papers

Publications (64)

astro-ph.GA2024

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies

Daizhong Liu, Amelie Saintonge, Caroline Bot +25

Understanding the physical processes that regulate star formation and galaxy evolution are major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunitie…

astro-ph.EP2016

Origin and evolution of two-component debris discs and an application to the q Eridani system

Christian Schüppler, Alexander V. Krivov, Torsten Löhne +3

Many debris discs reveal a two-component structure, with an outer Kuiper-belt analogue and a warm inner component whose origin is still a matter of debate. One possibility is that…

astro-ph.SR2025

Debris disks around M dwarfs: The Herschel DEBRIS survey

Jean-Francois Lestrade, Brenda C. Matthews, Grant M. Kennedy +7

The Herschel open-time key program Disc Emission via a Bias-free Reconnaissance in the Infrared and Sub-millimeter (DEBRIS) is an unbiased survey of the nearest ~100 stars for each…

astro-ph.EP2009

The History of the Solar System's Debris Disc: Observable Properties of the Kuiper Belt

Mark Booth, Mark C. Wyatt, Alessandro Morbidelli +2

The Nice model of Gomes et al. (2005) suggests that the migration of the giant planets caused a planetesimal clearing event which led to the Late Heavy Bombardment (LHB) at 880 Myr…

astro-ph.EP2023

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High Contrast Imaging of the Exoplanet HIP 65426 b from 2-16 m

Aarynn L. Carter, Sasha Hinkley, Jens Kammerer +108

We present JWST Early Release Science (ERS) coronagraphic observations of the super-Jupiter exoplanet, HIP 65426 b, with the Near-Infrared Camera (NIRCam) from 2-5 m, and with…

astro-ph.EP2022

Planet populations inferred from debris discs: insights from 178 debris systems in the ISPY, LEECH and LIStEN planet-hunting surveys

Tim D. Pearce, Ralf Launhardt, Robert Ostermann +11

We know little about the outermost exoplanets in planetary systems, because our detection methods are insensitive to moderate-mass planets on wide orbits. However, debris discs can…

astro-ph.EP2017

The Northern Arc of Eridani's Debris Ring as Seen by ALMA

Mark Booth, William R. F. Dent, Andrés Jordán +10

We present the first ALMA observations of the closest known extrasolar debris disc. This disc orbits the star Eridani, a K-type star just 3.2pc away. Due to the proximity of t…

astro-ph.EP2017

The First Scattered Light Image of the Debris Disk around the Sco-Cen target HD 129590

Elisabeth Matthews, Sasha Hinkley, Arthur Vigan +7

We present the first scattered light image of the debris disk around HD 129590, a ~1.3 M G1V member of the Scorpius Centaurus association with age ~10-16 Myr. The debris di…

astro-ph.EP2020

Observability of Debris Discs around M-stars

Patricia Luppe, Alexander V. Krivov, Mark Booth +1

Debris discs are second generation dusty discs formed by collisions of planetesimals. Many debris discs have been found and resolved around hot and solar-type stars. However, only…

astro-ph.EP2022

The JWST Early Release Science Program for the Direct Imaging & Spectroscopy of Exoplanetary Systems

Sasha Hinkley, Aarynn L. Carter, Shrishmoy Ray +83

The direct characterization of exoplanetary systems with high contrast imaging is among the highest priorities for the broader exoplanet community. As large space missions will be…

astro-ph.EP2020

Gas trapping of hot dust around main-sequence stars

Tim D. Pearce, Alexander V. Krivov, Mark Booth

In 2006 Vega was discovered to display excess near-infrared emission. Surveys now detect this phenomenon for one fifth of main-sequence stars, across various spectral types and age…

astro-ph.EP2025

Follow-Up Exploration of the TWA 7 Planet-Disk System with JWST NIRCam

Katie A. Crotts, Aarynn L. Carter, Kellen Lawson +39

The young M-star TWA 7 hosts a bright and near face-on debris disk, which has been imaged from the optical to the submillimeter. The disk displays multiple complex substructures su…

astro-ph.SR2015

The AU Mic Debris Disk: far-infrared and submillimeter resolved imaging

Brenda C. Matthews, Grant Kennedy, Bruce Sibthorpe +20

We present far-infrared and submillimeter maps from the Herschel Space Observatory and the James Clerk Maxwell Telescope of the debris disk host star AU Microscopii. Disk emission…

astro-ph.EP2020

Resolving the outer ring of HD 38206 using ALMA and constraining limits on planets in the system

Mark Booth, Michael Schulz, Alexander V. Krivov +3

HD 38206 is an A0V star in the Columba association, hosting a debris disc first discovered by IRAS. Further observations by Spitzer and Herschel showed that the disc has two compon…

astro-ph.EP2021

A detailed characterization of HR 8799's debris disk with ALMA in Band 7

Virginie Faramaz, Sebastian Marino, Mark Booth +8

The exoplanetary system of HR 8799 is one of the rare systems in which multiple planets have been directly imaged. Its architecture is strikingly similar to that of the Solar Syste…

astro-ph.SR2024

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Solar and stellar observations

Sven Wedemeyer, Miroslav Barta, Roman Brajsa +35

Observations at (sub-)millimeter wavelengths offer a complementary perspective on our Sun and other stars, offering significant insights into both the thermal and magnetic composit…

astro-ph.EP2024

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Planetary and Cometary Atmospheres

Martin A. Cordiner, Alexander E. Thelen, Thibault Cavalié +26

The study of planets and small bodies within our Solar System is fundamental for understanding the formation and evolution the Earth and other planets. Compositional and meteorolog…

astro-ph.CO2024

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Surveying the distant Universe

Eelco van Kampen, Tom Bakx, Carlos De Breuck +27

During the most active period of star formation in galaxies, which occurs in the redshift range 1<z<3, strong bursts of star formation result in significant quantities of dust, whi…

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.CO2025

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect

Luca Di Mascolo, Yvette Perrott, Tony Mroczkowski +23

An omnipresent feature of the multi-phase ``cosmic web'' is that warm/hot (> K) ionized gas pervades it. This gas constitutes a relevant contribution to the overall universal…

astro-ph.EP2011

The debris disk - terrestrial planet connection

Sean N. Raymond, Philip J. Armitage, Amaya Moro-Martín +5

The eccentric orbits of the known extrasolar giant planets provide evidence that most planet-forming environments undergo violent dynamical instabilities. Here, we numerically simu…

astro-ph.EP2019

From scattered-light to millimeter emission: A comprehensive view of the Gyr-old system of HD 202628 and its eccentric debris ring

Virginie Faramaz, John Krist, Karl R. Stapelfeldt +13

We present here new observations of the eccentric debris ring surrounding the Gyr-old solar-type star HD 202628: at millimeter wavelengths with ALMA, at far-infrared wavelengths wi…

astro-ph.SR2016

ALMA Observations of the Debris Disk of Solar Analogue Tau Ceti

Meredith A. MacGregor, Samantha M. Lawler, David J. Wilner +4

We present 1.3 mm observations of the Sun-like star Ceti with the Atacama Large Millimeter/submillimeter Array (ALMA) that probe angular scales of '' (4 AU). This first…

astro-ph.EP2011

Debris disk size distributions: steady state collisional evolution with P-R drag and other loss processes

Mark C. Wyatt, Cathie J. Clarke, Mark Booth

We present a new scheme for determining the shape of the size distribution, and its evolution, for collisional cascades of planetesimals undergoing destructive collisions and loss…

astro-ph.EP2016

Resolving the Planetesimal Belt of HR 8799 with ALMA

Mark Booth, Andrés Jordán, Simon Casassus +7

The star HR 8799 hosts one of the largest known debris discs and at least four giant planets. Previous observations have found evidence for a warm belt within the orbits of the pla…

astro-ph.EP2026

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) III: The vertical structure of debris disks

Brianna Zawadzki, Anna Fehr, A. Meredith Hughes +37

Debris disks -- collisionally sustained belts of dust and sometimes gas around main sequence stars -- are remnants of planet formation processes and are found in systems ${\gtrsim}…

astro-ph.SR2017

SONS: The JCMT legacy survey of debris discs in the submillimetre

Wayne S. Holland, Brenda C. Matthews, Grant M. Kennedy +32

Debris discs are evidence of the ongoing destructive collisions between planetesimals, and their presence around stars also suggests that planets exist in these systems. In this pa…

astro-ph2008

Dynamical Simulations of the Planetary System HD69830

Matthew J. Payne, Eric B. Ford, Mark C. Wyatt +1

HD 69830 exhibits radial velocity variations attributed to three planets as well as infrared emission attributed to a warm debris disk. Previous studies have developed models for t…

astro-ph.EP2025

Discovery of a Debris Disk Around TWA 20

Skyler Palatnick, Maxwell A. Millar-Blanchaer, Jingwen Zhang +20

We report the discovery of a debris disk surrounding the M3 star, TWA 20, revealed by JWST coronagraphic observations using the Near-infrared Camera (NIRCam). With reference-star d…

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.EP2023

The clumpy structure of Eridani's debris disc revisited by ALMA

Mark Booth, Tim D. Pearce, Alexander V. Krivov +8

Eridani is the closest star to our Sun known to host a debris disc. Prior observations in the (sub-)millimetre regime have potentially detected clumpy structure in the disc an…

astro-ph.EP2012

The debris disk around gamma Doradus resolved with Herschel

Hannah Broekhoven-Fiene, Brenda C. Matthews, Grant M. Kennedy +11

We present observations of the debris disk around gamma Doradus, an F1V star, from the Herschel Key Programme DEBRIS (Disc Emission via Bias-free Reconnaissance in the Infrared/Sub…

astro-ph.IM2024

The key science drivers for the Atacama Large Aperture Submillimeter Telescope (AtLAST)

Mark Booth, Pamela Klaassen, Claudia Cicone +14

Sub-mm and mm wavelengths provide a unique view of the Universe, from the gas and dust that fills and surrounds galaxies to the chromosphere of our own Sun. Current single-dish fac…

astro-ph.EP2022

Hot exozodis: cometary supply without trapping is unlikely to be the mechanism

Tim D. Pearce, Florian Kirchschlager, Gaël Rouillé +6

Excess near-infrared emission is detected around one fifth of main-sequence stars, but its nature is a mystery. These excesses are interpreted as thermal emission from populations…

astro-ph.EP2012

Resolved Debris Discs Around A Stars in the Herschel DEBRIS Survey

Mark Booth, Grant Kennedy, Bruce Sibthorpe +12

The majority of debris discs discovered so far have only been detected through infrared excess emission above stellar photospheres. While disc properties can be inferred from unres…

astro-ph.EP2018

Self-Stirring of Debris Discs by Planetesimals Formed by Pebble Concentration

Alexander V. Krivov, Mark Booth

When a protoplanetary disc loses gas, it leaves behind planets and one or more planetesimal belts. The belts get dynamically excited, either by planets ('planet stirring') or by em…

astro-ph.IM2024

AtLAST Science Overview Report

Mark Booth, Pamela Klaassen, Claudia Cicone +81

Submillimeter and millimeter wavelengths provide a unique view of the Universe, from the gas and dust that fills and surrounds galaxies to the chromosphere of our own Sun. Current…

astro-ph.EP2023

Inner edges of planetesimal belts: collisionally eroded or truncated?

Amaia Imaz Blanco, Sebastian Marino, Luca Matrà +9

The radial structure of debris discs can encode important information about their dynamical and collisional history. In this paper we present a 3-phase analytical model to analyse…

astro-ph.EP2009

How Common are Extrasolar, Late Heavy Bombardments?

Mark Booth, Mark C. Wyatt, Alessandro Morbidelli +2

The habitability of planets is strongly affected by impacts from comets and asteroids. Indications from the ages of Moon rocks suggest that the inner Solar System experienced an in…

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.EP2018

The Scattered Disc of HR 8799

Fabian Geiler, Alexander Krivov, Mark Booth +1

HR~8799 is a young F0-type star with four directly imaged giant planets and two debris belts, one located exterior and another one interior to the region occupied by the planetary…

astro-ph.EP2011

Debris disks as signposts of terrestrial planet formation

Sean N. Raymond, Philip J. Armitage, Amaya Moro-Martín +6

Circumstantial evidence suggests that most known extra-solar planetary systems are survivors of violent dynamical instabilities. Here we explore how giant planet instabilities affe…

astro-ph.EP2012

Debris disks as signposts of terrestrial planet formation. II Dependence of exoplanet architectures on giant planet and disk properties

Sean N. Raymond, Philip J. Armitage, Amaya Moro-Martin +6

We present models for the formation of terrestrial planets, and the collisional evolution of debris disks, in planetary systems that contain multiple unstable gas giants. We previo…

astro-ph.EP2021

Fomalhaut b could be massive and sculpting the narrow, eccentric debris disc, if in mean-motion resonance with it

Tim D. Pearce, Hervé Beust, Virginie Faramaz +4

The star Fomalhaut hosts a narrow, eccentric debris disc, plus a highly eccentric companion Fomalhaut b. It is often argued that Fomalhaut b cannot have significant mass, otherwise…

astro-ph.IM2026

The Atacama Large Aperture Submillimeter Telescope (AtLAST): enabling large-scale sub-mm science beyond 2030

Claudia Cicone, Tony Mroczkowski, Evanthia Hatziminaoglou +38

AtLAST is designed to be the largest (sub-)mm single-dish astronomical observatory and the first climate-neutral modern research infrastructure. It offers a unique combination of l…

astro-ph.EP2026

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems VIII: patchy forsterite and enstatite clouds in the atmosphere of VHS 1256 b, retrieval lessons learned and outlook to the future

Niall Whiteford, Jacqueline K. Faherty, Ben Burningham +123

JWST defines a new era for the data-driven approach of retrieval modelling, which has become a cornerstone tool for the statistical inference of exoplanetary and brown dwarf proper…

astro-ph.EP2019

The REASONS Survey: Resolved Millimeter Observations of a Large Debris Disk Around the Nearby F Star HD 170773

Aldo G. Sepulveda, Luca Matra, Grant M. Kennedy +15

Debris disks are extrasolar analogs to our own Kuiper Belt and they are detected around at least 17% of nearby Sun-like stars. The morphology and dynamics of a disk encode informat…

astro-ph.EP2023

The effect of sculpting planets on the steepness of debris-disc inner edges

Tim D. Pearce, Alexander V. Krivov, Antranik A. Sefilian +6

Debris discs are our best means to probe the outer regions of planetary systems. Many studies assume that planets lie at the inner edges of debris discs, akin to Neptune and the Ku…

astro-ph.IM2025

Debris disks and their properties with the Habitable Worlds Observatory

Isabel Rebollido, Yasuhiro Hasegawa, Meredith MacGregor +5

The study of the last stages of planet formation, also known as debris disks, is fundamental to place constrains on the formation of planetary sized bodies. Debris disks are compos…

astro-ph.IM2026

Detecting habitable exoplanet atmospheres with LIFE, the Large Interferometer for Exoplanets

Sarah Rugheimer, Aiden Weatherbee, James Fecanin +21

A key goal of astronomers with the next generation telescopes is to detect signs of life in exoplanet atmospheres. NASA's next flagship is the Habitable Worlds Observatory (HWO). I…

astro-ph.GA2024

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: The hidden circumgalactic medium

Minju M. Lee, Alice Schimek, Claudia Cicone +29

Our knowledge of galaxy formation and evolution has incredibly progressed through multi-wavelength observational constraints of the interstellar medium (ISM) of galaxies at all cos…

astro-ph.EP2026

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) II. The radial structure of debris discs

Yinuo Han, Elias Mansell, Jeff Jennings +38

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) was recently completed to cover the lack of high-resolution observations of debris discs and to investigate the preva…

astro-ph.GA2024

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Our Galaxy

Pamela Klaassen, Alessio Traficante, Maria T. Beltrán +38

As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas…

astro-ph.SR2020

The Age of the Carina Young Association and Potential Membership of HD 95086

Mark Booth, Carlos del Burgo, Valeri V. Hambaryan

Carina is a nearby young stellar association. So far, only a small number of stars have been clearly identified as members of this association. In this paper we reanalyse the membe…

astro-ph.EP2017

ALMA 1.3 Millimeter Map of the HD 95086 System

Kate Y. L. Su, Meredith A. Macgregor, Mark Booth +11

Planets and minor bodies such as asteroids, Kuiper-belt objects and comets are integral components of a planetary system. Interactions among them leave clues about the formation pr…

astro-ph.EP2026

JWST NIRCam Reveals the Largest Known M-dwarf Debris Disk Around TWA 10 and New Scattered-Light Observations of the TWA 25 Debris Disk

Katie A. Crotts, Aarynn L. Carter, Beth Biller +26

We present JWST NIRCam observations of two M-dwarf systems located in the TW Hydra association, TWA 10 and TWA 25. Both systems harbor detected debris disks in the F200W and F444W…

astro-ph.SR2013

Resolved Imaging of the HR 8799 Debris Disk with Herschel

Brenda C. Matthews, Grant Kennedy, Bruce Sibthorpe +5

We present Herschel far-infrared and submillimeter maps of the debris disk associated with the HR 8799 planetary system. We resolve the outer disk emission at 70, 100, 160 and 250…

astro-ph.CO2024

Atacama Large Aperture Submillimeter Telescope \mbox{(AtLAST)} Science: Probing the Transient and Time-variable Sky

John Orlowski-Scherer, Thomas J. Maccarone, Joe Bright +25

The study of transient and variable events, including novae, active galactic nuclei, and black hole binaries, has historically been a fruitful path for elucidating the evolutionary…

astro-ph.EP2024

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b

Brittany E. Miles, Beth A. Biller, Polychronis Patapis +101

We present the highest fidelity spectrum to date of a planetary-mass object. VHS 1256 b is a 20 M widely separated (8\arcsec, a = 150 au), young, planetary-…

astro-ph.EP2012

Millimeter Emission Structure in the first ALMA Image of the AU Mic Debris Disk

Meredith A. MacGregor, David J. Wilner, Katherine A. Rosenfeld +9

We present 1.3 millimeter ALMA Cycle 0 observations of the edge-on debris disk around the nearby, ~10 Myr-old, M-type star AU Mic. These observations obtain 0.6 arcsec (6 AU) resol…

astro-ph.EP2016

Inner mean-motion resonances with eccentric planets: A possible origin for exozodiacal dust clouds

Virginie Faramaz, Steve Ertel, Mark Booth +2

High levels of dust have been detected in the immediate vicinity of many stars, both young and old. A promising scenario to explain the presence of this short-lived dust is that th…

astro-ph.IM2024

Investing in the Unrivaled Potential of Wide-Separation Sub-Jupiter Exoplanet Detection and Characterisation with JWST -- Strategic Exoplanet Initiatives with HST and JWST White Paper

Aarynn L. Carter, Rachel Bowens-Rubin, Per Calissendorff +15

We advocate for a large scale imaging survey of nearby young moving groups and star-forming regions to directly detect exoplanets over an unexplored range of masses, ages and orbit…

astro-ph.IM2025

Finding New Debris Discs at Sub-millimetre Wavelengths

Mark Booth, Patricia Luppe, Sebastian Marino +9

Debris discs reveal the architectures and dynamical histories of planetary systems. Sub-millimetre observations trace large dust grains within debris discs, revealing their bulk pr…

astro-ph.EP2018

Deep ALMA Search for CO Gas in the HD 95086 Debris Disc

Mark Booth, Luca MatrÃ, Kate Y. L. Su +7

One of the defining properties of debris discs compared to protoplanetary discs used to be their lack of gas, yet small amounts of gas have been found around an increasing number o…