Science Team
Science Team
Principal Investigator: Jason Glenn (GSFC)
Deputy Principal Investigator: Margaret Meixner (JPL/Caltech)
Project Scientist: Matt Bradford (JPL/Caltech)
Deputy Project Scientist: Klaus Pontoppidan (JPL/Caltech)
Science Lead: Alexandra Pope (University of Massachusetts)
Deputy Science Lead: Tiffany Kataria (JPL/Caltech)
PRIMA Co-Investigators
  • Lee Armus IPAC/Caltech
  • Jochem Baselmans Netherlands Institute for Space Research, Leiden and Delft University of Technology
  • Cara Battersby University of Connecticut
  • Edwin (Ted) Bergin University of Michigan
  • Alberto Bolatto University of Maryland
  • Denis Burgarella Laboratoire d'Astrophysique de Marseille
  • Laure Ciesla Laboratoire d'Astrophysique de Marseille
  • Ilse Cleeves University of Virginia
  • Anna Di Giorgio INAF, Rome
  • Carlotta Gruppioni INAF OAS, Bologna
  • Thomas Henning MPIA, Heidelberg
  • Brandon Hensley JPL/Caltech
  • Hanae Inami, Provisional Co-I Hiroshima Univeristy, Japan
  • Willem Jellema Netherlands Institute for Space Research, Groningen
  • Oliver Krause MPIA, Heidelberg
  • Elisabeth Mills University of Kansas
  • Arielle Moullet (NRAO)
  • Marc Sauvage CEA/DRF/Irfu/Département d’Astrophysique
  • JD Smith University of Toledo
  • Rachel Somerville Rutgers University & Flatiron Institute
  • Johannes Staguhn JHU/GSFC
PRIMA Science Affiliates

Definition of Role: A Science Affiliate (SA) is an unfunded member of the PRIMA team that is identified by the team to take a specific active role in PRIMA. SAs may serve in a variety of ways to enhance PRIMA's Phase A work (examples below). SAs may be affiliated with an individual sponsoring Co-I for specific scientific contributions or affiliated with the science leadership for broader contributions to PRIMA's implementation or community engagement.

PRIMA intends for the total number of SAs to be modest (~20-30), and that all SAs will be renewed on an annual basis. New SA appointments will be considered on a rolling basis.

Example Activities:

  • SAs may work with individual PRIMA Co-Is to perform simulations, calculations, or other technical work to refine PRIMA's science program and articulate its capabilities.
  • SAs may act as working group (WG) leads and will meet as a group to provide oversight for all WGs. They will help in verifying applications from new working group members and manage WGs as appropriate. WG leads will be responsible for organizing recurring meetings and coordinating the development of community science cases for Volume 2 of the PRIMA GO Science Book.
  • SAs may help plan science enhancement options, citizen science opportunities and/or student collaborations.
  • Andrea Banzatti Texas State University
  • Matthieu Béthermin Observatoire de Strasbourg
  • Henrik Beuther MPIA, Heidelberg
  • Laura Bisigello INAF
  • Médéric Boquien Observatoire de Côte d'Azur
  • Dave Chuss Villanova University
  • Darren Dowell JPL/Caltech
  • Thomas Essinger-Hileman GSFC
  • Eduardo Gonzalez-Alfonso Universidad de Alcalá
  • Al Kogut GFSC
  • Dariusz Lis JPL/Caltech
  • Meredith MacGregor JHU
  • Jed McKinney University of Texas at Austin
  • Seb Oliver University of Sussex
  • Colette Salyk Vassar College
  • Irene Shivaei Centro de Astrobiología, Madrid
  • Thomas Stevenson GSFC