Searches for dark matter annihilation signatures in the Segue 1 satellite galaxy with the MAGIC-I telescope
| dc.contributor.author | Antoranz Canales, Pedro | |
| dc.contributor.author | Barrio Uña, Juan Abel | |
| dc.contributor.author | Contreras González, José Luis | |
| dc.contributor.author | Fonseca González, María Victoria | |
| dc.contributor.author | López Moya, Marcos | |
| dc.contributor.author | Miranda Pantoja, José Miguel | |
| dc.contributor.author | Scapin, Valeria | |
| dc.date.accessioned | 2023-06-20T03:33:56Z | |
| dc.date.available | 2023-06-20T03:33:56Z | |
| dc.date.issued | 2011-06 | |
| dc.description | © 2011 IOP Publishing Ltd and SISSA. We would like to thank the Instituto de Astrofisica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. The support of the German BMBF and MPG, the Italian INFN, the Swiss National Fund SNF, and the Spanish MICINN is gratefully acknowledged. This work was also supported by the Marie Curie program, by the CPAN CSD2007-00042 and MultiDark CSD2009-00064 projects of the Spanish Consolider-Ingenio 2010 programme, by grant DO02-353 of the Bulgarian NSF, by grant 127740 of the Academy of Finland, by the YIP of the Helmholtz Gemeinschaft, by the DFG Cluster of Excellence "Origin and Structure of the Universe", and by the Polish MNiSzW grant 745/N-HESS-MAGIC/2010/0. | |
| dc.description.abstract | We report the results of the observation of the nearly satellite galaxy Segue 1 performed by the MAGIC-I ground-based gamma-ray telescope between November 2008 and March 2009 for a total of 43.2 hours. No significant gamma-ray emission was found above the bmkground. Differential upper limits on the grimma-ray flux are derived assuming various power-law slopes for the possible emission spectrum. Integral upper limits are also calculated for several power-law spectra and for different energy thresholds. The values are of the order of 10(-11) ph cm(-2) s(-1) above 100 GeV and 10(-12) ph cm(-2) s(-1) above 200 GeV. Segue 1 is currently considered one of the most interesting targets for indirect dark matter searches. In these terms, the upper limits have been also interpreted in the context of annihilating dark matter particles. For such purpose, we performed a grid scan over a reasonable portion of the parameter space for the minimal SuperGravity model and computed the flux upper limit for each point separately, taking fully into account the peculiar spectral features of each model. We found that in order to match the experimental upper limits with the model predictions, a minimum flux boost of 10(3) is required, and that the upper limits are quite dependent on the shape of the gamma-ray energy spectrum predicted by each specific model. Finally we compared the upper limits with the predictions of some dark matter models able to explain the PAMELA rise in the positron ratio, finding that Segue 1 data are in tension with the dark matter explanation of the PAMELA spectrum in the case of a dark matter candidate annihilating into tau(+)tau(-). A complete exclusion however is not possible due to the uncertainties in the Segue 1 astrophysical factor. | |
| dc.description.department | Depto. de Estructura de la Materia, Física Térmica y Electrónica | |
| dc.description.faculty | Fac. de Ciencias Físicas | |
| dc.description.refereed | TRUE | |
| dc.description.sponsorship | German BMBF | |
| dc.description.sponsorship | German MPG | |
| dc.description.sponsorship | Italian INFN | |
| dc.description.sponsorship | Swiss National Fund SNF | |
| dc.description.sponsorship | Spanish MICINN | |
| dc.description.sponsorship | Marie Curie program | |
| dc.description.sponsorship | Spanish Consolider-Ingenio 2010 programme | |
| dc.description.sponsorship | Bulgarian NSF | |
| dc.description.sponsorship | Academy of Finland | |
| dc.description.sponsorship | YIP of the Helmholtz Gemeinschaft | |
| dc.description.sponsorship | DFG | |
| dc.description.sponsorship | Polish MNiSzW | |
| dc.description.status | pub | |
| dc.eprint.id | https://eprints.ucm.es/id/eprint/22091 | |
| dc.identifier.doi | 10.1088/1475-7516/2011/06/035 | |
| dc.identifier.issn | 1475-7516 | |
| dc.identifier.officialurl | http://dx.doi.org/10.1088/1475-7516/2011/06/035 | |
| dc.identifier.relatedurl | http://iopscience.iop.org | |
| dc.identifier.uri | https://hdl.handle.net/20.500.14352/43891 | |
| dc.issue.number | 6 | |
| dc.journal.title | Journal of Cosmology and Astroparticle Physics | |
| dc.language.iso | eng | |
| dc.publisher | Iop Publishing Ltd | |
| dc.relation.projectID | CSD2007-00042 | |
| dc.relation.projectID | CSD2009-00064 | |
| dc.relation.projectID | DO02-353 | |
| dc.relation.projectID | 127740 | |
| dc.relation.projectID | 745/N-HESS-MAGIC/2010/0 | |
| dc.rights | Atribución 3.0 España | |
| dc.rights.accessRights | open access | |
| dc.rights.uri | https://creativecommons.org/licenses/by/3.0/es/ | |
| dc.subject.cdu | 537 | |
| dc.subject.cdu | 539.1 | |
| dc.subject.keyword | Gamma-Ray Emission | |
| dc.subject.keyword | Dwarf Spheroidal Galaxies | |
| dc.subject.keyword | Large-Area Telescope | |
| dc.subject.keyword | Milky-Way Halo | |
| dc.subject.keyword | Spectroscopic Survey | |
| dc.subject.keyword | Galactic Satellites | |
| dc.subject.keyword | Particle | |
| dc.subject.keyword | Fermi | |
| dc.subject.keyword | Constraints | |
| dc.subject.keyword | Energies. | |
| dc.subject.ucm | Electrónica (Física) | |
| dc.subject.ucm | Electricidad | |
| dc.subject.ucm | Física nuclear | |
| dc.subject.unesco | 2202.03 Electricidad | |
| dc.subject.unesco | 2207 Física Atómica y Nuclear | |
| dc.title | Searches for dark matter annihilation signatures in the Segue 1 satellite galaxy with the MAGIC-I telescope | |
| dc.type | journal article | |
| dcterms.references | [1] CoGeNT collaboration, C.E. Aalseth et al., Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector, Phys. Rev. Lett. 106 (2011) 131301 [arXiv:1002.4703] [SPIRES]. [2] The Fermi LAT collaboration, A.A. Abdo et al., Measurement of the Cosmic Ray e+ plus espectrum from 20GeV to 1TeV with the Fermi Large Area Telescope, Phys. Rev. Lett. 102 (2009) 181101 [arXiv:0905.0025] [SPIRES]. [3] A.A. Abdo et al., Observations of Milky Way Dwarf Spheroidal galaxies with the Fermi-LAT detector and constraints on Dark Matter models, Astrophys. J. 712 (2010) 147 [arXiv:1001.4531] [SPIRES]. [4] The VERITAS collaboration, et al., VERITAS Search for VHE Gamma-ray Emission from Dwarf Spheroidal Galaxies, Astrophys. J. 720 (2010) 1174 [arXiv:1006.5955] [SPIRES]. [5] PAMELA collaboration, O. Adriani et al., An anomalous positron abundance in cosmic rays with energies 1.5–100 GeV, Nature 458 (2009) 607 [arXiv:0810.4995] [SPIRES]. [6] HESS collaboration, . F. Aharonian, Observations of the Sagittarius Dwarf galaxy by the H.E.S.S. experiment and search for a Dark Matter signal, Astropart. Phys. 29 (2008) 55 [arXiv:0711.2369] [SPIRES]. [7] H.E.S.S. collaboration, F. Aharonian et al., Probing the ATIC peak in the cosmic-ray electron spectrum with H.E.S.S, Astron. Astrophys. 508 (2009) 561 [arXiv:0905.0105] [SPIRES]. [8] HESS collaboration, . F. Aharonian, A search for a dark matter annihilation signal towards the Canis Major overdensity with H.E.S.S, arXiv:0809.3894 [SPIRES]. [9] The CDMS-II collaboration, Z. Ahmed et al., Dark Matter Search Results from the CDMS II Experiment, Science 327 (2010) 1619 [arXiv:0912.3592] [SPIRES]. [10] MAGIC collaboration, J. Albert et al., VHE Gamma-Ray Observation of the Crab Nebula and its Pulsar with the MAGIC telescope, Astrophys. J. 674 (2008) 1037 [arXiv:0705.3244] [SPIRES]. [11] MAGIC collaboration, J. Albert et al., Upper limit for gamma-ray emission above 140GeV from the dwarf spheroidal galaxy Draco, Astrophys. J. 679 (2008) 428 [arXiv:0711.2574][SPIRES]. [12] J. Albert et al., Implementation of the Random Forest Method for the Imaging Atmospheric Cherenkov Telescope MAGIC, Nucl. Instrum. Meth. A 588 (2008) 424 [arXiv:0709.3719] [SPIRES]. [13] MAGIC collaboration, J. Albert et al., FADC signal reconstruction for the MAGIC telescope, Nucl. Instrum. Meth. A 594 (2008) 407 [astro-ph/0612385] [SPIRES]. [14] MAGIC collaboration, E. Aliu et al., MAGIC upper limits on the VHE gamma-ray emission from the satellite galaxy Willman 1, Astrophys. J. 697 (2009) 1299 [arXiv:0810.3561] [SPIRES]. [15] T. Appelquist, H.-C. Cheng and B.A. Dobrescu, Bounds on universal extra dimensions, Phys. Rev. D 64 (2001) 035002 [hep-ph/0012100] [SPIRES]. [16] XENON100 collaboration, E. Aprile et al., First Dark Matter Results from the XENON100 Experiment, Phys. Rev. Lett. 105 (2010) 131302 [arXiv:1005.0380] [SPIRES]. [17] N. Arkani-Hamed, D.P. Finkbeiner, T.R. Slatyer and N. Weiner, A Theory of Dark Matter, Phys. Rev. D 79 (2009) 015014 [arXiv:0810.0713] [SPIRES]. [18] LAT collaboration, W.B. Atwood et al., The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission, Astrophys. J. 697 (2009) 1071 [arXiv:0902.1089] [SPIRES]. [19] F.E. Paige, S.D. Protopopescu, H. Baer and X. Tata, ISAJET 7.69: A Monte Carlo event generator for pp, ￣pp and e+e− reactions, hep-ph/0312045 [SPIRES]. [20] E.A. Baltz et al., Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation ignals, JCAP 07 (2008) 013 [arXiv:0806.2911] [SPIRES]. [21] SDSS collaboration, V. Belokurov et al., Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions, Astrophys. J. 654 (2007) 897 [astro-ph/0608448] [SPIRES]. [22] L. Bergstrom, P. Ullio and J.H. Buckley, Observability of gamma rays from dark matter neutralino annihilations in the Milky Way halo, Astropart. Phys. 9 (1998) 137 [astro-ph/9712318] [SPIRES]. [23] L. Bergstrom, J. Edsjo and G. Zaharijas, Dark matter interpretation of recent electron and positron data, Phys. Rev. Lett. 103 (2009) 031103 [arXiv:0905.0333] [SPIRES]. [24] DAMA collaboration, R. Bernabei et al., First results from DAMA/LIBRA and the combined results with DAMA/NaI, Eur. Phys. J. C 56 (2008) 333 [arXiv:0804.2741] [SPIRES]. [25] G. Bertone, D. Hooper and J. Silk, Particle dark matter: Evidence, candidates and constraints, Phys. Rept. 405 (2005) 279 [hep-ph/0404175] [SPIRES]. [26] L. Beiman, Random Forests, Mach. Learn. 45 (2001) 5. [27] T. Bringmann, L. Bergstrom and J. Edsjo, New Gamma-Ray Contributions to Supersymmetric Dark Matter Annihilation, JHEP 01 (2008) 049 [arXiv:0710.3169] [SPIRES]. [28] T. Bringmann, M. Doro and M. Fornasa, Dark Matter signals from Draco and Willman 1: Prospects for MAGIC II and CTA, JCAP 01 (2009) 016 [arXiv:0809.2269] [SPIRES]. [29] J.A.R. Cembranos, A. de la Cruz-Dombriz, A. Dobado, R.A. Lineros and A.L. Maroto, Photon spectra from WIMP annihilation, Phys. Rev. D 83 (2011) 083507 [arXiv:1009.4936] [SPIRES]. [30] A.H. Chamseddine, R.L. Arnowitt and P. Nath, Locally Supersymmetric Grand Unification, Phys. Rev. Lett. 49 (1982) 970. [31] J. Chang et al., An excess of cosmic ray electrons at energies of 300–800 GeV, Nature 456 (2008) 362. [32] S. Chang, J. Liu, A. Pierce, N. Weiner and I. Yavin, CoGeNT Interpretations, JCAP 08 (2010) 018 [arXiv:1004.0697] [SPIRES]. [33] H.-C. Cheng, K.T. Matchev and M. Schmaltz, Bosonic supersymmetry? Getting fooled at the CERN LHC, Phys. Rev. D 66 (2002) 056006 [hep-ph/0205314] [SPIRES]. [34] I. Cholis, D.P. Finkbeiner, L. Goodenough and N. Weiner, The PAMELA Positron Excess from Annihilations into a Light Boson, JCAP 12 (2009) 007 [arXiv:0810.5344] [SPIRES]. [35] I. Cholis, G. Dobler, D.P. Finkbeiner, L. Goodenough and N. Weiner, The Case for a 700+ GeV WIMP: Cosmic Ray Spectra from ATIC and PAMELA, Phys. Rev. D 80 (2009) 123518[arXiv:0811.3641] [SPIRES]. [36] M. Cirelli, M. Kadastik, M. Raidal and A. Strumia, Model-independent implications of the e+, e-, anti-proton cosmic ray spectra on properties of Dark Matter, Nucl. Phys. B 813 (2009) 1 [arXiv:0809.2409] [SPIRES]. [37] D. Clowe et al., A direct empirical proof of the existence of dark matter, Astrophys. J. 648 (2006) L109 [astro-ph/0608407] [SPIRES]. [38] S. Colafrancesco, S. Profumo and P. Ullio, Detecting dark matter WIMPs in the Draco dwarf: a multi-wavelength perspective, Phys. Rev. D 75 (2007) 023513 [astro-ph/0607073] [SPIRES]. [39] S. Colafrancesco, Dark Matter in Modern Cosmology, AIP Conf. Proc. 1206 (2010) 5 [arXiv:1004.3869] [SPIRES]. [40] for the MAGIC collaboration, P. Colin et al., Performance of the MAGIC telescopes in stereoscopic mode, arXiv:0907.0960 [SPIRES]. [41] J. Cortina, F. Goebel, T. Schweizer and f.t.M. Collaboration, Technical Performance of the MAGIC Telescopes, arXiv:0907.1211 [SPIRES]. [42] J. Diemand, M. Kuhlen and P. Madau, Dark matter substructure and gamma-ray annihilation in the Milky Way halo, Astrophys. J. 657 (2007) 262 [astro-ph/0611370] [SPIRES]. [43] J. Diemand et al., Clumps and streams in the local dark matter distribution, Nature 454 (2008) 735 [arXiv:0805.1244] [SPIRES]. [44] MAGIC collaboration, E. Domingo-Santamaria et al., The DISP analysis method for point-like or extended gamma source searches / studies with the MAGIC telescope, in The MAGIC Project. Contributions to ICRC 2005, Pune, India. Part 3: MAGIC detector and analysis details, contributed to 29th International Cosmic Ray Conference (ICRC 2005), Pune India, 3-11 Aug. 2005, pg. 23–27 [astro-ph/0508274] [SPIRES]. [45] R. Essig, N. Sehgal and L.E. Strigari, Bounds on Cross-sections and Lifetimes for Dark Matter Annihilation and Decay into Charged Leptons from Gamma-ray Observations of Dwarf Galaxies, Phys. Rev. D 80 (2009) 023506 [arXiv:0902.4750] [SPIRES]. [46] R. Essig, N. Sehgal, L.E. Strigari, M. Geha and J.D. Simon, Indirect Dark Matter Detection Limits from the Ultra-Faint Milky Way Satellite Segue 1, Phys. Rev. D 82 (2010) 123503 [arXiv:1007.4199] [SPIRES]. [47] D.P. Finkbeiner, L. Goodenough, T.R. Slatyer, M. Vogelsberger and N. Weiner, Consistent Scenarios for Cosmic-Ray Excesses from Sommerfeld-Enhanced Dark Matter Annihilation, JCAP 05 (2011) 002 [arXiv:1011.3082] [SPIRES]. [48] V.P. Fomin et al., New methods of atmospheric Cherenkov imaging for gamma-ray astronomy. 1: The False source method, Astropart. Phys. 2 (1994) 137. [49] N. Fornengo, L. Pieri and S. Scopel, Neutralino annihilation into gamma-rays in the Milky Way and in external galaxies, Phys. Rev. D 70 (2004) 103529 [hep-ph/0407342] [SPIRES]. [50] M. Geha, The Least Luminous Galaxy: Spectroscopy of the Milky Way Satellite Segue 1, Astrophys. J. 692 (2009) 1464 [arXiv:0809.2781] [SPIRES]. [51] G. Gilmore et al., The Observed properties of Dark Matter on small spatial scales, Astrophys. J. 663 (2007) 948 [astro-ph/0703308] [SPIRES]. [52] P. Gondolo et al., DarkSUSY: Computing supersymmetric dark matter properties numerically, JCAP 07 (2004) 008 [astro-ph/0406204] [SPIRES]. [53] A.M. Green, S. Hofmann and D.J. Schwarz, The power spectrum of SUSY-CDM on sub-galactic scales, Mon. Not. Roy. Astron. Soc. 353 (2004) L23 [astro-ph/0309621] [SPIRES]. [54] A.M. Hillas, Cherenkov Images of EAS produced by primary gamma rays and by nuclei, Proceedings of the 19th International Cosmic Ray Conference. Vol.3, La Jolla U.S.A. (1985), pg. 445. [55] D. Hooper, P. Blasi and P.D. Serpico, Pulsars as the Sources of High Energy Cosmic Ray Positrons, JCAP 01 (2009) 025 [arXiv:0810.1527] [SPIRES]. [56] T.C. Consortium, Design Concepts for the Cherenkov Telescope Array, arXiv:1008.3703 [SPIRES]. [57] G. Jungman, M. Kamionkowski and K. Griest, Supersymmetric dark matter, Phys. Rept. 267 (1996) 195 [hep-ph/9506380] [SPIRES]. [58] A.A. Klypin, A.V. Kravtsov, O. Valenzuela and F. Prada, Where are the missing galactic satellites?, Astrophys. J. 522 (1999) 82 [astro-ph/9901240] [SPIRES]. [59] WMAP collaboration, E. Komatsu et al., Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, Astrophys. J. Suppl. 192 (2011) 18 [arXiv:1001.4538] [SPIRES]. [60] A.V. Kravtsov, A.A. Klypin, J.S. Bullock and J.R. Primack, The Cores of Dark Matter Dominated Galaxies: theory vs. observations, Astrophys. J. 502 (1998) 48 [astro-ph/9708176] [SPIRES]. [61] A.V. Kravtsov, O.Y. Gnedin and A.A. Klypin, The tumultuous lives of galactic dwarfs and the missing satellites problem, Astrophys. J. 609 (2004) 482 [astro-ph/0401088] [SPIRES]. [62] M. Lattanzi and J.I. Silk, Can the WIMP annihilation boost factor be boosted by the Sommerfeld enhancement?, Phys. Rev. D 79 (2009) 083523 [arXiv:0812.0360] [SPIRES]. [63] ZEPLIN-III collaboration, V.N. Lebedenko et al., Limits on the spin-dependent WIMP-nucleon cross-sections from the first science run of the ZEPLIN-III experiment, Phys. Rev. Lett. 103 (2009) 151302 [arXiv:0901.4348] [SPIRES]. [64] T.-P. Li and Y.-Q. Ma, Analysis methods for results in gamma-ray astronomy, Astrophys. J. 272 (1983) 317. [65] S.P. Martin, A Supersymmetry Primer, hep-ph/9709356 [SPIRES]. [66] N.F. Martin, R.A. Ibata, S.C. Chapman, M. Irwin and G.F. Lewis, A Keck/DEIMOS spectroscopic survey of faint Galactic satellites: Searching for the least massive dwarf galaxies, Mon. Not. Roy. Astron. Soc. 380 (2007) 281 [arXiv:0705.4622] [SPIRES]. [67] G.D. Martinez, J.S. Bullock, M. Kaplinghat, L.E. Strigari and R. Trotta, Indirect Dark Matter Detection from Dwarf Satellites: Joint Expectations from Astrophysics and Supersymmetry, JCAP 06 (2009) 014 [arXiv:0902.4715] [SPIRES]. [68] G.D. Martinez et al., A Complete Spectroscopic Survey of the Milky Way satellite Segue 1: Dark matter content, stellar membership and binary properties from a Bayesian analysis, arXiv:1008.4585 [SPIRES]. [69] P. Meade, M. Papucci, A. Strumia and T. Volansky, Dark Matter Interpretations of the Electron/Positron Excesses after FERMI, Nucl. Phys. B 831 (2010) 178 [arXiv:0905.0480][SPIRES]. [70] N. Mirabal, Swift observation of Segue 1: constraints on sterile neutrino parameters in the darkest galaxy, arXiv:1010.4706 [SPIRES]. [71] B. Moore et al., Dark Matter Substructure in Galactic Halos, astro-ph/9907411 [SPIRES]. [72] B. Moore, T.R. Quinn, F. Governato, J. Stadel and G. Lake, Cold collapse and the core catastrophe, Mon. Not. Roy. Astron. Soc. 310 (1999) 1147 [astro-ph/9903164] [SPIRES]. [73] J.F. Navarro, C.S. Frenk and S.D.M. White, A Universal Density Profile from Hierarchical Clustering, Astrophys. J. 490 (1997) 493 [astro-ph/9611107] [SPIRES]. [74] J.F. Navarro et al., The Diversity and Similarity of Cold Dark Matter Halos, arXiv:0810.1522 [SPIRES]. [75] H.P. Nills, Supersymmetry, Supergravity and Particle Physics, Phys. Rept. 110 (1984) 1. [76] M. Niederste-Ostholt et al., The Origin of Segue 1, Mon. Not. Roy. Astron. Soc. 398 (2009) 1771 [arXiv:0906.3669] [SPIRES]. [77] M. Persic, P. Salucci and F. Stel, The Universal rotation curve of spiral galaxies: 1. The Dark matter connection, Mon. Not. Roy. Astron. Soc. 281 (1996) 27 [astro-ph/9506004] [SPIRES]. [78] L. Pieri, G. Bertone and E. Branchini, Dark Matter Annihilation in Substructures Revised, Mon. Not. Roy. Astron. Soc. 384 1627 [arXiv:0706.2101] [SPIRES]. [79] L. Pieri, M. Lattanzi and J. Silk, Constraining the Sommerfeld enhancement with Cherenkov telescope observations of dwarf galaxies, Mon. Not. Roy. Astron. Soc. 399 (2009) 2033 [arXiv:0902.4330] [SPIRES]. [80] M. Pospelov and A. Ritz, Astrophysical Signatures of Secluded Dark Matter, Phys. Lett. B 671 (2009) 391 [arXiv:0810.1502] [SPIRES]. [81] S. Profumo, Dissecting Pamela (and ATIC) with Occam’s Razor: existing, well-known Pulsars naturally account for the ’anomalous’ Cosmic-Ray Electron and Positron Data, arXiv:0812.4457 [SPIRES]. [82] W.A. Rolke, A.M. Lopez and J. Conrad, Limits and confidence intervals in the presence of nuisance parameters, Nucl. Instrum. Meth. A 551 (2005) 493 [physics/0403059]. [83] P. Salucci, F. Nesti, G. Gentile and C.F. Martins, The dark matter density at the Sun’s location, Astron. Astrophys. 523 (2010) A83 [arXiv:1003.3101] [SPIRES]. [84] M.A. S´anchez-Conde et al., Dark matter annihilation in Draco: New considerations of the expected gamma flux, Phys. Rev. D 76 (2007) 123509 [astro-ph/0701426] [SPIRES]. [85] M.A. S´anchez-Conde, M. Cannoni, F. Zandanel, M.E. Gomez and F. Prada, Dark matter searches with Cherenkov telescopes: nearby dwarf galaxies or local galaxy clusters?, arXiv:1104.3530 [SPIRES]. [86] P. Scott et al., Direct Constraints on Minimal Supersymmetry from Fermi-LAT Observations of the Dwarf Galaxy Segue 1, JCAP 01 (2010) 031 [arXiv:0909.3300] [SPIRES]. [87] G. Servant and T.M.P. Tait, Is the lightest Kaluza-Klein particle a viable dark matter candidate?, Nucl. Phys. B 650 (2003) 391 [hep-ph/0206071] [SPIRES]. [88] J.D. Simon et al., A Complete Spectroscopic Survey of the Milky Way Satellite Segue 1: The Darkest Galaxy, Astrophys. J. 733 (2011) 46 [arXiv:1007.4198] [SPIRES]. [89] J.D. Simon and M. Geha, The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite Problem, Astrophys. J. 670 (2007) 313 [arXiv:0706.0516] [SPIRES]. [90] V. Springel, Prospects for detecting supersymmetric dark matter in the Galactic halo, Nature 456 (2008) 73. [91] V. Springel et al., The Aquarius Project: the subhalos of galactic halos, Mon. Not. Roy. Astron. Soc. 391 (2008) 1685 [arXiv:0809.0898] [SPIRES]. [92] L.E. Strigari, S.M. Koushiappas, J.S. Bullock and M. Kaplinghat, Precise constraints on the dark matter content of Milky Way dwarf galaxies for gamma-ray experiments, Phys. Rev. D 75 (2007) 083526 [astro-ph/0611925] [SPIRES]. [93] L.E. Strigari et al., Redefining the Missing Satellites Problem, Astrophys. J. 669 (2007) 676[arXiv:0704.1817] [SPIRES]. [94] P. Ullio, L. Bergstrom, J. Edsjo and C.G. Lacey, Cosmological dark matter annihilations into gamma-rays: A closer look, Phys. Rev. D 66 (2002) 123502 [astro-ph/0207125] [SPIRES]. [95] R.G. Wagner and f.t.V. Collaboration, Indirect Dark Matter Searches with VERITAS, arXiv:0910.4563 [SPIRES]. [96] M. Wood et al., A Search for Dark Matter Annihilation with the Whipple 10m Telescope, arXiv:0801.1708 [SPIRES]. [97] SDSS-II SEGUE collaboration, B. Yanny et al., SEGUE: A Spectroscopic Survey of 240,000 stars with g=14–20, Astron. J. 137 (2009) 4377 [arXiv:0902.1781] [SPIRES]. [98] H. Yuksel, M.D. Kistler and T. Stanev, TeV Gamma Rays from Geminga and the Origin of the GeV Positron Excess, Phys. Rev. Lett. 103 (2009) 051101 [arXiv:0810.2784] [SPIRES]. [99] M. Xiang-Gruess, Y.-Q. Lou and W.J. Duschl, Dark matter dominated dwarf disc galaxy Segue 1, arXiv:0909.3496 [SPIRES]. [100] G. Bertone eds., Particle Dark Matter, first edition, Cambridge University Press, Cambridge U.K. (2010). [101] C. Farnier, Dark Matter Annihilations Search In Dwarfs Spheroidal Galaxies With Fermi, talk at Roma International Conference in Astro-Particle Physics, Roma Italy (2009). [102] T. Jeltema, Searching for dark matter annihilation in dwarf spheroidal galaxies with Fermi, tolk at TEV Particle Astrophysics Conference, Menlo Park U.S.A. 13–17 July 2009. [103] S. Murgia, Search for dark matter and new physics, tolk at TEV Particle Astrophysics Conference, Menlo Park U.S.A. 13–17 July 2009. | |
| dspace.entity.type | Publication | |
| relation.isAuthorOfPublication | 6bc87e5f-9b77-4982-b112-0d4f8aa128d0 | |
| relation.isAuthorOfPublication | 11e5fd8b-1a86-4f8d-85c6-135541232be4 | |
| relation.isAuthorOfPublication | 6a14529e-a65e-4709-9bc1-61f9429841c1 | |
| relation.isAuthorOfPublication | 9f2c0e34-0edd-497a-bbd0-fbd9d348e85c | |
| relation.isAuthorOfPublication | 8b5d96d7-bd11-4ee4-87d0-258a1e077e26 | |
| relation.isAuthorOfPublication | 328f9716-2012-44f9-aacc-ef8d48782a77 | |
| relation.isAuthorOfPublication.latestForDiscovery | 6bc87e5f-9b77-4982-b112-0d4f8aa128d0 |
Download
Original bundle
1 - 1 of 1
