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

Refereed Journals

  • Marcel R. Haas, Joop Schaye, Akila Jeeson-Daniel, MNRAS, 2012, 419, 2133, "Disentangling galaxy environment and host halo mass", [ADS] [ArXiV]
  • Akila Jeeson-Daniel, Claudio Dalla Vecchia, Marcel R. Haas, Joop Schaye, 2011, MNRAS Letters, 415L, 69 "The correlation structure of dark matter halo properties", [ADS] [ArXiV]
  • Freeke van de Voort, Joop Schaye, C.M. Booth, Marcel R. Haas, Claudio Dalla Vecchia, MNRAS, 2011, 414, 2458, "The rates and modes of gas accretion on to galaxies and their gaseous haloes" [ADS] [ArXiV]
  • 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]
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    Contact details

    Marcel R. Haas

    Address:

    Space Telescope Science Institute

    3700 San Martin Drive

    Baltimore, MD, 21218

    USA

    Bloomberg Building, Room P611

    Telephone:

    +1 - (410) 338 5012

    E-mail: mhaas_at_stsci_dot_edu