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exoALMA: a search for the youngest exoplanets

 

 

Peak intensity of CO emission from the fifteen sources surveyed by exoALMA.

Peak intensity of CO emission from the fifteen sources surveyed by exoALMA.

 

Project Overview

exoALMA is conducting a comprehensive planet hunting campaign in the sub-mm regime — the first to focus on still-forming planets. By leveraging the unparalleled spatial and spectral resolution of ALMA, the exoALMA program searches for still-forming planets embedded in their parental protoplanetary disks through their influence on the dynamics of the surrounding gas.

exoALMA focuses on 15 sources, studying some of the deepest and most sensitive images of these planet-forming nurseries taken to date. These observations are transforming our understanding of how planetary systems form and provide constraints on the mass distribution within these systems, mechanisms that concentrate grains into rings, and the 3D velocity structures of disks.

The exoALMA project is further described at https://www.exoalma.com/, including pages for Data, Publications, and Software.

 

Project Summary Table

 

Project code Title PIs
2021.1.01123.L exoALMA: a search for the youngest exoplanets Richard Teague (PI); Myriam Benisty, Stefano Facchini, Misato Fukagawa, Christophe Pinte (co-PIs)

 

Deliveries

The delivered data products are:

  • Calibration and imaging scripts
  • Fiducial line images
  • Measurement Sets (currently stored at NRAO while transfer to Dataverse for a DOI is completed)
  • High angular resolution line images
  • Continuum images
  • High surface brightness sensitivity line images

All exoALMA data products are made public through the exoALMA Dataverse. If you want the raw data, use the ALMA Archive and search for project ID 2021.1.01123.L. When using any of the data, please ensure to reference exoALMA I and exoALMA II. For direct links to commonly used products and paper-specific sub-repositories, see: https://www.exoalma.com/data.

 

PIs

 

Name Affiliation Country
Richard Teague (PI) Massachusetts Institute of Technology US
Myriam Benisty (co-PI) Max Planck Institute for Astronomy Germany
Stefano Facchini (co-PI) University of Milan Italy
Misato Fukagawa (co-PI) National Astronomical Observatory of Japan Japan
Christophe Pinte (co-PI) Univ. Grenoble Alpes France

 

Co-Is

Full consortium list (also maintained at https://www.exoalma.com/team):

Name Affiliation Country
Sean Andrews CfA Harvard US
Jaehan Bae University of Florida US
Marcelo Barraza Massachusetts Institute of Technology US
Gianni Cataldi National Astronomical Observatory of Japan Japan

Valentin Christiaens

Instituut voor Sterrenkunde Belgium

Nicolás Cuello

Univ. Grenoble Alpes France

Pietro Curone

Universidad de Chile Chile

Ian Czekala

Penn State US

Gaspard Duchene

UC Berkeley US

Daniele Fasano

Max Planck Institute for Astronomy Germany

Mario Flock

Max Planck Institute for Astronomy Germany

Maria Galloway-Sprietsma

University of Florida  US

Charlie Gardner

Rice University US

Himanshi Garg

Monash University Australia

Cassandra Hall

The University of Georgia

US

Iain Hammond

Monash University

Australia

Caitlyn Hardiman

Monash University Australia

Jun Hashimoto

ASIAA National Taiwan University  Taiwan

Tom Hilder

Monash University

Australia

Jane Huang

Columbia University

US

Kazuhiro Kanagawa

Ibaraki University 

Japan

John Ilee

University of Leeds UK

Andrea Isella

Rice University  US

Andrés Izquierdo

Leiden University The Netherlands

Geoffroy Lesur

Univ. Grenoble Alpes France

Giuseppe Lodato

University of Milan Italy

Cristiano Longarini

University of Milan Italy

Ryan Loomis

NRAO US

Francois Menard

Univ. Grenoble Alpes France

Munetake Momose

Ibaraki University  Japan

Ryuta Orihara

Ibaraki University  Japan

Daniel Price

Monash University

Australia

Giovanni Rosotti

University of Milan Italy

Jochen Stadler

Univ. Grenoble Alpes France

Jason Terry

University of Oxford UK

Leonardo Testi

University of Bologna Italy

Leon Trapman

University of Wisconsin at Madison US

Takashi Tsukagoshi

National Astronomical Observatory of Japan Japan

Hsi-Wei Yen

ASIAA National Taiwan University Taiwan

Gaylor Wafflard-Fernandez

Univ. Grenoble Alpes France

David Wilner

CfA Harvard US

Andrew Winter

Max Planck Institute for Astronomy Germany

Lisa Wölfer

Massachusetts Institute of Technology US

Tomohiro Yoshida

National Astronomical Observatory of Japan

Japan

Brianna Zawadzki

Wesleyan University US

 

Publications

The exoALMA papers are published in the Astrophysical Journal Letters exoALMA Focus Issue. For the most up-to-date list and the paper-by-paper summaries, use: https://www.exoalma.com/publications.

Paper Title Lead author ADS / journal
exoALMA I Science Goals, Project Design and Data Products Teague et al. ADS
exoALMA II Data Calibration and Imaging Pipeline Loomis et al. ADS
exoALMA III Line-intensity Modeling and System Property Extraction from Protoplanetary Disks Izquierdo et al. ADS
exoALMA IV Substructures, Asymmetries, and the Faint Outer Disk in Continuum Emission Curone et al. ADS
exoALMA V Gaseous Emission Surfaces and Temperature Structures Galloway-Sprietsma et al. ADS
exoALMA VI Rotating under Pressure: Rotation Curves, Azimuthal Velocity Substructures and Pressure Variations Stadler et al. ADS
exoALMA VII Benchmarking Hydrodynamics and Radiative Transfer Codes Bae et al. ADS
exoALMA VIII Probabilistic Moment Maps and Data Products Using Nonparametric Linear Models Hilder et al. ADS
exoALMA IX Regularized Maximum Likelihood Imaging of Non-Keplerian Features Zawadzki et al. ADS
exoALMA X Channel Maps Reveal Complex 12CO Abundance Distributions and a Variety of Kinematic Structures with Evidence for Embedded Planets Pinte et al. ADS
exoALMA XI ALMA Observations and Hydrodynamic Models of LkCa 15: Implications for Planetary Mass Companions in the Dust Continuum Cavity Gardener et al. ADS
exoALMA XII Weighing and Sizing exoALMA Disks with Rotation Curve Modeling Longarini et al. ADS
exoALMA XIII Gas Masses from N2H+ and C18O: A Comparison of Protoplanetary Gas Disk Mass Measurement Techniques Trapman et al. ADS
exoALMA XIV Gas Surface Densities in the RXJ1604.3-2130 A Disk from Pressure-Broadened CO Line Wings Yoshida et al. ADS
exoALMA XV Interpreting the Height of CO Emission Layer Rosotti et al. ADS
exoALMA XVI Predicting Signatures of Large-Scale Turbulence in Protoplanetary Disks Barraza-Alfaro et al. ADS
exoALMA XVII Characterizing the Gas Dynamics around Dust Asymmetries Wölfer et al. ADS
exoALMA XVIII Interpreting Large Scale Kinematic Structures as Moderate Warping Winter et al. ADS
exoALMA XIX Confirmation of Non-thermal Line Broadening in the DM Tau Protoplanetary Disk Hardiman et al. Journal

 

Software

The exoALMA software page is maintained at https://www.exoalma.com/software. A selection of tools (with links) is listed below.

Much of the calibration and imaging builds on scripts developed for DSHARP and MAPS; the final exoALMA scripts are included with the first data release (see the Data page).

 

Funding

Funding acknowledgements are maintained at https://www.exoalma.com/funding.

  • Dust Busters: A Marie SkĹ‚odowska Curie RISE action funded by the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 823823).
  • PROTOPLANETS ERC: ERC under EU Horizon 2020 (PROTOPLANETS), grant agreement No. 101002188.
  • UNVEIL ERC: ERC UNVEIL, 101076613 (standard EU/ERC disclaimer applies).
  • North American ALMA Science Center: funds supporting the December 2022 workshop at Endicott House; extensive computing resources for calibration and imaging; support for ApJL publication.
  • The Australian Research Council: FT170100040, DP180104235, DP220103767, DP240103290.
  • The University of Leeds: computing resources for imaging and analysis.
  • DiscEvol ERC: ERC DiscEvol, 101039651 (standard EU/ERC disclaimer applies).