Programme
The meeting starts at 10:00 and finishes at 17:00.
[Note: the programme was last updated on 10 Sept.]
| 10:00 | Coffee & welcome |
||
|---|---|---|---|
| 10.45 |
Session 1 |
Chair: TBC |
|
| 10.45 | Gillian James | Leicester | Black Holes in Short Period X-ray Binaries: the Transition to Radiatively Inefficient Accretion |
| 11.00 | Erin Kara | IoA, Cambridge | The Closest Look at 1H0707-495: X-ray Reverberation Lags with 1.3 Ms of Data |
| 11.15 | Daniel Plant | Southampton | Can we really measure black hole spin, and does it really power relativistic jets? |
| 11.30 | Amy Scott | Leicester | Broadband spectral properties of type 1 AGN |
| 11.45 | Wako Ishibashi | IoA, Cambridge | X-ray variability scaling in accreting black holes |
| 12.00 | John Richard Jones | Southampton | SPH modelling of high mass xray binaries (HMXRB) and the circumstellar disc therein. |
| 12.15 | Rhaana Starling | Leicester | Early thermal X-ray emission in Gamma-Ray Bursts |
| 12.30 | LUNCH (buffet) | ||
| 13.45 | Session 2 | Chair: TBC | |
| 13.45 |
Andrew Sutton | Durham | Energy dependent variability as a diagnostic of the ultraluminous state |
| 14:00 | Mat Page | MSSL/UCL | X-ray and submillimetre observations of star-forming QSOs in the epoch of galaxy formation. |
| 14:15 | James Mullaney | Durham | Evidence of a universal BH accretion to star formation rate ratio since z~2 |
| 14:30 | David Alexander | Durham | NuSTAR and the extragalactic surveys |
| 14:45 | Mike Watson | Leicester | Future X-ray astronomy missions |
| 15:00 | [Discussion] | ||
| 15:15 | COFFEE | ||
| 15.45 |
Session 3 |
Chair: TBC |
|
| 15:45 | Mark Burke | Birmingham | X-ray Binaries in Centaurus A |
| 16:00 | Beatriz Mingo | Hertfordshire | The Circinus galaxy, jet-driven outflows and the SNR connection. |
| 16:15 | Stephen Walker | IoA, Cambridge | Exploring the Outskirts of Galaxy Clusters with Suzaku |
| 16:30 | David Barnes | MSSL/UCL | X-ray and radio morphologies in galaxy clusters |
| 16:45 | Judith Ineson | Southampton | Radio-loud AGN: is there a link between luminosity and cluster environment? |
| 17:00 | CLOSE |
