{"paper":{"title":"Constraints on the Galactic Population of TEV Pulsar Wind Nebulae Using Fermi Large Area Telescope Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Allafort, A. B. Hill, A. Chekhtman, A. Drlica-Wagner, A. Franckowiak, A. K. Harding, A. Morselli, A. Okumura, A. Reimer, A. Schulz, A. S. Johnson, B. L. Winer, C. Cecchi, C. D. Dermer, C. Favuzzi, C. Monte, C. Sgr\\`o, D. A. Smith, D. Bastieri, D. F. Torres, D. Gasparrini, D. Hadasch, D. Horan, D. J. Suson, D. J. Thompson, D. Paneque, E. Bonamente, E. Bottacini, E. C. Ferrara, E. Charles, E. D. Bloom, E. do Couto e Silva, E. Hays, E. J. Siskind, E. Nuss, E. Orlando, E. Troja, F. Acero, F. D'Ammando, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Massaro, F. Piron, G. A. Caliandro, G. Barbiellini, G. Chiaro, G. Godfrey, G. J\\'ohannesson, G. Pivato, G. Spandre, G. Tosti, G. Vianello, H. Takahashi, I. A. Grenier, I. V. Moskalenko, J. Ballet, J. Bregeon, J. B. Thayer, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. E. Grove, J. E. McEnery, J. F. Ormes, J. G. Thayer, J. Hewitt, J. H. Panetta, J. Kn\\\"odlseder, J. Lande, J. Mehault, J. S. Perkins, J. Vandenbroucke, K. Bechtol, K. Hayashi, K. S. Wood, L. Baldini, L. Di Venere, L. Falletti, L. Latronico, L. Tibaldo, M. Ackermann, M. Ajello, M. Brigida, M. Dalton, M. E. Monzani, M. Giroletti, M. Hayashida, M.-H. Grondin, M. Kerr, M. Kuss, M. Lemoine-Goumard, M. Marelli, M. Mayer, M. N. Lovellette, M. N. Mazziotta, M. Orienti, M. Pesce-Rollins, M. Razzano, M. Roth, M. S. Jackson, M. Tinivella, M. Werner, N. Giglietto, O. Reimer, O. Tibolla, P. A. Caraveo, P. Bruel, P. F. Michelson, P. Fusco, P. Lubrano, P. M. Saz Parkinson, P. S. Drell, P. Spinelli, R. A. Cameron, R. Bellazzini, R. Buehler, R.C.G. Chaves, R. Claus, R. D. Blandford, R. E. Hughes, R. Nemmen, R. Rando, R. Rousseau, S. Buson, S. Ciprini, S. Cutini, S. Funk, S. Guiriec, S. J. Fegan, S. Larsson, S. Murgia, S. Rain\\`o, S. Ritz, T. A. Porter, T. Glanzman, T. Gr\\'egoire, T. J. Brandt, T. Jogler, T. Kamae, T. Kawano, T. Mizuno, T. Nakamori, T. Ohsugi, T. Reposeur, V. Vasileiou, V. Vitale, W. B. Focke, W. Mitthumsiri, X. Hou, Y. Fukazawa, Y. Hanabata, Y. Inoue, Y. Takeuchi, Y. Uchiyama, Z. Yang","submitted_at":"2013-06-24T19:58:23Z","abstract_excerpt":"Pulsar wind nebulae (PWNe) have been established as the most populous class of TeV gamma-ray emitters. Since launch, the Fermi Large Area Telescope (LAT)identified five high-energy (100MeV <E< 100 GeV) gamma-ray sources as PWNe, and detected a large number of PWNe candidates, all powered by young and energetic pulsars. The wealth of multi-wavelength data available and the new results provided by Fermi-LAT give us an opportunity to find new PWNe and to explore the radiative processes taking place in known ones. The TeV gamma-ray unidentifiedsources (UNIDs) are the best candidates for finding ne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.5735","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}