Yu-Ying Zhang

Selected presentations: colloquia, conferences, and workshops

1. (The eROSITA consortium meeting
   Munich, Germany, Nov, 28-29, 2012)
   
   
2. Science with eROSITA and ART-XC aboard Spectrum-RG "X-ray sky: from stars a\ nd black holes to cosmology"
   Kazan, Russia, Sep, 3-7, 2012
   Talk: Status on mass calibration using a representative cluster sample at z~0.2 and o\ n optical follow-up using mock surveys
   
   
3. XXVIII IAU General Assembly
   Beijing, China, Aug, 20-31, 2012
   Talk: Probing substructures in galaxy clusters and resulting systematic in cosmological applications with X-ray and optical surveys
   
   
4. (The eROSITA consortium meeting
   Hamburg, Germany, Jul, 23-24, 2012)
   
   
5. Local Cluster Substructure Survey team meeting
   Arizona, USA, Oct, 31 -- Nov 4, 2011
   Talk: Temperature cross-calibration between XMM-Newton and Chandra
   
   
6. University Observatory Munich
   Munich, Germany, Oct, 2011
   Seminar talk (invited): Understanding cluster mass measurements combining three independent probes: X-ray, weak lensing and velocity dispersion
   
   
7. First International eROSITA conference "Mapping the Structure of the Energetic Universe"
   Garmisch-Partenkirchen, Germany, Oct, 2011
   Poster: Where are we in calibrating mass proxies and baryon-mass fraction for cluster cosmology
   
   
8. (The eROSITA consortium meeting
   Garching, Germany, Oct, 23, 2011)
   
   
9. Schwerpunktprogramm "Witnesses of Cosmic History: Formation and evolution of black holes, galaxies and their environment" - final workshop
   Bad Honnef , Germany, Jul, 2011
   Talk: Calibrating mass proxies and baryon mass fraction for galaxy clusters
   
   
10. The X-ray Universe 2011
    Berlin, Germany, Jul, 2011
    Talk: Toward understanding mass proxies of galaxy clusters for modern cosmology
    
    
11. Tsinghua University
    Beijing, China, Jun, 2011
    Seminar talk (invited): Multi-wavelength studies of galaxy clusters for the eROSITA survey
    
    
12. National Astronomical Observatory Center
    Beijing, China, Oct, 2010
    Colloquium talk (invited): Biases of mass proxies of galaxy clusters and the origin
    
    
13. Institute of High Energy Physics
    Beijing, China, Oct, 2010
    Colloquium talk (invited): Controlling systematic uncertainties in future X-ray surveys of galaxy clusters
    
    
14. Galaxy Clusters: observations, physics and cosmology
    Garching, Germany, Jul, 26--30, 2010
    Poster: Testing cluster dynamical properties using X-ray and optical approaches
    
    
15. Local Cluster Substructure Survey team meeting
    Tokyo, Japan, Jul, 5--7, 2010
    Talk: XMM/Subaru mass comparison, and mass-Lx
    
    
16. CL J2010: from Massive Galaxy Formation to Dark Energy
    Tokyo, Japan Jun, 28--Jul, 2, 2010
    Poster: Testing Hydrostatic Equilibrium in Galaxy Clusters
    
    
17. Workshop: How to weigh clusters of galaxies
    Leiden, Netherland
    Apr, 19--23, 2010
    Talk (invited): Calibrating cluster mass proxies regarding to cluster morphology
    
    
18. High energy group at MPE
    Garching, Germany
    Jan, 14, 2010
    Talk (invited): What is the best mass proxy in X-ray cluster surveys - mass calibration with multi-wavelength data
    
    
19. X-ray cluster group at MPE
    Garching, Germany
    Jan, 13, 2010
    Talk (invited): Interesting cluster science with X-ray substructure
    
    
20. X-ray Astronomy 2009: Present status, multi-wavelength approach and future perspectives
    Bologna, Italy, Sep, 7--11, 2009
    Poster: Bias of Hydrostatic Equilibrium Mass and its Origin in Galaxy Clusters
    
    
21. SZ @ Bonn 2009: A multi-wavelength look at galaxy clusters
    Bonn, Germany, Jul, 15--17, 2009
    Talk (invited): Calibrating the scaling relations with multi-wavelength data
    
    
22. Kick-off meeting for the third period of the Schwerpunktprogramm "Witnesses of Cosmic History: Formation and evolution of black holes, galaxies and their environment")
    Bad Honnef, Germany, May, 21--23, 2009
    Talk: Galaxy Clusters: Mass estimates versus morphology
    
    
23. The 1st GCOE International Symposium: Weaving Science Web beyond Particle-Matter Hierarchy
    Sendai, Japan, Mar, 5--7, 2009
    Talk (invited): Galaxy Clusters: Mass estimates & Substructures
    
    
24. Schwerpunktprogramm "Witnesses of Cosmic History: Formation and evolution of black holes, galaxies and their environment"
    Bad Honnef, Germany, Jan, 23, 2009
    Poster: Complex interplay between the formation of dark matter halos and their baryon contents in galaxy cluster and galaxy group environments
    
    
25. Cluster Weighing Worshop
    Garching, Germany, Jul, 30--31, 2008
    Talk (invited): Do Mass Estimates agree with the True Mass?
    
    
26. Local Cluster Substructure Survey team meeting
    Chicago, USA, Jun, 3--5, 2008
    Talk: X-ray and Weak Lensing Observations vs. Simulations: LoCuSS vs. HIFLUGCS
    
    
27. The X-ray Universe 2008
    Granada, Spain, May, 26--30, 2008
    Poster: Scaling Relations of Galaxy Clusters: X-ray and Lensing vs. Simulations
    
    
28. An XXL extragalactic survey: prospects for the XMM next decade
    Paris, France, Apr, 14--16, 2008
    Talk: Scaling Relations of the LoCuSS Sample of Galaxy Clusters: X-ray and Lensing Observations Versus Simulations
    
    
29. IAP workshop -- Mass profiles of cosmic structures
    Paris, France, Nov, 14, 2007
    Talk (invited): Mass Estimates for Galaxy Clusters: Weak lensing vs X-ray mass & observations vs simulations
    
    
30. AIfA Workshop
    Bad Honnef, Germany, Oct, 26--27, 2007
    Talk: What does the M-Yx relation tell us?
    
    
31. Workshop of the Schwerpunktprogramm "Witnesses of Cosmic History: Formation and evolution of black holes, galaxies and their environment"
    Bad Honnef, Germany, Oct, 9--12, 2007
    Talk: Bias and scatter of weak lensing and X-ray cluster masses
    
    
32. Transregio 33 Meeting (Transregio 33: "The Dark Universe")
    Bad Honnef, Germany, Sep, 30--Oct, 3, 2007
    Talk: X-ray versus lensing masses for galaxy clusters
    
    
33. X-ray Surveys: Evolution of Accretion, Star-Formation and the Large Scale Structure
    Rhodes, Greece, Jul, 2--6, 2007
    Talk: Scaling relations for galaxy clusters
    
    
34. Tracing Cosmic Evolution with Clusters of Galaxies: Six Years Later
    Sesto, Italy, Jun, 25--29, 2007
    Poster: Weak lensing versus X-ray mass calibration for 37 LoCuSS galaxy clusters
    
    
35. REXCESS Cluster Workshop
    Chiemsee Frauenwoerth, Germany, May, 14--16, 2007
    Talk: X-ray versus lensing mass calibration
    
    
36. Cosmology group at Argelander-Institut fuer Astronomie
    Bonn, Germany, Feb, 22, 2007
    Talk (invited): Scaling relations and mass calibration: XMM observations of the pilot LoCuSS cluster sample
    
    
37. The Extreme Universe in the Suzaku Era
    Kyoto, Japan, Dec, 4--8, 2006
    Poster: Calibrating scaling relations using 2 large samples of galaxy clusters at z~0.2, 0.3: XMM-Newton observations
    
    
38. Meeting in the MPE high energy group
    Garching, Germany, Nov, 16, 2006
    Talk: XMM observations of a flux-limited sample of galaxy clusters at z~0.2
    
    
39. Black Holes: Power behind the Scene
    Kathmandu, Nepal, Oct, 23--27, 2006
    Talk: AGNs in Clusters of Galaxies: XMM observations of a flux-limited cluster sample at z~0.2
    
    
40. Local Cluster Substructure Survey: Data and Team Meeting
    School of Physics and Astronomy, University of Birmingham, UK, Sep, 18--20, 2006
    Talk: Scaling Relations and Mass Calibration: XMM observations of the Pilot Study Sample
    
    
41. Heating vs. Cooling in Galaxies and Clusters of Galaxies
    Garching, Germany, Aug, 6--11, 2006
    Poster: Scaling relations of massive galaxy clusters at medium redshifts
    
    
42. Galaxy Cluster Workshop with the Bonn Group
    Garching, Germany, Apr, 4--5, 2006
    Talk: Scaling relations: the REFLEX-DXL sample at z~0.3
    
    
43. Japan-Germany Colloquium on ``Relativistic Universe''
    Wildbad Kreuth, Germany, Feb, 27--Mar, 1, 2006
    Talk: Exploring the Scaling Relations of the REFLEX-DXL Galaxy Clusters at z~0.3
    
    
44. Institute of High Energy Physics
    Beijing, China, Nov, 2005
    Colloquium talk (invited): Strucure of galaxy clusters and their ICM as observed with XMM-Newton
    
    
45. National Astronomical Observatory Center
    Beijing, China, Oct, 2005
    Colloquium talk (invited): Self-similarity of massive galaxy clusters
    
    
46. The X-ray Universe 2005, El Escorial
    Spain, Sep, 26--30, 2005
    Poster: X-ray properties in Galaxy Clusters
    
    
47. XMM-Newton EPIC Consortium Meeting
    Ringberg, Germany, Apr, 11--13, 2005
    Poster: Exploring Galaxy Clusters: XMM-Newton observations of the REFLEX-DXL sample at z~0.3
    
    
48. The Future of Cosmology with Clusters of Galaxies
    Kona, USA, Feb, 26--Mar, 2, 2005
    Poster: Exploring Galaxy Clusters at z~0.3: XMM-Newton observations of the REFLEX-DXL sample
    
    
49. Ringberg Workshop: High Energy Studies
    Ringberg, Germany, Feb, 9--11, 2005
    Talk: The structure of galaxy clusters and their ICM as observed with XMM-Newton
    
    
50. XMM LP Workshop
    Garching, Germany, Jan, 25, 2005
    Talk: Temperature and Metallicity Profiles of 17 XMM-LP Galaxy Clusters
    
    
51. 35th COSPAR Scientific Assembly
    Paris, France, Jul, 18--25, 2004
    Poster: Spatial distributions of the galaxy clusters at medium redshifts observed by XMM-Newton
    
    
52. X-ray Studies of Galaxy Clusters and Deep X-ray Surveys
    Ringberg, Germany, May, 2--5, 2004
    Talk: XMM studies of medium distant clusters
    
    
53. MPE high energy group
    Garching, Germany, Nov, 6, 2003
    Talk: Spatial Distribution in the Core Region of the Supercluster
    
    
54. Modelling the Intergalactic and Intra-cluster Media
    Vucalno, Italy, Otc, 1--4, 2003
    Talk: Spatial distributions of the REFLEX-DXL galaxy clusters at z~0.3 observed by XMM-Newton
    
    
55. National Astronomical Observatory Center
    Beijing, China, Aug, 2003
    Colloquium talk (invited): Modeling spatially resolved properties of the ICM from the XMM-Newton observations
    
    

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