Visiting Scholars

Visiting Scholars

Visitor Period of stay Office Email address Research interests

John Carpenter

1 April 2025 to 3 April 2025 Dr. John Carpenter joined the ALMA Project in September 2015 as the ALMA Observatory Scientist. John received his PhD from the University of Massachusetts-Amherst, and was a James Clerk Maxwell Fellow at the University of Hawaii and an Postdoctoral Scholar at the California Institute of Technology (Caltech). While at Caltech, John conducted research using the Owens Valley Radio Observatory (OVR...

Past Visiting Scholars

Visitor Period of stay Research interests
Youkyung Ko
Department of Physics and Astronomy, Seoul National University, Korea.
16 Nov 2015 to 20 Nov 2015 Globular cluster system of early-type galaxies
Minjin Kim
Korea Astronomy and Space Science Institute (KASI)
11 Nov 2015 to 18 Nov 2015 Coevolution of galaxies and black holes
Sarah Bird
SHAO
29 Oct 2015 to 11 Nov 2015 Milky Way, stellar populations and dynamics
Alain Omont
Emeritus ‘Directeur de Recherche’ at Institut d’Astrophysique de Paris Universitè Pierre et Marie Curie (UPMC) and CNRS
26 Oct 2015 to 30 Oct 2015 High redshift dust and molecules Star formation and evolution of high redshift galaxies and QSOs
Roberto Maiolino
Kavli Institute for Cosmology and the Cavendish Laboratory
26 Oct 2015 to 30 Oct 2015 Observational investigation of galaxy formation and galaxy-black hole coevolution
Chengyuan Li
Purple Mountain Observatory
8 Oct 2015 to 14 Oct 2015 Multiple stellar populations in intermediate-age star clusters in the Magellanic Clouds
Matthias Kühtreiber
Department of Astrophysics, University of Vienna
17 Sep 2015 to 14 Dec 2015 the chemo-dynamical evolution of dwarf galaxies, dark matter and numerical simulations.
Angela Olinto
University of Chicago, KICP
17 Sep 2015 to 2 Oct 2015 Cosmic rays; magnetic fields
Yanfei Jiang
Harvard-Smithsonian CfA
24 Aug 2015 to 26 Aug 2015 Radiation transfer; Numerical simulations
Chin-Fei Lee
ASIAA
23 Jul 2015 to 21 Aug 2015 Star formation and Stellar Evolution; Radio Observations and MHD Numerical Simulations