Makidon Lab Operations in Wake of Covid-19
A message from the lab on operations and COVID-19.
A message from the lab on operations and COVID-19.
From January 4th-8th, lab members and collaborators attended the 235th meeting of the American Astronomical Society held in Honolulu, Hawaii.
In late October, a subset of the Makidon lab group set out to Tokyo to attend the “Spirit of Lyot” conference. Happening only every 3-5 years, this conference brings together everybody working in high-contrast imaging, sharing their work in the spirit of Bernard Lyot, the inventor of the coronagraph.
August 11- 15, lab members attended the 2019 SPIE Optics + Photonics conference in San Diego.
The optics lab takes a trip to Seattle, WA to present work on James Webb Space Telescope and Apodized Pupil Lyot Coronagraph designs.
From June 10th to June 15th, the lab team attended the SPIE conference in Austin-Texas to present the latest results it obtained on various on-going experiments.
The demanding requirements for HiCAT drives continual innovation. The precise optics work best in a controlled, enclosed area which has to be taken into account when designing the chamber.
Recently on HiCAT, we obtained a very first dark hole with a broadband light source, combining a segmented aperture, a coronagraph (Apodized Pupil Lyot Coronagraph or APLC), and wavefront control (the Speckle Nulling method, now running on demand in any configuration).
Last week, Jean-François Sauvage (from the Office National d’Etudes et de Recherches Aérospatiales and the Laboratoire d’Astrophysique de Marseille) has been invited by STScI to come to the Makidon Lab to implement and test the COFFEE wavefront sensor on HiCAT data.
For a couple of years now, our group had been doing really good work in developing first-class coronagraph technology and wavefront sensing techniques for segmented apertures. During this process, one of the focus points of the work is to create a concise python package which controls the HiCAT testbed and its environment and which would eventually be ready to be freely shared for implementation on other high-contrast testbeds.
Take a deeper look into how PASTIS is used for sensitivity analysis of segmented telescopes.
Out with the old, in with the new. JOST got a new camera that is brand-spanking-new!
Update on our second deformable mirror.
The PASTIS model provides a fast way to compute the contrast in the dark hole generated by a coronagraph, and affected by local errors on the segments. In this post, we introduce our very first results using this model and compare them with the outputs of a traditional end-to-end simulation.
For more information about the Russell B. Makidon Optics Laboratory, please contact Rémi Soummer.