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Related papers: The NASA Probe space mission concept, Cosmic Evolu…

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As part of a study funded by NASA Headquarters, we are developing a Probe-class mission concept called the Cosmic Evolution Through UV Spectroscopy (CETUS). CETUS includes a 1.5-m aperture diameter telescope with a large field-of-view…

The Far Ultraviolet Spectroscopic Explorer (FUSE) is a NASA astronomy mission that will explore the 905-1187 A wavelength region at high spectral resolution. Funded by NASA's Explorer Program, this Origins mission is scheduled for a 1999…

Astrophysics · Physics 2007-05-23 Kenneth R. Sembach

UV-SCOPE is a mission concept to determine the causes of atmospheric mass loss in exoplanets, investigate the mechanisms driving aerosol formation in hot Jupiters, and study the influence of the stellar environment on atmospheric evolution…

SPACE (SPectroscopic All-sky Cosmic Explorer) is a class-M mission proposed to ESA for the Cosmic Vision 2015-2025 call and recently promoted to the next assessment study phase. SPACE will produce the first all-sky spectroscopic survey of…

Astrophysics · Physics 2010-11-11 M. Robberto , A. Cimatti , the SPACE Science Team

The Star-Planet Activity Research CubeSat (SPARCS) is a NASA-funded 6U-CubeSat mission designed to monitor ultraviolet (UV) radiation from low-mass stars. These stars' relatively high-frequency and high-energy UV flares significantly affect…

For the first time in human history, technologies have matured sufficiently to enable a mission capable of discovering and characterizing habitable planets like Earth orbiting sunlike stars other than the Sun. At the same time, such a…

The Cosmic Origins Spectrograph (COS) was installed in the Hubble Space Telescope in May, 2009 as part of Servicing Mission 4 to provide high sensitivity, medium and low resolution spectroscopy at far- and near-ultraviolet wavelengths (FUV,…

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a…

Instrumentation and Methods for Astrophysics · Physics 2018-06-13 L. Amati , P. O'Brien , D. Goetz , E. Bozzo , C. Tenzer , F. Frontera , G. Ghirlanda , C. Labanti , J. P. Osborne , G. Stratta , N. Tanvir , R. Willingale , P. Attina , R. Campana , A. J. Castro-Tirado , C. Contini , F. Fuschino , A. Gomboc , R. Hudec , P. Orleanski , E. Renotte , T. Rodic , Z. Bagoly , A. Blain , P. Callanan , S. Covino , A. Ferrara , E. Le Floch , M. Marisaldi , S. Mereghetti , P. Rosati , A. Vacchi , P. D'Avanzo , P. Giommi , A. Gomboc , S. Piranomonte , L. Piro , V. Reglero , A. Rossi , A. Santangelo , R. Salvaterra , G. Tagliaferri , S. Vergani , S. Vinciguerra , M. Briggs , E. Campolongo , R. Ciolfi , V. Connaughton , B. Cordier , B. Morelli , M. Orlandini , C. Adami , A. Argan , J. -L. Atteia , N. Auricchio , L. Balazs , G. Baldazzi , S. Basa , R. Basak , P. Bellutti , M. G. Bernardini , G. Bertuccio , J. Braga , M. Branchesi , S. Brandt , E. Brocato , C. Budtz-Jorgensen , A. Bulgarelli , L. Burderi , J. Camp , S. Capozziello , J. Caruana , P. Casella , B. Cenko , P. Chardonnet , B. Ciardi , S. Colafrancesco , M. G. Dainotti , V. D'Elia , D. De Martino , M. De Pasquale , E. Del Monte , M. Della Valle , A. Drago , Y. Evangelista , M. Feroci , F. Finelli , M. Fiorini , J. Fynbo , A. Gal-Yam , B. Gendre , G. Ghisellini , A. Grado , C. Guidorzi , M. Hafizi , L. Hanlon , J. Hjorth , L. Izzo , L. Kiss , P. Kumar , I. Kuvvetli , M. Lavagna , T. Li , F. Longo , M. Lyutikov , U. Maio , E. Maiorano , P. Malcovati , D. Malesani , R. Margutti , A. Martin-Carrillo , N. Masetti , S. McBreen , R. Mignani , G. Morgante , C. Mundell , H. U. Nargaard-Nielsen , L. Nicastro , E. Palazzi , S. Paltani , F. Panessa , G. Pareschi , A. Pe'er , A. V. Penacchioni , E. Pian , E. Piedipalumbo , T. Piran , G. Rauw , M. Razzano , A. Read , L. Rezzolla , P. Romano , R. Ruffini , S. Savaglio , V. Sguera , P. Schady , W. Skidmore , L. Song , E. Stanway , R. Starling , M. Topinka , E. Troja , M. van Putten , E. Vanzella , S. Vercellone , C. Wilson-Hodge , D. Yonetoku , G. Zampa , N. Zampa , B. Zhang , B. B. Zhang , S. Zhang , S. -N. Zhang , A. Antonelli , F. Bianco , S. Boci , M. Boer , M. T. Botticella , O. Boulade , C. Butler , S. Campana , F. Capitanio , A. Celotti , Y. Chen , M. Colpi , A. Comastri , J. -G. Cuby , M. Dadina , A. De Luca , Y. -W. Dong , S. Ettori , P. Gandhi , E. Geza , J. Greiner , S. Guiriec , J. Harms , M. Hernanz , A. Hornstrup , I. Hutchinson , G. Israel , P. Jonker , Y. Kaneko , N. Kawai , K. Wiersema , S. Korpela , V. Lebrun , F. Lu , A. MacFadyen , G. Malaguti , L. Maraschi , A. Melandri , M. Modjaz , D. Morris , N. Omodei , A. Paizis , P. Pata , V. Petrosian , A. Rachevski , J. Rhoads , F. Ryde , L. Sabau-Graziati , N. Shigehiro , M. Sims , J. Soomin , D. Szecsi , Y. Urata , M. Uslenghi , L. Valenziano , G. Vianello , S. Vojtech , D. Watson , J. Zicha

The Large UV/Optical/Infrared Surveyor (LUVOIR) mission is one of four Decadal Survey Mission Concepts studied by NASA in preparation for the US National Academies' Astro2020 Decadal Survey. This observatory has the major goal of…

Instrumentation and Methods for Astrophysics · Physics 2019-12-16 The LUVOIR Team

The Star-Planet Activity Research CubeSat (SPARCS) is a NASA-funded astrophysics mission, devoted to the study of the ultraviolet (UV) time-domain behavior in low-mass stars. Given their abundance and size, low-mass stars are important…

The Spectral Imaging of the Coronal Environment (SPICE) instrument is a high-resolution imaging spectrometer operating at extreme ultraviolet (EUV) wavelengths. In this paper, we present the concept, design, and pre-launch performance of…

The Origins Space Telescope, one of four large Mission Concept studies sponsored by NASA for review in the 2020 US Astrophysics Decadal Survey, will open unprecedented discovery space in the infrared, unveiling our cosmic origins. We…

An outstanding, multi-disciplinary goal of modern science is the study of the diversity of potentially Earth-like planets and the search for life in them. This goal requires a bold new generation of space telescopes, but even the most…

Instrumentation and Methods for Astrophysics · Physics 2019-08-07 Daniel Apai , Tom D. Milster , Dae Wook Kim , Alex Bixel , Glenn Schneider , Ronguang Liang , Jonathan Arenberg

Atmospheric escape is a fundamental process that affects the structure, composition, and evolution of many planets. The signatures of escape are detectable on close-in, gaseous exoplanets orbiting bright stars, owing to the high levels of…

The Transient High-Energy Sky and Early Universe Surveyor (THESEUS) is a mission concept developed in the last years by a large European consortium, with interest in prospective participation by research groups in USA and other non-European…

High Energy Astrophysical Phenomena · Physics 2018-02-07 L. Amati , E. Bozzo , D. Götz , P. O'Brien , M. Della Valle

The purpose of this document is to discuss the scientific case of a space mission to the ice giants Uranus and Neptune and their satellite systems and its relevance to advance our understanding of the ancient past of the Solar System and,…

We describe the space observatory architecture and mission design of the SALTUS mission, a NASA Astrophysics Probe Explorer concept. SALTUS will address key far-infrared science using a 14-m diameter <45 K primary reflector (M1) and will…

XEUS, the X-ray Evolving Universe Spectroscopy mission, is at present an ESA-ISAS initiative for the study of the evolution of the hot Universe in the post-Chandra/XMM-Newton era. The key science objectives of XEUS are: Search for the…

Astrophysics · Physics 2016-08-30 Johan Bleeker , Mariano Mendez
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