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Erratum: “Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm” (2023, ApJ, 942, 4 )

The Astrophysical journal, 2023-04, Vol.947 (2), p.91

2023

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Measuring the density structure of an accretion hot spot

Nature (London), 2021-09, Vol.597 (7874), p.41-44

2021

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Using Multiwavelength Variability to Explore the Connection among X-Ray Emission, the Far-ultraviolet H2 Bump, and Accretion in T Tauri Stars

The Astrophysical journal, 2019-05, Vol.876 (2)

2019

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Addendum: “Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling with ALMA” (2023, ApJ, 944, 66)

The Astrophysical journal, 2023-09, Vol.954 (2), p.222

2023

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RW Aur A: SpeX Spectral Evidence for Differentiated Planetesimal Formation, Migration, and Destruction in an ∼3 Myr Old Excited CTTS System

The Astrophysical journal, 2022-04, Vol.928 (2), p.189

2022

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DETECTIONS OF TRANS-NEPTUNIAN ICE IN PROTOPLANETARY DISKS

The Astrophysical journal, 2015-01, Vol.799 (2), p.162

2015

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Probing CO and N2 Snow Surfaces in Protoplanetary Disks with N2H+ Emission

The Astrophysical journal, 2019-09, Vol.882 (2)

2019

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A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a

The Astrophysical journal, 2008, Vol.689 (2), p.L145-L148

2008

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Erratum: “Far-infrared to Millimeter Data of Protoplanetary Disks: Dust Growth in the Taurus, Ophiuchus, and Chamaeleon I Star-forming Regions” (2017, ApJ, 849, 63)

The Astrophysical journal, 2020-09, Vol.901 (1), p.88

2020

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Modeling protoplanetary disk SEDs with artificial neural networks

Astronomy and astrophysics (Berlin), 2020-10, Vol.642

2020

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PENELLOPE: The ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES): I. Survey presentation and accretion properties of Orion OB1 and σ -Orionis

Astronomy and astrophysics (Berlin), 2021-06, Vol.650, p.A196

2021

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A dusty streamer infalling onto the disk of a class I protostar

Astronomy and astrophysics (Berlin), 2024-02, Vol.682

2024

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A Model of the C iv λ λ1548, 1550 Doublet Line in T Tauri Stars

The Astrophysical journal, 2024-11, Vol.975 (2), p.193

2024

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A Model of the C ivλλ1548, 1550 Doublet Line in T Tauri Stars

The Astrophysical journal, 2024-11, Vol.975 (2), p.193

2024

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Sparse aperture masking interferometry survey of transitional discs

Astronomy and astrophysics (Berlin), 2016, Vol.595

2016

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Probing CO and N 2 Snow Surfaces in Protoplanetary Disks with N 2 H + Emission

The Astrophysical journal, 2019-09, Vol.882 (2), p.160

2019

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Herschel Observations of Protoplanetary Disks in Lynds 1641 Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA

The Astrophysical journal, 2018-08, Vol.863 (1)

2018

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ERRATUM: “THE DISK POPULATION OF THE TAURUS STAR-FORMING REGION” (2010, ApJS, 186, 111)

The Astrophysical journal. Supplement series, 2010-08, Vol.189 (2), p.353-354

2010

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Far-infrared to Millimeter Data of Protoplanetary Disks: Dust Growth in the Taurus, Ophiuchus, and Chamaeleon I Star-forming Regions ∗ Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA

The Astrophysical journal, 2017-10, Vol.849 (1)

2017

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PROBING DYNAMICAL PROCESSES IN THE PLANET-FORMING REGION WITH DUST MINERALOGY

The Astrophysical journal, 2012, Vol.759 (1)

2012

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THE DISK POPULATION OF THE TAURUS STAR-FORMING REGION

The Astrophysical journal. Supplement series, 2010-01, Vol.186 (1)

2010

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DM ORI: A YOUNG STAR OCCULTED BY A DISTURBANCE IN ITS PROTOPLANETARY DISK

The Astrophysical journal, 2016-11, Vol.831 (1)

2016

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MID-INFRARED SPECTRA OF TRANSITIONAL DISKS IN THE CHAMAELEON I CLOUD

The Astrophysical journal, 2009-08, Vol.700 (2)

2009

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Erratum: “Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm” (2023, ApJ, 942, 4 )

Measuring the density structure of an accretion hot spot

Using Multiwavelength Variability to Explore the Connection among X-Ray Emission, the Far-ultraviolet H2 Bump, and Accretion in T Tauri Stars

Addendum: “Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling with ALMA” (2023, ApJ, 944, 66)

RW Aur A: SpeX Spectral Evidence for Differentiated Planetesimal Formation, Migration, and Destruction in an ∼3 Myr Old Excited CTTS System

DETECTIONS OF TRANS-NEPTUNIAN ICE IN PROTOPLANETARY DISKS

Probing CO and N2 Snow Surfaces in Protoplanetary Disks with N2H+ Emission

A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a

Erratum: “Far-infrared to Millimeter Data of Protoplanetary Disks: Dust Growth in the Taurus, Ophiuchus, and Chamaeleon I Star-forming Regions” (2017, ApJ, 849, 63)

Modeling protoplanetary disk SEDs with artificial neural networks

PENELLOPE: The ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES): I. Survey presentation and accretion properties of Orion OB1 and σ -Orionis

A dusty streamer infalling onto the disk of a class I protostar

A Model of the C iv λ λ1548, 1550 Doublet Line in T Tauri Stars

A Model of the C ivλλ1548, 1550 Doublet Line in T Tauri Stars

Sparse aperture masking interferometry survey of transitional discs

A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. III. Optical Spectra Based on observations collected at the European Southern Observatory under ESO program 106.20Z8

Lyα Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems Based on observations collected at the European Southern Observatory under ESO program 106.20Z8

Probing CO and N 2 Snow Surfaces in Protoplanetary Disks with N 2 H + Emission

Herschel Observations of Protoplanetary Disks in Lynds 1641 Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA

ERRATUM: “THE DISK POPULATION OF THE TAURUS STAR-FORMING REGION” (2010, ApJS, 186, 111)

Far-infrared to Millimeter Data of Protoplanetary Disks: Dust Growth in the Taurus, Ophiuchus, and Chamaeleon I Star-forming Regions ∗ Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA

PROBING DYNAMICAL PROCESSES IN THE PLANET-FORMING REGION WITH DUST MINERALOGY

THE DISK POPULATION OF THE TAURUS STAR-FORMING REGION

DM ORI: A YOUNG STAR OCCULTED BY A DISTURBANCE IN ITS PROTOPLANETARY DISK

MID-INFRARED SPECTRA OF TRANSITIONAL DISKS IN THE CHAMAELEON I CLOUD

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