papers

Publications (31)

astro-ph.EP2019

Constraining Exoplanet Metallicities and Aerosols with ARIEL: An Independent Study by the Contribution to ARIEL Spectroscopy of Exoplanets (CASE) Team

Robert T. Zellem, Mark R. Swain, Nicolas B. Cowan +24

Launching in 2028, ESA's Atmospheric Remote-sensing Exoplanet Large-survey (ARIEL) survey of 1000 transiting exoplanets will build on the legacies of Kepler and TESS and comp…

astro-ph.SR2013

The Solar Neighborhood XXX: Fomalhaut C

Eric E. Mamajek, Jennifer L. Bartlett, Andreas Seifahrt +11

LP 876-10 is a nearby active M4 dwarf in Aquarius at a distance of 7.6 pc. The star is a new addition to the 10-pc census, with a parallax measured via the Research Consortium on N…

astro-ph.EP2022

Measuring the Obliquities of the TRAPPIST-1 Planets with MAROON-X

Madison Brady, Jacob Bean, Andreas Seifahrt +6

A star's obliquity with respect to its planetary system can provide us with insight into the system's formation and evolution, as well as hinting at the presence of additional obje…

astro-ph.EP2026

RV and TTV Measurements of Two Transiting Long-Period Giants around TOI-4600

Tong Hu, Zitao Lin, Sharon X. Wang +27

TOI-4600b and c, originally identified by the Transiting Exoplanet Survey Satellite (TESS) and reported by I. Mireles et al. (2023), are a rare pair of transiting long-period giant…

astro-ph.EP2025

An Earth-like Density for the Temperate Earth-sized Planet GJ 12b

Madison Brady, Jacob Bean, Ritvik Basant +9

While JWST has provided us with the opportunity to probe the atmospheres of potentially-habitable planets, observations of the TRAPPIST-1 system have shown us that active stars sev…

astro-ph.EP2019

Characterizing the Atmospheres of Irradiated Exoplanets at High Spectral Resolution

Diana Dragomir, Eliza Kempton, Jacob Bean +6

The best-characterized exoplanets to date are planets on close-in transiting orbits around their host stars. The high level of irradiation and transiting geometry of these objects…

stat.ME2021

Randomization Inference of Periodicity in Unequally Spaced Time Series with Application to Exoplanet Detection

Panos Toulis, Jacob Bean

The estimation of periodicity is a fundamental task in many scientific areas of study. Existing methods rely on theoretical assumptions that the observation times have equal or i.i…

astro-ph.EP2024

Searching for GEMS: Characterizing Six Giant Planets around Cool Dwarfs

Shubham Kanodia, Arvind F. Gupta, Caleb I. Canas +42

Transiting giant exoplanets around M-dwarf stars (GEMS) are rare, owing to the low-mass host stars. However, the all-sky coverage of TESS has enabled the detection of an increasing…

astro-ph.EP2017

Quantifying the Impact of Spectral Coverage on the Retrieval of Molecular Abundances from Exoplanet Transmission Spectra

John W. Chapman, Robert T. Zellem, Michael R. Line +14

Using forward models for representative exoplanet atmospheres and a radiometric instrument model, we have generated synthetic observational data to explore how well the major C- an…

astro-ph.EP2021

A Comprehensive Reanalysis of 's 4.5 m Phase Curves, and the Phase Variations of the Ultra-hot Jupiters MASCARA-1b and KELT-16b

Taylor J. Bell, Lisa Dang, Nicolas B. Cowan +12

We have developed an open-source pipeline for the analysis of \textit{Spitzer}/IRAC channel 1 and 2 time-series photometry, incorporating some of the most popular decorrelation met…

astro-ph.IM2022

Report on Community Cadence Observing to Maximize the Scientific Output of the Keck Planet Finder

Erik Petigura, Andrew Howard, Jacob Bean +11

The arrival of the Keck Planet Finder (KPF) in 2022 represents a major advance in the precision radial velocity (PRV) capabilities of the W. M. Keck Observatory. In preparation for…

astro-ph.EP2025

A Stellar Magnesium to Silicon ratio in the atmosphere of an exoplanet

Jorge A. Sanchez, Peter C. B. Smith, Krishna Kanumalla +17

The elemental compositions of exoplanets encode information about their formation environments and internal structures. While volatile ratios such as carbon-to-oxygen (C/O) are use…

astro-ph.EP2019

Astro2020 Science White Paper: Toward Finding Earth 2.0: Masses and Orbits of Small Planets with Extreme Radial Velocity Precision

David R. Ciardi, Jacob Bean, Jennifer Burt +9

Having discovered that Earth-sized planets are common, we are now embarking on a journey to determine if Earth-like planets are also common. Finding Earth-like planets is one of th…

astro-ph.EP2016

The Impact of Non-Uniform Thermal Structure on the Interpretation of Exoplanet Emission Spectra

Y. Katherina Feng, Michael R. Line, Jonathan J. Fortney +4

The determination of atmospheric structure and molecular abundances of planetary atmospheres via spectroscopy involves direct comparisons between models and data. While varying in…

astro-ph.IM2023

A First Look at the JWST MIRI/LRS Phase Curve of WASP-43b

Taylor J. Bell, Laura Kreidberg, Sarah Kendrew +7

We observed a full-orbit phase curve of the hot Jupiter WASP-43b with MIRI/LRS as part of the Transiting Exoplanet Community Early Release Science Program. Here we report prelimina…

astro-ph.IM2014

Observations of Transiting Exoplanets with the James Webb Space Telescope (JWST), Publications of the Astronomical Society of the Pacific (PASP), December 2014

Charles Beichman, Bjoern Benneke, Heather Knutson +44

This article summarizes a workshop held on March, 2014, on the potential of the James Webb Space Telescope (JWST) to revolutionize our knowledge of the physical properties of exopl…

astro-ph.EP2022

Assessing 's Yield of Rocky Planets Around Nearby M Dwarfs

Madison Brady, Jacob Bean

Terrestrial planets are easier to detect around M dwarfs than other types of stars, making them promising for next-generation atmospheric characterization studies. The missi…

astro-ph.SR2013

High Precision Abundances of the Old Solar Twin HIP 102152: Insights on Li Depletion from the Oldest Sun

TalaWanda R. Monroe, Jorge Meléndez, Iván Ramírez +13

We present the first detailed chemical abundance analysis of the old 8.2 Gyr solar twin, HIP 102152. We derive differential abundances of 21 elements relative to the Sun with preci…

astro-ph.EP2022

A New Analysis of 8 Spitzer Phase Curves and Hot Jupiter Population Trends: Qatar-1b, Qatar-2b, WASP-52b, WASP-34b, and WASP-140b

Erin May, Kevin Stevenson, Jacob Bean +16

With over 30 phase curves observed during the warm Spitzer mission, the complete data set provides a wealth of information relating to trends and three-dimensional properties of ho…

astro-ph.IM2020

Keys of a Mission to Uranus or Neptune, the Closest Ice Giants

Tristan Guillot, Jonathan Fortney, Emily Rauscher +26

Uranus and Neptune are the archetypes of "ice giants", a class of planets that may be among the most common in the Galaxy. They hold the keys to understand the atmospheric dynamics…

astro-ph.EP2019

Characterizing Transiting Exoplanets with JWST Guaranteed Time and ERS Observations

Thomas Greene, Jacob Bean, Thomas Beatty +10

We highlight how guaranteed time observations (GTOs) and early release science (ERS) will advance understanding of exoplanet atmospheres and provide a glimpse into what transiting…

astro-ph.EP2018

Simulated JWST/NIRISS Transit Spectroscopy of Anticipated TESS Planets Compared to Select Discoveries from Space-Based and Ground-Based Surveys

Dana R. Louie, Drake Deming, Loic Albert +3

The Transiting Exoplanet Survey Satellite (TESS) will embark in 2018 on a 2-year wide-field survey mission, discovering over a thousand terrestrial, super-Earth and sub-Neptune-siz…

astro-ph.EP2022

A close-in puffy Neptune with hidden friends: The enigma of TOI 620

Michael A. Reefe, Rafael Luque, Eric Gaidos +82

We present the validation of a transiting low-density exoplanet orbiting the M2.5 dwarf TOI 620 discovered by the NASA TESS mission. We utilize photometric data from both TESS and…

astro-ph.EP2021

The Dark World: A Tale of WASP-43b in Reflected Light with HST WFC3/UVIS

Jonathan Fraine, Laura C. Mayorga, Kevin B. Stevenson +14

Optical, reflected light eclipse observations provide a direct probe of the exoplanet scattering properties, such as from aerosols. We present here the photometric, reflected light…

astro-ph.EP2011

Observational evidence for a metal rich atmosphere on the super-Earth GJ1214b

Jean-Michel Désert, Jacob Bean, Eliza Miller-Ricci Kempton +6

We report observations of two consecutive transits of the warm super-Earth exoplanet GJ1214b at 3.6 and 4.5 microns with the Infrared Array Camera instrument on-board the Spitzer S…

astro-ph.EP2021

H-Alpha Variability of V1298 Tau c

Everett Schlawin, Ilya Ilyin, Adina D. Feinstein +5

The 23 Myr system V1298 Tau hosts four transiting planets and is a valuable laboratory for exploring the early stages of planet evolution soon after formation of the star. We obser…

astro-ph.EP2011

The GJ1214 Super-Earth System: Stellar Variability, New Transits, and a Search for Additional Planets

Zachory K. Berta, David Charbonneau, Jacob Bean +5

The super-Earth GJ1214b transits a nearby M dwarf that exhibits 1% intrinsic variability in the near-infrared. Here, we analyze new observations to refine the physical properties o…

astro-ph.EP2023

A Combined Ground-based and JWST Atmospheric Retrieval Analysis: Both IGRINS and NIRSpec Agree The Atmosphere of WASP-77A b is Metal-Poor

Peter Smith, Michael Line, Jacob Bean +12

Ground-based, high-resolution and space-based, low-resolution spectroscopy are the two main avenues through which transiting exoplanet atmospheres are studied. Both methods provide…

astro-ph.EP2016

No Thermal Inversion and a Solar Water Abundance for the Hot Jupiter HD209458b from HST WFC3 Emission Spectroscopy

Michael R. Line, Kevin B. Stevenson, Jacob Bean +6

The nature of the vertical thermal structure of hot Jupiter atmospheres is one of the key questions raised by the characterization of transiting exoplanets over the last decade. Th…

astro-ph.EP2023

Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST

Benjamin J. Hord, Eliza M. -R. Kempton, Thomas Mikal-Evans +142

JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5,000 confirmed planets, more than 4,000 TESS planet candidates a…

astro-ph.SR2024

Stellar Characterization and Chemical Abundances of Exoplanet Hosting M dwarfs from APOGEE Spectra: Future JWST Targets

Edypo Melo, Diogo Souto, Katia Cunha +11

Exoplanets hosting M dwarfs are the best targets to characterize Earth-like or super-Earth planetary atmospheres with the James Webb Space Telescope (JWST). We determine detailed s…