World Space Observatory-Ultraviolet: ISSIS, the imaging instrument
Ana I Gómez de Castro, Paola Sestito, Néstor Sánchez, Fátima López-Martínez, Juan Seijas, Maite Gómez, Pablo Rodríguez, José Quintana, Marcos Ubierna, Jacinto Muñoz
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Contribution presented to the 39th COSPAR Scientific Assembly held in Mysore, India and published in the Spacial volume of Advances in Space Research entitled: "Hot Stars, Galactic Star Formation and Cosmic Star Formation History: Ultraviolet Astrophysics using Space Mission"
The Imaging and Slitless Spectroscopy Instrument (ISSIS) will be flown as part of the Science Instrumentation in the World Space Observatory-Ultraviolet (WSO-UV). ISSIS will be the first UV imager to operate in a high Earth orbit from a 2-m class space telescope. In this contribution, the science driving to ISSIS design, as well as main characteristics of ISSIS are presented.
An Ultraviolet Instrument on the Habitable Worlds Observatory: Considerations and Capability Trades on the Multi-Object, Integral-field, and High-resolution modes of a potential UVI
University of Colorado, Boulder（科罗拉多大学博尔德分校）；Laboratory for Atmospheric and Space Physics（大气与空间物理实验室）；BAE Systems, Inc.（BAE系统公司）
The Smallsat Technology Accelerated Maturation Platform-1 (STAMP-1): A Proposal to Advance Ultraviolet Science, Workforce, and Technology for the Habitable Worlds Observatory
Building galaxies, stars, planets and the ingredients for life between the stars. A scientific proposal for a European Ultraviolet-Visible Observatory (EUVO)
The Ultraviolet Type Ia Supernova CubeSat (UVIa): Science Motivation & Mission Concept
University of Florida（佛罗里达大学）；Las Cumbres Observatory（拉思本斯天文台）；Jet Propulsion Laboratory, California Institute of Technology（加州理工学院喷气推进实验室）；University of Iowa（爱荷华大学）；University of California Santa Barbara（加州大学圣塔芭芭拉分校）；Steward Observatory, University of Arizona（亚利桑那大学斯图尔德天文台）；Texas A&M University（德克萨斯农工大学）
Pollux: decisions affecting the optical architecture of a high-resolution spectrograph and polarimeter for the Habitable Worlds Observatory
Department of Physics, University of Oxford（牛津大学物理系）；Space Research Institute, Austrian Academy of Sciences（奥地利科学院空间研究所）；LIRA, Observatoire de Paris, Universite PSL, CNRS, Sorbonne Universite, Universite Paris Cite, CY Cergy Universite（巴黎天文台 LIRA 实验室（隶属于 PSL 大学、CNRS、索邦大学、巴黎西岱大学、CY 塞尔吉大学））；Aix Marseille Univ, CNRS, CNES, LAM, Marseille（艾克斯-马赛大学）
Inverse diffraction for the Atmospheric Imaging Assembly in the Solar Dynamics Observatory
Università di Genova（热那亚大学）；Catholic University of America（美国天主教大学）；NASA Goddard Space Flight Center（美国国家航空航天局戈达德太空飞行中心）；Ecole Polytechnique（巴黎综合理工学院）；CNR - SPIN Genova（意大利国家研究委员会-SPIN热那亚）
Unraveling the Secrets of the lower Solar Atmosphere: One year of Operation of the Solar Ultraviolet Imaging Telescope (SUIT) on board Aditya-L1
Inter-University Centre for Astronomy and Astrophysics（大学间天文学与天体物理学中心）；Manipal Centre for Natural Sciences, Manipal Academy of Higher Education（马尼拉高等教育学院自然科学中心）；Department of Physics, University College, Research Centre, University of Kerala（喀拉拉大学研究学院物理系）；Tezpur University（特佐普尔大学）；Center of Excellence in Space Sciences India, Indian Institute of Science Education and Research Kolkata（印度空间科学卓越中心，加尔各答印度科学与教育研究所）
Bridging the UV Gap: The HST Ultraviolet Foundation for Star Formation Science in the Era of Roman, Euclid, and HWO
INAF-OACN（意大利国家天体物理研究所奥恰诺天文台）；ESO-Garching（欧洲南方天文台加兴）；INAF-Osservatorio Astronomico di Roma（意大利国家天体物理研究所罗马天文台）；University of Colorado Boulder（科罗拉多大学博尔德分校）；UH IfA（夏威夷大学天体物理研究所）；INAF-OAPA（意大利国家天体物理研究所帕尔马天文台）
