activity
20062023
most citedPlanet formation around stars of various masses: The snow line and the frequency of giant planets

499 citations · 6.2k across the 126 of their papers we have counts for

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90 papers · 1 filter

astro-ph.EP2023

A planetary collision afterglow and transit of the resultant debris cloud

Matthew Kenworthy, Simon Lock, Grant Kennedy +19

Planets grow in rotating disks of dust and gas around forming stars, some of which can subsequently collide in giant impacts after the gas component is removed from the disk. Monit…

astro-ph.EP2023★ 15 cited

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.EP2023★ 5 cited

ALMA and Keck analysis of Fomalhaut field sources: JWST's Great Dust Cloud is a background object

Grant M. Kennedy, Joshua B. Lovell, Paul Kalas +1

At 7.7 pc, the A-type star Fomalhaut hosts a bright debris disk with multiple radial components. The disk is eccentric and misaligned, strongly suggesting that it is sculpted by in…

astro-ph.EP2023★ 13 cited

Morphology of the gas-rich debris disk around HD 121617 with SPHERE observations in polarized light

Clément Perrot, Johan Olofsson, Quentin Kral +7

Debris disks are the signposts of collisionally eroding planetesimal circumstellar belts, whose study can put important constraints on the structure of extrasolar planetary systems…

astro-ph.EP2022★ 27 cited

ISPY-NACO Imaging Survey for Planets around Young stars. The demographics of forming planets embedded in protoplanetary disks

Gabriele Cugno, Timothy D. Pearce, Ralf Launhardt +11

We present the statistical analysis of a subsample of 45 young stars surrounded by protoplanetary disks (PPDs). This is the largest imaging survey uniquely focused on PPDs to date.…

astro-ph.EP2022★ 9 cited

High resolution ALMA and HST imaging of CrB: a broad debris disc around a post-main sequence star with low-mass companions

J. B. Lovell, M. C. Wyatt, P. Kalas +6

CrB is a Gyr old K1 sub-giant star, with an eccentric exo-Jupiter at au and a debris disc at tens of au. We present ALMA Band 6 (mm) and HST sca…

astro-ph.EP2022★ 17 cited

RVSPY -- Radial Velocity Survey for Planets around Young Stars. Target characterization and high-cadence survey

O. Zakhozhay, R. Launhardt, A. Mueller +15

We introduce our Radial Velocity Survey for Planets around Young stars (RVSPY), characterise our target stars, and search for substellar companions at orbital separations smaller t…

astro-ph.EP2022★ 176 cited

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.EP2022

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 t…

astro-ph.EP2022★ 79 cited

Direct discovery of the inner exoplanet in the HD206893 system. Evidence for deuterium burning in a planetary-mass companion

S. Hinkley, S. Lacour, G. -D. Marleau +110

Long term precise radial velocity (RV) monitoring of the nearby star HD206893, as well as anomalies in the system proper motion, have suggested the presence of an additional, inner…

astro-ph.EP2022★ 51 cited

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.EP2022★ 17 cited

A Star-sized Impact-Produced Dust Clump in the Terrestrial Zone of the HD 166191 System

Kate Y. L. Su, Grant M. Kennedy, Everett Schlawin +2

We report on five years of 3-5 micron photometry measurements obtained by warm Spitzer to track the dust debris emission in the terrestrial zone of HD 166191 in combination with si…

astro-ph.EP2022★ 6 cited

ALMA's view of the M-dwarf GSC 07396-00759's edge-on debris disc: AU Mic's coeval twin

Patrick F. Cronin-Coltsmann, Grant M. Kennedy, Christian Adam +7

We present new ALMA Band 7 observations of the edge-on debris disc around the M1V star GSC 07396-00759. At ~20 Myr old and in the beta Pictoris Moving Group along with AU Mic, GSC…

astro-ph.EP2022★ 21 cited

Circumbinary disk evolution in the presence of an outer companion star

Rebecca G. Martin, Stephen Lepp, Stephen H. Lubow +3

We consider a hierarchical triple system consisting of an inner eccentric binary with an outer companion. A highly misaligned circumbinary disk around the inner binary is subject t…

astro-ph.EP2022★ 61 cited

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.EP2021★ 24 cited

Carbon monoxide gas produced by a giant impact in the inner region of a young system

Tajana Schneiderman, Luca Matrà, Alan P. Jackson +7

Models of terrestrial planet formation predict that the final stages of planetary assembly, lasting tens of millions of years beyond the dispersal of young protoplanetary disks, ar…

astro-ph.EP2021★ 10 cited

Four new PLanetesimals Around TYpical and Pre-main seqUence Stars (PLATYPUS) Debris Discs at 8.8mm

Brodie J. Norfolk, Sarah T. Maddison, Jonathan P. Marshall +9

Millimetre continuum observations of debris discs can provide insights into the physical and dynamical properties of the unseen planetesimals that these discs host. The material pr…

astro-ph.EP2021

The formation of planetary systems with SPICA

I. Kamp, M. Honda, H. Nomura +38

In this era of spatially resolved observations of planet forming disks with ALMA and large ground-based telescopes such as the VLT, Keck and Subaru, we still lack statistically rel…

astro-ph.EP2021★ 37 cited

High resolution ALMA and HST images of q Eri: an asymmetric debris disc with an eccentric Jupiter

J. B. Lovell, S. Marino, M. C. Wyatt +10

We present \textit{ALMA} 1.3 mm and 0.86 mm observations of the nearby (17.34 pc) F9V star q1 Eri (HD 10647, HR 506). This system, with age Gyr, hosts a au ra…

astro-ph.EP2021★ 11 cited

ALMA imaging of the M-dwarf Fomalhaut C's debris disc

Patrick F. Cronin-Coltsmann, Grant M. Kennedy, Paul Kalas +9

Fomalhaut C (LP 876-10) is a low mass M4V star in the intriguing Fomalhaut triple system and, like Fomalhaut A, possesses a debris disc. It is one of very few nearby M-dwarfs known…

astro-ph.EP2021★ 15 cited

Discovery of an Edge-on Circumstellar Debris Disk Around BD+45598: a Newly Identifed Member of the Pictoris Moving Group

Sasha Hinkley, Elisabeth C. Matthews, Charlène Lefevre +24

We report the discovery of a circumstellar debris disk viewed nearly edge-on and associated with the young, K1 star BD+45598 using high-contrast imaging at 2.2m obtain…

astro-ph.EP2021★ 13 cited

The HOSTS survey: evidence for an extended dust disk and constraints on the presence of giant planets in the Habitable Zone of Leo

D. Defrère, P. M. Hinz, G. M. Kennedy +38

The young (50-400 Myr) A3V star Leo is a primary target to study the formation history and evolution of extrasolar planetary systems as one of the few stars with known hot ($\s…

astro-ph.EP2021★ 40 cited

A Occurrence Rate of Debris Discs around F stars in the Pic Moving Group

Nicole Pawellek, Mark Wyatt, Luca Matrà +2

Only 20\% of old field stars have detectable debris discs, leaving open the question of what disc, if any, is present around the remaining 80\%. Young moving groups allow to probe…

astro-ph.EP2020★ 15 cited

Rapid CO gas dispersal from NO Lup's class III circumstellar disc

J. B. Lovell, G. M. Kennedy, S. Marino +9

We observed the K7 class III star NO Lup in an ALMA survey of the 1-3 Myr Lupus association and detected circumstellar dust and CO gas. Here we show that the J = 3-2 CO emission is…