Jamal Chafi

Jamal Chafi
Verified
Jamal verified their affiliation via an institutional email.
Verified
Jamal verified their affiliation via an institutional email.
  • Doctor
  • Research Associate at Cadi Ayyad University

About

7
Publications
841
Reads
How we measure 'reads'
A 'read' is counted each time someone views a publication summary (such as the title, abstract, and list of authors), clicks on a figure, or views or downloads the full-text. Learn more
9
Citations
Introduction
I am a PhD student in Physics and Astrophysics at Cadi Ayyad University, specializing in direct imaging of exoplanets. I am a coronagraph designer in the Habitable Worlds Observatory (HWO) project using the Interferometric Apodization by Homothety (IAH) technique. As part of the Coronagraph Design sub-teams, I focus on creating new coronagraph designs for Exploratory Analytical Case 1 (EAC1), enhancing starlight suppression for future exoplanet observations.
Current institution
Cadi Ayyad University
Current position
  • Research Associate
Education
February 2021 - November 2024
Université Cadi Ayyad, Marrakech
Field of study
  • Astrophysique

Publications

Publications (7)
Article
Full-text available
This work presents the results of experimental laboratory tests on the apodization of circular and rectangular apertures using the Interferometric Apodization by Homothety (IAH) technique. The IAH approach involves splitting the amplitude of the instrumental PSF into two equal parts. One of the two produced PSFs undergoes a homothety to change its...
Preprint
This study is focused on the very high dynamic imaging field, specifically the direct observation of exoplanetary systems. The coronagraph is an essential technique for suppressing the star's light, making it possible to detect an exoplanet with a very weak luminosity compared to its host star. Apodization improves the rejection of the coronagraph,...
Article
This study is focused on the very high dynamic imaging field, specifically the direct observation of exoplanetary systems. The coronagraph is an essential technique for suppressing the star’s light, making it possible to detect an exoplanet with a very weak luminosity compared to its host star. Apodization improves the rejection of the coronagraph,...
Preprint
Full-text available
Atmospheric optical parameters play a significant role in high angular resolution and adaptive optics. The single star SCIDAR (hereafter SSS) is one of the methods by which we obtain the vertical profile of these parameters such as the refractive index structural constant C n ² . This technique is based on the study of the correlation functions of...
Poster
Full-text available
Principe de fonctionnement de coronographe

Network

Cited By