![]() Traub, "Observation of HD on Jupiter and the D/H Ratio," Astrophysical Journal Letters 184, L137, 1973. Mickelson, "Laboratory Absorption Strengths and Line Shape Parameters in the 4-0, 5-0, and 6-0 Vibration Bands of HD," Icarus 56, 176, 1983. Roesler, "A study of the Jovian nebula at high spectral resolution," Astrophysical Journal 236, 1035, 1980. Trauger, "The Jovian Nebula: a Post-Voyager Perspective," Nature 337, 341, 1984. Lunine, "Spectroscopy of Molecular Oxygen in the Atmospheres of Venus and Mars," Icarus 55, 272, 1983. Scheduled to launch no later than May 2027, NASA’s Nancy Grace Roman Space Telescope mission will help uncover some of the biggest mysteries in the cosmos. Westphal, "The on-orbit performance of WFPC2," Astrophysical Journal Letters 435, 元, 1994. Ballester, et al., "Saturn's hydrogen aurora: Wide Field and Planetary Camera 2 imaging from the Hubble Space Telescope," Journal of Geophysical Research 103, 237, 1998. Trauger, "High Contrast Coronagraphic Imaging with NGST," in Next Generation Space Telescope Science and Technology, Astronomical Society of the Pacific Conference Series 207, 165, 2000. ![]() Bagwell, "Performance of a precision high-density deformable mirror for extremely high contrast imaging astronomy from space," Proc. Traub, “A laboratory demonstration of the capability to image an Earth-like extrasolar planet,” Nature 446, 771, 2007. SPIE 7731, 773128, 2010 and Pathways towards Habitable Planets, ASP Conf. Trauger, et al., “ACCESS – A concept study for the direct imaging and spectroscopy of exoplanetary systems,” Final Report to the NASA Astrophysics Strategic Mission Concept Studies Program, Public Version, 2009 Proc. The approximately 166 million cost-plus-fixed-fee contract extension was issued as a sole-source procurement. One is called a high-contrast coronagrapha complex instrument that suppresses light inside a telescope and will be a feature of the Nancy Grace Roman Space Telescope, which is expected to. One of two main sections of the instrument, this layer houses the instrument. Trauger et al., “Complex apodization Lyot coronagraphy for the direct imaging of exoplanet systems: design, fabrication, and laboratory demonstration,” Proc. Engineers at NASAs Jet Propulsion Laboratory from left, Brandon Creager, Juan Gloria, Joshua Nachtigal, and Sonny Gutierrez are shown assembling the electronics palette for the Coronagraph Instrument on NASAs Roman Space Telescope in December 2022. Trauger et al., “The Hybrid Lyot Coronagraph, Final Report to the NASA Strategic Astrophysics Technology – Technology Demonstrations for Exoplanet Missions (SAT-TDEM) program, JPL Document D-78698, 2012. Gordon, “Complex apodized Lyot coronagraph for exoplanet imaging with partially obscured telescope apertures,” Proc. This in-space experience is a critical step toward future, larger missions targeted at. Trauger, "Development of the Wide Field and Planetary Camera 2," in "Hubble’s Legacy: Reflections by Those Who Dreamed It, Built It, and Observed the Universe with It, " R. The Coronagraph Instrument (CGI) on the Nancy Grace Roman Space Telescope will demonstrate the highcontrast technology necessary for visible-light exoplanet imaging and spectroscopy from space via direct imaging of Jupiter-size planets and debris disks. Simulation parameters: 10 hr exposure time, 525-580 nm, Hybrid Lyot Coronagraph. Simulated Nancy Grace Roman Space Telescope coronagraph image of the star 47 Ursae Majoris, showing two directly detected planets. The Roman spacecraft Mission objectives: The Roman telescope will be a cutting-edge space observatory for in-depth studies of the Universe in infrared light.The telescope’s large field of view, high sensitivity and advanced coronagraphic capabilities will allow astronomers to detect and study galaxies in the very early Universe, search for potentially habitable exoplanets and provide answers. Gordon, “Hybrid Lyot Coronagraph for WFIRST-AFTA: coronagraph design and performance metrics,” J. Simulated Nancy Grace Roman Space Telescope coronagraph image of 47 Ursae Majoris, showing two detected planets. This program element solicits proposals aimed at supporting the progress of and exploiting the scientific and technical data. Please contact Rob Zellem at JPL and/or Marie Ygouf if you are interested in giving a talk on work related to the Roman Space Telescope. Listed below are resources and information pertinent to the upcoming NASA Research Announcement for D.14 Nancy Grace Roman Space Telescope Research and Support Participation Opportunities, which is part of ROSES-2022. Talks are ~20 minutes with ~10 minutes for Q/A, and are scheduled for the 3rd Thursday of each month from 1-1:30 pm Pacific / 4-4:30 pm Eastern. All are welcome and encouraged to attend. These talks are open to the entire astronomy community and cover science, engineering, and technology related to the Roman mission. The Nancy Grace Roman Space Telescope monthly virtual lecture series is run jointly by JPL, IPAC, Goddard, and STScI.
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