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We have implemented upgrades to the University of Wyoming's Red Buttes Observatory (RBO) to allow remote and autonomous operations using the 0.6 m telescope. Detailed descriptions of hardware and software components provide sufficient…

Instrumentation and Methods for Astrophysics · Physics 2016-09-08 David H. Kasper , Tyler G. Ellis , Rex R. Yeigh , Henry A. Kobulnicky , Hannah Jang-Condell , Mark Kelley , Gerald J. Bucher , James S. Weger

The Wide-field Infrared Transient Explorer (WINTER) is a near-infrared time-domain survey instrument operating on a dedicated 1-meter robotic telescope at Palomar Observatory. The project takes advantage of recent technology advances in…

We have recently commissioned a novel infrared ($0.9-1.7$ $\mu$m) integral field spectrograph (IFS) called the Wide Integral Field Infrared Spectrograph (WIFIS). WIFIS is a unique instrument that offers a very large field-of-view…

The Wendelstein Observatory of Ludwig Maximilians University of Munich has recently been upgraded with a modern 2m robotic telescope. One Nasmyth port of the telescope has been equipped with a wide-field corrector which preserves the…

Instrumentation and Methods for Astrophysics · Physics 2015-06-22 Ralf Kosyra , Claus Goessl , Ulrich Hopp , Florian Lang-Bardl , Arno Riffeser , Ralf Bender , Stella Seitz

The ongoing development of large infrared array detectors has enabled wide field, deep surveys to be undertaken. There are, however, a number of challenges in building an infrared instrument which has both excellent optical quality and high…

Astrophysics · Physics 2021-07-22 Coryn A. L. Bailer-Jones , Peter Bizenberger , Clemens Storz

We present the current results from the development of a wide integral field infrared spectrograph (WIFIS). WIFIS offers an unprecedented combination of etendue and spectral resolving power for seeing-limited, integral field observations in…

The Wide-Field InfraRed Space Telescope (WFIRST) will be capable of delivering precise astrometry for faint sources over the enormous field of view of its main camera, the Wide-Field Imager (WFI). This unprecedented combination will be…

A large wide-field telescope and camera with optical throughput over 200 m^2 deg^2 -- a factor of 50 beyond what we currently have -- would enable the detection of faint moving or bursting optical objects: from Earth threatening asteroids…

Astrophysics · Physics 2009-11-07 J. Anthony Tyson , the LSST Collaboration

The World Space Observatory is an unconventional space project proceeding via distributed studies. The present design, verified for feasibilty, consists of a 1.7-meter telescope operating at the second Largangian point of the Earth-Sun…

The Sun Yat-sen University (SYSU) 80 cm telescope is a new generation near-infrared (NIR) facility in China dedicated to time-domain astronomy, while also serving as a testbed for emerging NIR cameras. Commissioned in October 2024 at the…

The World Space Observatory Project is a new space mission concept, grown out the needs of the Astronomical community to have access to the part of the electromagnetic spectrum where all known physics can be studied on all possible time…

We report on the upgraded One Degree Imager (ODI) at the WIYN 3.5 meter telescope at the Kitt Peak Observatory after the focal plane was expanded by an additional seventeen detectors in spring 2015. The now thirty Orthogonal Transfer Array…

Equipped with a suitable optical relay system, telescopes employing low-cost fixed primary mirrors could point and track while delivering high-quality images to a fixed location. Such an optical tracking system would enable liquid-mirror…

Astrophysics · Physics 2009-11-06 Paul Hickson

This paper reports on the current status of the World Space Observatory WSO-UV, a space mission for UV astronomy, planned for launch at the beginning of next decade. It is based on a 1.7 m telescope, with focal plane instruments including…

At a fraction the total cost of an equivalent orbital mission, scientific balloon-borne platforms, operating above 99.7% of the Earth's atmosphere, offer attractive, competitive, and effective observational capabilities -- namely space-like…

Wayne State University's Dan Zowada Memorial Observatory is a fully robotic 0.5m telescope and imaging system located under the dark skies of New Mexico. The observatory is particularly suited to time domain astronomy: the observation of…

Instrumentation and Methods for Astrophysics · Physics 2022-05-04 Robert Carr , David Cinabro , Edward Cackett , David Moutard , Russell Carroll

The Wide Field Monitor (WFM) is one of the three instruments on the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) mission, which was proposed in response to the NASA 2023 call for a probe class mission. The…

The James Webb Space Telescope (JWST) is a large, infrared space telescope that has recently started its science program which will enable breakthroughs in astrophysics and planetary science. Notably, JWST will provide the very first…

Instrumentation and Methods for Astrophysics · Physics 2023-05-31 Michael W. McElwain , Lee D. Feinberg , Marshall D. Perrin , Mark Clampin , C. Matt Mountain , Matthew D. Lallo , Charles-Philippe Lajoie , Randy A. Kimble , Charles W. Bowers , Christopher C. Stark , D. Scott Acton , Ken Aiello , Charles Atkinson , Beth Barinek , Allison Barto , Scott Basinger , Tracy Beck , Matthew D. Bergkoetter , Marcel Bluth , Rene A. Boucarut , Gregory R. Brady , Keira J. Brooks , Bob Brown , John Byard , Larkin Carey , Maria Carrasquilla , Sid Celeste , Dan Chae , David Chaney , Pierre Chayer , Taylor Chonis , Lester Cohen , Helen J. Cole , Thomas M. Comeau , Matthew Coon , Eric Coppock , Laura Coyle , Rick Davis , Bruce H. Dean , Kenneth J. Dziak , Michael Eisenhower , Nicolas Flagey , Randy Franck , Benjamin Gallagher , Larry Gilman , Tiffany Glassman , Gary Golnik , Joseph J. Green , John Grieco , Shari Haase , Theodore J. Hadjimichael , John G. Hagopian , Walter G. Hahn , George F. Hartig , Keith A. Havey , William L. Hayden , Robert Hellekson , Brian Hicks , Sherie T. Holfeltz , Joseph M. Howard , Jesse A. Huguet , Brian Jahne , Leslie A. Johnson , John D. Johnston , Alden S. Jurling , Jeffrey R. Kegley , Scott Kennard , Ritva A. Keski-Kuha , J. Scott Knight , Bernard A. Kulp , Joshua S. Levi , Marie B. Levine , Paul Lightsey , Robert A. Luetgens , John C. Mather , Gary W. Matthews , Andrew G. McKay , Kimberly I. Mehalick , Marcio Meléndez , Ted Messer , Gary E. Mosier , Jess Murphy , Edmund P. Nelan , Malcolm B. Niedner , Darin M. Noël , Catherine M. Ohara , Raymond G. Ohl , Eugene Olczak , Shannon B. Osborne , Sang Park , Kevin Patton , Charles Perrygo , Laurent Pueyo , Lisbeth Quesnel , Dale Ranck , David C. Redding , Michael W. Regan , Paul Reynolds , Rich Rifelli , Jane R. Rigby , Derek Sabatke , Babak N. Saif , Thomas R. Scorse , Byoung-Joon Seo , Fang Shi , Norbert Sigrist , Koby Smith , J. Scott Smith , Erin C. Smith , Sangmo Tony Sohn , John Spina , H. Philip Stahl , Randal Telfer , Todd Terlecki , Scott C. Texter , David Van Buren , Julie M. Van Campen , Begoña Vila , Mark F. Voyton , Mark Waldman , Chanda B. Walker , Nick Weiser , Conrad Wells , Garrett West , Tony L. Whitman , Eric Wick , Erin Wolf , Greg Young , Thomas P. Zielinski

The James Webb Space Telescope, launched in 2021, is an infrared observatory of novel design: deployable, with active optics, fully open to space for radiative cooling and orbiting the Lagrange point no. 2. This article explains the…

The prototype Robo-AO system at the Palomar Observatory 1.5-m telescope is the world's first fully automated laser adaptive optics instrument. Scientific operations commenced in June 2012 and more than 12,000 observations have since been…

Instrumentation and Methods for Astrophysics · Physics 2015-06-22 Christoph Baranec , Reed Riddle , Nicholas M. Law , Mark R. Chun , Jessica R. Lu , Michael S. Connelley , Donald Hall , Dani Atkinson , Shane Jacobson
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