!

List of bounds

List of bounds

MAGIC (Michele)

Fermi-LAT (Moritz)

  • [ ]

VERITAS (Michele)

  • Combined dSph galaxies 2017

HESS (Moritz)

  • GC 2011
  • GC line 2013
  • GC 2015
  • GC 2016
  • GC line 2016
  • GC line 2018
  • GC 2021
  • Sagittarius 2008
  • Canis Major 2009
  • dSph 2011
  • dSph 2014
  • dSph 2018/line
  • dSph 2020
  • Fornax cluster 2012
  • WLM 2021
  • M15 and NGC 6388 2011

CTA

`apt.txt` file

@moritzhuetten the apt.txt file should have a header for description. Also, it contains packages that are not available, for example I get

Error: Port texlive-generic-recommended not found
Error: Port texlive-latex-base not found
Error: Port texlive-science not found

the others I find. Also, it would be nice to add a description in the landing page to invite people to install these packages otherwise the program crashes becasue it cannot convert information to latex. Would you take care or should I do it?

HAWC limits

Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. A., Solares, H. A. A., Bautista-Elivar, N., Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Braun, J., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Castillo, M., Cotti, U., … Zhou, H. (2017). Dark Matter Limits From Dwarf Spheroidal Galaxies with The HAWC Gamma-Ray Observatory. The Astrophysical Journal, 853(2), 154. https://doi.org/10.3847/1538-4357/aaa6d8
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Casting of limits

Hi @kumark0 I propose we continue here the discussion about the casting of limits. As soon as you have updates, please post them here for proper book-keeping.

MAGIC-Fermi-LAT limits

MAGIC Collaboration, Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., Banerjee, B., Bangale, P., Barres De Almeida, U., Barrio, J. A., Becerra González, J., Bednarek, W., Bernardini, E., Biasuzzi, B., Biland, A., Blanch, O., Bonnefoy, S., Bonnoli, G., Borracci, F., … Strigari, L. (2016). Limits to dark matter annihilation cross-section from a combined analysis of MAGIC and Fermi-LAT observations of dwarf satellite galaxies. Journal of Cosmology and Astroparticle Physics, 2016(2). https://doi.org/10.1088/1475-7516/2016/02/039

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Direct and collider limits in sigmav plane

Bauer, D., Buckley, J., Cahill-Rowley, M., Cotta, R., Drlica-Wagner, A., Feng, J. L., Funk, S., Hewett, J., Hooper, D., Ismail, A., Kaplinghat, M., Kusenko, A., Matchev, K., McKinsey, D., Rizzo, T., Shepherd, W., Tait, T. M. P., Wijangco, A. M., & Wood, M. (2015). Dark matter in the coming decade: Complementary paths to discovery and beyond. Physics of the Dark Universe, 7–8, 16–23. https://doi.org/10.1016/j.dark.2015.04.001
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Choose project license

And propose to add
# %Part of https://github.com/moritzhuetten/DMbounds. Licensed under a XXX license - see LICENSE.rst
line at top of file. We also should agree which license we want to use for the project.

Originally posted by @moritzhuetten in #1 (comment)

CTA sensitivity

Acharyya, A., Adam, R., Adams, C., Agudo, I., Aguirre-Santaella, A., Alfaro, R., Alfaro, J., Alispach, C., Aloisio, R., Batista, R. A., Amati, L., Ambrosi, G., Angüner, E. O., Antonelli, L. A., Aramo, C., Araudo, A., Armstrong, T., Arqueros, F., Asano, K., … Živec, M. (2021). Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre. Journal of Cosmology and Astroparticle Physics, 2021(01), 057–057. https://doi.org/10.1088/1475-7516/2021/01/057

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Template for bound

I have added in the /templates/ folder a first proposal for the template file for the bounds. There are severa things to agree upon:

  • what columns do we put?
  • what metadata do we put?

I made a proposal: we can prepare one file per target per paper, including different channels (e.g. Segue in this paper for bb, tt channel). However, changing meta and columns we can change the number of files we generate (e.g. we can have one file per paper, one file per bound, etc). Think about it. It is clear that we better start with a final template for the data, so that later on importing would be easy.

MAGIC limits

Here is the limits provided by MAGIC (I will update this while adding files)

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