papers

Publications (75)

astro-ph.EP2022

Titanium oxide and chemical inhomogeneity in the atmosphere of the exoplanet WASP-189b

Bibiana Prinoth, H. Jens Hoeijmakers, Daniel Kitzmann +21

The temperature of an atmosphere decreases with increasing altitude, unless a shortwave absorber exists that causes a temperature inversion. Ozone plays this role in the Earth`s at…

astro-ph.EP2019

Linking the evolution of terrestrial interiors and an early outgassed atmosphere to astrophysical observations

Dan J. Bower, Daniel Kitzmann, Aaron S. Wolf +3

A terrestrial planet is molten during formation and may remain so if subject to intense insolation or tidal forces. Observations continue to favour the detection and characterisati…

astro-ph.EP2017

Analytical Models of Exoplanetary Atmospheres. IV. Improved Two-stream Radiative Transfer for the Treatment of Aerosols

Kevin Heng, Daniel Kitzmann

We present a novel generalization of the two-stream method of radiative transfer, which allows for the accurate treatment of radiative transfer in the presence of strong infrared s…

astro-ph.EP2026

A population view of transiting hot giant exoplanets: Tracing Fe and Ti chemistry with ESPRESSO and MAROON-X

Bibiana Prinoth, Vivien Parmentier, Stefan Pelletier +9

Hot and ultra-hot Jupiters offer a unique laboratory to study atmospheric chemistry at the population level using ground-based high-resolution spectroscopy. Fe and Ti are key trace…

astro-ph.SR2019

Supervised Machine Learning for Intercomparison of Model Grids of Brown Dwarfs: Application to GJ 570D and the Epsilon Indi B Binary System

Maria Oreshenko, Daniel Kitzmann, Pablo Marquez-Neila +6

Self-consistent model grids of brown dwarfs involve complex physics and chemistry, and are often computed using proprietary computer codes, making it challenging to identify the re…

astro-ph.EP2026

NCCR PlanetS: Observational and computational characterization of exoplanet atmospheres

Daniel Kitzmann, Elspeth K. H. Lee, Jens Hoeijmakers +1

This chapter reviews the current state of observational and theoretical efforts in the characterization of exoplanet atmospheres, with a focus on developments enabled through the S…

astro-ph.SR2020

Hunt for Starspots in HARPS Spectra of G and K Stars

Brett M. Morris, H. Jens Hoeijmakers, Daniel Kitzmann +1

We present a method for detecting starspots on cool stars using the cross-correlation function (CCF) of high resolution molecular spectral templates applied to archival high-resolu…

astro-ph.EP2019

The potassium absorption on HD189733b and HD209458b

Engin Keles, Matthias Mallonn, Carolina von Essen +9

In this work, we investigate the potassium excess absorption around 7699A of the exoplanets HD189733b and HD209458b. For this purpose, we used high spectral resolution transit obse…

astro-ph.EP2023

Retrieval study of cool, directly imaged exoplanet 51 Eri b

Niall Whiteford, Alistair Glasse, Katy L. Chubb +12

Retrieval methods are a powerful analysis technique for modelling exoplanetary atmospheres by estimating the bulk physical and chemical properties that combine in a forward model t…

astro-ph.EP2025

Competing chemical signatures in the atmosphere of TOI-270 d: Inference of sulfur and carbon chemistry

Lukas Felix, Daniel Kitzmann, Brice-Olivier Demory +1

Recent JWST measurements allow access to the near-infrared spectrum of the sub-Neptune TOI-270 d, for which two different interpretations, a high-metallicity miscible envelope and…

astro-ph.EP2020

Exploring the atmospheric dynamics of the extreme ultra-hot Jupiter KELT-9b using TESS photometry

Ian Wong, Avi Shporer, Daniel Kitzmann +24

We carry out a phase-curve analysis of the KELT-9 system using photometric observations from NASA's Transiting Exoplanet Survey Satellite (TESS). The measured secondary eclipse dep…

astro-ph.EP2022

The PEPSI Exoplanet Transit Survey (PETS) I: Investigating the presence of a silicate atmosphere on the super-Earth 55 Cnc e

Engin Keles, Matthias Mallonn, Daniel Kitzmann +26

The study of exoplanets and especially their atmospheres can reveal key insights on their evolution by identifying specific atmospheric species. For such atmospheric investigations…

astro-ph.EP2021

A Comparative Study of Atmospheric Chemistry with VULCAN

Shang-Min Tsai, Matej Malik, Daniel Kitzmann +4

We present an update of the open-source photochemical kinetics code VULCAN (Tsai et al. 2017; https://github.com/exoclime/VULCAN) to include C-H-N-O-S networks and photochemistry.…

astro-ph.EP2026

Climates of Terrestrial Exoplanets and Biosignatures

Siddharth Bhatnagar, Emeline Bolmont, Nikita J. Boeren +18

Understanding the climates of terrestrial exoplanets and the detectability of biosignatures is an inherently interdisciplinary challenge, requiring the integration of insights from…

astro-ph.EP2025

Parameter degeneracies associated with interpreting HST WFC3 transmission spectra of exoplanetary atmospheres

Aline Novais, Chloe Fisher, Luan Ghezzi +3

The Wide Field Camera 3 (WFC3) instrument on the Hubble Space Telescope has provided an abundance of exoplanet spectra over the years. These spectra have enabled analysis studies u…

astro-ph.EP2021

Simulating gas giant exoplanet atmospheres with Exo-FMS: Comparing semi-grey, picket fence and correlated-k radiative-transfer schemes

Elspeth K. H. Lee, Vivien Parmentier, Mark Hammond +5

Radiative-transfer (RT) is a fundamental part of modelling exoplanet atmospheres with general circulation models (GCMs). An accurate RT scheme is required for estimates of the atmo…

astro-ph.EP2021

Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability & diversity

Sascha P. Quanz, Olivier Absil, Daniel Angerhausen +45

Exoplanet science is one of the most thriving fields of modern astrophysics. A major goal is the atmospheric characterization of dozens of small, terrestrial exoplanets in order to…

astro-ph.EP2016

HELIOS: An Open-source, GPU-accelerated Radiative Transfer Code For Self-consistent Exoplanetary Atmospheres

Matej Malik, Luc Grosheintz, João M. Mendonça +10

We present the open-source radiative transfer code named HELIOS, which is constructed for studying exoplanetary atmospheres. In its initial version, the model atmospheres of HELIOS…

astro-ph.EP2023

FastChem Cond: Equilibrium chemistry with condensation and rainout for cool planetary and stellar environments

Daniel Kitzmann, Joachim W. Stock, A. Beate C. Patzer

Cool astrophysical objects, such as (exo)planets, brown dwarfs, or asymptotic giant branch stars, can be strongly affected by condensation. Condensation does not only directly affe…

astro-ph.EP2024

Observations of scattered light from exoplanet atmospheres

Brett M. Morris, Kevin Heng, Daniel Kitzmann

Optical phase curves of hot Jupiters can reveal global scattering properties. We implement a Bayesian inference framework for optical phase curves with flux contributions from: ref…

astro-ph.EP2025

JWST NIRSpec finds no clear signs of an atmosphere on TOI-1685 b

Chloe E. Fisher, Matthew J. Hooton, Amélie Gressier +21

Determining the prevalence of atmospheres on terrestrial planets is a core objective in exoplanetary science. While M dwarf systems offer a promising opportunity, conclusive observ…

astro-ph.EP2022

Retrieval Study of Brown Dwarfs Across the L-T Sequence

Anna Lueber, Daniel Kitzmann, Brendan P. Bowler +2

A large suite of 228 atmospheric retrievals is performed on a curated sample of 19 brown dwarfs spanning the L0 to T8 spectral types using the open-source Helios-r2 retrieval code,…

astro-ph.EP2024

A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST

TRAPPIST-1 JWST Community Initiative, :, Julien de Wit +80

Ultra-cool dwarf stars are abundant, long-lived, and uniquely suited to enable the atmospheric study of transiting terrestrial companions with JWST. Amongst them, the most prominen…

astro-ph.EP2026

An Ultra-Short Period Super-Earth and a Sub-Neptune Orbiting the K dwarf TOI-4311

Yoshi Nike Emilia Eschen, Thomas G. Wilson, Andrew Collier Cameron +95

We report the discovery and characterisation of the multi-planetary system around TOI-4311, a K dwarf kinematically between the Galactic thick disk and Hercules stream. TOI-4311 ho…

astro-ph.EP2020

Helios-r2 -- A new Bayesian, open-source retrieval model for brown dwarfs and exoplanet atmospheres

Daniel Kitzmann, Kevin Heng, Maria Oreshenko +5

We present an improved, hybrid CPU-GPU atmospheric retrieval code, Helios-r2, which is applicable to medium-resolution emission spectra of brown dwarfs, in preparation for precisio…

astro-ph.EP2018

Towards Consistent Modeling of Atmospheric Chemistry and Dynamics in Exoplanets: Validation and Generalization of Chemical Relaxation Method

Shang-Min Tsai, Daniel Kitzmann, James R. Lyons +3

Motivated by the work of Cooper & Showman, we revisit the chemical relaxation method, which seeks to enhance the computational efficiency of chemical-kinetics calculations by repla…

astro-ph.EP2024

Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3

Michaël Gillon, Peter P. Pedersen, Benjamin V. Rackham +81

Located at the bottom of the main sequence, ultracool dwarf stars are widespread in the solar neighbourhood. Nevertheless, their extremely low luminosity has left their planetary p…

astro-ph.EP2018

Analytical Models of Exoplanetary Atmospheres. VI. Full Solutions for Improved Two-stream Radiative Transfer Including Direct Stellar Beam

Kevin Heng, Matej Malik, Daniel Kitzmann

Two-stream radiative transfer is a workhorse in the Earth, planetary and exoplanetary sciences due to its simplicity and ease of implementation. However, a longstanding limitation…

astro-ph.EP2022

3D radiative-transfer for exoplanet atmospheres. gCMCRT: a GPU accelerated MCRT code

Elspeth K. H. Lee, Joost P. Wardenier, Bibiana Prinoth +10

Radiative-transfer (RT) is a key component for investigating atmospheres of planetary bodies. With the 3D nature of exoplanet atmospheres being important in giving rise to their ob…

astro-ph.EP2024

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems V: Do Self-Consistent Atmospheric Models Represent JWST Spectra? A Showcase With VHS 1256 b

Simon Petrus, Niall Whiteford, Polychronis Patapis +119

The unprecedented medium-resolution (R~1500-3500) near- and mid-infrared (1-18um) spectrum provided by JWST for the young (140+/-20Myr) low-mass (12-20MJup) L-T transition (L7) com…

astro-ph.EP2020

High-resolution Transmission Spectroscopy of MASCARA-2 b with EXPRES

H. Jens Hoeijmakers, Samuel H. C. Cabot, Lily Zhao +10

We report detections of atomic species in the atmosphere of MASCARA-2 b, using the first transit observations obtained with the newly commissioned EXPRES spectrograph. EXPRES is a…

astro-ph.EP2023

The Mantis Network I: A standard grid of templates and masks for cross-correlation analyses of ultra-hot Jupiter transmission spectra

Daniel Kitzmann, Jens H. Hoeijmakers, Simon L. Grimm +3

The atmospheres of ultra-hot Jupiters are highly interesting and unique chemical laboratories. Due to the very high atmospheric temperatures, their chemical composition is dominate…

astro-ph.EP2022

The Mantis Network II: Examining the 3D high-resolution observable properties of the UHJs WASP-121b and WASP-189b through GCM modelling

Elspeth K. H. Lee, Bibiana Prinoth, Daniel Kitzmann +4

The atmospheres of ultra hot Jupiters (UHJs) are prime targets for the detection of molecules and atoms at both low and high spectral resolution. We study the atmospheres of the UH…

astro-ph.EP2020

Atmospheric Characterization via Broadband Color Filters on the PLAnetary Transits and Oscillations of stars (PLATO) Mission

John Lee Grenfell, Mareike Godolt, Juan Cabrera +5

We assess broadband color filters for the two fast cameras on the PLAnetary Transits and Oscillations (PLATO) of stars space mission with respect to exoplanetary atmospheric charac…

astro-ph.EP2025

Modelling the 3D atmospheric structure of the cold Jupiter WD1856+534b orbiting a white dwarf

Pascal A. Noti, Elspeth K. H. Lee, Daniel Kitzmann +5

WD-1856b+534b (WD-1856b) is to date the only detected cold Jupiter outside of our Solar System. This cold Jupiter can provide useful information about the cold giants in our Solar…

astro-ph.EP2024

The Retrieved Atmospheric Properties of the Sub-stellar Object VHS 1256 b from Analyzing HST, VLT and JWST Spectra

Anna Lueber, Kevin Heng, Brendan P. Bowler +3

Motivated by the observed ~30% variations in flux from the L7 dwarf VHS 1256 b, we subjected its time-resolved Hubble Space Telescope (HST) WFC3 spectra (measured in two epochs in…

astro-ph.EP2025

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Mark Fortune, Neale P. Gibson, Hannah Diamond-Lowe +14

Time-series photometry at mid-infrared wavelengths is becoming a common technique to search for atmospheres around rocky exoplanets. This method constrains the brightness temperatu…

astro-ph.EP2020

Interpreting High-Resolution Spectroscopy of Exoplanets Using Cross-Correlations and Supervised Machine Learning

Chloe Fisher, H. Jens Hoeijmakers, Daniel Kitzmann +4

We present a new method for performing atmospheric retrieval on ground-based, high-resolution data of exoplanets. Our method combines cross-correlation functions with a random fore…

astro-ph.EP2025

An Ultra-Short Period Super-Earth and Sub-Neptune Spanning the Radius Valley Orbiting the Kinematic Thick Disk Star TOI-2345

Yoshi Nike Emilia Eschen, Thomas G. Wilson, Andrea Bonfanti +94

A crucial chemical link between stars and their orbiting exoplanets is thought to exist. If universal, this connection could affect the formation and evolution of all planets. Ther…

astro-ph.EP2025

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems III: Aperture Masking Interferometric Observations of the star HIP 65426 at 3.8 um

Shrishmoy Ray, Steph Sallum, Sasha Hinkley +121

We present aperture masking interferometry (AMI) observations of the star HIP 65426 at as a part of the JWST Direct Imaging Early Release Science (ERS) program obta…

astro-ph.EP2017

Optical properties of potential condensates in exoplanetary atmospheres

Daniel Kitzmann, Kevin Heng

The prevalence of clouds in currently observable exoplanetary atmospheres motivates the compilation and calculation of their optical properties. First, we present a new open-source…

astro-ph.EP2017

VULCAN: an Open-Source, Validated Chemical Kinetics Python Code for Exoplanetary Atmospheres

Shang-Min Tsai, James R. Lyons, Luc Grosheintz +3

We present an open-source and validated chemical kinetics code for studying hot exoplanetary atmospheres, which we name VULCAN. It is constructed for gaseous chemistry from 500 to…

astro-ph.EP2025

Differentiable Modeling of Planet and Substellar Atmosphere: High-Resolution Emission, Transmission, and Reflection Spectroscopy with ExoJAX2

Hajime Kawahara, Yui Kawashima, Shotaro Tada +11

Modeling based on differentiable programming holds great promise for astronomy, enabling advanced techniques such as gradient-based posterior sampling and optimization. This paradi…

astro-ph.EP2018

The Peculiar Atmospheric Chemistry of KELT-9b

Daniel Kitzmann, Kevin Heng, Paul B. Rimmer +6

The atmospheric temperatures of the ultra-hot Jupiter KELT-9b straddle the transition between gas giants and stars, and therefore between two traditionally distinct regimes of atmo…

astro-ph.EP2022

FastChem 2: An improved computer program to determine the gas-phase chemical equilibrium composition for arbitrary element distributions

Joachim W. Stock, Daniel Kitzmann, A. Beate C. Patzer

The computation of complex neutral/ionised chemical equilibrium compositions is invaluable to obtain scientific insights of, for example, the atmospheres of extrasolar planets and…

astro-ph.IM2018

Exoplanet science with a space-based mid-infrared nulling interferometer

Sascha P. Quanz, Jens Kammerer, Denis Defrère +3

One of the long-term goals of exoplanet science is the (atmospheric) characterization of a large sample (>100) of terrestrial planets to assess their potential habitability and ove…

astro-ph.EP2026

Hot Rocks Survey V: Secondary Eclipse Photometry of GJ 3473 b with JWST/MIRI

Måns Holmberg, Hannah Diamond-Lowe, João M. Mendonça +16

JWST is transforming our ability to characterise small exoplanets, from sub-Neptunes to rocky worlds. A key open question is whether highly irradiated rocky planets can retain atmo…

astro-ph.EP2024

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems IV: NIRISS Aperture Masking Interferometry Performance and Lessons Learned

Steph Sallum, Shrishmoy Ray, Jens Kammerer +120

We present a performance analysis for the aperture masking interferometry (AMI) mode on board the James Webb Space Telescope Near Infrared Imager and Slitless Spectrograph (JWST/NI…

astro-ph.EP2013

Clouds and Hazes in Exoplanet Atmospheres

Mark S. Marley, Andrew S. Ackerman, Jeffrey N. Cuzzi +1

Clouds and hazes are commonplace in the atmospheres of solar system planets and are likely ubiquitous in the atmospheres of extrasolar planets as well. Clouds affect every aspect o…

astro-ph.EP2026

FastChem 4: New chemical elements and improved convergence behaviour

Daniel Kitzmann, Joachim W. Stock, A. Beate C. Patzer

Chemical equilibrium calculations are a key ingredient for modelling and interpreting spectroscopic observations of (exo)planets, brown dwarfs, cool stars, and protoplanetary disks…

astro-ph.EP2026

The Goldilocks problem for detecting water in terrestrial planets: Constraining water abundances in the mid-IR with LIFE

Sarah Rugheimer, Eleonora Alei, Björn S. Konrad +7

We investigate how well the Large Interferometer for Exoplanets (LIFE) mission concept can detect habitable conditions on exoplanets through the presence of atmospheric water vapor…

astro-ph.EP2025

Kinetic and photochemical disequilibrium in the potentially carbon-rich atmosphere of the warm-Jupiter WASP-69b

Nidhi Bangera, Christiane Helling, Gloria Guilluy +5

High-resolution transmission spectroscopy of the warm gas-giant WASP-69b has revealed the presence of H2O, CO, CH4, NH3, and C2H2 in its atmosphere. This study investigates the imp…

astro-ph.EP2021

Visible-light Phase Curves from the Second Year of the TESS Primary Mission

Ian Wong, Daniel Kitzmann, Avi Shporer +10

We carried out a systematic study of full-orbit phase curves for known transiting systems in the northern ecliptic sky that were observed during Year 2 of the TESS primary mission.…

astro-ph.EP2024

JWST/NIRISS and HST: Exploring the improved ability to characterise exoplanet atmospheres in the JWST era

Chloe Fisher, Jake Taylor, Vivien Parmentier +6

The Hubble Space Telescope has been a pioneering instrument for studying the atmospheres of exoplanets, specifically its WFC3 and STIS instruments. With the launch of JWST, we are…

astro-ph.EP2017

Clouds in the atmospheres of extrasolar planets. V. The impact of CO2 ice clouds on the outer boundary of the habitable zone

Daniel Kitzmann

Clouds have a strong impact on the climate of planetary atmospheres. The potential scattering greenhouse effect of CO2 ice clouds in the atmospheres of terrestrial extrasolar plane…

astro-ph.EP2020

Information content of JWST-NIRSPEC transmission spectra of warm Neptunes

Andrea Guzmán-Mesa, Daniel Kitzmann, Chloe Fisher +7

Warm Neptunes offer a rich opportunity for understanding exo-atmospheric chemistry. With the upcoming James Webb Space Telescope (JWST), there is a need to elucidate the balance be…

astro-ph.SR2022

Sunbathing under white light -- 3D modelling of brown dwarf - white dwarf atmospheres with strong UV irradiation

Elspeth K. H. Lee, Joshua D. Lothringer, Sarah L. Casewell +3

The atmospheres of brown dwarfs orbiting in close proximity to their parent white dwarf represent some of the most extreme irradiated environments known. Understanding their comple…

astro-ph.EP2018

Atomic iron and titanium in the atmosphere of the exoplanet KELT-9b

H. Jens Hoeijmakers, David Ehrenreich, Kevin Heng +10

The chemical composition of an exoplanet is a key ingredient in constraining its formation history. Iron is the most abundant transition metal, but has never been directly detected…

astro-ph.EP2026

Ultra-hot Jupiter atmospheres at high spectral resolution

Stefan Pelletier, Daniel Kitzmann, Valentina Vaulato +3

Observations of ultra-hot Jupiters offer an unprecedented opportunity to study the physics of some of the most extreme planetary atmospheres known. With exceedingly high amounts of…

astro-ph.SR2023

Intercomparison of Brown Dwarf Model Grids and Atmospheric Retrieval Using Machine Learning

Anna Lueber, Daniel Kitzmann, Chloe E. Fisher +4

Understanding differences between sub-stellar spectral data and models has proven to be a major challenge, especially for self-consistent model grids that are necessary for a thoro…

astro-ph.SR2022

Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-Dwarf Companion in the Hyades

Kyle Franson, Brendan P. Bowler, Mariangela Bonavita +28

Benchmark brown dwarf companions with well-determined ages and model-independent masses are powerful tools to test substellar evolutionary models and probe the formation of giant p…

astro-ph.EP2021

Physically-motivated basis functions for temperature maps of exoplanets

Brett M. Morris, Kevin Heng, Kathryn Jones +4

Thermal phase curves of exoplanet atmospheres have revealed temperature maps as a function of planetary longitude, often by sinusoidal decomposition of the phase curve. We construc…

astro-ph.EP2024

Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c

Alexander D. Rathcke, Lars A. Buchhave, Julien De Wit +8

Stellar surface heterogeneities, such as spots and faculae, often contaminate exoplanet transit spectra, hindering precise atmospheric characterization. We demonstrate a novel, epo…

astro-ph.EP2021

HELIOS-K 2.0 Opacity Calculator and Open-source Opacity Database for Exoplanetary Atmospheres

Simon L. Grimm, Matej Malik, Daniel Kitzmann +12

Computing and using opacities is a key part of modeling and interpreting data of exoplanetary atmospheres. Since the underlying spectroscopic line lists are constantly expanding an…

astro-ph.EP2021

Lithologic Controls on Silicate Weathering Regimes of Temperate Planets

Kaustubh Hakim, Dan J. Bower, Meng Tian +6

Weathering of silicate rocks at a planetary surface can draw down CO from the atmosphere for eventual burial and long-term storage in the planetary interior. This process is th…

astro-ph.EP2016

Revisiting the scattering greenhouse effect of CO2 ice clouds

Daniel Kitzmann

Carbon dioxide ice clouds are thought to play an important role for cold terrestrial planets with thick CO2 dominated atmospheres. Various previous studies showed that a scattering…

astro-ph.EP2019

Self-luminous and irradiated exoplanetary atmospheres explored with HELIOS

Matej Malik, Daniel Kitzmann, João M. Mendonça +5

We present new methodological features and physical ingredients included in the 1D radiative transfer code HELIOS, improving the hemispheric two-stream formalism. We conduct a thor…

astro-ph.EP2023

Time-resolved transmission spectroscopy of the ultra-hot Jupiter WASP-189 b

Bibiana Prinoth, H. Jens Hoeijmakers, Stefan Pelletier +14

Ultra-hot Jupiters are tidally locked with their host stars dividing their atmospheres into a hot dayside and a colder nightside. As the planet moves through transit, different reg…

astro-ph.EP2018

A ground-based NUV secondary eclipse observation of KELT-9b

Matthew J. Hooton, Christopher A. Watson, Ernst J. W. de Mooij +2

KELT-9b is a recently discovered exoplanet with a 1.49 d orbit around a B9.5/A0-type star. The unparalleled levels of UV irradiation it receives from its host star put KELT-9b in i…

astro-ph.EP2021

Closed-formed ab initio solutions of geometric albedos and reflected light phase curves of exoplanets

Kevin Heng, Brett M. Morris, Daniel Kitzmann

Studying the albedos of the planets and moons of the Solar System dates back at least a century. Of particular interest is the relationship between the albedo measured at superior…

astro-ph.EP2025

Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b

Prune C. August, Lars A. Buchhave, Hannah Diamond-Lowe +18

M dwarf systems offer an opportunity to study terrestrial exoplanetary atmospheres due to their small size and cool temperatures. However, the extreme conditions imposed by these h…

astro-ph.EP2017

The theory of transmission spectra revisited: a semi-analytical method for interpreting WFC3 data and an unresolved challenge

Kevin Heng, Daniel Kitzmann

The computation of transmission spectra is a central ingredient in the study of exoplanetary atmospheres. First, we revisit the theory of transmission spectra, unifying ideas from…

astro-ph.EP2025

Hot Rocks Survey IV: Emission from LTT 3780 b is consistent with a bare rock

Natalie H. Allen, Néstor Espinoza, Hannah Diamond-Lowe +19

It is an open question whether small planets around M dwarfs are able to maintain atmospheres. The Hot Rocks Survey aims to address this question by observing 9 rocky exoplanets or…

astro-ph.EP2024

Sulphur dioxide in the mid-infrared transmission spectrum of WASP-39b

Diana Powell, Adina D. Feinstein, Elspeth K. H. Lee +70

The recent inference of sulphur dioxide (SO) in the atmosphere of the hot (1100 K), Saturn-mass exoplanet WASP-39b from near-infrared JWST observations suggests that phot…

astro-ph.EP2021

TOI-2109b: An Ultrahot Gas Giant on a 16 hr Orbit

Ian Wong, Avi Shporer, George Zhou +56

We report the discovery of an ultrahot Jupiter with an extremely short orbital period of days (16 hr). The plane…