Thomas Henning, Inga Kamp, Matthias Samland, Aditya M. Arabhavi, Jayatee Kanwar, Ewine F. van Dishoeck, Manuel Guedel, Pierre-Olivier Lagage, Christoffel Waelke… 展开作者
Thomas Henning, Inga Kamp, Matthias Samland, Aditya M. Arabhavi, Jayatee Kanwar, Ewine F. van Dishoeck, Manuel Guedel, Pierre-Olivier Lagage, Christoffel Waelkens, Alain Abergel, Olivier Absil, David Barrado, Anthony Boccaletti, Jeroen Bouwman, Alessio Caratti o Garatti, Vincent Geers, Adrian M. Glauser, Fred Lahuis, Cyrine Nehme, Goeran Olofsson, Eric Pantin, Tom P. Ray, Bart Vandenbussche, L. B. F. M. Waters, Gillian Wright, Valentin Christiaens, Riccardo Franceschi, Danny Gasman, Rodrigo Guadarrama, Hyerin Jang, Maria Morales-Calderon, Nicole Pawellek, Giulia Perotti, Donna Rodgers-Lee, Juergen Schreiber, Kamber Schwarz, Benoit Tabone, Milou Temmink, Marissa Vlasblom, Luis Colina, Thomas R. Greve, Goeran Oestlin
The study of protoplanetary disks has become increasingly important with the Kepler satellite finding that exoplanets are ubiquitous around stars in our galaxy and the discovery of enormous diversity in planetary system architectures and planet properties. High-resolution near-IR and ALMA images show strong evidence for ongoing planet formation in young disks. The JWST MIRI mid-INfrared Disk Survey (MINDS) aims to (1) investigate the chemical inventory in the terrestrial planet-forming zone across stellar spectral type, (2) follow the gas evolution into the disk dispersal stage, and (3) study the structure of protoplanetary and debris disks in the thermal mid-IR. The MINDS survey will thus build a bridge between the chemical inventory of disks and the properties of exoplanets. The survey comprises 52 targets (Herbig Ae stars, T Tauri stars, very low-mass stars and young debris disks). We primarily obtain MIRI/MRS spectra with high S/N (~100-500) covering the complete wavelength range from 4.9 to 27.9 μm. For a handful of selected targets we also obtain NIRSpec IFU high resolution spectroscopy (2.87-5.27 μm). We will search for signposts of planet formation in thermal emission of micron-sized dust - information complementary to near-IR scattered light emission from small dust grains and emission from large dust in the submillimeter wavelength domain. We will also study the spatial structure of disks in three key systems that have shown signposts for planet formation, TW Hya and HD 169142 using the MIRI coronagraph at 15.5 μm and 10.65 μm respectively and PDS70 using NIRCam imaging in the 1.87 μm narrow and the 4.8 μm medium band filter. ...
Investigating aerosols as a way to reconcile K2-18 b JWST MIRI and NIRISS/NIRSpec observations
Laboratoire d’astrophysique de Bordeaux, Univ. Bordeaux, CNRS（波尔多天体物理学实验室，波尔多大学，法国国家科学研究中心）；ETH University, Center for Origin and Prevalence of Life, Department of Earth and Planetary Sciences（苏黎世联邦理工学院，生命起源与普遍性中心，地球与行星科学系）
NIRCam yells at cloud: JWST MIRI imaging can directly detect exoplanets of the same temperature, mass, age, and orbital separation as Saturn and Jupiter
JWST/MIRI Imaging of the Warm Dust Component of the Epsilon Eridani Debris Disk
Steward Observatory and the Department of Astronomy, The University of Arizona（亚利桑那大学天文学系斯图尔德天文台）；Jet Propulsion Laboratory, California Institute of Technology（加州理工学院喷气推进实验室）
本研究利用JWST/MIRI多波段成像和辐射转移建模，揭示了Epsilon Eridani碎片盘的平滑尘埃分布及内盘结构，确认了行星Epsilon Eri b与尘埃的相互作用，并指出尘埃主要来自外行星带向内迁移。
A Homogeneous Survey of JWST MIRI Transmission Spectra of 10 Exoplanets
Institute of Astronomy, University of Cambridge（剑桥大学天文学研究所）；Space Telescope Science Institute（太空望远镜科学研究所）；School of Physics and Astronomy, Cardiff University（卡迪夫大学物理与天文学院）
JWST/MIRI coronagraphic search for planets in systems with gapped exoKuiper belts and proper motion anomalies
University of Exeter（埃克塞特大学）；Space Telescope Science Institute (STScI)（太空望远镜科学研究所）；University of Arizona（亚利桑那大学）；University of Warwick（华威大学）；Friedrich-Schiller-Universität Jena（耶拿弗里德里希·席勒大学）；University of Birmingham（伯明翰大学）；University of Queensland（昆士兰大学）；University of Cambridge（剑桥大学）
Hot Rocks Survey V: Secondary Eclipse Photometry of GJ 3473 b with JWST/MIRI
Space Telescope Science Institute（太空望远镜科学研究所）；Technical University of Denmark（丹麦技术大学）；University of Southampton（南安普顿大学）；University of Bern（伯尔尼大学）；Johns Hopkins University（约翰斯·霍普金斯大学）；Trinity College Dublin, University of Dublin（都柏林三一学院，都柏林大学）
JWST/MIRI observations of the young TWA 27 system: hydrocarbon disk chemistry, silicate clouds, evidence for a CPD
ETH Zürich（苏黎世联邦理工学院）；Centro de Astrobiología (CAB), CSIC-INTA（天体生物学中心 (CAB)，西班牙国家航空航天技术研究委员会-国家航空技术研究所）；Kapteyn Astronomical Institute, University of Groningen（格罗宁根大学卡普坦天文研究所）；Institute of Astronomy, KU Leuven（荷语鲁汶大学天体物理研究所）；Department of Astronomy, University of Michigan（密歇根大学天文学系）；Department of Astrophysics, University of Zurich（苏黎世大学天体物理学系）；Max-Planck-Institut für Astronomie (MPIA)（马克斯·普朗克天文学研究所）；Johns Hopkins University（约翰斯·霍普金斯大学）；Space Telescope Science Institute（太空望远镜科学研究所）；American Museum of Natural History（美国自然历史博物馆）；Université Paris-Saclay（巴黎萨克雷大学）；Radboud University（拉德堡德大学）；SRON Netherlands Institute for Space Research（荷兰空间研究研究所）；University of Vienna（维也纳大学）；STAR Institute, Université de Liège（列日大学STAR研究所）；LESIA, Observatoire de Paris（巴黎天文台LESIA实验室）；LERMA, Observatoire de Paris（巴黎天文台LERMA实验室）；Leiden Observatory, Leiden University（莱顿大学莱顿天文台）；UK Astronomy Technology Centre, Royal Observatory Edinburgh（爱丁堡皇家天文台英国天文学技术中心）；Carnegie Institution for Science（卡内基科学机构）；Max-Planck-Institut für Extraterrestrische Physik（马克斯·普朗克地外物理研究所）；European Space Agency（欧洲空间局）；Stockholm University（斯德哥尔摩大学）；University of Leicester（莱斯特大学）；Sun Yat-sen University（中山大学）；Dublin Institute for Advanced Studies（都柏林高等研究院）
First Demonstration of Kernel Phase Interferometry on JWST/MIRI: Prospects for Future Planet Searches Around Post Main Sequence Stars
University of California, Irvine（加州大学尔湾分校）；University of California, Santa Cruz（加州大学圣克鲁兹分校）；University of Texas at Austin（德克萨斯大学奥斯汀分校）；University of Arizona（亚利桑那大学）
Direct emission spectroscopy of exoplanets with the medium resolution imaging spectrometer on board JWST MIRI: I. Molecular mapping and sensitivity to instrumental effects
Simultaneous retrieval of orbital phase resolved JWST/MIRI emission spectra of the hot Jupiter WASP-43b: evidence of water, ammonia and carbon monoxide
Inspecting Cloudy Substellar Atmospheres with JWST MIRI Synthetic Magnitudes from Spitzer Mid-infrared Spectra
Department of Physics, Graduate Center, City University of New York（纽约市立大学研究生中心物理系）；Department of Astronomy, Columbia University（哥伦比亚大学天文学系）；Department of Astrophysics, American Museum of Natural History（美国自然历史博物馆天体物理学系）；School of Physics, Trinity College Dublin, The University of Dublin（都柏林三一学院物理学院，都柏林大学）；Department of Physics and Astronomy, Western University（韦仕敦大学物理与天文系）；Institute for Earth and Space Exploration, Western University（韦仕敦大学地球与太空探索研究所）；Department of Physics and Astronomy, Hunter College, City University of New York（纽约市立大学亨特学院物理与天文系）
A Binary Flux Calibrator Reveals the Scientific Potential of Short-integration JWST MIRI Imaging to Directly Detect sub-Jupiter Exoplanets
Eureka Scientific Inc.（Eureka科学公司）；University of Michigan（密歇根大学）；Max Planck Institute for Astronomy（马克斯·普朗克天文学研究所）；University of California Santa Cruz（加州大学圣克鲁兹分校）；Massachusetts Institute of Technology（麻省理工学院）；Johns Hopkins APL（约翰斯·霍普金斯大学应用物理实验室）
Protoplanetary disk cavities with JWST-MIRI: a dichotomy in molecular emission
Texas State University（德克萨斯州立大学）；Vassar College（瓦瑟学院）；University of Arizona（亚利桑那大学）；Mullard Space Science Laboratory, University College London（伦敦大学学院穆拉德空间科学实验室）；NSF’s NOIRLab（美国国家科学基金会NOIR实验室）；Jet Propulsion Laboratory, California Institute of Technology（加州理工学院喷气推进实验室）；University of Exeter（埃克塞特大学）；California Institute of Technology（加州理工学院）；Université Paris-Saclay（巴黎萨克雷大学）
JWST MIRI reveals a potential atmosphere on the ultra-hot rocky planet TOI-431b
University of Maryland（马里兰大学）；University of Chicago（芝加哥大学）；Instituto de Astrofísica de Andalucía (IAA-CSIC)（安达卢西亚天体物理研究所）；University of Birmingham（伯明翰大学）；Carnegie Science（卡内基科学研究所）；Space Telescope Science Institute（太空望远镜科学研究所）；Peking University（北京大学）
JWST/MIRI Imaging Search for Kinematically Detected Protoplanetary Candidates
University of Zürich（苏黎世大学）；Max-Planck Institute for Astronomy (MPIA)（马克斯·普朗克天文学研究所）；Massachusetts Institute of Technology（麻省理工学院）；Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité（巴黎天文台，巴黎文理研究大学，法国国家科学研究中心，索邦大学，巴黎第七大学，巴黎索邦城）；Space Telescope Science Institute（太空望远镜科学研究所）；Johns Hopkins University（约翰斯·霍普金斯大学）；ETH Zürich, Institute for Particle Physics and Astrophysics（苏黎世联邦理工学院，粒子物理与天体物理研究所）
A Characterization of JWST MIRI Detector Persistence and Implications for High-Contrast Imaging
University of Michigan（密歇根大学）；Massachusetts Institute of Technology（麻省理工学院）；Eureka Scientific Inc.（尤里卡科学公司）；JHU Applied Physics Laboratory（约翰霍普金斯大学应用物理实验室）
Coordinated Space and Ground-Based Monitoring of Accretion Bursts in a Protoplanetary Disk: Establishing Mid-Infrared Hydrogen Lines as Accretion Diagnostics for JWST-MIRI
本文利用 JWST-MIRI 对 DQ Tau 双星系统三个轨道周期的协调监测，首次确立并校准了中红外氢复合线作为原行星盘吸积光度诊断指标，并据此为 38 个已发表的原行星盘 MRS 光谱档案样本提供了吸积光度。
Silicate Clouds, SiO, and Molecular Trends across the L-T Sequence: A JWST/MIRI LRS Spectral Library of Brown Dwarfs
The University of Western Ontario（韦仕敦大学）；American Museum of Natural History（美国自然历史博物馆）；Centro de Astrobiología, CSIC-INTA（天体生物学中心，CSIC-INTA）；Université de Montréal（蒙特利尔大学）
A new window in time: a mid-infrared slit spectroscopy mode for precision time-series astronomy with JWST/MIRI
Space Telescope Science Institute（太空望远镜科学研究所）；AURA for the European Space Agency (ESA), Space Telescope Science Institute（为欧洲空间局（ESA）工作的美国大学研究协会，太空望远镜科学研究所）；Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM（巴黎萨克雷大学，巴黎西岱大学，法国原子能和替代能源委员会，法国国家科学研究中心，天体物理学分子图像实验室）；European Space Agency, Space Telescope Science Institute（欧洲空间局，太空望远镜科学研究所）；Instituto de Astrofísica de Canarias (IAC)（加那利群岛天体物理研究所）；Departamento de Astrofísica, Universidad de La Laguna (ULL)（拉帕拉马大学天体物理学系）；Instituto de Astrofísica de Andalucía (IAA-CSIC)（安达卢西亚天体物理研究所）；SRON Space Research Organisation Netherlands（荷兰空间研究组织）
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. VII. Molecular Mapping Performance with JWST/MIRI MRS: VHS 1256 b as a case study
Johns Hopkins University（约翰斯·霍普金斯大学）；Space Telescope Science Institute（太空望远镜科学研究所）；Observatoire de Paris（巴黎天文台）；CNRS（法国国家科学研究中心）；Sorbonne Université（索邦大学）；Laboratoire d’Astrophysique de Bordeaux（波尔多天体物理学实验室）
The Volatile Inventory of 3I/ATLAS as seen with JWST/MIRI
California Institute of Technology（加州理工学院）；Space Telescope Science Institute（太空望远镜科学研究所）；Eureka Scientific（尤里卡科学）；Auburn University（奥本大学）；Johns Hopkins University Applied Physics Laboratory（约翰斯·霍普金斯大学应用物理实验室）
A Next-Generation Exoplanet Atmospheric Retrieval Framework for Transmission Spectroscopy (NEXOTRANS): Comparative Characterization for WASP-39 b Using JWST NIRISS, NIRSpec PRISM, and MIRI Observations
JWST-MIRI's multi-dimensional view of mass loss in the irradiated disks of NGC 1977
Center for Astrophysics | Harvard & Smithsonian（哈佛-史密森天体物理中心）；Steward Observatory, University of Arizona（亚利桑那大学斯图尔德天文台）；Jet Propulsion Laboratory, California Institute of Technology（加州理工学院喷气推进实验室）；Division of Geological and Planetary Sciences, California Institute of Technology（加州理工学院地质与行星科学系）；Astronomy Unit, Department of Physics and Astronomy, Queen Mary University of London（伦敦玛丽女王大学物理与天文学系天文学组）；Lunar and Planetary Laboratory, The University of Arizona（亚利桑那大学月球与行星实验室）；National Radio Astronomy Observatory（国家射电天文台）
JWST/MIRI Finds ISM-like Amorphous Silicates in Interstellar Comet 3I/ATLAS
California Institute of Technology（加州理工学院）；Space Telescope Science Institute（太空望远镜科学研究所）；Johns Hopkins University Applied Physics Laboratory（约翰斯·霍普金斯大学应用物理实验室）；University of California San Diego（加利福尼亚大学圣地亚哥分校）；Eureka Scientific（尤里卡科学公司）；Jet Propulsion Laboratory（喷气推进实验室）
MINDS. Young binary systems with JWST/MIRI: Variable water-rich primaries and extended emission
Carnegie Institution for Science（卡内基科学机构）；Leiden University（莱顿大学）；Max-Planck-Institut für Astronomie (MPIA)（马克斯·普朗克天文学研究所）；Rijksuniversiteit Groningen（格罗宁根大学）；KU Leuven（荷语鲁汶大学）；Université de Liège（列日大学）；Texas State University（德克萨斯州立大学）；University of Exeter（埃克塞特大学）
