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Related papers: Incorporating Wavefront Error, Wavefront Sensing a…

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NASA's Habitable Worlds Observatory (HWO) will be the first space telescope capable of directly imaging Earth-like planets in the habitable zones of Sun-like stars to probe their atmospheres for signs of life. Now in its early stages of…

Earth and Planetary Astrophysics · Physics 2025-06-30 Katie E. Painter , Brendan P. Bowler , Kyle Franson , Juliette C. Becker , Jennifer A. Burt

Executive Summary: The Habitable Worlds Observatory (HWO) is the first astrophysics flagship mission with a key cross-divisional astrobiology science goal of searching for signs of life on rocky planets beyond our solar system. The Living…

The James Webb Space Telescope is orders of magnitude more sensitive than any other facility across the near to mid-infrared wavelengths. Many approved programs take advantage of its highly stable point spread function (PSF) to directly…

A lower bound on unbiased estimates of wavefront errors (WFE) is presented for the linear regime of small perturbation and active control of a high-contrast region (dark hole). Analytical approximations and algorithms for computing the…

Instrumentation and Methods for Astrophysics · Physics 2021-10-13 Leonid Pogorelyuk , Laurent Pueyo , Jared R. Males , Kerri Cahoy , N. Jeremy Kasdin

Future space missions that aim to detect and characterize Earth-like exoplanets will require an instrument that efficiently measures spectra of these planets, placing strict requirements on detector performance. The upcoming Roman Space…

Instrumentation and Methods for Astrophysics · Physics 2024-05-16 Alex R. Howe , Christopher C. Stark , John E. Sadleir

The primary scientific objective of this Habitable Worlds Observatory (HWO) Science Case Development Document (SCDD) is to measure planetary rotation rates of transiting exoplanets to determine the structure, composition, circulation, and…

Direct imaging simulations of starshades and other proposed mission concepts are needed to characterize planet detection performance and inform mission design trades. In order to assess the complementary role of a 60 m starshade for the…

Instrumentation and Methods for Astrophysics · Physics 2025-11-20 Jamila Taaki , Farzad Kamalabadi , Athol Kemball , Lia Corrales , Alfred O. Hero

Astrometry, one of the oldest branches of astronomy, has been revolutionized by missions like Hipparcos and especially Gaia, which mapped billions of stars with extraordinary precision. However, challenges such as detecting Earth-like…

The Habitable Worlds Observatory (HWO), NASA's next flagship science mission, follows in the tradition of the Nancy Grace Roman Space Telescope and other preceding great observatories. HWO will directly image and characterize Earth-like…

Focal plane wavefront sensing and control is a critical approach to reducing non-common path errors between the a conventional astronomical adaptive optics (AO) wavefront sensor (WFS) detector and science camera. However, in addition to…

Instrumentation and Methods for Astrophysics · Physics 2023-03-01 Benjamin L. Gerard , Daren Dillon , Sylvain Cetre , Rebecca Jensen-Clem

Exoplanet direct imaging allows us to directly probe and characterize an exoplanet's atmosphere, searching for signs of life in its atmospheric signatures. Directly imaging an Earth-like planet around a Sun-like star requires reaching…

The Habitable Worlds Observatory (HWO) offers a unique opportunity to revolutionize our understanding of planetary formation and evolution. The goal of this Science Case Development Document (SCDD) is to investigate the physical and…

We assess archival high-energy data for key stars on the Habitable Worlds Observatory (HWO) Target Stars and Systems 2025 list, as stellar radiation is critical to shaping and interpreting planetary atmospheres. Using a sample of 98 nearby…

High-contrast imaging will be a challenge for future ELTs, because their vibrations create low-order aberrations - mostly tip/tilt - that reduce coronagraphic performances at 1.2 lambda/D and above. A Low-Order WaveFront Sensor (LOWFS) is…

Instrumentation and Methods for Astrophysics · Physics 2015-06-17 Julien Lozi , Ruslan Belikov , Glenn Schneider , Olivier Guyon , EugenePluzhnik , Sandrine J. Thomas , Frantz Martinache

As of October 2021 (Period 108), the European Southern Observatory (ESO) offers a new mode of the ESPRESSO spectrograph designed to use the High Resolution grating with 4x2 binning (spatial by spectral; HR42 mode) with the specific…

Astrophysics of Galaxies · Physics 2022-06-08 Trystyn A. M. Berg , Guido Cupani , Pedro Figueira , Andrea Mehner

Characterizing the surface and atmosphere of Earth-like planets in reflected light is a key goal for upcoming direct imaging surveys. NASA's next flagship-class astrophysics mission concept, the Habitable Worlds Observatory (HWO), is a…

Earth and Planetary Astrophysics · Physics 2026-03-27 Aiden S. Zelakiewicz , Elijah Mullens , Lisa Kaltenegger , Dmitry Savransky

Habitable Worlds Observatory (HWO) presents a key challenge for technology development in the coming years, requiring a $>$ $100\times$ more stable system than \textit{JWST}. WaveDriver is a concept for a laser guide star spacecraft coupled…

The James Webb Space Telescope (JWST) presents the opportunity to transform our understanding of planets and the origins of life by revealing the atmospheric compositions, structures, and dynamics of transiting exoplanets in unprecedented…

Earth and Planetary Astrophysics · Physics 2018-10-17 Jacob L. Bean , Kevin B. Stevenson , Natalie M. Batalha , Zachory Berta-Thompson , Laura Kreidberg , Nicolas Crouzet , Björn Benneke , Michael R. Line , David K. Sing , Hannah R. Wakeford , Heather A. Knutson , Eliza M. -R. Kempton , Jean-Michel Désert , Ian Crossfield , Natasha E. Batalha , Julien de Wit , Vivien Parmentier , Joseph Harrington , Julianne I. Moses , Mercedes Lopez-Morales , Munazza K. Alam , Jasmina Blecic , Giovanni Bruno , Aarynn L. Carter , John W. Chapman , Leen Decin , Diana Dragomir , Thomas M. Evans , Jonathan J. Fortney , Jonathan D. Fraine , Peter Gao , Antonio García Muñoz , Neale P. Gibson , Jayesh M. Goyal , Kevin Heng , Renyu Hu , Sarah Kendrew , Brian M. Kilpatrick , Jessica Krick , Pierre-Olivier Lagage , Monika Lendl , Tom Louden , Nikku Madhusudhan , Avi M. Mandell , Megan Mansfield , Erin M. May , Giuseppe Morello , Caroline V. Morley , Nikolay Nikolov , Seth Redfield , Jessica E. Roberts , Everett Schlawin , Jessica J. Spake , Kamen O. Todorov , Angelos Tsiaras , Olivia Venot , William C. Waalkes , Peter J. Wheatley , Robert T. Zellem , Daniel Angerhausen , David Barrado , Ludmila Carone , Sarah L. Casewell , Patricio E. Cubillos , Mario Damiano , Miguel de Val-Borro , Benjamin Drummond , Billy Edwards , Michael Endl , Nestor Espinoza , Kevin France , John E. Gizis , Thomas P. Greene , Thomas K. Henning , Yucian Hong , James G. Ingalls , Nicolas Iro , Patrick G. J. Irwin , Tiffany Kataria , Fred Lahuis , Jérémy Leconte , Jorge Lillo-Box , Stefan Lines , Joshua D. Lothringer , Luigi Mancini , Franck Marchis , Nathan Mayne , Enric Palle , Emily Rauscher , Gaël Roudier , Evgenya L. Shkolnik , John Southworth , Mark R. Swain , Jake Taylor , Johanna Teske , Giovanna Tinetti , Pascal Tremblin , Gregory S. Tucker , Roy van Boekel , Ingo P. Waldmann , Ian C. Weaver , Tiziano Zingales

Ground-based high contrast imaging (HCI) and extreme adaptive optics (AO) technologies have advanced to the point of enabling direct detections of gas-giant exoplanets orbiting beyond the snow lines around nearby young star systems.…