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Record W1658758220 · doi:10.1007/s10686-015-9484-8

The EChO science case

2015· article· en· W1658758220 on OpenAlexaff
G. Tinetti, P. Drossart, Paul Eccleston, P. Hartogh, K. G. Isaak, Martin Linder, C. Lovis, Marc Ollivier, Ludovic Puig, I. Ribas, I. A. G. Snellen, B. Swinyard, F. Allard, J. K. Barstow, James Cho, A. Coustenis, Charles Cockell, A. C. M. Correia, L. Decin, Remco de Kok, Pieter Deroo, Thérèse Encrenaz, F. Forget, Alistair Glasse, Caitlin Griffith, T. Guillot, Tommi Koskinen, H. Lammer, Jérémy Leconte, Pierre Maxted, Ingo Mueller‐Wodarg, Richard P. Nelson, C. North, Ε. Πάλλη, Isabella Pagano, G. Piccioni, D. J. Pinfield, Franck Selsis, A. Sozzetti, Lars Stixrude, Jonathan Tennyson, D. Turrini, M. R. Zapatero Osorio, Jean‐Philippe Beaulieu, Denis Grodent, M. Guêdel, David Luz, H. U. Nørgaard-Nielsen, H. Rickman, Avri Selig, Mark Swain, Marek Banaszkiewicz, Neil E. Bowles, G. Branduardi‐Raymont, Vincent Coudé du Foresto, Jean‐Claude Gérard, L. Gizon, A. Hornstrup, Christopher J. Jarchow, F. Kerschbaum, G. Kovács, Pierre-Olivier Lagage, Tanya Lim, Mercedes López‐Morales, G. Malaguti, E. Pace, E. Pascale, B. Vandenbussche, Gillian Wright, Gonzalo Ramos Zapata, A. Adriani, R. Azzollini, Ana Balado, Ian Bryson, Raymond Burston, J. Colomé, M. Vives Crook, A. Di Giorgio, Matt Griffin, Ruud Hoogeveen, R. Ottensamer, Ranah Irshad, Kevin Middleton, G. Morgante, Frederic Pinsard, M. Rataj, Jean-Michel Réess, G. Savini, Jan-Rutger Schrader, R. Stamper, Berend Winter, L. Abe, Manuel Abreu, N. Achilleos, P. A. R. Ade, V. Adybekian, L. Affer, C. B. Agnor, M. Agúndez, C. Alard, J. M. Alcalá, C. Allende Prieto, F. J. Alonso Floriano, Francesca Altieri, C. A. Alvarez Iglesias, P. J. Amado, Anja C. Andersen, A. D. Aylward, C. Baffa, G. Á. Bakos, P. Ballerini, M. Banaszkiewicz, R. J. Barber, D. Barrado, Emma J. Barton, V. Batista, G. Bellucci, Juan Antonio Belmonte Avilés, David Berry, Bruno Bézard, D. Biondi, M. I. Błęcka, Bertrand Bonfond, P. Bordé, P. Börner, H. Bouy, L. Brown, Lars A. Buchhave, J. Budaj, A. Bulgarelli, M. R. Burleigh, Alexandre Cabral, M. T. Capria, A. Cassan, C. Cavarroc, C. Cecchi‐Pestellini, R. Cerulli, Joshua Chadney, S. Chamberlain, S. Charnoz, Niels Christian Jessen, A. Ciaravella, A. Claret, R. Claudi, A. J. Coates, R. Cole, A. Collura, D. Cordier, E. Covino, Camilla Danielski, M. Damasso, H. J. Deeg, Ciro Del Vecchio, O. D. S. Demangeon, A. De Sio, J. De Wit, M. Dobrijévic, P. Doel, C. Dominic, E. A. Dorfi, S. Eales, C. Eiroa, M. Espinoza Contreras, Marco Esposito, V. Eymet, N. Fabrizio, M. Fernández, B. Femenía Castella, P. Figueira, G. Filacchione, Leigh N. Fletcher, Mauro Focardi, S. J. Fossey, P. Fouqué, J. Frith, M. Galand, L. Gambicorti, P. Gaulme, R. J. Garcı́a López, Á. García-Piquer, W. K. Gear, J.-C. Gerard, L. Gesa, E. Giani, F. Gianotti, M. Gillon, E. Giro, M. Giuranna, H. L. Gomez, I. Gómez‐Leal, J. I. Gónzalez Hernández, B. González Merino, Rafał Graczyk, D. Grassi, P. Guio, Jillian Gustin, Peter Hargrave, Joanna D. Haigh, Éric Hébrard, U. Heiter, R. L. Heredero, E. Herrero, F. Hersant, David Heyrovský, Morgan Hollis, B. Hubert, R. Hueso, G. Israelian, Nicolas Iro, P. G. J. Irwin, Stéphane Jacquemoud, G. Jones, H. Jones, K. Justtanont, T. Kehoe, E. Kerins, P. Kervella, David Kipping, T. Koskinen, N. Krupp, O. Lahav, B. Laken, N. Lanza, E. Lellouch, G. Leto, J. Licandro Goldaracena, C. Lithgow-Bertelloni, S. J. Liu, U. Lo Cicero, N. Lodieu, Philippe Lognonné, M. López‐Puertas, M. Á. López‐Valverde, I. Rasmussen, A. Luntzer, P. Machado, C. MacTavish, A. Maggio, J. P. Maillard, W. Magnes, J. Maldonado, U. Mall, J. B. Marquette, P. Mauskopf, A. S. Maurin, Alexander S. Medvedev, Chloé Michaut, Paulo A. Miles-Páez, M. Montalto, P. Montañés‐Rodríguez, M. A. Monteiro, D. Montes, H. Morais, J. C. Morales, M. Morales‐Calderón, Giuseppe Morello, Julianne I. Moses, A. Moya Bedon, F. Murgas Alcaino, E. Oliva, G. Orton, F. Palla, M. Pancrazzi, E. Pantin, Vivien Parmentier, H. Parviainen, Karla Peña Ramírez, Javier Peralta, S. Pérez‐Hoyos, R. Petrov, S. Pezzuto, R. Pietrzak, Elke Pilat‐Lohinger, N. Piskunov, R. Prinja, L. Prisinzano, Inna Polichtchouk, E. Poretti, Aikaterini Radioti, A. A. Ramos, T. Rank-Lüftinger, K. Readorn, José M. Rebordão, M. Rengel, L. Rezac, M. Rocchetto, F. Rodler, V. J. S. Béjar, A. Sánchez‐Lavega, E. Sanromá, N. C. Santos, J. Sanz‐Forcada, G. Scandariato, F. X. Schmider, A. Scholz, Salvatore Scuderi, J. Sethenadh, S. N. Shore, A. P. Showman, B. Sicardy, P. Sitek, A. Smith, Lauriane Soret, S. G. Sousa, A. Stiepen, M. Stolarski, G. Strazzulla, H. M. Tabernero, P. Tanga, M. Tecsa, J. Temple, L. Terenzi, M. Tessenyi, L. Testi, S. Thompson, H. Thrastarson, B. W. Tingley, M. Trifoglio, Javier Martín‐Torres, Andrea Tozzi, D. Turrini, R. Varley, F. Vakili, M. de Val-Borro, M. L. Valdivieso, Olivia Vénot, E. Villaver, Sandrine Vinatier, S. Viti, I. Waldmann, D. Waltham, D. Ward–Thompson, Rens Waters, C. Watkins, D. Watson, P. Wawer, A. Wawrzaszk, G. White, T. Widemann, W. Winek, T. Wiśniowski, R. Yelle, Yuk L. Yung, S. N. Yurchenko

Bibliographic record

VenueExperimental Astronomy · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersEuropean Research CouncilScience and Technology Facilities Council
KeywordsEcho (communications protocol)Computer sciencePhysics

Abstract

fetched live from OpenAlex

The discovery of almost two thousand exoplanets has revealed an unexpectedly diverse planet population. We see gas giants in few-day orbits, whole multi-planet systems within the orbit of Mercury, and new populations of planets with masses between that of the Earth and Neptune-all unknown in the Solar System. Observations to date have shown that our Solar System is certainly not representative of the general population of planets in our Milky Way. The key science questions that urgently need addressing are therefore: What are exoplanets made of? Why are planets as they are? How do planetary systems work and what causes the exceptional diversity observed as compared to the Solar System? The EChO (Exoplanet Characterisation Observatory) space mission was conceived to take up the challenge to explain this diversity in terms of formation, evolution, internal structure and planet and atmospheric composition. This requires in-depth spectroscopic knowledge of the atmospheres of a large and well-defined planet sample for which precise physical, chemical and dynamical information can be obtained. In order to fulfil this ambitious scientific program, EChO was designed as a dedicated survey mission for transit and eclipse spectroscopy capable of observing a large, diverse and well-defined planet sample within its 4-year mission lifetime. The transit and eclipse spectroscopy method, whereby the signal from the star and planet are differentiated using knowledge of the planetary ephemerides, allows us to measure atmospheric signals from the planet at levels of at least 10 -4 relative to the star. This can only be achieved in conjunction with a carefully designed stable payload and satellite platform. It is also necessary to provide broad instantaneous wavelength coverage to detect as many molecular species as possible, to probe the thermal structure of the planetary atmospheres and to correct for the contaminating effects of the stellar photosphere. This requires wavelength coverage of at least 0.55 to 11 m with a goal of covering from 0.4 to 16 m. Only modest spectral resolving power is needed, with R~300 for wavelengths less than 5 m and R~30 for wavelengths greater than this. The transit

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.004
metaresearch head score (Gemma)0.017
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.090
Threshold uncertainty score0.301

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.017
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0070.006
Scholarly communication0.0100.007
Open science0.0020.009
Research integrity0.0110.013
Insufficient payload (model declined to judge)0.0900.021

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.017
GPT teacher head0.268
Teacher spread0.251 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designTheoretical or conceptual
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations34
Published2015
Admission routes1
Has abstractyes

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