Origins Space Telescope Mission Concept Study Report
arXiv:1912.06213
Abstract
The Origins Space Telescope (Origins) traces our cosmic history, from the formation of the first galaxies and the rise of metals to the development of habitable worlds and present-day life. Origins does this through exquisite sensitivity to infrared radiation from ions, atoms, molecules, dust, water vapor and ice, and observations of extra-solar planetary atmospheres, protoplanetary disks, and large-area extragalactic fields. Origins operates in the wavelength range 2.8 to 588 microns and is 1000 times more sensitive than its predecessors due to its large, cold (4.5 K) telescope and advanced instruments. Origins was one of four large missions studied by the community with support from NASA and industry in preparation for the 2020 Decadal Survey in Astrophysics. This is the final study report.
376 pages
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- Observing H2 Emission in Forming Galaxies
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Cited by in corpus (28)
- Large Interferometer For Exoplanets (LIFE): I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer mission
- Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy
- ALMA uncovers the [CII] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
- Vertically resolved magma ocean-protoatmosphere evolution: H, HO, CO, CH, CO, O, and N as primary absorbers
- Photochemistry of Anoxic Abiotic Habitable Planet Atmospheres: Impact of New HO Cross-Sections
- Accurate dust temperature determination in a galaxy
- JWST Noise Floor II: Systematic Error Sources in JWST NIRCam Time Series
- Concepts for future missions to search for technosignatures
- Evaluating the Plausible Range of N2O Biosignatures on Exo-Earths: An Integrated Biogeochemical, Photochemical, and Spectral Modeling Approach
- The Past and Future of Mid-Infrared Studies of AGN
- Possibilities for an Aerial Biosphere in Temperate Sub Neptune-Sized Exoplanet Atmospheres
- Bioverse: a simulation framework to assess the statistical power of future biosignature surveys
- A New Method For Studying Exoplanet Atmospheres Using Planetary Infrared Excess
- Disruption of a Planetary Nitrogen Cycle as Evidence of Extraterrestrial Agriculture
- The Demographics of Wide-Separation Planets
- The Role of Atmospheric Exchange in False-Positive Biosignature Detection
- The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena
- Phase Modeling of the TRAPPIST-1 Planetary Atmospheres
- Mapping the Universe in HD
- The Phase-curve Signature of Condensible Water-rich Atmospheres on Slowly Rotating Tidally Locked Exoplanets
- Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
- Boosting Line Intensity Map Signal-to-Noise with the Ly- Forest Cross-Correlation
- High-sensitivity transition-edge-sensed bolometers: improved speed and characterization with AC and DC bias
- Demonstration of ultra-low noise equivalent power using a longitudinal proximity effect transition-edge sensor
- Galaxy evolution through infrared and submillimeter spectroscopy: Measuring star formation and black hole accretion with JWST and ALMA
- A Decade of NASA Strategic Astrophysics Technology Investments: Technology Maturation, Infusion, and Other Benefits
- Redshift Horizon for the Origins Space Telescope from Primordial Dust Emission
- Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey