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1. Blind Source Separation of Multispectral Astronomical Images

   Multispectral images lead to classify pixels, but often with the drawback that each pixel value is the result of a combination of different sources....

   Albert Bijaoui, Danielle Nuzillard in Mining the Sky

   Conference paper
   

2. Extracting Knowledge from Very Large Datasets in a Multi-Wavelength Context

   The ability to extract knowledge from very large data catalogues resulting from sky surveys or from deep wide fields, observed at various wavelength...

   Daniel Egret in Mining the Sky

   Conference paper
   

3. OPTICON and the Virtual Observatory

   The challenges of multi-wavelength astrophysics require new outlooks from those appropriate to traditional astronomy. The next generation of research...

   Gerry Gilmore in Mining the Sky

   Conference paper
   

4. Mining the CDS Collection: A Learning Experience

   The experiences gained as a result of the CDS/ESO Datamining project are described in this paper as well as a brief outline of the tools developed...

   Patricio F. Ortiz, François Ochsenbein in Mining the Sky

   Conference paper
   

5. DEEP: Pre-DEIMOS Surveys to $I \sim 24$ of Galaxy Evolution and Kinematics

   DEEP is a two-phase program designed to undertake spectroscopic surveys of faint field galaxies with the Keck Telescopes. The scientific goals...

   David C. Koo in Deep Fields

   Conference paper
   

6. Constraining Models of Galaxy Formation with Deep Multicolor Galaxy Surveys

   We present a comparison between the observed properties of high redshift galaxies, as they result from the analysis of deep multicolor imaging...

   Adriano Fontana, Nicola Menci, ... Paolo Saracco in Deep Fields

   Conference paper
   

7. Modeling Faint Morphological Number Counts

   We revisit our recent results concerning comparisons of magnitude and photometric redshift data from the Hubble Deep Fields to statistical...

   Paul Bristow, Steve Phillipps in Deep Fields

   Conference paper
   

8. Distant Disk Galaxies: Kinematics and Evolution to $z \sim 1$

   High resolution HST images have been combined with Keck+LRIS and VLT+ISAAC spectra to study the internal kinematics of 100 faint disk galaxies in the...

   Nicole P. Vogt in Deep Fields

   Conference paper
   

9. Optical and Near-IR Identifications of (Sub)Millimeter Background Sources

   We summarise preliminary results of our search for optical and near-infrared counterparts to millimeter continuum background sources discovered in...

   Helmut Dannerbauer, Frank Bertoldi, ... Frazer Owen in Deep Fields

   Conference paper
   

10. The Star Formation Density in the High-Redshift Universe

    We use images of the Hubble Deep Fields (HDFs) to estimate the universal star formation density (SFD) and its evolution. We find that it increases...

    Alberto Fernández-Soto, Kenneth M. Lanzetta, ... Noriaki Yahata in Deep Fields

    Conference paper
    

11. Population of Cl1601+42 at z = 0.54

    We use photometric redshifts to determine the rest frame cluster luminosity function (LF) to...

    Tomas Dahlén, Claes Fransson, Magnus Näslund in Deep Fields

    Conference paper
    

12. High-Energy Large-Area Surveys: From BeppaSAX to Chandra and XMM

    Optical identification of hard X-ray selected BeppoSAX and Chandra sources indicates that a large fraction of the sources are “intermediate” AGN,...

    Fabrizio Fiore, Andrea Comastri, ... the HELLAS Collaboration in Deep Fields

    Conference paper
    

13. Deep Observations of Lyman Break Galaxies

    We summarise the main results of recent work on the Lyman break galaxy population which takes advantage of newly commissioned instrumentation on the...

    Max Pettini, Charles C. Steidel, ... Mauro Giavalisco in Deep Fields

    Conference paper
    

14. VLT Imaging of Quasar Host Galaxies at $z \sim 1.5$

    We present high spatial resolution near-infrared H-band ( $1.65 \mu$...

    Renato Falomo, Jari Kotilainen, ... Nicoletta Carangelo in Deep Fields

    Conference paper
    

15. Galaxies Near Distant Damped Ly- $\alpha$ Clouds

    We are obtaining deep, broad band images with MOSAIC and IRIM at the KPNO 4-m of 5 QSO fields controlling damped Ly...

    Nicolas Bouché, James D. Lowenthal in Deep Fields

    Conference paper
    

16. Deep Surveys with SIRTF’s Infrared Array Camera

    The Infrared Array Camera (IRAC) on NASA’s Space Infrared Telescope Facility (SIRTF) will provide imaging at 3.6, 4.6, 5.8 and 8 μm. The four bands...

    Peter Eisenhardt, Giovanni Fazio, ... Edward Wright in Deep Fields

    Conference paper
    

17. Optical/Infrared Survey of Galaxy Clusters

    In this contribution the ongoing effort to build a statistical sample of clusters of galaxies over a wide range of redshifts to study the evolution...

    Luiz da Costa, S. Arnouts, ... E. Zucca in Deep Fields

    Conference paper
    

18. The Present: Capodimonte Deep Field. The Future: Science with VST

    The VLT Survey Telescope (VST) project is a cooperation between ESO, the Capodimonte Astronomical Observatory (OAC) in Naples, Italy, and the...

    Massimo Capaccioli, Juan M. Alcalá, ... Roberto Silvotti in Deep Fields

    Conference paper
    

19. The BMW Deep X-Ray Cluster Survey

    We briely describe the main features and first results of the BMW survey of serendipitous X-ray clusters, based on the still unexploited ROSAT-HRI...

    Luigi Guzzo, Alberto Moretti, ... Gianpiero Tagliaferri in Deep Fields

    Conference paper
    

20. XMM-Newton Deep Fields

    The XMM-Newton Observatory offers unprecedented effective collecting area in the X-ray energy range 0.1-15keV, and excellent angular resolution. This...

    David H. Lumb in Deep Fields

    Conference paper