Prof. James E. Rhoads Profile

Prof. James E. Rhoads

Associate Professor at Arizona State Univ

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Publications (4)

Proceedings Article | 22 August 2018 Presentation + Paper

ATLAS probe for the study of galaxy evolution with 300,000,000 galaxy spectra

Robert Content, Yun Wang, Massimo Roberto, Mark Dickinson, Henry Ferguson, Lynne Hillenbrand, Wesley Fraser, Peter Behroozi, Jarle Brinchmann, Andrea Cimatti, Emanuele Daddi, Christopher Hirata, Michael Hudson, J. Davy Kirkpatrick, Robert Barkhouser, James Bartlett, Robert Benjamin, Ranga Chary, Charlie Conroy, Megan Donahue, Olivier Doré, Peter Eisenhardt, Karl Glazebrook, George Helou, Sangeeta Malhotra, Lauro Moscardini, Zoran Ninkov, Alvaro Orsi, Michael Ressler, James Rhoads, Jason Rhodes, Alice Shapley, Stephen Smee

Proc. SPIE. 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave

KEYWORDS: Telescopes, Mirrors, Spectrographs, Prisms, Cameras, Sensors, Space telescopes, Digital micromirror devices, Galactic astronomy, Galaxy evolution

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ATLAS (Astrophysics Telescope for Large Area Spectroscopy) Probe is a mission concept for a NASA probe-class space mission with primary science goal the definitive study of galaxy evolution through the capture of 300,000,000 galaxy spectra up to z=7. It is made of a 1.5-m Ritchey-Chretien telescope with a field of view of solid angle 0.4 deg². The wavelength range is at least 1 μm to 4 μm with a goal of 0.9 μm to 5 μm. Average resolution is 600 but with a possible trade-off to get 1000 at the longer wavelengths. The ATLAS Probe instrument is made of 4 identical spectrographs each using a Digital Micro-mirror Device (DMD) as a multi-object mask. It builds on the work done for the ESA SPACE and Phase-A EUCLID projects. Three-mirror fore-optics re-image each sub-field on its DMD which has 2048 x 1080 mirrors 13.6 μm wide with 2 possible tilts, one sending light to the spectrograph, the other to a light dump. The ATLAS Probe spectrographs use prisms as dispersive elements because of their higher and more uniform transmission, their larger bandwidth, and the ability to control the resolution slope with the choice of glasses. Each spectrograph has 2 cameras. While the collimator is made of 4 mirrors, each camera is made of only one mirror which reduces the total number of optics. All mirrors are aspheric but with a relatively small P-V with respect to their best fit sphere making them easily manufacturable. For imaging, a simple mirror to replace the prism is not an option because the aberrations are globally corrected by the collimator and camera together which gives large aberrations when the mirror is inserted. An achromatic grism is used instead. There are many variations of the design that permit very different packaging of the optics. ATLAS Probe will enable ground-breaking science in all areas of astrophysics. It will (1) revolutionize galaxy evolution studies by tracing the relation between galaxies and dark matter from the local group to cosmic voids and filaments, from the epoch of reionization through the peak era of galaxy assembly; (2) open a new window into the dark universe by mapping the dark matter filaments to unveil the nature of the dark Universe using 3D weak lensing with spectroscopic redshifts, and obtaining definitive measurements of dark energy and modification of gravity using cosmic large-scale structure; (3) probe the Milky Way's dust-shrouded regions, reaching the far side of our Galaxy; and (4) characterize asteroids and other objects in the outer solar systems.

Proceedings Article | 11 August 2010 Paper

Design and implementation of the NUV/optical widefield Star Formation Camera for the Theia Observatory

Paul Scowen, Rolf Jansen, Matthew Beasley, Daniella Calzetti, Steve Desch, Alex Fullerton, John Gallagher, P. Douglas Lisman, Steven Macenka, Sangeeta Malhotra, Mark McCaughrean, Shouleh Nikzad, Robert O'Connell, Sally Oey, Deborah Padgett, James Rhoads, Aki Roberge, Oswald H. W. Siegmund, Stuart Shaklan, Nathan Smith, Daniel Stern, Jason Tumlinson, Rogier Windhorst, Robert Woodruff

Proc. SPIE. 7731, Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave

KEYWORDS: Staring arrays, Optical filters, Astronomy, Stars, Imaging systems, Cameras, Sensors, Silicon, Space telescopes, Galactic astronomy

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Proceedings Article | 21 July 2010 Paper

Multiband filters for near-infrared astronomical applications

James Rhoads, Sangeeta Malhotra, Paul Scowen, Ron Probst, Don McCarthy

Proc. SPIE. 7735, Ground-based and Airborne Instrumentation for Astronomy III

KEYWORDS: Optical filters, Astronomy, Cameras, Coating, Optical coatings, Smoothing, Image filtering, Astronomical imaging, Boxcar filters, Bandpass filters

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Proceedings Article | 12 July 2008 Paper

The Star Formation Observatory (SFO) mission to study cosmic origins near and far

Paul Scowen, Rolf Jansen, Matthew Beasley, Brian Cooke, Shouleh Nikzad, Oswald Siegmund, Robert Woodruff, Daniela Calzetti, Steven Desch, Alex Fullerton, John Gallagher, Sangeeta Malhotra, Mark McCaughrean, Robert O'Connell, Sally Oey, Debbie Padgett, James Rhoads, Aki Roberge, Nathan Smith, Daniel Stern, Jason Tumlinson, Rogier Windhorst

Proc. SPIE. 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter

KEYWORDS: Observatories, Stars, Sensors, Spectroscopy, Microchannel plates, Silicon, Quantum efficiency, Imaging spectroscopy, Planets, Galactic astronomy

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