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Science Highlight

 

 

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Large ALMA Programs

Large Programs are designed to address strategic scientific issues that will lead to a major advance or breakthrough in the field. The Large Program proposal teams produce high level data products and documentation which are made available to the scientific community within one year after the final delivery of calibrated data. Large Programs are distinguished from Regular Proposals in the following ways:

  • They are programs with an estimated execution time of greater than 50 hours on the 12-m Array (with or without accompanying ACA time) or 150 hours on the ACA in stand-alone mode.
  • They are designed to be coherent science projects that are not reproducible by a combination of Regular Proposals. 
  • Investigators must deliver high level data products and relevant documentation in a manner consistent with the management plan of their proposal.

 

The following table contains the full list of ALMA Large Programs, as well as links to the data products delivered by the teams:

 

Nickname       PIDs

PIDs

Cycle

Title

Primary Investigator - Institution

Primary Article

Team’s Site

Data Deliveries

Cosmology and High Redshift Universe

ASPECS

2016.1.00324.L

4

ASPECS: The ALMA SPECtral line Survey in the UDL - An ALMA Large Program

Fabian Walter / MPIA Heidelberg

link

link

 

ALPINE

2017.1.00428.L

5

ALPINE: The ALMA Large Program to INvestigate CII at Early Times

Olivier Le Fèvre / Laboratoire D’Astrophysique de Marseille

 

 

 

 

2018.1.00035.L

6

ALMA Lensing Cluster Survey

Kotaro Kohno / University of Tokyo

 

 

 

Galaxies and Galactic Nuclei

PHANGS

2017.1.00886.L

5

100,000 Molecular Clouds Across the Main Sequence: GMCs as the Drivers of Galaxy Evolution

Eva Schinnerer / MPIA Heidelberg

 

link

 

ALCHEMI

2017.1.00161.L

5

ALCHEMi: the ALMA Comprehensive High-resolution Extragalactic Molecular Inventory

Sergio Martin / IRAM

 

 

 

ISM, Star Formation, and Astrochemistry

ALMA-IMF

2017.1.01355.L

5

ALMA_IMF: ALMA transforms our view of the origin of stellar masses

Frédérique Motte / CNRS

 

 

 

FAUST

2018.1.01205.L

6

Fifty AU Study of the chemistry in the disk/envelope system of Solar-like protostars (FAUST)

Satoshi Yamamoto / Tokyo University

 

 

 

Circumstellar Disks, Exoplanets, and the Solar System

DSHARP

2016.1.00484.L

4

Small-Scale Substructures in Protoplanetary Disks

Sean Andrews / CfA Harvard

 

 

link

 

2018.1.01055.L

6

The Chemistry of Planet Formation

Karin Oberg / Harvard

 

 

 

Stellar Evolution and the Sun

ATOMIUM

2018.1.00659.L

6

ATOMIUM: ALMA Tracing the Origins of Molecular In dUst-forming oxygen-rich M-type stars

Leen Decin / K.U. Leuven