{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:VYE6MSYRHG2FRAO4QPLFNDVCAC","short_pith_number":"pith:VYE6MSYR","schema_version":"1.0","canonical_sha256":"ae09e64b1139b45881dc83d6568ea20095ef7b6a56c27a62383348ffed686b3d","source":{"kind":"arxiv","id":"1012.0908","version":1},"attestation_state":"computed","paper":{"title":"Sensitivity Studies for Third-Generation Gravitational Wave Observatories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. Chincarini, A. Cumming, A. Di Virgilio, A. Freise, A. Gennai, A. Giazotto, A. Gurkovsky, A. Paoli, A. Pasqualetti, A. Rocchi, A. R\\\"udiger, A. Sintes, A. Th\\\"uring, A. Vecchio, A. Vicere, B. Barr, B. Krishnan, B Mours, B. Sassolas, B. Sathyaprakash, B. Willke, C. Bradaschia, C. Colacino, C. D. Ott, C. Gr\\\"af, C. Michel, C. Palomba, C. Schwarz, C. Van Den Broeck, D. Friedrich, D. Heinert, D. Passuello, D. Rabeling, E. Calloni, E. Chassande Mottin, E. Coccia, E. Cuoco, E. Genin, E. Hennes, E. Majorana, F. Acernese, F. Barone, F. Frasconi, F. Khalili, F. Ricci, F. Richard, F. Speirits, F. Vetrano, G. Cella, G. Gemme, G. Guidi, G. Hammond, G. Jones, G. Parguez, G. Woan, H. Grote, H. L\\\"uck, H. M\\\"uller-Ebhardt, H. Rehbein, I. Heng, I. Mandel, I. Martin, J. Clark, J. Colas, J. Franc, J. Gair, J. Harms, J. Hough, J. Nelson, J. Read, J. van den Brand, J. Veitch, K. Arun, K. Danzmann, K. Glampedakis, K. Kokeyama, K. Kokkotas, K. Somiya, K. Strain, K. Yamamoto, L. Bosi, L. Cunningham, L. Di Fiore, L. Pinard, L. Santamar\\'ia, M. Abernathy, M. Barsuglia, M. Beker, M. Doets, M. Granata, M. Hannam, M. Hendry, M. Lorenzini, M. Mantovani, M. Prato, M. Punturo, M. van Veggel, N. Andersson, N. Beveridge, N. Morgado, P. Amaro-Seoane, P. Falferi, P. Fulda, P. Murray, P. Popolizio, P. Puppo, P. Rapagnani, P. Seidel, P. Sutton, R. De Rosa, R. De Salvo, R. Flaminio, R. Nawrodt, R. Oshaughnessy, R. Passaquieti, R. Poggiani1, R. Schnabel, S. Birindelli, S. Bose, S. Braccini, S. Chelkowski, S. Danilishin, S. Hild, S. Husa, S. Huttner, S. Mosca, S. Reid, S. Rowan, S Strigin, S. Tarabrin, S. Vyatchanin, T. Bulik, T. Dent, T.G.F. Li, T. Regimbau, V. Fafone, V. Mandic, W. Plastino, Y. Minenkov","submitted_at":"2010-12-04T12:17:06Z","abstract_excerpt":"Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension t"},"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":"1012.0908","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-12-04T12:17:06Z","cross_cats_sorted":[],"title_canon_sha256":"de2b50bbb8f290b898880c01269c5ad03257ba4cd1da512112909c33849e1afe","abstract_canon_sha256":"a6f96467ecaaf27efb3ad4159c655fb8970af0ef7cf16216d17df62211e29334"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:33.011258Z","signature_b64":"f87RKhbx3HYuNuhokQDj9DPVKf4YJCZ25e1FFG+1BJhuhJNwxy0pE9WbQ0Hglzz/8LiDsQNbaLi5ZdCoRQvkAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae09e64b1139b45881dc83d6568ea20095ef7b6a56c27a62383348ffed686b3d","last_reissued_at":"2026-05-18T02:04:33.010517Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:33.010517Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Sensitivity Studies for Third-Generation Gravitational Wave Observatories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. Chincarini, A. Cumming, A. Di Virgilio, A. Freise, A. Gennai, A. Giazotto, A. Gurkovsky, A. Paoli, A. Pasqualetti, A. Rocchi, A. R\\\"udiger, A. Sintes, A. Th\\\"uring, A. Vecchio, A. Vicere, B. Barr, B. Krishnan, B Mours, B. Sassolas, B. Sathyaprakash, B. Willke, C. Bradaschia, C. Colacino, C. D. Ott, C. Gr\\\"af, C. Michel, C. Palomba, C. Schwarz, C. Van Den Broeck, D. Friedrich, D. Heinert, D. Passuello, D. Rabeling, E. Calloni, E. Chassande Mottin, E. Coccia, E. Cuoco, E. Genin, E. Hennes, E. Majorana, F. Acernese, F. Barone, F. Frasconi, F. Khalili, F. Ricci, F. Richard, F. Speirits, F. Vetrano, G. Cella, G. Gemme, G. Guidi, G. Hammond, G. Jones, G. Parguez, G. Woan, H. Grote, H. L\\\"uck, H. M\\\"uller-Ebhardt, H. Rehbein, I. Heng, I. Mandel, I. Martin, J. Clark, J. Colas, J. Franc, J. Gair, J. Harms, J. Hough, J. Nelson, J. Read, J. van den Brand, J. Veitch, K. Arun, K. Danzmann, K. Glampedakis, K. Kokeyama, K. Kokkotas, K. Somiya, K. Strain, K. Yamamoto, L. Bosi, L. Cunningham, L. Di Fiore, L. Pinard, L. Santamar\\'ia, M. Abernathy, M. Barsuglia, M. Beker, M. Doets, M. Granata, M. Hannam, M. Hendry, M. Lorenzini, M. Mantovani, M. Prato, M. Punturo, M. van Veggel, N. Andersson, N. Beveridge, N. Morgado, P. Amaro-Seoane, P. Falferi, P. Fulda, P. Murray, P. Popolizio, P. Puppo, P. Rapagnani, P. Seidel, P. Sutton, R. De Rosa, R. De Salvo, R. Flaminio, R. Nawrodt, R. Oshaughnessy, R. Passaquieti, R. Poggiani1, R. Schnabel, S. Birindelli, S. Bose, S. Braccini, S. Chelkowski, S. Danilishin, S. Hild, S. Husa, S. Huttner, S. Mosca, S. Reid, S. Rowan, S Strigin, S. Tarabrin, S. Vyatchanin, T. Bulik, T. Dent, T.G.F. Li, T. Regimbau, V. Fafone, V. Mandic, W. Plastino, Y. Minenkov","submitted_at":"2010-12-04T12:17:06Z","abstract_excerpt":"Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.0908","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":"1012.0908","created_at":"2026-05-18T02:04:33.010638+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.0908v1","created_at":"2026-05-18T02:04:33.010638+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.0908","created_at":"2026-05-18T02:04:33.010638+00:00"},{"alias_kind":"pith_short_12","alias_value":"VYE6MSYRHG2F","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_16","alias_value":"VYE6MSYRHG2FRAO4","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_8","alias_value":"VYE6MSYR","created_at":"2026-05-18T12:26:15.391820+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":26,"internal_anchor_count":17,"sample":[{"citing_arxiv_id":"2605.21310","citing_title":"Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection","ref_index":60,"is_internal_anchor":true},{"citing_arxiv_id":"2605.20332","citing_title":"Cosmological History of Flavour Deconstruction Models: Constraints from Monopole Production","ref_index":91,"is_internal_anchor":true},{"citing_arxiv_id":"2605.17813","citing_title":"Positive Running of the Spectral Index for Scalar Theory and Modified Gravity","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19336","citing_title":"Recombination Thickness as an Uncertainty in Inflationary Observables","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2508.09965","citing_title":"GW231123: A Possible Primordial Black Hole Origin","ref_index":114,"is_internal_anchor":true},{"citing_arxiv_id":"2509.14924","citing_title":"Residual Test for the Third Gravitational-Wave Transient Catalog","ref_index":86,"is_internal_anchor":true},{"citing_arxiv_id":"2509.19009","citing_title":"Finite-temperature Yang-Mills theories with the density of states method: towards the continuum limit","ref_index":93,"is_internal_anchor":true},{"citing_arxiv_id":"2510.05400","citing_title":"Binary Neutron Stars from the Moon: Early Warnings and Precision Science for the Artemis Era","ref_index":24,"is_internal_anchor":true},{"citing_arxiv_id":"2510.22137","citing_title":"Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2511.08692","citing_title":"Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors","ref_index":21,"is_internal_anchor":true},{"citing_arxiv_id":"2303.15923","citing_title":"Science with the Einstein Telescope: a comparison of different designs","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2512.10344","citing_title":"Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2512.09978","citing_title":"Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2601.02458","citing_title":"Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter","ref_index":122,"is_internal_anchor":true},{"citing_arxiv_id":"2601.20939","citing_title":"Probing Bose-enhanced Inflaton Decay with Gravitational Waves","ref_index":37,"is_internal_anchor":true},{"citing_arxiv_id":"1912.02622","citing_title":"Science Case for the Einstein Telescope","ref_index":25,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15197","citing_title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","ref_index":245,"is_internal_anchor":true},{"citing_arxiv_id":"2605.04896","citing_title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","ref_index":99,"is_internal_anchor":false},{"citing_arxiv_id":"2605.01992","citing_title":"Reviving Motivated Inflationary Potentials with $K$-inflation in the light of ACT","ref_index":60,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20792","citing_title":"Irreducible Gravitational Wave Background as a Particle Detector","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11871","citing_title":"Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09081","citing_title":"Probing High-Quality Axions with Gravitational Waves","ref_index":84,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09350","citing_title":"Gravitational Memory from Hairy Binary Black Hole Mergers","ref_index":145,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06306","citing_title":"Uncool soft-wall transitions and gravitational waves","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14099","citing_title":"Electro-Weak Phase Transitions and Collider Signals in the Aligned 2-Higgs Doublet Model","ref_index":113,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC","json":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC.json","graph_json":"https://pith.science/api/pith-number/VYE6MSYRHG2FRAO4QPLFNDVCAC/graph.json","events_json":"https://pith.science/api/pith-number/VYE6MSYRHG2FRAO4QPLFNDVCAC/events.json","paper":"https://pith.science/paper/VYE6MSYR"},"agent_actions":{"view_html":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC","download_json":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC.json","view_paper":"https://pith.science/paper/VYE6MSYR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.0908&json=true","fetch_graph":"https://pith.science/api/pith-number/VYE6MSYRHG2FRAO4QPLFNDVCAC/graph.json","fetch_events":"https://pith.science/api/pith-number/VYE6MSYRHG2FRAO4QPLFNDVCAC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC/action/storage_attestation","attest_author":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC/action/author_attestation","sign_citation":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC/action/citation_signature","submit_replication":"https://pith.science/pith/VYE6MSYRHG2FRAO4QPLFNDVCAC/action/replication_record"}},"created_at":"2026-05-18T02:04:33.010638+00:00","updated_at":"2026-05-18T02:04:33.010638+00:00"}