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20152025
most citedThe Mass-Metallicity Relation for Giant Planets

437 citations · 2.8k across the 62 of their papers we have counts for

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60 papers · 1 filter

astro-ph.EP2025

A Compact Multi-Planet System of Three Transiting Giant Planets Around TIC118798035

Rafael Brahm, Trifon Trifonov, Andrés Jordán +20

We report the discovery and characterization of three transiting giant planets in the TIC118798035 system. The three planets were identified as transiting candidates from data of t…

astro-ph.EP2025★ 21 cited

Revising the Giant Planet Mass-Metallicity Relation: Deciphering the Formation Sequence of Giant Planets

Yayaati Chachan, Jonathan J. Fortney, Kazumasa Ohno +2

The rate at which giant planets accumulate solids and gas is a critical component of planet formation models, yet it is extremely challenging to predict from first principles. Char…

astro-ph.EP2025★ 10 cited

A transiting giant planet in orbit around a 0.2-solar-mass host star

Edward M. Bryant, Andrés Jordán, Joel D. Hartman +56

Planet formation models suggest that the formation of giant planets is significantly harder around low-mass stars, due to the scaling of protoplanetary disc masses with stellar mas…

astro-ph.EP2025★ 7 cited

Cloudy mornings and clear evenings on a gas giant exoplanet

Sagnick Mukherjee, David K. Sing, Guangwei Fu +25

The spectra of exoplanet atmospheres are affected by aerosols (clouds and hazes) of uncertain origin. Proposed aerosol formation mechanisms include gas condensation or photochemica…

astro-ph.EP2025

A Revised Density Estimate for the Largest Known Exoplanet, HAT-P-67 b

Gavin Wang, William O. Balmer, Laurent Pueyo +7

Low-density () hot Saturns are expected to quickly ( Myr) lose their atmospheres due to stellar irradiation, explaining their rarity. HAT-P-67 b seems…

astro-ph.EP2025

The Super-Puff WASP-193b is On A Well-Aligned Orbit

Samuel W. Yee, Gudmundur Stefansson, Daniel Thorngren +8

The "super-puffs" are a population of planets that have masses comparable to that of Neptune but radii similar to Jupiter, leading to extremely low bulk densities ($ρ_p \lesssim 0.…

astro-ph.EP2025

Statistical trends in JWST transiting exoplanet atmospheres

Guangwei Fu, Kevin B. Stevenson, David K. Sing +13

Our brains are hardwired for pattern recognition as correlations are useful for predicting and understanding nature. As more exoplanet atmospheres are being characterized with JWST…

astro-ph.EP2025★ 4 cited

A Comprehensive Reanalysis of K2-18 b's JWST NIRISS+NIRSpec Transmission Spectrum

Stephen P. Schmidt, Ryan J. MacDonald, Shang-Min Tsai +13

Sub-Neptunes are the most common type of planet in our galaxy. Interior structure models suggest that the coldest sub-Neptunes could host liquid water oceans underneath their hydro…

astro-ph.EP2024

VLTI/GRAVITY Observations of AF Lep b: Preference for Circular Orbits, Cloudy Atmospheres, and a Moderately Enhanced Metallicity

William O. Balmer, Kyle Franson, Antoine Chomez +26

Direct imaging observations are biased towards wide-separation, massive companions that have degenerate formation histories. Although the majority of exoplanets are expected to for…

astro-ph.EP2024

Reassessing Sub-Neptune Structure, Radii, and Thermal Evolution

Yao Tang, Jonathan J. Fortney, Francis Nimmo +3

We present a novel python-based 1D sub-Neptune evolution model that emphasizes the thermal evolution and potential solidification of the rock/iron core and the structure of the rad…

astro-ph.EP2024★ 23 cited

BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b

James Kirk, Eva-Maria Ahrer, Alastair B. Claringbold +23

We present a transmission spectrum of the misaligned hot Jupiter WASP-15b from 2.8-5.2 microns observed with JWST's NIRSpec/G395H grating. Our high signal to noise data, which has…

astro-ph.EP2024★ 3 cited

The Featherweight Giant: Unraveling the Atmosphere of a 17 Myr Planet with JWST

Pa Chia Thao, Andrew W. Mann, Adina D. Feinstein +29

The characterization of young planets (< 300 Myr) is pivotal for understanding planet formation and evolution. We present the 3-5m transmission spectrum of the 17 Myr, Jupiter-s…

astro-ph.EP2024★ 1 cited

Separating Super-Puffs vs. Hot Jupiters Among Young Puffy Planets

Amalia Karalis, Eve J. Lee, Daniel P. Thorngren

Discoveries of close-in young puffy (R 6 R) planets raise the question of whether they are bona fide hot Jupiters or puffed-up Neptunes, potentially plac…

astro-ph.EP2024

Surviving in the Hot Neptune Desert: The Discovery of the Ultra-Hot Neptune TOI-3261b

Emma Nabbie, Chelsea X. Huang, Jennifer A. Burt +45

The recent discoveries of Neptune-sized ultra-short period planets (USPs) challenge existing planet formation theories. It is unclear whether these residents of the Hot Neptune Des…

astro-ph.EP2024★ 92 cited

A warm Neptune's methane reveals core mass and vigorous atmospheric mixing

David K. Sing, Zafar Rustamkulov, Daniel P. Thorngren +18

Observations of transiting gas giant exoplanets have revealed a pervasive depletion of methane, which has only recently been identified atmospherically. The depletion is thought to…

astro-ph.EP2024

Giant Outer Transiting Exoplanet Mass (GOT `EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away

Yayaati Chachan, Paul A. Dalba, Daniel P. Thorngren +6

Systems hosting multiple giant planets are important laboratories for understanding planetary formation and migration processes. We present a nearly decade-long Doppler spectroscop…

astro-ph.EP2024

Helium in the Extended Atmosphere of the Warm Super-Puff TOI-1420b

Shreyas Vissapragada, Michael Greklek-McKeon, Dion Linssen +11

Super-puffs are planets with exceptionally low densities (~g~cm) and core masses (). Many lower-mass () super-…

astro-ph.EP2024★ 29 cited

JWST Reveals CH, CO, and HO in a Metal-rich Miscible Atmosphere on a Two-Earth-Radius Exoplanet

Björn Benneke, Pierre-Alexis Roy, Louis-Philippe Coulombe +28

Even though sub-Neptunes likely represent the most common outcome of planet formation, their natures remain poorly understood. In particular, planets near 1.5-2.5 often…

astro-ph.EP2024★ 14 cited

Three Warm Jupiters around Solar-analog stars detected with TESS

Jan Eberhardt, Melissa J. Hobson, Thomas Henning +32

We report the discovery and characterization of three giant exoplanets orbiting solar-analog stars, detected by the \tess space mission and confirmed through ground-based photometr…

astro-ph.EP2024★ 1 cited

Muted Features in the JWST NIRISS Transmission Spectrum of Hot-Neptune LTT 9779 b

Michael Radica, Louis-Philippe Coulombe, Jake Taylor +13

The hot-Neptune desert is one of the most sparsely populated regions of the exoplanet parameter space, and atmosphere observations of its few residents can provide insights into ho…

astro-ph.EP2024

Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets

Paul A. Dalba, Stephen R. Kane, Howard Isaacson +29

Discovering and characterizing exoplanets at the outer edge of the transit method's sensitivity has proven challenging owing to geometric biases and the practical difficulties asso…

astro-ph.EP2023★ 13 cited

Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey: III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-Transit Jupiter Orbiting TOI-2010

Christopher R. Mann, Paul A. Dalba, David Lafrenière +48

Large-scale exoplanet surveys like the TESS mission are powerful tools for discovering large numbers of exoplanet candidates. Single-transit events are commonplace within the resul…

astro-ph.EP2023★ 11 cited

TESS Giants Transiting Giants V -- Two hot Jupiters orbiting red-giant hosts

Filipe Pereira, Samuel K. Grunblatt, Angelica Psaridi +24

In this work we present the discovery and confirmation of two hot Jupiters orbiting red-giant stars, TOI-4377 b and TOI-4551 b, observed by TESS in the southern ecliptic hemisphere…

astro-ph.EP2023

TESS Spots a Super-Puff: The Remarkably Low Density of TOI-1420b

Stephanie Yoshida, Shreyas Vissapragada, David W. Latham +51

We present the discovery of TOI-1420b, an exceptionally low-density ( g cm) transiting planet in a day orbit around a late G dwarf star. Using tra…