Rubin LSST-France, APC Paris, 27-29/11/2024

Session

Plenary

27 nov. 2024, 14:00

Amphithéâtre Pierre Gilles de Gennes (sous-sol) (APC)

Présidents de session

Plenary: General updates

• Cyrille Doux (LPSC)

Plenary: Invited talks

• Cyrille Doux (LPSC)

Plenary: General updates

• Cyrille Doux (LPSC)

Plenary: Invited/flash talks

• Cyrille Doux (LPSC)

Plenary: LSST quizz and ComCam bubbles

• Il n'a pas de président de session pour ce bloc

Plenary: Final remarks

• Il n'a pas de président de session pour ce bloc

15. Welcome

Cyrille Doux (LPSC)

27/11/2024 14:00

16. News from Rubin and DESC

Dr Johan Bregeon (IN2P3 LSPC)

27/11/2024 14:10

17. EDIM

Clara Déplantes, Marina Ricci

27/11/2024 14:30

18. LSST France communication

Dr Johan Bregeon (IN2P3 LSPC)

27/11/2024 14:50

19. Computing

Fabio Hernandez (CC-IN2P3)

27/11/2024 15:10

30. Simons Observatory: status update and synergies with LSST

Ema TSANG KING SANG (APC-CNRS), Simon Biquard (APC / CNRS)

27/11/2024 15:30

The Simons Observatory (SO) is a new cosmic microwave background (CMB) experiment, located on Cerro Toco in Chile, that began observing in 2024. SO plans to measure the temperature and polarization variations in the CMB across six frequency bands, spanning 27 to 280 GHz. The initial setup includes three small-aperture (0.5-meter) telescopes (SATs) and one large-aperture (6-meter) telescope...

23. Camera filter exchange system

Alexandre Boucaud (APC / IN2P3), Eric AUBOURG (APC), Pierre Antilogus (LPNHE)

27/11/2024 16:30

21. Commissioning plan focal

Dr Johan Bregeon (IN2P3 LSPC), Thibault Guillemin (LAPP), Yassine Faris (LPNHE)

27/11/2024 16:50

22. AuxTel

Jérémy Neveu (LPNHE), Dr Sylvie Dagoret (IJCLab), marc moniez (LAL-IN2P3)

27/11/2024 17:10

14. Tomographic study of the anomalous cosmic dipole with LSST

Roya Mohayaee (Institut d'Astrophysique de Paris/Sorbonne université)

27/11/2024 17:30

The recent data from high redshift Universe demonstrates that our velocity with respect to distant sources, for example quasars and radio galaxies at redshifts of more than one,
is at least twice as large as our velocity with respect to the rest frame of cosmic microwave background (CMB). If the Universe is homogeneous and isotropic on large scales then the restframe of CMB is expected to...

32. Lightning talks

Cyrille Doux (LPSC)

27/11/2024 17:50

20. 180s flash talks!

Cyrille Doux (LPSC)

27/11/2024 18:00