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Particle and nuclear physics

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  1. Galaxy Masses: Disks and Their Halos

    I review what we currently do and do not know about the masses of disk galaxies and their dark matter halos. The prognosis for disks is good: the...
    Stacy McGaugh in The Mass of Galaxies at Low and High Redshift
    Conference paper

  2. Luminosities of Radio-Loud Active Galaxies

    We investigate the host galaxy luminosities of three different samples of radio loud active nuclei at z<0.5 including BL Lac Objects (BLLs), Radio...
    Aldo Treves, Nicoletta Carangelo, Renato Falomo in The Mass of Galaxies at Low and High Redshift
    Conference paper

  3. Probing the Evolution of Massive Galaxies with the K20 Survey

    The motivations and the status of the K20 survey are presented. The first results on the evolution of massive galaxies and the comparison with the...
    Andrea Cimatti in The Mass of Galaxies at Low and High Redshift
    Conference paper

  4. The Evolution of Galaxy Mass in Hierarchical Models

    Advances in extragalactic astronomy have prompted the development of increasingly realistic models which aim to describe the formation and evolution...
    C. M. Baugh, A. J. Benson, ... C. Lacey in The Mass of Galaxies at Low and High Redshift
    Conference paper

  5. Studying the Dynamics of Star Forming and IR Luminous Galaxies with Infrared Spectroscopy

    With the advent of efficient near-IR spectrometers on 10m-class telescopes, exploiting the new generation of low readout noise, large format...
    Reinhard Genzel, Linda J. Tacconi, ... Niranjan Thatte in The Mass of Galaxies at Low and High Redshift
    Conference paper

  6. What Does the Local Black Hole Mass Distribution Tell Us About the Evolution of the Quasar Luminosity Function?

    We present a robust method to derive the duty cycle of QSO activity based on the empirical QSO luminosity function and on the present-day linear...
    Luca Ciotti, Zoltan Haiman, Jeremiah P. Ostriker in The Mass of Galaxies at Low and High Redshift
    Conference paper

  7. Spheroidal Galaxies/QSOs Connection

    In view of the extensive evidence of a tight inter-relationship between spheroidal galaxies (and galactic bulges) and massive black holes hosted at...
    Luigi Danese, Gian Luigi Granato, ... Gianfranco De Zotti in The Mass of Galaxies at Low and High Redshift
    Conference paper

  8. The Mass of Radio Galaxies from Low to High Redshift

    Using a new radio sample, 6C* designed to find radio galaxies at z > 4 along with the complete 3CRR and 6CE sample we extend the radio galaxy K-z...
    Matt J. Jarvis, Steve Rawlings, ... Chris J. Willott in The Mass of Galaxies at Low and High Redshift
    Conference paper

  9. Estimating the Mass of Local Disk Galaxies from the NIR Luminosity

    The relation between the dynamical mass ( $\propto V_{max}^2 \times r_{opt}$...
    Giuseppe Gavazzi in The Mass of Galaxies at Low and High Redshift
    Conference paper

  10. Clustering at High Redshift

    The addition of deep near infrared images to the database provided by the HDF WFPC2 is essential to monitor the SEDs of the objects on a wide...
    S. Cristiani, S. Arnouts, ... E. Vanzella in The Mass of Galaxies at Low and High Redshift
    Conference paper

  11. Detection of CDM Substructure

    The properties of multiple image gravitational lenses require a fractional surface mass density in satellites of f...
    C. S. Kochanek, N. Dalal in The Mass of Galaxies at Low and High Redshift
    Conference paper

  12. Lens Galaxies vs. CDM

    By directly probing mass distributions, gravitational lensing offers several new tests of the CDM paradigm. Lens statistics place upper limits on the...
    Charles R. Keeton in The Mass of Galaxies at Low and High Redshift
    Conference paper

  13. Galaxy-Galaxy Lensing in the FORS Deep Field

    We demonstrate the presence of a galaxy-galaxy lensing signal of z=0.5-1.0 foreground galaxies by analyzing the distortion of z=2.5-4.5 background...
    Stella Seitz, Thomas Erben, ... the FDF-Team in The Mass of Galaxies at Low and High Redshift
    Conference paper

  14. The Mass Function of Field Galaxies at 0.4 < z < 1.2 as Derived from the MUNICS K-Selected Sample

    We derive the number density evolution of massive field galaxies in the redshift range 0.4 < z < 1.2 using the K-band selected field galaxy sample...
    Niv Drory, Ralf Bender, ... Claudia Mendes de Oliveira in The Mass of Galaxies at Low and High Redshift
    Conference paper

  15. Nuclear Stellar Disks in Spiral Galaxies

    We report the discovery of a nuclear stellar disk in 3 early-type spirals, namely NGC 1425, NGC 3898 and NGC 4698, revealed by WFPC2/F606W images out...
    A. Pizzella, E. M. Corsini, ... F. Bertola in The Mass of Galaxies at Low and High Redshift
    Conference paper

  16. Gas Minor-Axis Velocity Gradients in Early-Type Spiral Galaxies

    We measured a remarkable gas velocity gradient along the minor axis of 5 early-type spiral galaxies. This phenomenon suggests the presence of a...
    E. M. Corsini, A. Pizzella, ... F. Bertola in The Mass of Galaxies at Low and High Redshift
    Conference paper

  17. The Evolution of Distant Cluster Spirals

    Ground-based and HST observations indicate that the disk galaxy population in rich galaxy clusters has experienced remarkable evolution since z = 1....
    Bo Milvang-Jensen, Alfonso Aragón-Salamanca, ... Jens Hjorth in The Mass of Galaxies at Low and High Redshift
    Conference paper

  18. Measuring Galaxy Disk Mass with the SparsePak Integral Field Unit on WIYN

    We present first results from the commissioning data of the SparsePak Integral Field Unit on the WIYN telescope. SparsePak is a bundle of 82 fibers,...
    Marc Verheijen, Matthew Bershady, David Andersen in The Mass of Galaxies at Low and High Redshift
    Conference paper

  19. Constraining the Mass Assembly in Ellipticals from ERO Clustering

    The redshift evolution of clustering is a powerful tool to constrain the models of galaxy assembly. In particular, the strong clustering of EROs, if...
    Emanuele Daddi in The Mass of Galaxies at Low and High Redshift
    Conference paper

  20. Evolution in the Linewidth-Magnitude Relation to z > 1 from the DEEP Groth Strip Survey

    Galaxy kinematics are potentially a powerful tool to measure the evolution of Tully-Fisher-type relations and to see how properties of distant...
    Benjamin J. Weiner, the DEEP Collaboration in The Mass of Galaxies at Low and High Redshift
    Conference paper
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