Intergalactic Interconnections

›9:00 (1h40)

Intergalactic Medium Cosmology meets Intergalactic Medium properties
Sebastian Lopez

› Amphitheatre Gastaut

9:00 - 10:40 (1h40)

Intergalactic Medium Cosmology meets Intergalactic Medium properties

Amphitheatre Gastaut

Sebastian Lopez

› The IGM as a biased tracer of large-scale fluctuations: the transmission and the absorber bias factors - Jordi Miralda-Escude, Institut de Ciencies del Cosmos 09:00-09:30 (30min)

› Classifying Damped Lyman Alpha Systems (DLAs) with their metal lines, a new window to the high redshift cosmos - Andreu Arinyo i Prats, Institut de Ciencies del Cosmos, Universitat de Barcelona 09:30-09:50 (20min)

› Measuring baryon acoustic oscillations using the distribution of intergalactic gas - Michael Blomqvist, Laboratoire dÁstrophysique de Marseille 09:50-10:20 (30min)

› Three-point correlation function of the Lyman-alpha forest - Suk Sien Tie, The Ohio State University 10:20-10:40 (20min)

›10:40 (20min)

Coffee break

› Salle des Voutes

10:40 - 11:00 (20min)

Coffee break

Salle des Voutes

›11:00 (2h)

Intergalactic Medium Cosmology meets Intergalactic Medium properties
Sebastian Lopez

› Amphitheatre Gastaut

11:00 - 13:00 (2h)

Intergalactic Medium Cosmology meets Intergalactic Medium properties

Amphitheatre Gastaut

Sebastian Lopez

› The Thermal History of the Universe - Joe Hennawi, Physics Department [Santa Barbara] 11:00-11:30 (30min)

› WDM and Lya-forest: the importance of thermal history - Antonella Garzilli, Niels Bohr Institute & University of Copenhagen 11:30-11:50 (20min)

› Small scale structure of the IGM: A Dark Matter Tale - Vid Irsic, University of Washington 11:50-12:10 (20min)

› The prospects for IGM cosmology in future surveys - Matthew Pieri, Laboratoire d'Astrophysique de Marseille 12:10-12:30 (20min)

› Discussion: What can IGM/CGM scientists do for IGM cosmologists and vice versa for further progress? - (Chair Mat Pieri) 12:30-13:00 (30min)