Rise And Shine 2018
@2018_rise
I'm the official twitter account for the Rise and Shine 2018 conference. June 18-22 Strasbourg, France. Managed by @domaubr
Naoki Yoshida: this video looks boring, but believe me, it is done with a very sofisticated code.
We can discuss escape fractions for ever... maybe we should organise another dedicated workshop about this. #riseshine18 #lycleak
Worseck : Disagreement with quasar-driven HeII reionization models predicting ubiquitous GP throughs at z>3 #riseshine18
Boutsia : escape fraction of faint agn at z>4 could be ~75% #riseshine18
Bradac :Spitzer is the high-redshift killer #riseshine18
Oesch : only 9 reliable z=10 galaxies today. Typically one order of magnitude drop in the observed SFRD between z=8 and 10. #riseshine18
Oesch : Hubble frontier fields can probe turn over in the LF at low luminosities thanks to lensing. 3 Mag fainter than HUDF. LF at high z remains steep until Muv ~-15 #riseshine18
Anne Hutter : 21cm - LyA emitters cross-correlations still require large surveys (>20 deg2) when looking at moderately bright LAE to distinguish between different Universe ionization state #riseshine18
Second day for Rise and Shine 2018, starting with Catherine Watkinson about "Non Gaussianity during the Cosmic Dawn" #riseshine18
Extension to Garrelt Mellema's talk. It was missing a picture of the foreground filter. #riseshine18 @2018_rise
And that’s it for the first day of Rise and Shine 2018 ! #riseshine18
Iliev : scales relevant for cosmological reionization and observations ~100s of Mpc but typical hydro simulations model ~10s of Mpc #riseshine18
Bethermin : separating high-z CII from CO lines at lower z is one of the challenges of CONCERTO. But also an opportunity to understand molecular gas. #riseshine18
Bethermin : CONCERTO, an intensity mapping experiment using the CII line between z=4.5 and 9 (200-360 GHz). First results planned 2021. Probe dusty SFRD for z>4, fait number counts and bright-end of the LF. #riseshine18
Sambit Giri : the 21 cm signature of the BAO can be obtained using statistics such as the squeezed-limit bispectrum #riseshine18
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