English
Related papers

Related papers: The Advanced X-ray Imaging Satellite

200 papers

A deep 75 ks {\it Chandra} ACIS--I data of NGC 2024 was analyzed, aiming at a search for diffuse X-ray emission in this one of the most nearby (415 pc) massive star-forming regions. After removing point sources, an extended emission was…

In order to take full advantage of the U.S. Department of Energy's billion-dollar investments into the next-generation research infrastructure (e.g., exascale, light sources, colliders), advances are required not only in detector technology…

Instrumentation and Detectors · Physics 2022-05-24 Antonino Miceli , Kazutomo Yoshii , Ian T. Foster

We describe the expected scientific capabilities of CHARIS, a high-contrast integral-field spectrograph (IFS) currently under construction for the Subaru telescope. CHARIS is part of a new generation of instruments, enabled by extreme…

The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interactions and also happens to be an excellent dark matter candidate. Axions constituting the dark matter halo of our galaxy may be detected by…

An X-ray Interferometer (XRI) has recently been proposed as a theme for ESA's Voyage 2050 planning cycle, with the eventual goal to observe the X-ray sky with an unprecedented angular resolution better than 1 micro arcsec (5 prad) [1]. A…

Instrumentation and Methods for Astrophysics · Physics 2021-07-19 Roland den Hartog , Phil Uttley , Richard Willingale , Henk Hoevers , Jan-Willem den Herder , Michael Wise

Since its launch on October 2002, the INTEGRAL satellite has revolutionized our knowledge of the hard X-ray sky thanks to its unprecedented imaging capabilities and source detection positional accuracy above 20 keV. Nevertheless, many of…

SPHEREx, a NASA explorer satellite launched on 11 March 2025, is carrying out the first all-sky near-infrared spectral survey. The satellite observes in 102 spectral bands from 0.75 to 5.0 um with a resolving power ranging from 35 to 130 in…

Instrumentation and Methods for Astrophysics · Physics 2025-12-19 James J. Bock , Asad M. Aboobaker , Joseph Adamo , Rachel Akeson , John M. Alred , Farah Alibay , Matthew L. N. Ashby , Yoonsoo P. Bach , Lindsey E. Bleem , Douglas Bolton , David F. Braun , Sean Bruton , Sean A. Bryan , Tzu-Ching Chang , Shuang-Shuang Chen , Yun-Ting Cheng , James R. Cheshire , Yi-Kuan Chiang , Jean Choppin de Janvry , Samuel Condon , Walter R. Cook , Asantha Cooray , Brendan P. Crill , Ari J. Cukierman , Olivier Dore , C. Darren Dowell , Gregory P. Dubois-Felsmann , Tim Eifler , Spencer Everett , Beth E. Fabinsky , Andreas L. Faisst , James L. Fanson , Allen H. Farrington , Tamim Fatahi , Candice M. Fazar , Richard M. Feder , Eric H. Frater , Henry S. Grasshorn Gebhardt , Utkarsh Giri , Tatiana Goldina , Varoujan Gorjian , Salman Habib , William G. Hart , Chen Heinrich , Joseph L. Hora , Zhaoyu Huai , Howard Hui , Young-Soo Jo , Woong-Seob Jeong , Jae Hwan Kang , Miju Kang , Branislav Kecman , Chul-Hwan Kim , Jaeyeong Kim , Minjin Kim , Young-Jun Kim , Yongjung Kim , J. Davy Kirkpatrick , Yosuke Kobayashi , Phil M. Korngut , Elisabeth Krause , Bomee Lee , Ho-Gyu Lee , Jae-Joon Lee , Jeong-Eun Lee , Carey M. Lisse , Giacomo Mariani , Daniel C. Masters , Philip D. Mauskopf , Gary J. Melnick , Mary H. Minasyan , Jordan Mirocha , Hiromasa Miyasaka , Anne Moore , Bradley D. Moore , Giulia Murgia , Bret J. Naylor , Christina Nelson , Chi H. Nguyen , Hien T. Nguyen , Jinyoung K. Noh , Stephen Padin , Roberta Paladini , Sung-Joon Park , Konstantin I. Penanen , Dustin S. Putnam , Jeonghyun Pyo , Nesar Ramachandra , Keshav Ramanathan , Zafar Rustamkulov , Daniel J. Reiley , Eric B. Rice , Jennifer M. Rocca , Ji Yeon Seok , Roger Smith , Jeremy Stober , Sara Susca , Harry I. Teplitz , Michael P. Thelen , Volker Tolls , Gabriela Torrini , Amy R. Trangsrud , Stephen Unwin , Phani Velicheti , Pao-Yu Wang , Robin Y. Wen , Michael-W. -Werner , Abby E. Williams , Ross Williamson , James Wincentsen , Rogier A. Windhorst , Soung-Chul Yang , Yujin Yang , Michael Zemcov

The launch of the Chandra X-ray Observatory in July 1999 opened a new era in X-ray astronomy. Its unprecedented, <0.5" spatial resolution and low background are providing views of the X-ray sky 10-100 times fainter than previously possible.…

The Lynx X-ray Surveyor Mission is one of 4 large missions being studied by NASA Science and Technology Definition Teams as mission concepts to be evaluated by the upcoming 2020 Decadal Survey. By utilizing optics that couple fine angular…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Abraham D. Falcone , Ralph P. Kraft , Marshall W. Bautz , Jessica A. Gaskin , John A. Mulqueen , Doug A. Swartz

We study the feasibility of a new generation axion helioscope, the most ambitious and promising detector of solar axions to date. We show that large improvements in magnetic field volume, x-ray focusing optics and detector backgrounds are…

The Swift mission, scheduled for launch in early 2004, is a multiwavelength observatory for gamma-ray burst (GRB) astronomy. It is the first-of-its-kind autonomous rapid-slewing satellite for transient astronomy and pioneers the way for…

The Advanced Telescope for High-energy Astrophysics (Athena+) is being proposed to ESA as the L2 mission (for a launch in 2028) and is specifically designed to answer two of the most pressing questions for astrophysics in the forthcoming…

High-mass X-ray binary systems are powered by the stellar wind of their donor stars. The X-ray state of Cygnus X-1 is correlated with the properties of the wind which defines the environment of mass accretion. Chandra-HETGS observations…

XEUS is under study by ESA as part of the Horizon 2000+ program to utilize the International Space Station (ISS) for astronomical applications. XEUS will be a long-term X-ray observatory with an initial mirror area of 6m2 at 1 keV that will…

[NIRSS is one of three concepts that contributed to the Wide-Field Infrared Survey Telescope (WFIRST) mission advocated by the Decadal Survey.] Operating beyond the reaches of the Earth's atmosphere, free of its limiting absorption and…

Lynx is the next-generation observatory which will provide unprecedented X-ray vision into the otherwise invisible Universe to gain understanding of origins and physics of the cosmos. Lynx will see the dawn of black holes, reveal what…

Instrumentation and Methods for Astrophysics · Physics 2018-10-10 The Lynx Team

Far-infrared astronomy has advanced rapidly since its inception in the late 1950's, driven by a maturing technology base and an expanding community of researchers. This advancement has shown that observations at far-infrared wavelengths are…

Using new cosmological models for galaxy evolution, predictions for the next generation of deep mid-IR surveys are presented for both the ASTRO-F space telescope (due for launch 2003) and the proposed HII/L2 mission (2010). Although ASTRO-F…

Astrophysics · Physics 2007-05-23 Chris Pearson