Hunting for Hidden Galaxies at the Universe's Peak Star-Formation Epoch: How Do Galaxies Form, Grow and

Thesis topic details

General information

Organisation

The French Alternative Energies and Atomic Energy Commission (CEA) is a key player in research, development and innovation in four main areas :
• defence and security,
• nuclear energy (fission and fusion),
• technological research for industry,
• fundamental research in the physical sciences and life sciences.

Drawing on its widely acknowledged expertise, and thanks to its 16000 technicians, engineers, researchers and staff, the CEA actively participates in collaborative projects with a large number of academic and industrial partners.

The CEA is established in ten centers spread throughout France
  

Reference

SL-DRF-27-0094  

Direction

DRF

Thesis topic details

Category

Corpuscular physics and outer space

Thesis topics

Hunting for Hidden Galaxies at the Universe's Peak Star-Formation Epoch: How Do Galaxies Form, Grow and Die in the Early Universe?

Contract

Thèse

Job description

Nearly 10 billion years ago, the Universe was forming stars at its peak rate. Galaxies were assembling, growing and being transformed at a pace we no longer see today. Hidden in that era is a rare gem: a massive group of galaxies at redshift 1.85, caught in the act of building itself around a starbursting central galaxy.
By a stroke of luck, the light emitted by hydrogen atoms in this group (the Halpha line, a direct tracer of newborn stars) is shifted into exactly the right wavelength for one of JWST's narrow-band filters. Our accepted JWST program uses this to produce a panoramic, sharply resolved map of where stars are forming across the whole group. We expect to detect around 100 star-forming galaxies, including dwarfs about a hundred times less massive than the Milky Way, at a time when such objects are essentially unexplored.
The PhD student will analyse these brand-new data and tackle three open questions:
1) How many small galaxies does a group hold? Simulations of cold dark matter predict many more small satellites than we observe nearby. Counting them in a distant group offers a new test of this 'Missing Satellite Problem' and of alternative dark-matter models.
2) How do galaxies build themselves? JWST can resolve giant star-forming clumps inside galaxies, making it possible to measure how often they form and how they shape galaxy growth.
3) How do galaxies get switched off? The student will search for signs of ram-pressure stripping, the removal of a galaxy's gas as it plunges through the hot intragroup medium, at the highest redshift ever probed.
The student will work with JWST imaging and spectroscopy, learn state-of-the-art techniques in astronomical data analysis, and confront the results with cosmological simulations. No prior JWST experience is needed. Curiosity, rigor, programming skills (Python is ideal) and a taste for big questions matter most.
The student will join a dynamic research team in Paris, one of Europe's leading centres for extragalactic astrophysics, with opportunities to collaborate internationally, attend conferences, and present their own discoveries.

University / doctoral school

Astronomie et Astrophysique d’Île de France (ED A&A)
Paris-Saclay

Thesis topic location

Site

Saclay

Requester

Position start date

01/10/2027

Person to be contacted by the applicant

DADDI Emanuele edaddi@cea.fr
CEA
DRF/IRFU/DAP/LCEG
Orme des Merisiers

Tutor / Responsible thesis director

DADDI Emanuele edaddi@cea.fr
CEA
DRF/IRFU/DAP/LCEG
Orme des Merisiers

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