I do neither guarantee completeness nor uniqueness via the links in the subtitle at all!

Refereed Journals

  • Marcel R. Haas et al., 2010, in prep., "Envrionmental effects in galaxy formation from hydrodynamical cosmological simulations"
  • Marcel R. Haas et al., 2010, in prep., "Simulated galaxy luminosity functions: evolution, input physics and dust attenuatio"
  • Marcel R. Haas et al., 2010, in prep., "Galaxy environmental parameters compared"
  • Marcel R. Haas et al., 2010, in prep., "Physical properties of simulated galaxies from varying input physics"
  • M.R. Haas, P. Anders, 2010, A&A, 512, 79, "Variations in integrated galactic initial mass functions due to sampling method and cluster mass function", [ADS] [ArXiV]
  • Joop Schaye, Claudio Dalla Vecchia, C.M. Booth, Robert P.C. Wiersma, Tom Theuns, Marcel R. Haas, Serena Bertone, Alan R. Duffy, I.G. McCarthy, Luca Tornatore, Freeke van de Voort, 2010, MNRAS, 402, 1536, "The physics driving the cosmic star formation history", [ADS] [ArXiV]
  • Laura V. Sales, Julio F. Navarro, Joop Schaye, Claudio Dalla Vecchia, Volker Springel, Marcel R. Haas, Amina Helmi, 2009, MNRAS Letters, 399, L64, "The origin of extended disk galaxies at z=2", [ADS] [ArXiV]
  • M.R. Haas, M. Gieles, R.A. Scheepmaker, S.S. Larsen, H.J.G.L.M. Lamers, 2008, A&A, 487, 937, "ACS imaging of star clusters in M51. II. The luminosity function and mass function across the disk", [ADS] [ArXiV]
  • R.A. Scheepmaker, M.R. Haas, M.Gieles, N.Bastian, S.S. Larsen, H.J.G.L.M. Lamers, 2007, A&A, 469, 925, "ACS imaging of star clusters in M51. I. Identification and radius distribution", [ADS] [ArXiV]
  • M. Gieles, S.S. Larsen, R.A. Scheepmaker, N. Bastian, M.R. Haas, H.J.G.L.M. Lamers, 2006, A&A Letters, 446, L9-L12, "Observational evidence for a truncation of the star cluster initial mass function at the high mass end", [ADS] [ArXiV]
  • Conference Proceedings

  • M.R.Haas, P. Anders, 2009, "Galactic consequences of clustered star formation", Star clusters - Basic Galactic Building Blocks Throughout Time And Space (IAU S266) [ADS] [ArXiV]
  • M.R.Haas, P. Anders, 2009, "Population synthesis from clustered star formation", Population synthesis planning for the next decade (IAU S262)
  • M.R. Haas, M. Gieles, R.A. Scheepmaker, S.S. Larsen, H.J.G.L.M. Lamers, N. Bastian, 2008, "Variation of the cluster luminosity function across the disk of M51", Mass loss from stars and the evolution of stellar clusters [ADS] [ArXiV]
  • R.A. Scheepmaker, M. Gieles, M.R. Haas, N. Bastian, H.J.G.L.M. Lamers, 2008, "Thousands of Star Clusters in M51 with HST/ACS", Mass loss from stars and the evolution of stellar clusters [ADS]
  • R.A. Scheepmaker, M. Gieles, M.R. Haas, N. Bastian, S.S. Larsen, H.J.G.L.M. Lamers, 2006, "The radii of thousands of star clusters in M51 with HST/ACS", Globular Clusters: Guides to Galaxies, [ADS] [ADS] [ArXiV]
  • M. Gieles, S.S. Larsen, M.R. Haas, R.A. Scheepmaker, N. Bastian, 2006, "The Maximum Mass of Star Clusters", Globular Clusters Guides to Galaxies, [ADS] [ArXiV]
  • Navigation

    Contact details

    Marcel R. Haas

    Address:

    Leiden Observatory

    Niels Bohrweg 2

    2333 CA Leiden

    The Netherlands

    Oort Building, Room 436

    Telephone:

    +31 - (0)71 - 527 8436

    E-mail: mail@marcelhaas.com