Marshall Perrin: I develop and employ advanced instrumentation for imaging planets and disks around other stars, in particular making extensive use of infrared integral field spectroscopy and imaging polarimetry. I have been a part of the Gemini Planet Imager team since the project's inception over a decade ago, and these days I co-lead GPI's Data Analysis & Data Pipeline team. I carry out observations of nearby circumstellar disks using HST, GPI, and other facilities, and collaborate in the development of our lab testbeds for high contrast and wavefront control.
Dean Hines: I use ultraviolet, optical and infrared imaging, spectropolarimetry and spectroscopy, to investigate active galaxies, quasars, post-main-sequence stars, and the formation and evolution of planetary systems including the Solar System. My research has a particular emphasis on polarimetry and high-contrast imaging of these astrophysical phenomenon. I am a member of the HST/NICMOS and Spitzer/MIPS instrument and science teams, and the JWST/MIRI science and the MIRI Instrument Team Lead at STScI. I am also the PI for the Polarimetry Experiment for Zodiacal Dust, and the Deputy PI for the EXCEDE mission, which is a proposed dedicated coronagraphic imaging polarimetry space telescope designed to investigate the environments of nearby stars.
Laurent Pueyo: High contrast imaging of nearby stars opens new avenues to map regions of the planetary formation phase-space yet unexplored with indirect methods. This technique is also the most promising to search for biomarkers in the atmosphere of earth-like planets in order to eventually address the fascinating question: “Are we alone?” Such observations are however quite challenging: they rely on detecting sources fainter than their host stars by factors ranging from 105 − 107 for young gas giants, to 1010 for earth analogs. I investigate a broad range of problems aimed at facilitating and carrying out direct imaging exo-planetary science. More specifically, I am currently working on:
[a.] High-contrast imaging instrumentation to prepare the ELT/post-JWST era, with long term goals aimed at capturing in-situ planetary formation phenomena and probing for biomarkers in the atmosphere of earth analogs.
[b.] Direct imaging surveys with today’s state of the art facilities, aimed at revealing a broader range of planetary systems, unveiling their formation history and exploring their atmospheric compositions
Charles Lajoie: My work focuses on preparing for the on-orbit alignment of the James Webb Space Telescope. In order to prepare for such a complex task, we will use JOST (James Webb Space Telescope Optical Simulator Testbed), a three-lens transmissive model of JWST that includes a segmented deformable mirror, to exercise the software that will be used to commission JWST. JOST will allow us to become intimately familiar with various steps of the JWST commissioning process and develop contingency strategies for aligning it. I also work on simulations of JWST coronagraphic observations and methods for optimizing coronagraphic performance.
STScI projects: ALICE, HICAT.
Johan Mazoyer: I am interested in the imaging and study of the close vicinity of young stars, in which often hide debris disks and exoplanets. Both in simulation and experimentally on test beds, I develop wavefront control techniques which, associated to coronagraphs, achieve high contrast imaging in broad spectral bands. I also use image processing methods to detect and analyze circumstellar debris disks.
JHU Graduate Students
Elena Gofas Salas