activity
20172026
most citedA non-energetic mechanism for glycine formation in the interstellar medium

127 citations · 395 across the 25 of their papers we have counts for

collaborators

27 papers

astro-ph.EP2026

Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model

E. Mamonova, K. Herbst, V. Kofman +4

Context. M dwarfs are key targets for terrestrial exoplanet studies, with prospects for atmospheric spectroscopy. However, strong stellar magnetic activity and frequent flaring req…

astro-ph.EP2026

Impact of Climate States and Seasons on Future Exo-Earth Observations

Kyle Batra, Stephanie Olson, Vincent Kofman

Many planetary parameters impact the climate state of Earth-like exoplanets and could vary significantly from those on Earth. However, some of these parameters may be impossible to…

astro-ph.EP2026★ 1 cited

Retrieving the Red Edge on Earth-like Planets with Heterogeneous Clouds and Surfaces

Zachary Burr, Mario Damiano, Vincent Kofman +2

The detection and characterization of potentially habitable exoplanets is one of the chief goals of astrophysics for the coming decades. Imaging in reflected light is well suited f…

astro-ph.EP2026

Spectral signatures from the habitable zone

Vincent Kofman

This work describes the context and approach for the detection of spectroscopic signatures from planets in the habitable zone of nearby stars. By understanding the limitations of c…

astro-ph.EP2026

Multi-bandpass Photometry for Exoplanet Atmosphere Reconnaissance (MPEAR) with the Habitable Worlds Observatory (HWO) -- I. Differentiating Earth from Neptunes During Discovery

Eleonora Alei, Avi M. Mandell, Miles H. Currie +7

As the architecture for the Habitable Worlds Observatory (HWO) is being developed, it is crucial to optimize the observing strategies for a survey to detect and characterize Earth-…

astro-ph.IM2026

Habitable Worlds Observatory (HWO): Living Worlds Community Working Group: The Search for Life on Potentially Habitable Exoplanets

Giada Arney, Niki Parenteau, Natalie Hinkel +25

The discovery of a biosphere on another planet would transform how we view ourselves, and our planet Earth, in relation to the rest of the cosmos. We now know Earth is one planet a…

astro-ph.EP2025

Determining the Detectability of H2O with Photometric Observations using Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE)

Natasha Latouf, Chris Stark, Avi Mandell +1

We examine the detectability of water (H2O) in the reflected-light spectrum of an Earth-like exoplanet assuming a photometric observational approach rather than spectroscopic. By q…

astro-ph.EP2025★ 2 cited

Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging

Corey Beard, Paul Robertson, Jack Lubin +31

We present the discovery of GJ 251 c, a candidate super-Earth orbiting in the Habitable Zone (HZ) of its M dwarf host star. Using high-precision Habitable-zone Planet Finder (HPF)…

astro-ph.EP2025

A comprehensive spectroscopic reference of the solar system and its application to exoplanet direct imaging

Allison Payne, Geronimo L. Villanueva, Vincent Kofman +5

We present a calibrated database of reflectance spectra for the solar system planets (i.e., Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune) and for Titan, spanning f…

astro-ph.EP2025★ 1 cited

Detecting alien living worlds and photosynthetic life using imaging polarimetry with the HWO coronagraph

Svetlana Berdyugina, Lucas Patty, Jonathan Grone +10

Our Earth, being the only living planet that we know, provides us with clues that photosynthetic life-forms may be dominant on other exoplanets for billions of years. Spectropolari…

astro-ph.EP2025★ 2 cited

From Global Climate Models (GCMs) to Exoplanet Spectra with the Global Emission Spectra (GlobES)

Thomas J. Fauchez, Geronimo L. Villanueva, Vincent Kofman +2

In the quest to understand the climates and atmospheres of exoplanets, 3D global climate models (GCMs) have become indispensable. The ability of GCMs to predict atmospheric conditi…

astro-ph.EP2025★ 1 cited

The climates and thermal emission spectra of prime nearby temperate rocky exoplanet targets

Tobi Hammond, Thaddeus D. Komacek, Ravi K. Kopparapu +9

Over the course of the past decade, advances in the radial velocity and transit techniques have enabled the detection of rocky exoplanets in the habitable zones of nearby stars. Fu…

astro-ph.EP2024

Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE) \RNum{3}: Introducing the KEN

Natasha Latouf, Michael D. Himes, Avi M. Mandell +4

We deploy a newly-generated set of geometric albedo spectral grids to examine the detectability of methane (CH4) in the reflected-light spectrum of an Earth-like exoplanet at visib…

astro-ph.EP2024★ 11 cited

The pale blue dot: using the Planetary Spectrum Generator to simulate signals from hyper realistic exo-Earths

Vincent Kofman, Geronimo Villanueva, Thomas Fauchez +5

The atmospheres and surfaces of planets show tremendous amount of spatial variation, which has a direct effect on the spectrum of the object, even if this may not be spatially reso…

astro-ph.EP2024

Detectability Simulations of a NIR Surface Biosignature on Proxima Centauri b with Future Space Observatories

Connor O. Metz, Nancy Y. Kiang, Geronimo L. Villanueva +2

Telescope missions are currently being designed which will make direct imaging of habitable exoplanets possible in the near future, and studies are needed to quantify the detectabi…

astro-ph.EP2024★ 1 cited

The challenge of detecting remote spectroscopic signatures from radionuclides

Jacob Haqq-Misra, Vincent Kofman, Ravi K. Kopparapu

The characterization of exoplanetary atmospheres through transit spectra is becoming increasingly feasible, and technology for direct detection remains ongoing. The possibility of…

astro-ph.EP2024★ 20 cited

Large Interferometer For Exoplanets (LIFE): XIII. The Value of Combining Thermal Emission and Reflected Light for the Characterization of Earth Twins

E. Alei, S. P. Quanz, B. S. Konrad +9

Following the recommendations to NASA and ESA, the search for life on exoplanets will be a priority in the next decades. Two direct imaging space mission concepts are being develop…

astro-ph.IM2024

Detectability of Solar Panels as a Technosignature

Ravi Kopparapu, Vincent Kofman, Jacob Haqq-Misra +2

In this work, we assess the potential detectability of solar panels made of silicon on an Earth-like exoplanet as a potential technosignature. Silicon-based photovoltaic cells have…

astro-ph.EP2024

Modeling Atmospheric Lines By the Exoplanet Community (MALBEC) version 1.0: A CUISINES radiative transfer intercomparison project

Geronimo L. Villanueva, Thomas J. Fauchez, Vincent Kofman +15

Radiative transfer (RT) models are critical in the interpretation of exoplanetary spectra, in simulating exoplanet climates and when designing the specifications of future flagship…

astro-ph.EP2023★ 1 cited

Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE) II: Using Grid-Based Nested Sampling in Coronagraphy Observation Simulations for O2 and O3

Natasha Latouf, Avi Mandell, Geronimo Villanueva +8

We present the results for the detectability of the O2 and O3 molecular species in the atmosphere of an Earth-like planet using reflected light at the visible wavelengths. By quant…

astro-ph.EP2023★ 2 cited

Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE) I: Using Grid-Based Nested Sampling in Coronagraphy Observation Simulations for H2O

Natasha Latouf, Avi Mandell, Geronimo Villanueva +4

Detecting H2O in exoplanet atmospheres is the first step on the path to determining planet habitability. Coronagraphic design currently limits the observing strategy used to detect…

astro-ph.EP2023★ 2 cited

JWST molecular mapping and characterization of Enceladus' water plume feeding its torus

G. L. Villanueva, H. B. Hammel, S. N. Milam +18

Enceladus is a prime target in the search for life in our solar system, having an active plume likely connected to a large liquid water subsurface ocean. Using the sensitive NIRSpe…

astro-ph.EP2022★ 37 cited

Phosphine in the Venusian Atmosphere: A Strict Upper Limit from SOFIA GREAT Observations

M. A. Cordiner, G. L. Villanueva, H. Wiesemeyer +13

The presence of phosphine (PH) in the atmosphere of Venus was reported by Greaves et al. (2021a), based on observations of the J=1-0 transition at 267 GHz using ground-based, m…

astro-ph.IM2020★ 127 cited

A non-energetic mechanism for glycine formation in the interstellar medium

S. Ioppolo, G. Fedoseev, K. -J. Chuang +8

The detection of the amino acid glycine and its amine precursor methylamine on the comet 67P/Churyumov-Gerasimenko by the Rosetta mission provides strong evidence for a cosmic orig…