Slide 1The disc-jet-spin connection: 3C273 Chris Done Charles Finn, Emma Gardner… University of Durham Slide 2 AGN/QSO Zoo!!! Optical Mass, mass accretion rate, spin and…
ar X iv :1 40 9. 56 32 v1 [ as tro -p h.C O] 1 9 S ep 20 14 Accepted for ApJL Preprint typeset using LATEX style emulateapj v. 5/2/11 LYα FOREST TOMOGRAPHY FROM BACKGROUND…
“Anillo de Cosmología” internal meeting, January 13th 2014 Deep I,V imaging with Warsaw telescope of the Extended Hubble Deep Field South (E-HDFS) Carlos Hervías! Departamento…
Slide 1 Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly = ionizing…
What’s New with Peculiar Velocities? hundreds of 5% distances within 6 Mpc galaxies gather in groups; few are isolated modest group masses; don’t account for much of…
“Surveying the low frequency sky with LOFAR” 8-12 March 2010, Leiden, The Netherlands INAF-Istituto di Radioastronomia, Bologna, ITALY Cluster Radio Halos in the LOFAR…
The Z-burst effect A Z-boson is produced at the neutrino resonance energy “Visible” decay products have energies 10-40 times smaller. Fargion, Weiler, Yoshida Main problems…
Future Science at cm wavelengths, Chicago II, Aug 2006, C.Carilli Major efforts: EVLA I+II, ATA… Three year process: Quantified ‘experiments’ for future large area…
Cosmological observables after recombination Antony Lewis Institute of Astronomy, Cambridge http://cosmologist.info/ Anthony Challinor (IoA, DAMTP); astro-ph/0702600 + in…
Effects of Primordial Magnetic Helicity and Detection Possibilities Tina Kahniashvili Kansas State University New Views of the Universe Papers: C. Caprini, R.Durrer, T.K.,…