Theia: Faint objects in motion or the new astrometry frontier

null The Theia Collaboration; Celine Boehm; Alberto Krone-Martins; Antonio Amorim; Guillem Anglada-Escude; Alexis Brandeker; Frederic Courbin; Torsten Ensslin; Antonio Falcao; Katherine Freese; Berry Holl; Lucas Labadie; Alain Leger; Fabien Malbet; Gary Mamon; Barbara McArthur; Alcione Mora; Michael Shao; Alessandro Sozzetti; Douglas Spolyar; Eva Villaver; Conrado Albertus; Stefano Bertone; Herve Bouy; Michael Boylan-Kolchin; Anthony Brown; Warren Brown; Vitor Cardoso; Laurent Chemin; Riccardo Claudi; Alexandre C. M. Correia; Mariateresa Crosta; Antoine Crouzier; Francis-Yan Cyr-Racine; Mario Damasso; Antonio da Silva; Melvyn Davies; Payel Das; Pratika Dayal; Miguel de Val-Borro; Antonaldo Diaferio; Adrienne Erickcek; Malcolm Fairbairn; Morgane Fortin; Malcolm Fridlund; Paulo Garcia; Oleg Gnedin; Ariel Goobar; Paulo Gordo; Renaud Goullioud; Nigel Hambly; Nathan Hara; David Hobbs; Erik Hog; Andrew Holland; Rodrigo Ibata; Carme Jordi; Sergei Klioner; Sergei Kopeikin; Thomas Lacroix; Jacques Laskar; Christophe Le Poncin-Lafitte; Xavier Luri; Subhabrata Majumdar; Valeri Makarov; Richard Massey; Bertrand Mennesson; Daniel Michalik; Andre Moitinho de Almeida; Ana Mourao; Leonidas Moustakas; Neil Murray; Matthew Muterspaugh; Micaela Oertel; Luisa Ostorero; Angeles Perez-Garcia; Imants Platais; Jordi Portell i de Mora; Andreas Quirrenbach; Lisa Randall; Justin Read; Eniko Regos; Barnes Rory; Krzysztof Rybicki; Pat Scott; Jean Schneider; Jakub Scholtz; Arnaud Siebert; Ismael Tereno; John Tomsick; Wesley Traub; Monica Valluri; Matt Walker; Nicholas Walton; Laura Watkins; Glenn White; Dafydd Wyn Evans; Lukasz Wyrzykowski; Rosemary Wyse

Theia: Faint objects in motion or the new astrometry frontier

The Theia Collaboration, Celine Boehm, Alberto Krone-Martins, Antonio Amorim, Guillem Anglada-Escude, Alexis Brandeker, Frederic Courbin, Torsten Ensslin, Antonio Falcao, Katherine Freese, Berry Holl, Lucas Labadie, Alain Leger, Fabien Malbet, Gary Mamon, Barbara McArthur, Alcione Mora, Michael Shao, Alessandro Sozzetti, Douglas SpolyarEva Villaver, Conrado Albertus, Stefano Bertone, Herve Bouy, Michael Boylan-Kolchin, Anthony Brown, Warren Brown, Vitor Cardoso, Laurent Chemin, Riccardo Claudi, Alexandre C. M. Correia, Mariateresa Crosta, Antoine Crouzier, Francis-Yan Cyr-Racine, Mario Damasso, Antonio da Silva, Melvyn Davies, Payel Das, Pratika Dayal, Miguel de Val-Borro, Antonaldo Diaferio, Adrienne Erickcek, Malcolm Fairbairn, Morgane Fortin, Malcolm Fridlund, Paulo Garcia, Oleg Gnedin, Ariel Goobar, Paulo Gordo, Renaud Goullioud, Nigel Hambly, Nathan Hara, David Hobbs, Erik Hog, Andrew Holland, Rodrigo Ibata, Carme Jordi, Sergei Klioner, Sergei Kopeikin, Thomas Lacroix, Jacques Laskar, Christophe Le Poncin-Lafitte, Xavier Luri, Subhabrata Majumdar, Valeri Makarov, Richard Massey, Bertrand Mennesson, Daniel Michalik, Andre Moitinho de Almeida, Ana Mourao, Leonidas Moustakas, Neil Murray, Matthew Muterspaugh, Micaela Oertel, Luisa Ostorero, Angeles Perez-Garcia, Imants Platais, Jordi Portell i de Mora, Andreas Quirrenbach, Lisa Randall, Justin Read, Eniko Regos, Barnes Rory, Krzysztof Rybicki, Pat Scott, Jean Schneider, Jakub Scholtz, Arnaud Siebert, Ismael Tereno, John Tomsick, Wesley Traub, Monica Valluri, Matt Walker, Nicholas Walton, Laura Watkins, Glenn White, Dafydd Wyn Evans, Lukasz Wyrzykowski, Rosemary Wyse

School of Physics and Astronomy

Research output: Other contribution

Abstract

In the context of the ESA M5 (medium mission) call we proposed a new satellite mission, Theia, based on relative astrometry and extreme precision to study the motion of very faint objects in the Universe. Theia is primarily designed to study the local dark matter properties, the existence of Earth-like exoplanets in our nearest star systems and the physics of compact objects. Furthermore, about 15 $\%$ of the mission time was dedicated to an open observatory for the wider community to propose complementary science cases. With its unique metrology system and "point and stare" strategy, Theia's precision would have reached the sub micro-arcsecond level. This is about 1000 times better than ESA/Gaia's accuracy for the brightest objects and represents a factor 10-30 improvement for the faintest stars (depending on the exact observational program). In the version submitted to ESA, we proposed an optical (350-1000nm) on-axis TMA telescope. Due to ESA Technology readiness level, the camera's focal plane would have been made of CCD detectors but we anticipated an upgrade with CMOS detectors. Photometric measurements would have been performed during slew time and stabilisation phases needed for reaching the required astrometric precision.

Original language	English
Type	arXiv e-prints repository
Media of output	pdf
Publication status	Published - 6 Jul 2017

Keywords

Astrophysics - Instrumentation and Methods for Astrophysics

Access to Document

pdfFinal published version, 8.15 MB

http://adsabs.harvard.edu/abs/2017arXiv170701348T

Cite this

The Theia Collaboration, Boehm, C., Krone-Martins, A., Amorim, A., Anglada-Escude, G., Brandeker, A., Courbin, F., Ensslin, T., Falcao, A., Freese, K., Holl, B., Labadie, L., Leger, A., Malbet, F., Mamon, G., McArthur, B., Mora, A., Shao, M., Sozzetti, A., ... Wyse, R. (2017, Jul 6). Theia: Faint objects in motion or the new astrometry frontier. http://adsabs.harvard.edu/abs/2017arXiv170701348T

@misc{c315fb01a8fe42a99c13f8ce164fc011,

title = "Theia: Faint objects in motion or the new astrometry frontier",

abstract = "In the context of the ESA M5 (medium mission) call we proposed a new satellite mission, Theia, based on relative astrometry and extreme precision to study the motion of very faint objects in the Universe. Theia is primarily designed to study the local dark matter properties, the existence of Earth-like exoplanets in our nearest star systems and the physics of compact objects. Furthermore, about 15 $\%$ of the mission time was dedicated to an open observatory for the wider community to propose complementary science cases. With its unique metrology system and {"}point and stare{"} strategy, Theia's precision would have reached the sub micro-arcsecond level. This is about 1000 times better than ESA/Gaia's accuracy for the brightest objects and represents a factor 10-30 improvement for the faintest stars (depending on the exact observational program). In the version submitted to ESA, we proposed an optical (350-1000nm) on-axis TMA telescope. Due to ESA Technology readiness level, the camera's focal plane would have been made of CCD detectors but we anticipated an upgrade with CMOS detectors. Photometric measurements would have been performed during slew time and stabilisation phases needed for reaching the required astrometric precision.",

keywords = "Astrophysics - Instrumentation and Methods for Astrophysics",

author = "{The Theia Collaboration} and Celine Boehm and Alberto Krone-Martins and Antonio Amorim and Guillem Anglada-Escude and Alexis Brandeker and Frederic Courbin and Torsten Ensslin and Antonio Falcao and Katherine Freese and Berry Holl and Lucas Labadie and Alain Leger and Fabien Malbet and Gary Mamon and Barbara McArthur and Alcione Mora and Michael Shao and Alessandro Sozzetti and Douglas Spolyar and Eva Villaver and Conrado Albertus and Stefano Bertone and Herve Bouy and Michael Boylan-Kolchin and Anthony Brown and Warren Brown and Vitor Cardoso and Laurent Chemin and Riccardo Claudi and Correia, {Alexandre C. M.} and Mariateresa Crosta and Antoine Crouzier and Francis-Yan Cyr-Racine and Mario Damasso and {da Silva}, Antonio and Melvyn Davies and Payel Das and Pratika Dayal and {de Val-Borro}, Miguel and Antonaldo Diaferio and Adrienne Erickcek and Malcolm Fairbairn and Morgane Fortin and Malcolm Fridlund and Paulo Garcia and Oleg Gnedin and Ariel Goobar and Paulo Gordo and Renaud Goullioud and Nigel Hambly and Nathan Hara and David Hobbs and Erik Hog and Andrew Holland and Rodrigo Ibata and Carme Jordi and Sergei Klioner and Sergei Kopeikin and Thomas Lacroix and Jacques Laskar and {Le Poncin-Lafitte}, Christophe and Xavier Luri and Subhabrata Majumdar and Valeri Makarov and Richard Massey and Bertrand Mennesson and Daniel Michalik and {Moitinho de Almeida}, Andre and Ana Mourao and Leonidas Moustakas and Neil Murray and Matthew Muterspaugh and Micaela Oertel and Luisa Ostorero and Angeles Perez-Garcia and Imants Platais and {de Mora}, {Jordi Portell i} and Andreas Quirrenbach and Lisa Randall and Justin Read and Eniko Regos and Barnes Rory and Krzysztof Rybicki and Pat Scott and Jean Schneider and Jakub Scholtz and Arnaud Siebert and Ismael Tereno and John Tomsick and Wesley Traub and Monica Valluri and Matt Walker and Nicholas Walton and Laura Watkins and Glenn White and Evans, {Dafydd Wyn} and Lukasz Wyrzykowski and Rosemary Wyse",

year = "2017",

month = jul,

day = "6",

language = "English",

type = "Other",

}

The Theia Collaboration, Boehm, C, Krone-Martins, A, Amorim, A, Anglada-Escude, G, Brandeker, A, Courbin, F, Ensslin, T, Falcao, A, Freese, K, Holl, B, Labadie, L, Leger, A, Malbet, F, Mamon, G, McArthur, B, Mora, A, Shao, M, Sozzetti, A, Spolyar, D, Villaver, E, Albertus, C, Bertone, S, Bouy, H, Boylan-Kolchin, M, Brown, A, Brown, W, Cardoso, V, Chemin, L, Claudi, R, Correia, ACM, Crosta, M, Crouzier, A, Cyr-Racine, F-Y, Damasso, M, da Silva, A, Davies, M, Das, P, Dayal, P, de Val-Borro, M, Diaferio, A, Erickcek, A, Fairbairn, M, Fortin, M, Fridlund, M, Garcia, P, Gnedin, O, Goobar, A, Gordo, P, Goullioud, R, Hambly, N, Hara, N, Hobbs, D, Hog, E, Holland, A, Ibata, R, Jordi, C, Klioner, S, Kopeikin, S, Lacroix, T, Laskar, J, Le Poncin-Lafitte, C, Luri, X, Majumdar, S, Makarov, V, Massey, R, Mennesson, B, Michalik, D, Moitinho de Almeida, A, Mourao, A, Moustakas, L, Murray, N, Muterspaugh, M, Oertel, M, Ostorero, L, Perez-Garcia, A, Platais, I, de Mora, JPI, Quirrenbach, A, Randall, L, Read, J, Regos, E, Rory, B, Rybicki, K, Scott, P, Schneider, J, Scholtz, J, Siebert, A, Tereno, I, Tomsick, J, Traub, W, Valluri, M, Walker, M, Walton, N, Watkins, L, White, G, Evans, DW, Wyrzykowski, L & Wyse, R 2017, Theia: Faint objects in motion or the new astrometry frontier.. <http://adsabs.harvard.edu/abs/2017arXiv170701348T>

TY - GEN

T1 - Theia: Faint objects in motion or the new astrometry frontier

AU - The Theia Collaboration, null

AU - Boehm, Celine

AU - Krone-Martins, Alberto

AU - Amorim, Antonio

AU - Anglada-Escude, Guillem

AU - Brandeker, Alexis

AU - Courbin, Frederic

AU - Ensslin, Torsten

AU - Falcao, Antonio

AU - Freese, Katherine

AU - Holl, Berry

AU - Labadie, Lucas

AU - Leger, Alain

AU - Malbet, Fabien

AU - Mamon, Gary

AU - McArthur, Barbara

AU - Mora, Alcione

AU - Shao, Michael

AU - Sozzetti, Alessandro

AU - Spolyar, Douglas

AU - Villaver, Eva

AU - Albertus, Conrado

AU - Bertone, Stefano

AU - Bouy, Herve

AU - Boylan-Kolchin, Michael

AU - Brown, Anthony

AU - Brown, Warren

AU - Cardoso, Vitor

AU - Chemin, Laurent

AU - Claudi, Riccardo

AU - Correia, Alexandre C. M.

AU - Crosta, Mariateresa

AU - Crouzier, Antoine

AU - Cyr-Racine, Francis-Yan

AU - Damasso, Mario

AU - da Silva, Antonio

AU - Davies, Melvyn

AU - Das, Payel

AU - Dayal, Pratika

AU - de Val-Borro, Miguel

AU - Diaferio, Antonaldo

AU - Erickcek, Adrienne

AU - Fairbairn, Malcolm

AU - Fortin, Morgane

AU - Fridlund, Malcolm

AU - Garcia, Paulo

AU - Gnedin, Oleg

AU - Goobar, Ariel

AU - Gordo, Paulo

AU - Goullioud, Renaud

AU - Hambly, Nigel

AU - Hara, Nathan

AU - Hobbs, David

AU - Hog, Erik

AU - Holland, Andrew

AU - Ibata, Rodrigo

AU - Jordi, Carme

AU - Klioner, Sergei

AU - Kopeikin, Sergei

AU - Lacroix, Thomas

AU - Laskar, Jacques

AU - Le Poncin-Lafitte, Christophe

AU - Luri, Xavier

AU - Majumdar, Subhabrata

AU - Makarov, Valeri

AU - Massey, Richard

AU - Mennesson, Bertrand

AU - Michalik, Daniel

AU - Moitinho de Almeida, Andre

AU - Mourao, Ana

AU - Moustakas, Leonidas

AU - Murray, Neil

AU - Muterspaugh, Matthew

AU - Oertel, Micaela

AU - Ostorero, Luisa

AU - Perez-Garcia, Angeles

AU - Platais, Imants

AU - de Mora, Jordi Portell i

AU - Quirrenbach, Andreas

AU - Randall, Lisa

AU - Read, Justin

AU - Regos, Eniko

AU - Rory, Barnes

AU - Rybicki, Krzysztof

AU - Scott, Pat

AU - Schneider, Jean

AU - Scholtz, Jakub

AU - Siebert, Arnaud

AU - Tereno, Ismael

AU - Tomsick, John

AU - Traub, Wesley

AU - Valluri, Monica

AU - Walker, Matt

AU - Walton, Nicholas

AU - Watkins, Laura

AU - White, Glenn

AU - Evans, Dafydd Wyn

AU - Wyrzykowski, Lukasz

AU - Wyse, Rosemary

PY - 2017/7/6

Y1 - 2017/7/6

N2 - In the context of the ESA M5 (medium mission) call we proposed a new satellite mission, Theia, based on relative astrometry and extreme precision to study the motion of very faint objects in the Universe. Theia is primarily designed to study the local dark matter properties, the existence of Earth-like exoplanets in our nearest star systems and the physics of compact objects. Furthermore, about 15 $\%$ of the mission time was dedicated to an open observatory for the wider community to propose complementary science cases. With its unique metrology system and "point and stare" strategy, Theia's precision would have reached the sub micro-arcsecond level. This is about 1000 times better than ESA/Gaia's accuracy for the brightest objects and represents a factor 10-30 improvement for the faintest stars (depending on the exact observational program). In the version submitted to ESA, we proposed an optical (350-1000nm) on-axis TMA telescope. Due to ESA Technology readiness level, the camera's focal plane would have been made of CCD detectors but we anticipated an upgrade with CMOS detectors. Photometric measurements would have been performed during slew time and stabilisation phases needed for reaching the required astrometric precision.

AB - In the context of the ESA M5 (medium mission) call we proposed a new satellite mission, Theia, based on relative astrometry and extreme precision to study the motion of very faint objects in the Universe. Theia is primarily designed to study the local dark matter properties, the existence of Earth-like exoplanets in our nearest star systems and the physics of compact objects. Furthermore, about 15 $\%$ of the mission time was dedicated to an open observatory for the wider community to propose complementary science cases. With its unique metrology system and "point and stare" strategy, Theia's precision would have reached the sub micro-arcsecond level. This is about 1000 times better than ESA/Gaia's accuracy for the brightest objects and represents a factor 10-30 improvement for the faintest stars (depending on the exact observational program). In the version submitted to ESA, we proposed an optical (350-1000nm) on-axis TMA telescope. Due to ESA Technology readiness level, the camera's focal plane would have been made of CCD detectors but we anticipated an upgrade with CMOS detectors. Photometric measurements would have been performed during slew time and stabilisation phases needed for reaching the required astrometric precision.

KW - Astrophysics - Instrumentation and Methods for Astrophysics

M3 - Other contribution

ER -

Theia: Faint objects in motion or the new astrometry frontier

Abstract

Keywords

Access to Document

Fingerprint

Cite this