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Browsing Tag

astro-ph.IM

9 posts
SScience
Connecting Polarization To Exoplanet Yield Calculations For Habitable Worlds Observatory (HWO)
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Connecting Polarization To Exoplanet Yield Calculations For Habitable Worlds Observatory (HWO)

  • June 14, 2026
Overview of the simulation pipeline components used in this work. The modeling begins with hwo pol, a Poke…
SScience
Japan’s Possible Contributions For Coronagraph Of The Habitable Worlds Observatory (HWO)
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Japan’s Possible Contributions For Coronagraph Of The Habitable Worlds Observatory (HWO)

  • June 13, 2026
Example of the optical design for the NIR coronagraph. (Top) Overall layout of the optical system, where the…
SScience
Prospects for Astrobiology And Technosignature Searches With The Vera C. Rubin Observatory Legacy Survey Of Space And Time
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Prospects for Astrobiology And Technosignature Searches With The Vera C. Rubin Observatory Legacy Survey Of Space And Time

  • June 13, 2026
Simulated multiband light-curve populations in the Cchroma–Ccross diagnostic plane. Left: noise-dominated, natural, and coherent variability classes (N ≈…
SScience
The Unique Ability Of The Hubble Space Telescope To Characterize Young Exoplanet Environments
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The Unique Ability Of The Hubble Space Telescope To Characterize Young Exoplanet Environments

  • May 30, 2026
Modified Pass et al. (2025) Figure 2 showing an updated Cosmic Shoreline for exoplanets orbiting full convective M…
SScience
PEEPSS: Photonic-Enabled ExoPlanet Spectroscopic Sensor for the Habitable Worlds Observatory
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PEEPSS: Photonic-Enabled ExoPlanet Spectroscopic Sensor for the Habitable Worlds Observatory

  • April 30, 2026
The complete proposed wavefront sensing process. (Starting from the top left and going around clockwise) The full coronagraph…
SScience
Planetary Exploration 3.0: A Roadmap for Software-Defined, Radically Adaptive Space Systems
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Planetary Exploration 3.0: A Roadmap for Software-Defined, Radically Adaptive Space Systems

  • April 25, 2026
Planetary exploration is characterized by unknowns, which are both the primary reason and challenge for exploration. (a) The…
SScience
Continuing To Advance European High Contrast Imaging Research And Development Towards HWO And LIFE
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Continuing To Advance European High Contrast Imaging Research And Development Towards HWO And LIFE

  • April 20, 2026
Artist’s impression of the LIFE nulling-interferometry mission, consisting of four collector spacecraft in a rectangular array configuration sending…
SScience
Narrowband Radio Technosignature Search Toward 3I/ATLAS With FAST
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Narrowband Radio Technosignature Search Toward 3I/ATLAS With FAST

  • March 21, 2026
Scatter plots of potential candidate in frequency, drift rate and signal-to-noise ratio for each polarization channel. The color…
SScience
Searching For Life-As-We-Don’t-Know-It: Mission-relevant Application of Assembly Theory For Exoplanet Life Detection
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Searching For Life-As-We-Don’t-Know-It: Mission-relevant Application of Assembly Theory For Exoplanet Life Detection

  • March 14, 2026
Potentially habitable worlds – Grok via Astrobiology.com This white paper introduces a framework for applying Assembly Theory (AT)…
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