Observing the millimeter Universe with the NIKA2 camera

Session

Wednesday Morning-2

5 juin 2019, 11:00

30. NOEMA

Dr Charlène LEFEVRE (Institut de RadioAstronomie Millimétrique)

05/06/2019 11:00

I will introduce NOEMA interferometer, its latest upgrades and capabilities. In particular, I will detail the increase of sensitivity with more antennas, increase of spatial resolution with track extension, and increase of bandwidth with new receiver generation as well as future dual band upgrade. Finally, I will discuss the complementarity between NOEMA and NIKA2 and possible synergies from...

31. Constraining dust physics with NIKA2 polarization : new road maps after Planck

Dr Vincent Guillet (IAS)

05/06/2019 11:30

The Planck mission has brought considerable constraints on the properties of dust, and their evolution from the most diffuse, high-latitude, Galactic ISM to the densest regions of the Gould Belt (Planck 2013 results. XI, Planck Int. Results 2015, XXIX). The combined analysis of ancillary and Planck HFI data has imposed a revision of dust models for the diffuse/translucent ISM, both in total...

60. Unveiling the AGN-galaxy connection at high-z with NIKA2 and radio facilities

Ivan Delvecchio (CEA Saclay)

05/06/2019 12:00

The relationship between supermassive black hole (SMBH) accretion and star formation has lead to controversial studies claiming that Active Galactic Nuclei (AGN) activity might both quench and enhance galaxies' star-forming content. Especially at high redshift (z>2), their interplay is still poorly understood, also due to the lack of accurate estimates of star formation rate (SFR) and AGN...