The meeting starts at 10:00 and finishes at 17:00. Lunch and two coffee breaks are included.
10:00-10:30 | Coffee and welcome | |
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10:30-10:45 | Carlos Frenk | X-ray coronae around spiral galaxies? |
10:45-11:00 | Ryan Hickox | The edge of detection: The unresolved cosmic X-ray background in the Chandra Deep Fields |
11:00-11:15 | Mike Hill | The X-ray AGN contribution to the FIR and sub-mm backgrounds |
11:15-11:30 | Agnese Del Moro | Revealing the most obscured distant AGNs: new insights from X-ray and infrared spectroscopy |
11:30-11:45 | Paul Giles | X-ray Properties of Galaxy Clusters and comparisons to Weak-Lensing Measurements |
11:45-12:00 | Kathy Romer | XMM Cluster Survey: the first cluster data release (500 temperatures and 1000 redshifts) |
12:00-12:15 | Beatriz Mingo Fernandez | Upset AGNs: bubbles and shocks in Markarian 6 and beyond |
12:15-12:30 | Adam Patrick | Iron Line Profiles in Suzaku Spectra of Bare Seyfert Galaxies |
12:30-13:30 | Lunch | |
13:30-13:45 | Dan Wilkins | Determination of the Emissivity Profiles of AGN Accretion Discs and their Physical Implications |
13:45-14:00 | Simon Vaughan | What can we learn from multiple XMM-Newton observations of NGC 4051? |
14:00-14:15 | Missagh Mehdipour | The optical-UV-X-ray variability connection in Mrk 509 |
14:15-14:30 | Dom Walton | Ultraluminous X-ray Sources in Nearby Galaxies |
14:30-14:45 | Roberto Soria | X-ray hot spots, optical nebula and radio lobes of a powerful microquasar in NGC 7793 |
14:45-15:00 | Antonia Rowlinson | The unusual X-ray emission of the short Swift GRB 090515: Evidence for the formation of a magnetar? |
15:00-15:30 | Coffee | |
15:30-15:45 | Wynn Ho | Lessons from the youngest neutron star in the Galaxy |
15:45-16:00 | Adam Ingram | Low frequency QPOs: a precession model in the context of mass accretion rate fluctuations |
16:00-16:15 | Pablo Cassatella | Time lags from reflection in BHXRBs |
16:15-16:30 | Lucy Heil | The rms-flux relation in Black hole binaries |
16:30-16:45 | Tony Wilkinson | GX 339-4 in 2004 and 2009: Is the PSD break time-scale a signature of the disc truncation radius? |
16:45-17:00 | Mike Watson | The next 15 years: future developments in X-ray astronomy |
17:00 | Close |