{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:3RU2YIB2YBTHD7GMNZBQ6YFJPT","short_pith_number":"pith:3RU2YIB2","schema_version":"1.0","canonical_sha256":"dc69ac203ac06671fccc6e430f60a97cfe0f3ac22418cf5626f5b778db8b7e42","source":{"kind":"arxiv","id":"2308.09617","version":1},"attestation_state":"computed","paper":{"title":"Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adam Dustor, Adam Popowicz, Aida Behmard, Akihiko Fukui, Alessandro Sozzetti, Alexander Belinski, Alexander Tarasenkov, Alex S. Polanski, Allyson Bieryla, Andr\\'es Jord\\'an, Andrew Vanderburg, Andrew W. Howard, Andrew W. Mayo, Antonio Frasca, Ashley Chontos, Aviad Panahi, Avi Shporer, Avraham Binnenfeld, Benjamin Fulton, Benjamin J. Hord, Bob Massey, Carl Ziegler, Caroline V. Morley, Catherine A. Clark, Chris Stockdale, Christopher R. Mann, Coel Hellier, Courtney Dressing, Cristilyn N. Watkins, Daniel Huber, David Baker, Davide Gandolfi, David R. Ciardi, David W. Latham, Dennis M. Conti, Diana Dragomir, Don J. Radford, Edward J. Michaels, Elena Lee, Elisabeth Matthews, Elise Furlan, Eliza M.-R. Kempton, Emily A. Gilbert, Emmanuel Jehin, Enric Palle, Erica Gonzales, Eric B. Ting, Eric Girardin, Eric L. N. Jensen, Fei Dai, Ferran Grau Horta, Fran\\c{c}ois Bouchy, Francisco J. Pozuelos, Franco Mallia, Gabrielle Ross, George Zhou, Georgia Mraz, Georgina Dransfield, Gilbert Esquerdo, Giovanni Isopi, Giuseppe Marino, Gregor Srdoc, Howard Isaacson, Howard M. Relles, Hugh Osborn, Ian J. M. Crossfield, Ian Waite, Jack Lubin, Jacob Bean, J. D. Hartman, Jegug Ih, Jerome P. de Leon, Jerzy Fio{\\l}ka, Joao Gregorio, John F. Kielkopf, John H. Livingston, Jon M. Jenkins, Jose A. Mu\\~noz, Joseph E. Rodriguez, Joshua Schlieder, JP Vignes, Judah Van Zandt, Justin Wittrock, Karen A. Collins, Keith Horne, Kevin I. Collins, Khalid Barkaoui, Kim K. McLeod, Knicole D. Col\\'on, Krzysztof Bernacki, Krzysztof G. He{\\l}miniak, Lars A. Buchhave, Lauren M. Weiss, Lee J. Rosenthal, Louise Dyregaard Nielsen, Malena Rice, Marion Cointepas, Marshall C. Johnson, Mathilde Timmermans, Mayuko Mori, Michael B. Lund, Michael Calkins, Micha\\\"el Gillon, Michael Greklek-McKeon, Michelle L. Hill, Mourad Ghachoui, Natalie M. Batalha, Nataliia Maslennikova, Nicolas B. Cowan, Nicole Schanche, Noriharu Watanabe, Norio Narita, Pablo Lewin, Pau Bosch-Cabot, Paul Benni, Paul Robertson, Pere Guerra, Phil Evans, Phillip A. Reed, Rachel Matson, Rafael Brahm, Ramotholo Sefako, Raquel For\\'es-Toribio, Riccardo Papini, Richard P. Schwarz, Ryan A. Rubenzahl, Ryan Cloutier, Samuel N. Quinn, Sergio B. Fajardo-Acosta, Shay Zucker, S{\\l}awomir Lasota, Stephen R. Kane, Steve B. Howell, Steven Giacalone, Tansu Daylan, Teo Mo\\v{c}nik, Thiam-Guan Tan, Thomas Henning, Thomas Mikal-Evans, Tianjun Gan, Tsevi Mazeh, Vadim Krushinsky, Valerio Bozza, Zoe L. de Beurs, Zouhair Benkhaldoun","submitted_at":"2023-08-18T15:20:39Z","abstract_excerpt":"JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5,000 confirmed planets, more than 4,000 TESS planet candidates are still unconfirmed and many of the best planets for atmospheric characterization may remain to be identified. We present a sample of TESS planets and planet candidates that we identify as \"best-in-class\" for transmission and emission spectroscopy with JWST. These targets are sorted into bins across equilibrium temperature $T_{\\mathrm{eq}}$ and planetary radius $R{_\\mathrm{p}}$ and are ranked by transmission and emi"},"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":"2308.09617","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-08-18T15:20:39Z","cross_cats_sorted":[],"title_canon_sha256":"5b8604cadd7378da4a7bb8d00dd16bbbb17e5da74fb2dafc9e2b6b24dbe44aaf","abstract_canon_sha256":"2506c9bdc6289d547030f90f73207ed3e4d191beb0607814137297c6d79053e8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:42:36.115462Z","signature_b64":"FHD2FyKZDoMB3m91P2FQPvukePcFDGVENtFq1uDjnoMLKs70wWve5SR0Mdsdr89JvNAbtMYhimz5a9pvNIebDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dc69ac203ac06671fccc6e430f60a97cfe0f3ac22418cf5626f5b778db8b7e42","last_reissued_at":"2026-07-05T06:42:36.114914Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:42:36.114914Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adam Dustor, Adam Popowicz, Aida Behmard, Akihiko Fukui, Alessandro Sozzetti, Alexander Belinski, Alexander Tarasenkov, Alex S. Polanski, Allyson Bieryla, Andr\\'es Jord\\'an, Andrew Vanderburg, Andrew W. Howard, Andrew W. Mayo, Antonio Frasca, Ashley Chontos, Aviad Panahi, Avi Shporer, Avraham Binnenfeld, Benjamin Fulton, Benjamin J. Hord, Bob Massey, Carl Ziegler, Caroline V. Morley, Catherine A. Clark, Chris Stockdale, Christopher R. Mann, Coel Hellier, Courtney Dressing, Cristilyn N. Watkins, Daniel Huber, David Baker, Davide Gandolfi, David R. Ciardi, David W. Latham, Dennis M. Conti, Diana Dragomir, Don J. Radford, Edward J. Michaels, Elena Lee, Elisabeth Matthews, Elise Furlan, Eliza M.-R. Kempton, Emily A. Gilbert, Emmanuel Jehin, Enric Palle, Erica Gonzales, Eric B. Ting, Eric Girardin, Eric L. N. Jensen, Fei Dai, Ferran Grau Horta, Fran\\c{c}ois Bouchy, Francisco J. Pozuelos, Franco Mallia, Gabrielle Ross, George Zhou, Georgia Mraz, Georgina Dransfield, Gilbert Esquerdo, Giovanni Isopi, Giuseppe Marino, Gregor Srdoc, Howard Isaacson, Howard M. Relles, Hugh Osborn, Ian J. M. Crossfield, Ian Waite, Jack Lubin, Jacob Bean, J. D. Hartman, Jegug Ih, Jerome P. de Leon, Jerzy Fio{\\l}ka, Joao Gregorio, John F. Kielkopf, John H. Livingston, Jon M. Jenkins, Jose A. Mu\\~noz, Joseph E. Rodriguez, Joshua Schlieder, JP Vignes, Judah Van Zandt, Justin Wittrock, Karen A. Collins, Keith Horne, Kevin I. Collins, Khalid Barkaoui, Kim K. McLeod, Knicole D. Col\\'on, Krzysztof Bernacki, Krzysztof G. He{\\l}miniak, Lars A. Buchhave, Lauren M. Weiss, Lee J. Rosenthal, Louise Dyregaard Nielsen, Malena Rice, Marion Cointepas, Marshall C. Johnson, Mathilde Timmermans, Mayuko Mori, Michael B. Lund, Michael Calkins, Micha\\\"el Gillon, Michael Greklek-McKeon, Michelle L. Hill, Mourad Ghachoui, Natalie M. Batalha, Nataliia Maslennikova, Nicolas B. Cowan, Nicole Schanche, Noriharu Watanabe, Norio Narita, Pablo Lewin, Pau Bosch-Cabot, Paul Benni, Paul Robertson, Pere Guerra, Phil Evans, Phillip A. Reed, Rachel Matson, Rafael Brahm, Ramotholo Sefako, Raquel For\\'es-Toribio, Riccardo Papini, Richard P. Schwarz, Ryan A. Rubenzahl, Ryan Cloutier, Samuel N. Quinn, Sergio B. Fajardo-Acosta, Shay Zucker, S{\\l}awomir Lasota, Stephen R. Kane, Steve B. Howell, Steven Giacalone, Tansu Daylan, Teo Mo\\v{c}nik, Thiam-Guan Tan, Thomas Henning, Thomas Mikal-Evans, Tianjun Gan, Tsevi Mazeh, Vadim Krushinsky, Valerio Bozza, Zoe L. de Beurs, Zouhair Benkhaldoun","submitted_at":"2023-08-18T15:20:39Z","abstract_excerpt":"JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5,000 confirmed planets, more than 4,000 TESS planet candidates are still unconfirmed and many of the best planets for atmospheric characterization may remain to be identified. We present a sample of TESS planets and planet candidates that we identify as \"best-in-class\" for transmission and emission spectroscopy with JWST. These targets are sorted into bins across equilibrium temperature $T_{\\mathrm{eq}}$ and planetary radius $R{_\\mathrm{p}}$ and are ranked by transmission and emi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.09617","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2308.09617/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2308.09617","created_at":"2026-07-05T06:42:36.114971+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.09617v1","created_at":"2026-07-05T06:42:36.114971+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.09617","created_at":"2026-07-05T06:42:36.114971+00:00"},{"alias_kind":"pith_short_12","alias_value":"3RU2YIB2YBTH","created_at":"2026-07-05T06:42:36.114971+00:00"},{"alias_kind":"pith_short_16","alias_value":"3RU2YIB2YBTHD7GM","created_at":"2026-07-05T06:42:36.114971+00:00"},{"alias_kind":"pith_short_8","alias_value":"3RU2YIB2","created_at":"2026-07-05T06:42:36.114971+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/3RU2YIB2YBTHD7GMNZBQ6YFJPT","json":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT.json","graph_json":"https://pith.science/api/pith-number/3RU2YIB2YBTHD7GMNZBQ6YFJPT/graph.json","events_json":"https://pith.science/api/pith-number/3RU2YIB2YBTHD7GMNZBQ6YFJPT/events.json","paper":"https://pith.science/paper/3RU2YIB2"},"agent_actions":{"view_html":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT","download_json":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT.json","view_paper":"https://pith.science/paper/3RU2YIB2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.09617&json=true","fetch_graph":"https://pith.science/api/pith-number/3RU2YIB2YBTHD7GMNZBQ6YFJPT/graph.json","fetch_events":"https://pith.science/api/pith-number/3RU2YIB2YBTHD7GMNZBQ6YFJPT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT/action/storage_attestation","attest_author":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT/action/author_attestation","sign_citation":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT/action/citation_signature","submit_replication":"https://pith.science/pith/3RU2YIB2YBTHD7GMNZBQ6YFJPT/action/replication_record"}},"created_at":"2026-07-05T06:42:36.114971+00:00","updated_at":"2026-07-05T06:42:36.114971+00:00"}