Chalk talk archive 2015

Raw date Event date Title Speakers Host Summary Links
20150108 Jan. 8, 2015 Cancelled
20150108 Jan. 8, 2015 Cancelled
20150115 Jan. 15, 2015 Dark Matter-Neutrino Interactions
20150115 Jan. 15, 2015 Dark Matter-Neutrino Interactions
20150122 Jan. 22, 2015 Cancelled
20150129 Jan. 29, 2015 The SPT-3G Sinuous Antenna
20150129 Jan. 29, 2015 The SPT-3G Sinuous Antenna
20150205 Feb. 5, 2015 Cancelled
20150205 Feb. 5, 2015 Cancelled
20150212 Feb. 12, 2015 SPT-3G observing bands defined by the SPT-3G triplexer
20150212 Feb. 12, 2015 SPT-3G observing bands defined by the SPT-3G triplexer
20150305 March 5, 2015 What is a photoneutron source and how is it useful for SuperCDMS?
20150305 March 5, 2015 What is a photoneutron source and how is it useful for SuperCDMS?
20150312 March 12, 2015 On the Solar Modulation of Cosmic Rays
20150402 April 2, 2015 The Dispersion Measure Distance
20150409 April 9, 2015 Is the Fermi Source J2212.50703 a DM sub halo?
20150423 April 23, 2015 TBA
20150430 April 30, 2015 Doping for better results - not just for cyclists
20150514 May 14, 2015 Neutrinoless Double Electron Capture on Ar36
20150521 May 21, 2015 Scalable DAQ for high throughput data astrophysics experiments, MKIDS and more
20150910 Sept. 10, 2015 Multi-wavelength Constraints for Galactic Cosmic Ray Leptons
20150924 Sept. 24, 2015 Exotic Rotational Fluctuations
20151001 Oct. 1, 2015 Intensity Interferometry in the Era of Giant Telescopes
20151008 Oct. 8, 2015 The Heavenly Fire of Reionization
20151022 Oct. 22, 2015 Readout system for a 1 kg CCD based detector for DM and CNNS (DAMIC and CONIE)
20151029 Oct. 29, 2015 Neutron yield measurements and neutron sources
20151105 Nov. 5, 2015 CCD Calibration with Neutrons for DAMIC and CONNIE
20151112 Nov. 12, 2015 The Latin American Giant Observatory (LAGO)
20151119 Nov. 19, 2015 An Introduction to the Neutron Electric Dipole Moment
20151210 Dec. 10, 2015 Magnetization of High Temperature Superconducting Bulks
20151217 Dec. 17, 2015 Likelihood - free cosmological parameter estimation from supernovae observations