中文
相关论文

相关论文: The Visible and Near Infrared module of EChO

200 篇论文

Transit-spectroscopy of exoplanets is one of the key observational techniques to characterize the extrasolar planet and its atmosphere. The observational challenges of these measurements require dedicated instrumentation and only the space…

A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context and by addressing the suitability of planets for the…

地球与行星天体物理 · 物理学 2015-06-03 G. Tinetti , J. P. Beaulieu , T. Henning , M. Meyer , G. Micela , I. Ribas , D. Stam , M. Swain , O. Krause , M. Ollivier , E. Pace , B. Swinyard , A. Aylward , R. van Boekel , A. Coradini , T. Encrenaz , I. Snellen , M. R. Zapatero-Osorio , J. Bouwman , J. Y-K. Cho , V. Coudé du Foresto , T. Guillot , M. Lopez-Morales , I. Mueller-Wodarg , E. Palle , F. Selsis , A. Sozzetti , P. A. R. Ade , N. Achilleos , A. Adriani , C. B. Agnor , C. Afonso , C. Allende Prieto , G. Bakos , R. J. Barber , M. Barlow , P. Bernath , B. Bezard , P. Bordé , L. R. Brown , A. Cassan , C. Cavarroc , A. Ciaravella , C. O. U. Cockell , A. Coustenis , C. Danielski , L. Decin , R. De Kok , O. Demangeon , P. Deroo , P. Doel , P. Drossart , L. N. Fletcher , M. Focardi , F. Forget , S. Fossey , P. Fouqué , J. Frith , M. Galand , P. Gaulme , J. I. González Hernández , O. Grasset , D. Grassi , J. L. Grenfell , M. J. Griffin , C. A. Griffith , U. Grözinger , M. Guedel , P. Guio , O. Hainaut , R. Hargreaves , P. H. Hauschildt , K. Heng , D. Heyrovsky , R. Hueso , P. Irwin , L. Kaltenegger , P. Kervella , D. Kipping , T. T. Koskinen , G. Kovács , A. La Barbera , H. Lammer , E. Lellouch , G. Leto , M. Lopez Morales , M. A. Lopez Valverde , M. Lopez-Puertas , C. Lovis , A. Maggio , J. P. Maillard , J. Maldonado Prado , J. B. Marquette , F. J. Martin-Torres , P. Maxted , S. Miller , S. Molinari , D. Montes , A. Moro-Martin , J. I. Moses , O. Mousis , N. Nguyen Tuong , R. Nelson , G. S. Orton , E. Pantin , E. Pascale , S. Pezzuto , D. Pinfield , E. Poretti , R. Prinja , L. Prisinzano , J. M. Rees , A. Reiners , B. Samuel , A. Sanchez-Lavega , J. Sanz Forcada , D. Sasselov , G. Savini , B. Sicardy , A. Smith , L. Stixrude , G. Strazzulla , J. Tennyson , M. Tessenyi , G. Vasisht , S. Vinatier , S. Viti , I. Waldmann , G. J. White , T. Widemann , R. Wordsworth , R. Yelle , Y. Yung , S. N. Yurchenko

Radial velocities (RV) measured from near-infrared (NIR) spectra are a potentially excellent tool to search for extrasolar planets around cool or active stars. High resolution infrared (IR) spectrographs now available are reaching the high…

天体物理仪器与方法 · 物理学 2016-04-07 I. Carleo , N. Sanna , R. Gratton , S. Benatti , M. Bonavita , E. Oliva , L. Origlia , S. Desidera , R. Claudi , E. Sissa

Space telescopes such as EChO (Exoplanet Characterisation Observatory) and JWST (James Webb Space Telescope) will be important for the future study of extrasolar planet atmospheres. Both of these missions are capable of performing high…

地球与行星天体物理 · 物理学 2012-12-21 Joanna K. Barstow , Suzanne Aigrain , Patrick G. J. Irwin , Neil Bowles , Leigh N. Fletcher , Jae-Min Lee

The Near-InfraRed Planet Searcher (NIRPS) is a high-resolution, high-stability near-infrared (NIR) spectrograph equipped with an AO system. Installed on the ESO 3.6-m telescope, it was developed to enable radial velocity (RV) measurements…

天体物理仪器与方法 · 物理学 2025-07-30 Francois Bouchy , Rene Doyon , Francesco Pepe , Claudio Melo , Etienne Artigau , Lison Malo , Francois Wildi , Frederique Baron , Xavier Delfosse , Jose Renan De Medeiros , Rafael Rebolo , Nuno C. Santos , Gregg Wade , Romain Allart , Khaled Al Moulla , Nicolas Blind , Charles Cadieux , Bruno L. Canto Martins , Neil J. Cook , Xavier Dumusque , Yolanda Frensch , Frederic Genest , Jonay I. Gonzalez Hernandez , Nolan Grieves , Gaspare Lo Curto , Christophe Lovis , Lucile Mignon , Louise D. Nielsen , Anne-Sophie Poulin-Girard , Jose Luis Rasilla , Vladimir Reshetov , Danuta Sosnowska , Michael Sordet , Jonathan Saint-Antoine , Alejandro Suarez Mascareno , Simon Thibault , Philippe Vallee , Thomas Vandal , Manuel Abreu , Jose L. A. Aguiar , Guillaume Allain , Tomy Arial , Hugues Auger , Susana C. C. Barros , Luc Bazinet , Bjorn Benneke , Xavier Bonfils , Anne Boucher , Vincent Bourrier , Sebastien Bovay , Christopher Broeg , Denis Brousseau , Vincent Bruniquel , Marta Bryan , Alexandre Cabral , Andres Carmona , Yann Carteret , Zalpha Challita , Bruno Chazelas , Ryan Cloutier , Joao Coelho , Marion Cointepas , Uriel Conod , Nicolas B. Cowan , Eduardo Cristo , Joao Gomes da Silva , Laurie Dauplaise , Antoine Darveau-Bernier , Roseane de Lima Gomes , Daniel Brito de Freitas , Elisa Delgado-Mena , Jean-Baptiste Delisle , David Ehrenreich , Joao Faria , Pedro Figueira , Dasaev O. Fontinele , Thierry Forveille , Jonathan Gagne , Ludovic Genolet , Felix Gracia Temich , Olivier Hernandez , Melissa J. Hobson , Jens Hoeijmakers , Norbert Hubin , Farbod Jahandar , Ray Jayawardhana , Hans-Ulrich Kauf , Dan Kerley , Johann Kolb , Vigneshwaran Krishnamurthy , David Lafreniere , Pierrot Lamontagne , Pierre Larue , Henry Leath , Alexandrine L Heureux , Izan de Castro Leao , Olivia Lim , Allan M. Martins , Jaymie Matthews , Jean-Sebastien Mayer , Yuri S. Messias , Stan Metchev , Leslie Moranta , Christoph Mordasini , Dany Mounzer , Nicola Nari , Ares Osborn , Mathieu Ouellet , Jon Otegi , Lena Parc , Luca Pasquini , Vera M. Passegger , Stefan Pelletier , Celine Peroux , Caroline Piaulet-Ghorayeb , Mykhaylo Plotnykov , Emanuela Pompei , Jason Rowe , Mirsad Sarajlic , Alex Segovia , Julia Seidel , Damien Segransan , Robin Schnell , Ana Rita Costa Silva , Avidaan Srivastava , Valentina Vaulato , Atanas K. Stefanov , Marcio A. Teixeira , Stephane Udry , Joost P. Wardenier , Bachar Wehbe , Drew Weisserman , Vincent Yariv , Gerard Zins

Giant exoplanets on 10-100 au orbits have been directly imaged around young stars. The peak of the thermal emission from these warm young planets is in the near-infrared (~1-5 microns), whereas mature, temperate exoplanets (i.e., those…

EChO is a three-modules (VNIR, SWIR, MWIR), highly integrated spectrometer, covering the wavelength range from 0.55 $\mu$m, to 11.0 $\mu$m. The baseline design includes the goal wavelength extension to 0.4 $\mu$m while an optional LWIR…

天体物理仪器与方法 · 物理学 2015-06-18 M. Focardi , A. M. Di Giorgio , M. Farina , M. Pancrazzi , R. Ottensamer , T. L. Lim , S. Pezzuto , G. Micela , E. Pace

EChO is a dedicated mission to investigate exoplanetary atmospheres. When extracting the planetary signal, one has to take care of the variability of the hosting star, which introduces spectral distortion that can be mistaken as planetary…

天体物理仪器与方法 · 物理学 2015-06-18 G. Scandariato , G. Micela

The CHIRON optical high-resolution echelle spectrometer was commissioned at the 1.5m telescope at CTIO in 2011. The instrument was designed for high throughput and stability, with the goal of monitoring radial velocities of bright stars…

Observations of circumstellar environments to look for the direct signal of exoplanets and the scattered light from disks has significant instrumental implications. In the past 15 years, major developments in adaptive optics, coronagraphy,…

The VLTI Spectro Imager (VSI) was proposed as a second-generation instrument of the Very Large Telescope Interferometer providing the ESO community with spectrally-resolved, near-infrared images at angular resolutions down to 1.1…

Integrated electro-optic (EO) modulators are fundamental photonics components with utility in domains ranging from digital communications to quantum information processing. At telecommunication wavelengths, thin-film lithium niobate…

Motivated by the development of high-dispersion spectrographs in the mid-infrared (MIR) range, we study their application to the atmospheric characterization of nearby non-transiting temperate terrestrial planets around M-type stars. We…

地球与行星天体物理 · 物理学 2021-03-24 Yuka Fujii , Taro Matsuo

VOR, the versatile optimal resolution chopper spectrometer, is designed to probe dynamic phenomena that are currently inaccessible for inelastic neutron scattering due to flux limitations. VOR is a short instrument by the standards of the…

仪器与探测器 · 物理学 2015-06-22 P. P. Deen , A. Vickery , K. H. Andersen , R. Hall-Wilton

The past decade has seen increasing efforts in detecting and characterising exoplanets by high contrast imaging in the near/mid-infrared, which is the optimal wavelength domain for studying old, cold planets. In this work, we present deep…

Integral-field spectroscopy is the most effective method of exploiting the superb image quality of the ESO-VLT, allowing complex astrophysical processes to be probed on the angular scales currently accessible only for imaging data, but with…

The Mini-EUSO instrument is a UV telescope to be placed inside the International Space Station (ISS), looking down on the Earth from a nadir-facing window in the Russian Zvezda module. Mini-EUSO will map the earth in the UV range (300 - 400…

天体物理仪器与方法 · 物理学 2018-09-18 Francesca Capel , Alexander Belov , Marco Casolino , Pavel Klimov

Context. Detailed characterizations of exoplanets are moving to the forefront of planetary science. Temperature is a key marker for understanding atmospheric physics and chemistry. Aims. We aim to retrieve temperatures of N2-O2 dominated…

地球与行星天体物理 · 物理学 2019-12-23 Franz Schreier , Steffen Städt , Fabian Wunderlich , Mareike Godolt , John Lee Grenfell

The World Space Observatory for Ultraviolet (WSO-UV) is an orbital optical telescope with a 1.7 m-diameter primary mirror currently under development. The WSO-UV is aimed to operate in the 115-310 nm UV spectral range. Its two major science…

Mini-EUSO (Multiwavelength Imaging New Instrument for the Extreme Universe Space Observatory) is a telescope observing the Earth from the International Space Station since 2019. The instrument employs a Fresnel-lens optical system and a…

‹ 上一页 1 2 3 10 下一页 ›