{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:QZE7B6YNQVTQ5G7DRGXXDB2AAL","short_pith_number":"pith:QZE7B6YN","schema_version":"1.0","canonical_sha256":"8649f0fb0d85670e9be389af71874002e4da0fc2322c97f42fe3b31b4f3f0c06","source":{"kind":"arxiv","id":"1108.2855","version":1},"attestation_state":"computed","paper":{"title":"Discovery of the source HESS J1356-645 associated with the young and energetic PSR J1357-6429","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Zdziarski, A. Balzer, A. Barnacka, A. Bochow, A.C. Clapson, A. Charbonnier, A. Cheesebrough, A. Djannati-Ata\\\"i, A. Fiasson, A. F\\\"orster, A.G. Akhperjanian, A. Hoffmann, A. Jacholkowska, A. Lopatin, A. Marcowith, A. Quirrenbach, A. Reimer, A. Santangelo, A. Schulz, A. Szostek, A. Viana, A. Wierzcholska, A. Zajczyk, A. Zech, B. Behera, B. Degrange, B. Giebels, B. Gl\\\"uck, B. Kh\\'elifi, B. Nicholas, B. Opitz, B. Rudak, C. Boisson, C.B. Rulten, C.-C. Lu, C. Deil, C. Farnier, C. Jahn, C.L. Naumann, C. Stegmann, C. van Eldik, C. Venter, D. Gerbig, D. G\\\"oring, D. Hampf, D. Horns, D. Keogh, D. Khangulyan, D. Klochkov, D. Lennarz, D. Maurin, D. Nedbal, D. Nekrassov, D. Sanchez, E. de Ona Wilhelmi, E. Moulin, F. Acero, F. Aharonian, F. Brun, F. Dubois, F. Feinstein, F.M. Sch\\\"ock, F. Rieger, F. Stinzing, F. Volpe, G. Anton, G. Coignet, G. Cologna, G. Dubus, G. Fontaine, G. Heinzelmann, G. Henri, G. Hermann, G. Lamanna, G. Pedaletti, G. Pelletier, G. P\\\"uhlhofer, G. Rowell, G. Spengler, G. Vasileiadis, HESS Collaboration: A. Abramowski, H. Gast, H.J. Dickinson, H.J. V\\\"olk, H. Laffon, H. Sol, H.-S. Zechlin, I. B\\\"usching, I.D. Davids, I. Jung, I. Oya, I. Sushch, J.A. Hinton, J. Becker, J. Bolmont, J. Brucker, J. Conrad, J.D. Hague, J. Dyks, J.F. Glicenstein, J.L. Skilton, J. Masbou, J. M\\'ehault, J. Niemiec, J.-P. Tavernet, J.P. Vialle, J. Ripken, J. Ruppel, K. Bernl\\\"ohr, K. Dutson, K. Egberts, K. Katarzynski, K. Kosack, K. Stycz, K. Valerius, L. Fallon, L. G\\'erard, L.-M. Chounet, L.O'C. Drury, L. Rob, L. Stawarz, M.A. Kastendieck, M. Cerruti, M.C. Medina, M. Dalton, M. de Naurois, M. Dyrda, M. F\\\"ussling, M. Hauser, M. Holler, M. Jamrozy, M.K. Daniel, M. Mayer, M. Naumann-Godo, M. Ostrowski, M. Panter, M. Paz Arribas, M. Punch, M. Raue, M. Renaud, M. Sikora, M. Tluczykont, M.V. Fernandes, M. Vorster, M. Ward, M. Zacharias, N. Maxted, N. Nguyen, Nu. Komin, O.C. de Jager, O. Reimer, P. Bordas, P. Brun, P. Eger, P. Espigat, P. Goret, P. Hofverberg, P.M. Chadwick, P.-O. Petrucci, P. Vincent, R.C.G. Chaves, R. de los Reyes, R. Kossakowski, R. Moderski, R. Schlickeiser, R. Steenkamp, R. Terrier, R. White, S. Carrigan, S. Casanova, S. Fegan, S. H\\\"affner, S. Heinz, S.J. Nolan, S.J. Wagner, S. Kaufmann, S.M. Rayner, S. Ohm, S. Pita, S. Rosier-Lees, S. Schwarzburg, S. Schwemmer, S. Vorobiov, T. Bulik, T.J.L. McComb, T. Kneiske, T. Lohse, U. Barres de Almeida, U. Katz, U. Schwanke, V. Marandon, V. Sahakian, W. Domainko, W. Hofmann, W. Kluzniak, Y.A. Gallant, Y. Becherini","submitted_at":"2011-08-14T10:16:06Z","abstract_excerpt":"Several newly discovered very-high-energy (VHE; E > 100 GeV) gamma-ray sources in the Galaxy are thought to be associated with energetic pulsars. Among them, middle-aged (> 1E+4 yr) systems exhibit large centre-filled VHE nebulae, offset from the pulsar position, which result from the complex relationship between the pulsar wind and the surrounding medium, and reflect the past evolution of the pulsar. Imaging Atmospheric Cherenkov Telescopes (IACTs) have been successful in revealing extended emission from these sources in the VHE regime. Together with radio and X-ray observations, this observa"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1108.2855","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-08-14T10:16:06Z","cross_cats_sorted":[],"title_canon_sha256":"a8483db04cd7dd14371ee869b573163fab8d0e5828b6d3dcf2755963c8efead5","abstract_canon_sha256":"8b168517c190a7626c93aca9c9f8c050fbc66bbec9ad3f4bea9aea8211ac0d66"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:54.185974Z","signature_b64":"QR6UqcfmoQMuFfMute5YmCJCOVqiWmHIO8TWBSix/dVtBVOK91D3eWbn6/v1w6CsgPPqdo6C+V8VRI2DCh70Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8649f0fb0d85670e9be389af71874002e4da0fc2322c97f42fe3b31b4f3f0c06","last_reissued_at":"2026-05-18T02:00:54.185197Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:54.185197Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery of the source HESS J1356-645 associated with the young and energetic PSR J1357-6429","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Zdziarski, A. Balzer, A. Barnacka, A. Bochow, A.C. Clapson, A. Charbonnier, A. Cheesebrough, A. Djannati-Ata\\\"i, A. Fiasson, A. F\\\"orster, A.G. Akhperjanian, A. Hoffmann, A. Jacholkowska, A. Lopatin, A. Marcowith, A. Quirrenbach, A. Reimer, A. Santangelo, A. Schulz, A. Szostek, A. Viana, A. Wierzcholska, A. Zajczyk, A. Zech, B. Behera, B. Degrange, B. Giebels, B. Gl\\\"uck, B. Kh\\'elifi, B. Nicholas, B. Opitz, B. Rudak, C. Boisson, C.B. Rulten, C.-C. Lu, C. Deil, C. Farnier, C. Jahn, C.L. Naumann, C. Stegmann, C. van Eldik, C. Venter, D. Gerbig, D. G\\\"oring, D. Hampf, D. Horns, D. Keogh, D. Khangulyan, D. Klochkov, D. Lennarz, D. Maurin, D. Nedbal, D. Nekrassov, D. Sanchez, E. de Ona Wilhelmi, E. Moulin, F. Acero, F. Aharonian, F. Brun, F. Dubois, F. Feinstein, F.M. Sch\\\"ock, F. Rieger, F. Stinzing, F. Volpe, G. Anton, G. Coignet, G. Cologna, G. Dubus, G. Fontaine, G. Heinzelmann, G. Henri, G. Hermann, G. Lamanna, G. Pedaletti, G. Pelletier, G. P\\\"uhlhofer, G. Rowell, G. Spengler, G. Vasileiadis, HESS Collaboration: A. Abramowski, H. Gast, H.J. Dickinson, H.J. V\\\"olk, H. Laffon, H. Sol, H.-S. Zechlin, I. B\\\"usching, I.D. Davids, I. Jung, I. Oya, I. Sushch, J.A. Hinton, J. Becker, J. Bolmont, J. Brucker, J. Conrad, J.D. Hague, J. Dyks, J.F. Glicenstein, J.L. Skilton, J. Masbou, J. M\\'ehault, J. Niemiec, J.-P. Tavernet, J.P. Vialle, J. Ripken, J. Ruppel, K. Bernl\\\"ohr, K. Dutson, K. Egberts, K. Katarzynski, K. Kosack, K. Stycz, K. Valerius, L. Fallon, L. G\\'erard, L.-M. Chounet, L.O'C. Drury, L. Rob, L. Stawarz, M.A. Kastendieck, M. Cerruti, M.C. Medina, M. Dalton, M. de Naurois, M. Dyrda, M. F\\\"ussling, M. Hauser, M. Holler, M. Jamrozy, M.K. Daniel, M. Mayer, M. Naumann-Godo, M. Ostrowski, M. Panter, M. Paz Arribas, M. Punch, M. Raue, M. Renaud, M. Sikora, M. Tluczykont, M.V. Fernandes, M. Vorster, M. Ward, M. Zacharias, N. Maxted, N. Nguyen, Nu. Komin, O.C. de Jager, O. Reimer, P. Bordas, P. Brun, P. Eger, P. Espigat, P. Goret, P. Hofverberg, P.M. Chadwick, P.-O. Petrucci, P. Vincent, R.C.G. Chaves, R. de los Reyes, R. Kossakowski, R. Moderski, R. Schlickeiser, R. Steenkamp, R. Terrier, R. White, S. Carrigan, S. Casanova, S. Fegan, S. H\\\"affner, S. Heinz, S.J. Nolan, S.J. Wagner, S. Kaufmann, S.M. Rayner, S. Ohm, S. Pita, S. Rosier-Lees, S. Schwarzburg, S. Schwemmer, S. Vorobiov, T. Bulik, T.J.L. McComb, T. Kneiske, T. Lohse, U. Barres de Almeida, U. Katz, U. Schwanke, V. Marandon, V. Sahakian, W. Domainko, W. Hofmann, W. Kluzniak, Y.A. Gallant, Y. Becherini","submitted_at":"2011-08-14T10:16:06Z","abstract_excerpt":"Several newly discovered very-high-energy (VHE; E > 100 GeV) gamma-ray sources in the Galaxy are thought to be associated with energetic pulsars. Among them, middle-aged (> 1E+4 yr) systems exhibit large centre-filled VHE nebulae, offset from the pulsar position, which result from the complex relationship between the pulsar wind and the surrounding medium, and reflect the past evolution of the pulsar. Imaging Atmospheric Cherenkov Telescopes (IACTs) have been successful in revealing extended emission from these sources in the VHE regime. Together with radio and X-ray observations, this observa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.2855","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1108.2855","created_at":"2026-05-18T02:00:54.185330+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.2855v1","created_at":"2026-05-18T02:00:54.185330+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.2855","created_at":"2026-05-18T02:00:54.185330+00:00"},{"alias_kind":"pith_short_12","alias_value":"QZE7B6YNQVTQ","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_16","alias_value":"QZE7B6YNQVTQ5G7D","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_8","alias_value":"QZE7B6YN","created_at":"2026-05-18T12:26:39.201973+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL","json":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL.json","graph_json":"https://pith.science/api/pith-number/QZE7B6YNQVTQ5G7DRGXXDB2AAL/graph.json","events_json":"https://pith.science/api/pith-number/QZE7B6YNQVTQ5G7DRGXXDB2AAL/events.json","paper":"https://pith.science/paper/QZE7B6YN"},"agent_actions":{"view_html":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL","download_json":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL.json","view_paper":"https://pith.science/paper/QZE7B6YN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.2855&json=true","fetch_graph":"https://pith.science/api/pith-number/QZE7B6YNQVTQ5G7DRGXXDB2AAL/graph.json","fetch_events":"https://pith.science/api/pith-number/QZE7B6YNQVTQ5G7DRGXXDB2AAL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL/action/storage_attestation","attest_author":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL/action/author_attestation","sign_citation":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL/action/citation_signature","submit_replication":"https://pith.science/pith/QZE7B6YNQVTQ5G7DRGXXDB2AAL/action/replication_record"}},"created_at":"2026-05-18T02:00:54.185330+00:00","updated_at":"2026-05-18T02:00:54.185330+00:00"}