An Updated Study of Potential Targets for Ariel
An Updated Study of Potential Targets for Ariel
复制标题
Ariel 潜在目标的最新研究
DOI:
10.3847/1538-3881/ab1cb9
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发表时间:
2019
期刊:
影响因子:
--
通讯作者:
Subhajit Sarkar
中科院分区:
文献类型:
--
作者:
B. Edwards;L. Mugnai;G. Tinetti;E. Pascale;Subhajit Sarkar
Ariel has been selected as ESA’s M4 mission for launch in 2028 and is designed for the characterization of a large and diverse population of exoplanetary atmospheres to provide insights into planetary formation and evolution within our Galaxy. Here we present a study of Ariel’s capability to observe currently known exoplanets and predicted Transiting Exoplanet Survey Satellite (TESS) discoveries. We use the Ariel radiometric model (ArielRad) to simulate the instrument performance and find that ∼2000 of these planets have atmospheric signals which could be characterized by Ariel. This list of potential planets contains a diverse range of planetary and stellar parameters. From these we select an example mission reference sample (MRS), comprised of 1000 diverse planets to be completed within the primary mission life, which is consistent with previous studies. We also explore the mission capability to perform an in-depth survey into the atmospheres of smaller planets, which may be enriched or secondary. Earth-sized planets and super-Earths with atmospheres heavier than H/He will be more challenging to observe spectroscopically. However, by studying the time required to observe ∼110 Earth-sized/super-Earths, we find that Ariel could have substantial capability for providing in-depth observations of smaller planets. Trade-offs between the number and type of planets observed will form a key part of the selection process and this list of planets will continually evolve with new exoplanet discoveries replacing predicted detections. The Ariel target list will be constantly updated and the MRS re-selected to ensure maximum diversity in the population of planets studied during the primary mission life.
影响因子:
4.8
作者:
Arazi Pinhas;N. Madhusudhan;S. Gandhi;R. MacDonald
通讯作者:
Arazi Pinhas;N. Madhusudhan;S. Gandhi;R. MacDonald
影响因子:
3
作者:
G. Tinetti;P. Drossart;P. Eccleston;P. Hartogh;A. Heske;J. Leconte;G. Micela;M. Ollivier;G. Pilbratt;L. Puig;D. Turrini;B. Vandenbussche;Paulina Wolkenberg;J. Beaulieu;L. A. Buchave;Martin Ferus;M. Griffin;M. Guedel;K. Justtanont;P. Lagage;Pedro Machado;G. Malaguti;Michiel Min;H. Nørgaard-Nielsen;Mirek Rataj;T. Ray;Ignasi Ribas;M. Swain;R. Szabó;Stephanie C. Werner;J. Barstow;Matt Burleigh;James Cho;V. C. du Foresto;A. Coustenis;L. Decin;T. Encrenaz;M. Galand;M. Gillon;R. Helled;J. C. Morales;A. G. Muñoz;A. Moneti;Isabella Pagano;E. Pascale;G. Piccioni;David Pinfield;Subhajit Sarkar;F. Selsis;J. Tennyson;A. Triaud;O. Venot;I. Waldmann;David Waltham;Gillian S. Wright;J. Amiaux;J. Auguères;M. Berthé;N. Bezawada;G. Bishop;Neil Bowles;Deirdre Coffey;J. Colomé;M. Crook;P. Crouzet;Vania Da Peppo;I. E. Sanz;M. Focardi;M. Frericks;Tom Hunt;R. Kohley;K. Middleton;G. Morgante;R. Ottensamer;E. Pace;Chris Pearson;R. Stamper;K. Symonds;M. Rengel;E. Renotte;P. Ade;L. Affer;Christophe Alard;Nicole F. Allard;F. Altieri;Yves André;Claudio Arena;I. Argyriou;Alan Aylward;C. Baccani;Gáspár Á. Bakos;M. Banaszkiewicz;Mike Barlow;V. Batista;G. Bellucci;S. Benatti;Pernelle Bernardi;Bruno Bézard;M. Błęcka;É. Bolmont;B. Bonfond;R. Bonito;A. Bonomo;J. Brucato;Allan Sacha Brun;I. Bryson;W. Bujwan;S. Casewell;B. Charnay;C. Pestellini;Guo Chen;A. Ciaravella;R. Claudi;R. Clédassou;M. Damasso;M. Damiano;C. Danielski;Pieter Deroo;A. D. di Giorgio;Carsten Dominik;V. Doublier;S. Doyle;René Doyon;Benjamin Drummond;Bastien Duong;S. Eales;Billy Edwards;Maria Farina;E. Flaccomio;Leigh Fletcher;F. Forget;Steve Fossey;Markus Fränz;Yuka Fujii;A. Garcia-Piquer;W. Gear;H. Geoffray;Jean-Claude Gérard;L. Gesa;H. Gomez;Rafał Graczyk;C. Griffith;D. Grodent;M. Guarcello;J. Gustin;K. Hamano;P. Hargrave;Y. Hello;Kevin Heng;E. Herrero;A. Hornstrup;Benoît Hubert;Shigeru Ida;M. Ikoma;N. Iro;Patrick Irwin;C. Jarchow;Jean Jaubert;Hugh R. A. Jones;Queyrel Julien;Shingo Kameda;F. Kerschbaum;P. Kervella;T. Koskinen;M. Krijger;N. Krupp;M. Lafarga;F. Landini;E. Lellouch;G. Leto;A. Luntzer;T. Rank-Lüftinger;Antonio Maggio;J. Maldonado;Jean-Pierre Maillard;Urs Mall;J. Marquette;Stéphane Mathis;P. Maxted;T. Matsuo;A. Medvedev;Yamila Miguel;V. Minier;G. Morello;Alessandro Mura;N. Narita;V. Nascimbeni;N. Nguyen Tong;V. Noce;F. Oliva;E. Pallé;Paul Palmer;M. Pancrazzi;A. Papageorgiou;V. Parmentier;M. Perger;A. Petralia;S. Pezzuto;Ray Pierrehumbert;I. Pillitteri;G. Piotto;G. Pisano;L. Prisinzano;A. Radioti;J. Réess;L. Rezac;M. Rocchetto;A. Rosich;N. Sanna;A. Santerne;G. Savini;G. Scandariato;B. Sicardy;Carles Sierra;G. Sindoni;K. Skup;I. Snellen;M. Sobiecki;L. Soret;A. Sozzetti;A. Stiepen;A. Strugarek;Jake Taylor;William Taylor;L. Terenzi;M. Tessenyi;A. Tsiaras;C. Tucker;Diana Valencia;G. Vasisht;A. Vazan;F. Vilardell;S. Vinatier;S. Viti;Rens Waters;P. Wawer;A. Wawrzaszek;A. Whitworth;Yuk L. Yung;S. Yurchenko;M. Z. Osorio;R. Zellem;T. Zingales;F. Zwart
通讯作者:
G. Tinetti;P. Drossart;P. Eccleston;P. Hartogh;A. Heske;J. Leconte;G. Micela;M. Ollivier;G. Pilbratt;L. Puig;D. Turrini;B. Vandenbussche;Paulina Wolkenberg;J. Beaulieu;L. A. Buchave;Martin Ferus;M. Griffin;M. Guedel;K. Justtanont;P. Lagage;Pedro Machado;G. Malaguti;Michiel Min;H. Nørgaard-Nielsen;Mirek Rataj;T. Ray;Ignasi Ribas;M. Swain;R. Szabó;Stephanie C. Werner;J. Barstow;Matt Burleigh;James Cho;V. C. du Foresto;A. Coustenis;L. Decin;T. Encrenaz;M. Galand;M. Gillon;R. Helled;J. C. Morales;A. G. Muñoz;A. Moneti;Isabella Pagano;E. Pascale;G. Piccioni;David Pinfield;Subhajit Sarkar;F. Selsis;J. Tennyson;A. Triaud;O. Venot;I. Waldmann;David Waltham;Gillian S. Wright;J. Amiaux;J. Auguères;M. Berthé;N. Bezawada;G. Bishop;Neil Bowles;Deirdre Coffey;J. Colomé;M. Crook;P. Crouzet;Vania Da Peppo;I. E. Sanz;M. Focardi;M. Frericks;Tom Hunt;R. Kohley;K. Middleton;G. Morgante;R. Ottensamer;E. Pace;Chris Pearson;R. Stamper;K. Symonds;M. Rengel;E. Renotte;P. Ade;L. Affer;Christophe Alard;Nicole F. Allard;F. Altieri;Yves André;Claudio Arena;I. Argyriou;Alan Aylward;C. Baccani;Gáspár Á. Bakos;M. Banaszkiewicz;Mike Barlow;V. Batista;G. Bellucci;S. Benatti;Pernelle Bernardi;Bruno Bézard;M. Błęcka;É. Bolmont;B. Bonfond;R. Bonito;A. Bonomo;J. Brucato;Allan Sacha Brun;I. Bryson;W. Bujwan;S. Casewell;B. Charnay;C. Pestellini;Guo Chen;A. Ciaravella;R. Claudi;R. Clédassou;M. Damasso;M. Damiano;C. Danielski;Pieter Deroo;A. D. di Giorgio;Carsten Dominik;V. Doublier;S. Doyle;René Doyon;Benjamin Drummond;Bastien Duong;S. Eales;Billy Edwards;Maria Farina;E. Flaccomio;Leigh Fletcher;F. Forget;Steve Fossey;Markus Fränz;Yuka Fujii;A. Garcia-Piquer;W. Gear;H. Geoffray;Jean-Claude Gérard;L. Gesa;H. Gomez;Rafał Graczyk;C. Griffith;D. Grodent;M. Guarcello;J. Gustin;K. Hamano;P. Hargrave;Y. Hello;Kevin Heng;E. Herrero;A. Hornstrup;Benoît Hubert;Shigeru Ida;M. Ikoma;N. Iro;Patrick Irwin;C. Jarchow;Jean Jaubert;Hugh R. A. Jones;Queyrel Julien;Shingo Kameda;F. Kerschbaum;P. Kervella;T. Koskinen;M. Krijger;N. Krupp;M. Lafarga;F. Landini;E. Lellouch;G. Leto;A. Luntzer;T. Rank-Lüftinger;Antonio Maggio;J. Maldonado;Jean-Pierre Maillard;Urs Mall;J. Marquette;Stéphane Mathis;P. Maxted;T. Matsuo;A. Medvedev;Yamila Miguel;V. Minier;G. Morello;Alessandro Mura;N. Narita;V. Nascimbeni;N. Nguyen Tong;V. Noce;F. Oliva;E. Pallé;Paul Palmer;M. Pancrazzi;A. Papageorgiou;V. Parmentier;M. Perger;A. Petralia;S. Pezzuto;Ray Pierrehumbert;I. Pillitteri;G. Piotto;G. Pisano;L. Prisinzano;A. Radioti;J. Réess;L. Rezac;M. Rocchetto;A. Rosich;N. Sanna;A. Santerne;G. Savini;G. Scandariato;B. Sicardy;Carles Sierra;G. Sindoni;K. Skup;I. Snellen;M. Sobiecki;L. Soret;A. Sozzetti;A. Stiepen;A. Strugarek;Jake Taylor;William Taylor;L. Terenzi;M. Tessenyi;A. Tsiaras;C. Tucker;Diana Valencia;G. Vasisht;A. Vazan;F. Vilardell;S. Vinatier;S. Viti;Rens Waters;P. Wawer;A. Wawrzaszek;A. Whitworth;Yuk L. Yung;S. Yurchenko;M. Z. Osorio;R. Zellem;T. Zingales;F. Zwart