{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:2P54TG2CTQJUOBNSUFCK5YMHNW","short_pith_number":"pith:2P54TG2C","schema_version":"1.0","canonical_sha256":"d3fbc99b429c134705b2a144aee1876d8bec9504e1c117fb7552793b249f5557","source":{"kind":"arxiv","id":"0805.2366","version":5},"attestation_state":"computed","paper":{"title":"LSST: from Science Drivers to Reference Design and Anticipated Data Products","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"LSST will image 18,000 square degrees of sky about 800 times across six bands over 10 years to a coadded depth of r~27.5, producing a public database of 40 billion objects and 32 trillion observations.","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Aaron Roodman, Abhijit Saha, Alexander Szalay, Alfred Dellapenna, Alice L. Callen, Amanda E. Bauer, Anders W. Borgland, Andrei Nomerotski, Andrew Bradshaw, Andrew C. Becker, Andrew J. Connolly, Andrew P. Rasmussen, Andrew Serio, Anthony S. Johnson, Asantha Cooray, Ashish Mahabal, Augustin Guyonnet, Aurelian Barrau, Benoit Sassolas, Beth Willman, Bhuvnesh Jain, Bob Abel, Bo Xin, Brian J. Bauman, Brian Selvy, Brian Walsh, Bryce Kalmbach, Carol Chirino, Cathy E. Petry, Cecille Roucelle, Charles F. Claver, Charles J. B. Gessner, Chris Cribbs, Chris J. Lintott, Christine Soldahl, Christopher Montgomery, Christopher W. Stubbs, Christopher W. Walter, Claire Juramy-Gilles, Colin T. Slater, Connor Miraval, Constanza Araujo, Craig A. Brackett, Craig Hogan, Craig S. Lage, Cristina Beldica, Dajun Huang, Daniel A. Goldstein, Daniel Calabrese, Daniel L. Wang, Daniel Vanden Berk, Darko Jevremovi\\'c, Darren S. Marsh, David Alonso, David E. Trilling, David G. Monet, David J. Mills, David J. Reiss, David Kirkby, David L. Burke, David R. Ciardi, David Wittman, Deborah J. Bard, Deborah Levine, Derek Chow, D. Kirk Gilmore, Dominique Boutigny, Donald L. Petravick, Donald P. Schneider, Donald Sweeney, Douglas R. Neill, Eduardo Serrano, Edward Hileman, Edward Stover, Elliott C. Cheu, Emily Acosta, Emmanuel Gangler, Enrique Figueroa, \\'Eric Aubourg, Eric Gawiser, Fabio Hernandez, Fabrice Jammes, Federica B. Bianco, Felipe Daruich, Francesco Pierfederici, Francisco Delgado, Francoise Virieux, Freddy Mu\\~noz Arancibia, Fritz Mueller, Frossie Economou, Garrett Jernigan, Gary P. Muller, George Z. Angeli, German Schumacher, Gianpietro Cagnoli, Glenaver Charles-Emerson, Glenn H. Sembroski, Greg Daues, Gregory P. Dubois-Felsmann, Guillaume Blanc, Guillaume Daubard, Gunther Haller, Heather Kelly, Henry Ferguson, Hsin-Fang Chiang, Hu Zhan (for the LSST Collaboration), Iain Goodenow, Ian Shipsey, Ian S. Sullivan, Ivan V. Kotov, Jacek Becla, Jacques Sebag, J. Allyn Smith, James B. Parsons, James Chiang, James F. Bosch, James Frank, James G. Bartlett, James Jee, James Roger P. Angel, James S. Bullock, J. Anthony Tyson, Jason S. Kalirai, Jayadev Rajagopal, J. Brian Langton, Jean-Yves Nief, Jeff D. Barr, Jeffrey P. Kantor, Jeffrey Tice, J. Matt Peterson, Joachim Moeyens, Joanne Bogart, Johann Cohen-Tanugi, John A. Hodgson, John Andrew, John C. Geary, John D. Swinbank, John Gregg Thayer, John K. Parejko, John Ku, John Kuczewski, John Oliver, John R. Peterson, Jonathan Blazek, Jonathan Sick, Jon J. Thaler, Josef Durech, Joseph J. Cockrum, Josh S. Bloom, Joshua Hoblitt, Joshua Meyers, Justine Haupt, Kem H. Cook, Kenneth Johns, Kevin A. Reil, Kevin E. Long, Kevin R. Covey, Kian-Tat Lim, Kirk Borne, Kirk T. Arndt, Knut Olsen, K. Simon Krughoff, Kurt Vetter, Lauren A. MacArthur, Laurent Le Guillou, Leanne P. Guy, Lisa Storrie-Lombardi, Lloyd Knox, Lucianne Walkowicz, Lynn G. Seppala, Mansi M. Kasliwal, Marc Moniez, Margaret W.G. Johnson, Margaux Lopez, Mario Juri\\'c, Marla Geha, Martin Nordby, Matthew R. Rumore, Max Turri, Megan E. Schwamb, M.E. Libby Petrick, Melissa L. Graham, Merlin Fisher-Levine, Michael A. Reuter, Michael A. Strauss, Michael D. Foss, Michael D. Freemon, Michael D. Schneider, Michael E. Brown, Michael E. Huffer, Michael Eracleous, Michael Prouza, Michael Warner, Michelle McQueen, Michelle Miller, Miguel de Val-Borro, Ming Liang, Morgan May, Myriam Migliore, Nadine R. Kurita, Nate B. Lust, Nathan M. Pease, Nicolas Regnault, Nicole Auza, Nicole Silvestri, Nitya J. Kallivayalil, Oliver Wiecha, Patricia Burchat, Patrick A. Hascall, Patrick Ingraham, Paul A. Price, Paul E. Palecek, Paul J. Lotz, Paul O'Connor, Perry Gee, Peter Doherty, Peter Takacs, Peter Yoachim, Petr Kub\\'anek, Philip A. Pinto, Philip J. Marshall, Philip N. Daly, Philippe Gris, Pierre Antilogus, Pierre Astier, Pierre Karst, Pim Schellart, Rachel A. Street, Rachel Mandelbaum, Rafe H. Schindler, Rahul Biswas, Raymond Plante, R. Chris Smith, Rebecca Coles, Reynald Pain, Reza Ansari, Richard A. Shaw, Richard Dubois, Richard Kessler, Richard Van Berg, R. Lynne Jones, Robert Armstrong, Robert de Peyster, Robert H. Lupton, Robert McKercher, Robert R. Gibson, Rob Pike, Robyn Allsman, Roc Cutri, Roger D. Blandford, Ron Harris, Ron Lambert, Russell E. Owen, Samuel Schmidt, Sandra Ortiz, Sandrine Thomas, Scot S. Olivier, Scott E. Winters, Scott F. Anderson, Scott F. Daniel, Scott P. Newbry, Sean Robinson, Serge Monkewitz, Seth W. Digel, Shahram Sobhani, Shawn Callahan, Shawn Osier, Shin-Yawn Wang, Shri Kulkarni, Sidney C. Wolff, Srinivasan Chandrasekharan, Stefano Russo, Stephen A. Tether, Stephen Pietrowicz, Stephen Plate, Stephen T. Ridgway, Steve Bellavia, Steve Chesley, Steven M. Kahn, Steve Ritz, Stuart Marshall, Suzanne H. Jacoby, Sven Herrmann, Sylvain Baumont, Tatiana Goldina, Terry L. Schalk, Thomas Glanzman, Tim Jenness, Tim S. Axelrod, Tim W. Bond, Tomislav Vucina, Travis Lange, Vaikunth Thukral, Veljko Radeka, Veronica Kinnison, Victor L. Krabbendam, Vincent J. Riot, \\v{Z}eljko Ivezi\\'c, Walter R. Innes, Warren Focke, Wayne Rosing, Wei Cui, William Dawson, William Glick, William J. Gressler, William Nielsen Brandt, William O'Mullane, William Roby, William Schoening, William Wahl, W. Michael Wood-Vasey, Xiuqin Wu, Yusra Alsayyad","submitted_at":"2008-05-15T18:10:13Z","abstract_excerpt":"(Abridged) We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). A vast array of science will be enabled by a single wide-deep-fast sky survey, and LSST will have unique survey capability in the faint time domain. The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the Solar System, exploring the transient optical sky, and mapping the Milky Way. LSST will be a wide-field ground-based system sited at Cerro Pach\\'{o}n in northern Chile. The telescope will have an 8.4 "},"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":true,"formal_links_present":false},"canonical_record":{"source":{"id":"0805.2366","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-05-15T18:10:13Z","cross_cats_sorted":[],"title_canon_sha256":"db6a2b76bf6f4a5c49e1a4f207ae0e9c7e963c20d7e5f08d8df2c0b33796dc86","abstract_canon_sha256":"61732fa96c9901f5bcbfc202c424a57f0420d02da74c4309d2c5427ad47038bf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:38:14.524991Z","signature_b64":"8eF5nu/wNzRgsDUK2z8p40b0xt2O/FO68LYiAvLE4JpgKZ7isO2PtplNJ80CVeJuJhCO2ypTE2urnyWKEVwhCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d3fbc99b429c134705b2a144aee1876d8bec9504e1c117fb7552793b249f5557","last_reissued_at":"2026-05-17T23:38:14.524269Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:38:14.524269Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"LSST: from Science Drivers to Reference Design and Anticipated Data Products","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"LSST will image 18,000 square degrees of sky about 800 times across six bands over 10 years to a coadded depth of r~27.5, producing a public database of 40 billion objects and 32 trillion observations.","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Aaron Roodman, Abhijit Saha, Alexander Szalay, Alfred Dellapenna, Alice L. Callen, Amanda E. Bauer, Anders W. Borgland, Andrei Nomerotski, Andrew Bradshaw, Andrew C. Becker, Andrew J. Connolly, Andrew P. Rasmussen, Andrew Serio, Anthony S. Johnson, Asantha Cooray, Ashish Mahabal, Augustin Guyonnet, Aurelian Barrau, Benoit Sassolas, Beth Willman, Bhuvnesh Jain, Bob Abel, Bo Xin, Brian J. Bauman, Brian Selvy, Brian Walsh, Bryce Kalmbach, Carol Chirino, Cathy E. Petry, Cecille Roucelle, Charles F. Claver, Charles J. B. Gessner, Chris Cribbs, Chris J. Lintott, Christine Soldahl, Christopher Montgomery, Christopher W. Stubbs, Christopher W. Walter, Claire Juramy-Gilles, Colin T. Slater, Connor Miraval, Constanza Araujo, Craig A. Brackett, Craig Hogan, Craig S. Lage, Cristina Beldica, Dajun Huang, Daniel A. Goldstein, Daniel Calabrese, Daniel L. Wang, Daniel Vanden Berk, Darko Jevremovi\\'c, Darren S. Marsh, David Alonso, David E. Trilling, David G. Monet, David J. Mills, David J. Reiss, David Kirkby, David L. Burke, David R. Ciardi, David Wittman, Deborah J. Bard, Deborah Levine, Derek Chow, D. Kirk Gilmore, Dominique Boutigny, Donald L. Petravick, Donald P. Schneider, Donald Sweeney, Douglas R. Neill, Eduardo Serrano, Edward Hileman, Edward Stover, Elliott C. Cheu, Emily Acosta, Emmanuel Gangler, Enrique Figueroa, \\'Eric Aubourg, Eric Gawiser, Fabio Hernandez, Fabrice Jammes, Federica B. Bianco, Felipe Daruich, Francesco Pierfederici, Francisco Delgado, Francoise Virieux, Freddy Mu\\~noz Arancibia, Fritz Mueller, Frossie Economou, Garrett Jernigan, Gary P. Muller, George Z. Angeli, German Schumacher, Gianpietro Cagnoli, Glenaver Charles-Emerson, Glenn H. Sembroski, Greg Daues, Gregory P. Dubois-Felsmann, Guillaume Blanc, Guillaume Daubard, Gunther Haller, Heather Kelly, Henry Ferguson, Hsin-Fang Chiang, Hu Zhan (for the LSST Collaboration), Iain Goodenow, Ian Shipsey, Ian S. Sullivan, Ivan V. Kotov, Jacek Becla, Jacques Sebag, J. Allyn Smith, James B. Parsons, James Chiang, James F. Bosch, James Frank, James G. Bartlett, James Jee, James Roger P. Angel, James S. Bullock, J. Anthony Tyson, Jason S. Kalirai, Jayadev Rajagopal, J. Brian Langton, Jean-Yves Nief, Jeff D. Barr, Jeffrey P. Kantor, Jeffrey Tice, J. Matt Peterson, Joachim Moeyens, Joanne Bogart, Johann Cohen-Tanugi, John A. Hodgson, John Andrew, John C. Geary, John D. Swinbank, John Gregg Thayer, John K. Parejko, John Ku, John Kuczewski, John Oliver, John R. Peterson, Jonathan Blazek, Jonathan Sick, Jon J. Thaler, Josef Durech, Joseph J. Cockrum, Josh S. Bloom, Joshua Hoblitt, Joshua Meyers, Justine Haupt, Kem H. Cook, Kenneth Johns, Kevin A. Reil, Kevin E. Long, Kevin R. Covey, Kian-Tat Lim, Kirk Borne, Kirk T. Arndt, Knut Olsen, K. Simon Krughoff, Kurt Vetter, Lauren A. MacArthur, Laurent Le Guillou, Leanne P. Guy, Lisa Storrie-Lombardi, Lloyd Knox, Lucianne Walkowicz, Lynn G. Seppala, Mansi M. Kasliwal, Marc Moniez, Margaret W.G. Johnson, Margaux Lopez, Mario Juri\\'c, Marla Geha, Martin Nordby, Matthew R. Rumore, Max Turri, Megan E. Schwamb, M.E. Libby Petrick, Melissa L. Graham, Merlin Fisher-Levine, Michael A. Reuter, Michael A. Strauss, Michael D. Foss, Michael D. Freemon, Michael D. Schneider, Michael E. Brown, Michael E. Huffer, Michael Eracleous, Michael Prouza, Michael Warner, Michelle McQueen, Michelle Miller, Miguel de Val-Borro, Ming Liang, Morgan May, Myriam Migliore, Nadine R. Kurita, Nate B. Lust, Nathan M. Pease, Nicolas Regnault, Nicole Auza, Nicole Silvestri, Nitya J. Kallivayalil, Oliver Wiecha, Patricia Burchat, Patrick A. Hascall, Patrick Ingraham, Paul A. Price, Paul E. Palecek, Paul J. Lotz, Paul O'Connor, Perry Gee, Peter Doherty, Peter Takacs, Peter Yoachim, Petr Kub\\'anek, Philip A. Pinto, Philip J. Marshall, Philip N. Daly, Philippe Gris, Pierre Antilogus, Pierre Astier, Pierre Karst, Pim Schellart, Rachel A. Street, Rachel Mandelbaum, Rafe H. Schindler, Rahul Biswas, Raymond Plante, R. Chris Smith, Rebecca Coles, Reynald Pain, Reza Ansari, Richard A. Shaw, Richard Dubois, Richard Kessler, Richard Van Berg, R. Lynne Jones, Robert Armstrong, Robert de Peyster, Robert H. Lupton, Robert McKercher, Robert R. Gibson, Rob Pike, Robyn Allsman, Roc Cutri, Roger D. Blandford, Ron Harris, Ron Lambert, Russell E. Owen, Samuel Schmidt, Sandra Ortiz, Sandrine Thomas, Scot S. Olivier, Scott E. Winters, Scott F. Anderson, Scott F. Daniel, Scott P. Newbry, Sean Robinson, Serge Monkewitz, Seth W. Digel, Shahram Sobhani, Shawn Callahan, Shawn Osier, Shin-Yawn Wang, Shri Kulkarni, Sidney C. Wolff, Srinivasan Chandrasekharan, Stefano Russo, Stephen A. Tether, Stephen Pietrowicz, Stephen Plate, Stephen T. Ridgway, Steve Bellavia, Steve Chesley, Steven M. Kahn, Steve Ritz, Stuart Marshall, Suzanne H. Jacoby, Sven Herrmann, Sylvain Baumont, Tatiana Goldina, Terry L. Schalk, Thomas Glanzman, Tim Jenness, Tim S. Axelrod, Tim W. Bond, Tomislav Vucina, Travis Lange, Vaikunth Thukral, Veljko Radeka, Veronica Kinnison, Victor L. Krabbendam, Vincent J. Riot, \\v{Z}eljko Ivezi\\'c, Walter R. Innes, Warren Focke, Wayne Rosing, Wei Cui, William Dawson, William Glick, William J. Gressler, William Nielsen Brandt, William O'Mullane, William Roby, William Schoening, William Wahl, W. Michael Wood-Vasey, Xiuqin Wu, Yusra Alsayyad","submitted_at":"2008-05-15T18:10:13Z","abstract_excerpt":"(Abridged) We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). A vast array of science will be enabled by a single wide-deep-fast sky survey, and LSST will have unique survey capability in the faint time domain. The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the Solar System, exploring the transient optical sky, and mapping the Milky Way. LSST will be a wide-field ground-based system sited at Cerro Pach\\'{o}n in northern Chile. The telescope will have an 8.4 "},"claims":{"count":3,"items":[{"kind":"strongest_claim","text":"The LSST system is capable of imaging about 10,000 square degrees of sky in a single filter in three nights. The typical 5 sigma point-source depth in a single visit in r will be ~24.5 (AB). The survey will yield a coadded map to r~27.5.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The design assumes that the 8.4m telescope, 3.2 gigapixel camera, and site conditions at Cerro Pachon will deliver the stated image quality, depth, and operational efficiency starting in 2022.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"LSST will image 18,000 square degrees of sky about 800 times across six bands over 10 years to a coadded depth of r~27.5, producing a public database of 40 billion objects and 32 trillion observations.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"}],"snapshot_sha256":"60d35744a03a32a70232cb31e1876567b19585b8a0231218fd2ee43d47595e66"},"source":{"id":"0805.2366","kind":"arxiv","version":5},"verdict":{"id":"0050e4e7-5565-42dd-b621-d06e08646058","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-17T08:58:01.567908Z","strongest_claim":"The LSST system is capable of imaging about 10,000 square degrees of sky in a single filter in three nights. The typical 5 sigma point-source depth in a single visit in r will be ~24.5 (AB). The survey will yield a coadded map to r~27.5.","one_line_summary":"LSST will image 18,000 square degrees of sky about 800 times across six bands over 10 years to a coadded depth of r~27.5, producing a public database of 40 billion objects and 32 trillion observations.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The design assumes that the 8.4m telescope, 3.2 gigapixel camera, and site conditions at Cerro Pachon will deliver the stated image quality, depth, and operational efficiency starting in 2022.","pith_extraction_headline":""},"references":{"count":300,"sample":[{"doi":"10.1088/0067-0049/182/2/543","year":2009,"title":"Abazajian , K. N., Adelman-McCarthy , J. K., Ag \\\"u eros , M. A., et al. 2009, , 182, 543, 10.1088/0067-0049/182/2/543","work_id":"a2b8de51-d046-42bd-ab8a-a181bcd0ef82","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2016,"title":"Abazajianet al.[CMB-S4],CMB-S4 Science Book, First Edition","work_id":"a36703d1-7c55-4314-a1b3-cb1dfe4aaf4d","ref_index":2,"cited_arxiv_id":"1610.02743","is_internal_anchor":true},{"doi":"10.3847/2041-8213/aa91c9","year":2017,"title":"2017 b , , 848, L12, 10.3847/2041-8213/aa91c9","work_id":"ce1335b7-ca12-4b4a-b721-056fa43cba78","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1038/nature24471","year":2017,"title":"P., Abbott, R., Abbott, T","work_id":"086c1f01-a887-42a0-aba2-60f9920a63da","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2004,"title":"A'Hearn , M. F. 2004, in Comets II, ed. M. C. Festou , H. U. Keller , & H. A. Weaver (University of Arizona Press), 17--22","work_id":"a49b599b-206b-4e7c-8ed8-3ece9d89460d","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":300,"snapshot_sha256":"88749ba40f83e71de703ed07215ba45cbb8d163240ff4ac610e2f3fda6a46d16","internal_anchors":22},"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":"0805.2366","created_at":"2026-05-17T23:38:14.524407+00:00"},{"alias_kind":"arxiv_version","alias_value":"0805.2366v5","created_at":"2026-05-17T23:38:14.524407+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0805.2366","created_at":"2026-05-17T23:38:14.524407+00:00"},{"alias_kind":"pith_short_12","alias_value":"2P54TG2CTQJU","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_16","alias_value":"2P54TG2CTQJUOBNS","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_8","alias_value":"2P54TG2C","created_at":"2026-05-18T12:25:56.245647+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":38,"internal_anchor_count":38,"sample":[{"citing_arxiv_id":"1906.11346","citing_title":"Maximizing LSST Solar System Science: Approaches, Software Tools, and Infrastructure Needs","ref_index":70,"is_internal_anchor":true},{"citing_arxiv_id":"1907.04443","citing_title":"SETI in the Spatio-Temporal Survey Domain","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2301.09655","citing_title":"Perturbation-theory informed integrators for cosmological simulations","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2411.07970","citing_title":"MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2411.14748","citing_title":"Cosmological Analysis with Calibrated Neural Quantile Estimation and Approximate Simulators","ref_index":5,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21578","citing_title":"Gravitational wave detectability range informed by external messengers","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2605.22353","citing_title":"Prospects for detecting surface color heterogeneity on asteroid surfaces from sparse multiband photometric survey data","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"2509.06929","citing_title":"Edges In Coadded Images","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2511.05653","citing_title":"Probing Dark Energy Microphysics with kSZ Tomography","ref_index":22,"is_internal_anchor":true},{"citing_arxiv_id":"2603.09278","citing_title":"Constraining Neutrino Mass with the Void Weak Lensing Effect","ref_index":109,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21436","citing_title":"Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum","ref_index":155,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12482","citing_title":"Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles","ref_index":107,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19059","citing_title":"VarWISE: Infrared Variability via NEOWISE Single Exposure Photometry","ref_index":18,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19217","citing_title":"Taking Inventory of the Most Promising Lensed Radio Sources for Constraining Fundamental Properties of Dark Matter","ref_index":168,"is_internal_anchor":true},{"citing_arxiv_id":"2605.17005","citing_title":"Red novae, their progenitors, and remnants","ref_index":209,"is_internal_anchor":true},{"citing_arxiv_id":"2508.19106","citing_title":"Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid","ref_index":88,"is_internal_anchor":true},{"citing_arxiv_id":"2509.03360","citing_title":"The Early Career Workshop of GR-Amaldi 2025","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2509.06929","citing_title":"Edges In Coadded Images","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2509.15890","citing_title":"Fast and accurate Gaia-unWISE quasar mock catalogs from LPT and Eulerian bias","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2303.15923","citing_title":"Science with the Einstein Telescope: a comparison of different designs","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2511.16971","citing_title":"Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2511.18134","citing_title":"Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2602.03110","citing_title":"Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing","ref_index":144,"is_internal_anchor":true},{"citing_arxiv_id":"2603.13053","citing_title":"A unified harmonic framework for dark siren cosmology","ref_index":71,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12482","citing_title":"Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles","ref_index":94,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW","json":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW.json","graph_json":"https://pith.science/api/pith-number/2P54TG2CTQJUOBNSUFCK5YMHNW/graph.json","events_json":"https://pith.science/api/pith-number/2P54TG2CTQJUOBNSUFCK5YMHNW/events.json","paper":"https://pith.science/paper/2P54TG2C"},"agent_actions":{"view_html":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW","download_json":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW.json","view_paper":"https://pith.science/paper/2P54TG2C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0805.2366&json=true","fetch_graph":"https://pith.science/api/pith-number/2P54TG2CTQJUOBNSUFCK5YMHNW/graph.json","fetch_events":"https://pith.science/api/pith-number/2P54TG2CTQJUOBNSUFCK5YMHNW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW/action/storage_attestation","attest_author":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW/action/author_attestation","sign_citation":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW/action/citation_signature","submit_replication":"https://pith.science/pith/2P54TG2CTQJUOBNSUFCK5YMHNW/action/replication_record"}},"created_at":"2026-05-17T23:38:14.524407+00:00","updated_at":"2026-05-17T23:38:14.524407+00:00"}