Advisor: Renaud Foy †
8 years, 7 months and counting
8 years
2 years
With the extreme Adaptive Optics SPHERE instrument at the VLT we imaged (in the near-infrared) the transition disk and for the first time planet b in its large disk gap, south of the star.
Keppler+ 2018 Müller+ 2018, A&A
A year later with the integral field instrument MUSE also at the VLT we imaged (in H⍺ at 656 nm) not one but two planets in the large gap, south of the star. (Haffert et al. 2018)
Haffert+ 2019, Nature Astronomy
These planets are forming "in-situ", probably by gravitational instability (of the circumstellar material). Learn more with this PBS/Nova Video from an interview I gave then or click on the image to read one of the press releases.
Using the NACO instrument at the VLT, we observed Luhman 16 AB, the closest brown dwarf pair in polarimetry mode taking advantage of the infrared wavefront sensor to close the adaptive optics loop on the two brown dwarfs themselves separated by ~1-1.5 arcsecond.
We detect a tiny signal of circular polarization on the A component which we interpret as the presense of cloud bands (like Jupiter's).
Millar-Blanchaer, Girard+ 2020, ApJCheck the Caltech Press Release and Video.
or click on the image to read the press release.
JWST is our largest space telescope but its primary mirror only 6.5m across. Moreover when using NIRCam's coronagraphs this the Lyot stop limits that to ~5.2m. Our angular resolution is thus affected but we compensate this loss thanks to the telescope's extreme stability and sensitivity in space. Then we apply all our PSF subtraction and post-processing technique to remove the stellar glare and detect planets 10,000 to 100,000 fainter than the host star.
In this work we were able to detect a strong drop in the spectral energy distribution of planet e between 4.1 and 4.3 µm, the evidence of the presence of Carbone Dioxide in its atmosphere. Click on the image below to access the NASA Press Release.

Girard+ 2022, SPIE is the reference publication for the first light and commissioning of the JWST/NIRCam Coronagraphy mode.
These are refereed papers for which I consider myself a lead author (typically among the first 5 authors). I always prefer to help and provide expertise to impcatful and student-led projects than publish as first author.
(Current projects are on top and older/past ones towards the bottom)
Funded Project Team member, I contribute to calibration and commissioning programs, observation planning, simulations and community engagement
Between 2018 and 2021 I coordinated this challenge to get the community acquainted with Roman CGI data.
With Program PI Sasha Hinkley and a large team we tested and validate the main high contrast modes of JWST.
While spending nearly a thousand nights in the Atacama desert in northern Chile I picked up nightscape photography and even became the 13th ESO Photo Ambassador.
What I truly love is working with creative and talented individuals who inspire me everyday. I also love to be part of big adventures and visit incredible places.