CLUMPY: a code for gamma-ray signals from dark matter structures
arXiv:1201.4728 · doi:10.1016/j.cpc.2011.10.017
Abstract
We present the first public code for semi-analytical calculation of the gamma-ray flux astrophysical J-factor from dark matter annihilation/decay in the Galaxy, including dark matter substructures. The core of the code is the calculation of the line of sight integral of the dark matter density squared (for annihilations) or density (for decaying dark matter). The code can be used in three modes: i) to draw skymaps from the Galactic smooth component and/or the substructure contributions, ii) to calculate the flux from a specific halo (that is not the Galactic halo, e.g. dwarf spheroidal galaxies) or iii) to perform simple statistical operations from a list of allowed DM profiles for a given object. Extragalactic contributions and other tracers of DM annihilation (e.g. positrons, antiprotons) will be included in a second release.
15 pages, 7 figures, published in CPC. The CLUMPY code and its documentation can be found at http://lpsc.in2p3.fr/clumpy
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- Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
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- Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
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- Sensitivity of the Cherenkov Telescope Array to the detection of a dark matter signal in comparison to direct detection and collider experiments
- Search for -ray emission from dark matter particle interactions from Andromeda and Triangulum Galaxies with the Fermi Large Area Telescope
- The Smith Cloud and its dark matter halo: Survival of a Galactic disc passage
- Decaying dark matter: a stacking analysis of galaxy clusters to improve on current limits
- Search for Gamma-ray Spectral Lines from Dark Matter Annihilation in Dwarf Galaxies with the High-Altitude Water Cherenkov Observatory
- Constraining the dark matter contribution of rays in Cluster of galaxies using Fermi-LAT data
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- Dark Matter Density Profiles in Dwarf Galaxies: Linking Jeans Modeling Systematics and Observation
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- Constraints on dark matter annihilation and decay from the large-scale structure of the nearby universe
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- Investigating the detection of dark matter subhalos as extended sources with Fermi-LAT
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- Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
- Search for Dark Matter Gamma-ray Emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory
- Dark Matter search in dwarf irregular galaxies with the Fermi Large Area Telescope
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- Gamma-ray sensitivity to dark matter subhalo modelling at high latitudes
- Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.S
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- Spatial extension of dark subhalos as seen by Fermi-LAT and implications for WIMP constraints
- Search for heavy dark matter from dwarf spheroidal galaxies: leveraging cascades and subhalo models
- Harnessing the Population Statistics of Subhalos to Search for Annihilating Dark Matter
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- Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
- Dependence of accessible dark matter annihilation cross-sections on the density profiles of dwarf spheroidal galaxies with the Cherenkov Telescope Array
- Indirect detection prospects for d(2380) dark matter
- Searching for dark matter subhalos in the Fermi-LAT catalog with Bayesian neural networks
- Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
- Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
- The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
- Statistics for dark matter subhalo searches in gamma rays from a kinematically constrained population model: Fermi-LAT-like telescopes
- Sensitivity of CTA to gamma-ray emission from the Perseus galaxy cluster
- How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
- Prospects for annihilating dark matter from M31 and M33 observations with the Cherenkov Telescope Array
- Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced - and -wave -ray signals
- Extragalactic Searches for Dark Matter Annihilation
- Search for Galactic dark matter substructures with Cherenkov telescopes