"Galaxy redsfhit estimation from multi-band images with Deep Learning : strengths and challenges". The thesis will be presented in French (slides in English). For those who would like to attend the defense online, it will also be available on Zoom.
"Dust properties of low surface brightness galaxies and their implications for future large sky surveys" by JUNAIS (National Centre for the Nuclear Research - Astrophysics Division, Warsaw), The cafe-club will take place at 13:00 **in the Mistral room** (2nd floor) >>> UNUSUAL TIME <<< and on the usual AMU virtual room: You can find the […]
The idea is to continue with the format of a round table, with a lively and informal discussion for basic to advanced subjects. This time we will have the presence of Samuel Boissier as main moderators on the discussion, as well as Junais M. and Eloise Bernaud who will also be present to encourage discussion […]
Tuesday each 2/3 weeks to discuss galactic/extra-galactic transients with the perspective of SVOM, Colibri, etc.
Wednedays, 15:00. Informal (short) presentations with coffee Find all informations at this link.
Discussions about extra-galactic transients Latest news (SVOM, LISA, ...) Presentation byNy-Avo : extinction curves in host galaxies of GRBs.
The JWST is revolutionizing our understanding of the early Universe by unveiling a wealth of bright galaxies at z>9 and faint AGNs at z>5. I will present the latest constraints on the overabundance of UV-bright galaxies at z>9, which is 10–100 times higher than galaxy formation models. I will discuss to what extent recent theoretical […]
For our next G.E. Circle ( 15 March - 15h @ Mistral ) we propose to talk about quenching at high redshift. The idea is to continue with the format of a round table, with a lively and informal discussion for basic to advanced subjects. This time we will have the presence of Thibaud Moutard […]
Wavefront architecture of the ELT The ELT Wavefront Control manages the 5 mirrors of the telescope in position and shape and delivers at the interface with the instruments a beam quality compatible with diffraction-limited performance after correction by post-focal AO systems. This is obtained if the spectral distribution of aberrations in the temporal and spatial […]
