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  1. Integral Field Spectroscopy at High Spectral Resolution with an Imaging FTS

    The properties of an Imaging Fourier Transform Spectrometer (IFTS) are reminded to show its unique capability of high spectral resolution on a wide...
    Conference paper
  2. Basics of Plasma Physics

    Basic properties of plasmas are introduced, which are valid for an extremely wide range of plasma parameters. Plasmas are classified by different...
    U. Schumacher in Plasma Physics
    Chapter
  3. Strongly Coupled Plasmas

    We give a brief introduction into the basic many-particle effectes in strongly coupled plasmas and their theoretical treatment. Exemplary results are...
    R. Redmer in Plasma Physics
    Chapter
  4. X-rays from the First Massive Black Holes

    We briefly review some recent results from Chandra and XMM-Newton studies of the highest redshift ( ) active galactic...
    W.N. Brandt, C. Vignali, ... I.V. Strateva in Growing Black Holes: Accretion in a Cosmological Context
    Conference paper
  5. A Search for the First Massive Galaxy Clusters

    We have obtained deep, multi-band imaging observations around three of the most distant known quasars at redshifts z>6. Standard accretion theory...
    C.J. Willott, D. Crampton, ... W.J. Percival in Growing Black Holes: Accretion in a Cosmological Context
    Conference paper
  6. Accretion onto a Dupermassive Black Hole in Sgr A*

    We propose a model of accretion onto a black hole at the center of our Galaxy. This model describes a situation in which Sgr A* is accreting a hot...
    M. Moscibrodzka, B. Czerny, V. Beskin in Growing Black Holes: Accretion in a Cosmological Context
    Conference paper
  7. Narrow Line Seyfert 1 Galaxies and the “Anti-hierarchical” Black Hole Growth

    Using a complete sample of soft X-ray selected AGNs, we show that highly accreting AGNs do not follow the MBH–σ relation of normal galaxies. This...
    Conference paper
  8. Torus Models for Obscuration in Type 2 AGN

    We discuss a clumpy model of obscuring dusty tori around AGN. Cloud-cloud collisions lead to an effective viscosity and a geometrically thick...
    T. Beckert, W.J. Duschl, B. Vollmer in Growing Black Holes: Accretion in a Cosmological Context
    Conference paper
  9. Gravitational Waves from Massive Black Holes Binaries

    We compute the expected gravitational wave (GW) signal from coalescing massive black hole (MBH) binaries in a hierarchical structure formation...
    A. Sesana, F. Haardt, ... M. Volonteri in Growing Black Holes: Accretion in a Cosmological Context
    Conference paper
  10. Black Hole Growth in a Cosmological Context and the Associated Cosmic Star Formation History

    Based on a co-evolution scenario of massive black holes (MBH) and their host spheroids, we trace the BH growth and the joint cosmic star formation...
    Y. P. Wang, T. Yamada, Y. Taniguchi in Growing Black Holes: Accretion in a Cosmological Context
    Conference paper
  11. Planet Formation

    Motivating the study of planet formation is not difficult for any curious audience. One of the fundamental human questions is that of origins: “where...
    Chapter
  12. The RASS-SDSS Galaxy Cluster Survey

    Solid observational evidences indicate a strong dependence of the galaxy formation and evolution on the environment. In order to study in particular...
    Paola Popesso, Hans Böhringer, Wolfgang Voges in Multiwavelength Map** of Galaxy Formation and Evolution
    Conference paper
  13. SED Diagnostics of Submillimetre Galaxies

    We apply an evolutionary SED model of starbursts to submm galaxies, in order to predict the present-day colour, magnitude, and size of submm...
    Toshinobu Takagi, Nobuo Arimoto, Hitoshi Hanami in Multiwavelength Map** of Galaxy Formation and Evolution
    Conference paper
  14. High Redshift Lyman Break Galaxies

    Two of the most outstanding issues in modern astrophysics are what reionized the Universe and how did the first objects form. Observations of...
    Conference paper
  15. Extremely Red Galaxies: Dust Attenuation and Classification

    The “extremely red galaxies” (ERGs) constitute a controversial population in deep near-IR surveys. Their extremely-red observed colours (I...
    Daniele Pierini, Claudia Maraston, ... Adolf N. Witt in Multiwavelength Map** of Galaxy Formation and Evolution
    Conference paper
  16. The Deepest Near-Infrared View of the Universe

    We present very deep near-infrared imaging in the J s , H and K s -bands of the HDF-S and...
    Ivo Labbé, Marijn Franx, ... Paul van der Werf in Multiwavelength Map** of Galaxy Formation and Evolution
    Conference paper
  17. A Spectroscopic Survey of the Submillimeter Galaxy Population: 85 Redshifts Using Keck/LRIS-B

    We present spectroscopic identifications for a sample of 85 millimeter and submillimeter galaxies detected with the SCUBA/JCMT and MAMBO/IRAM30m...
    Scott C. Chapman, Andrew Blain, ... Ian Smail in Multiwavelength Map** of Galaxy Formation and Evolution
    Conference paper
  18. Galaxy Evolution in Three Dimensions: Time, Space and Mass

    There are three major axes to describe the evolution of galaxies, namely, time (redshift), space (environment) and mass (stellar mass). In this...
    Tadayuki Kodama, Richard Bower, ... Masayuki Tanaka in Multiwavelength Map** of Galaxy Formation and Evolution
    Conference paper
  19. Chemo-Photometric Models of Ring Galaxies

    The peculiar ring galaxies are formed as a result of cosmic interaction. An intruder galaxy plunges through the center of a disk galaxy triggering...
    Conference paper
  20. Deep Submillimetre Imaging of Distant AGN: Visualising the Formation of Cluster Ellipticals

    We Rob Ivison, Jason Stevens, James Dunlop, Ian Smail, Wil Percival, David Hughes, Huub Röttgering, Wil van Breugel and Michel...
    Conference paper
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