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The top documents tagged [high redshift galaxies]

Current Topics: Lyman Break Galaxies - Lecture 3 Current Topics Lyman Break Galaxies Dr Elizabeth Stanway (E.R.Stanway@Bristol.ac.uk)
Current Topics: Lyman Break Galaxies - Lecture 3 Current Topics Lyman Break Galaxies Dr Elizabeth Stanway ([email protected])
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Target Selection and photo-z Filipe B. Abdalla. Usual spectroscopic targets: KAOS/WFMOS/BigBOSS/Sumire/DESpec etc… LRG galaxies out to z~1 with absorption
Target Selection and photo-z Filipe B. Abdalla. Usual spectroscopic targets: KAOS/WFMOS/BigBOSS/Sumire/DESpec etc… LRG galaxies out to z~1 with absorption
215 views
High Redshift Galaxies in the Great Observatories Origins Deep Survey (GOODS) Mark Dickinson (National Optical Astronomy Observatory) for the GOODS team
High Redshift Galaxies in the Great Observatories Origins Deep Survey (GOODS) Mark Dickinson (National Optical Astronomy Observatory) for the GOODS team
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Dark Energy & overview of Cosmological parameters Today: Review last time Revisit the accelerating universe Look at values of cosmological parameters from
Dark Energy & overview of Cosmological parameters Today: Review last time Revisit the accelerating universe Look at values of cosmological parameters from
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Binary Quasars in the Sloan Digital Sky Survey Joseph F. Hennawi Berkeley Hubble Symposium April 7, 2005
Binary Quasars in the Sloan Digital Sky Survey Joseph F. Hennawi Berkeley Hubble Symposium April 7, 2005
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Far-infrared properties of UV selected galaxies from z=4 to z=1.5: unveiling obscured star formation Véronique Buat & Sebastien Heinis With the contribution
Far-infrared properties of UV selected galaxies from z=4 to z=1.5: unveiling obscured star formation Véronique Buat & Sebastien Heinis With the contribution
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High Redshift Galaxies (Ever Increasing Numbers)
High Redshift Galaxies (Ever Increasing Numbers)
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Molecules in high redshift galaxies as probes of star formation and galaxy evolution Alain Omont (IAP, CNRS and Université Paris 6)
Molecules in high redshift galaxies as probes of star formation and galaxy evolution Alain Omont (IAP, CNRS and Université Paris 6)
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Receiver Schematic The figure below shows a schematic of the receiver. Each pixel in the spectrometer comprises a feedhorn that couples the incoming radiation
Receiver Schematic The figure below shows a schematic of the receiver. Each pixel in the spectrometer comprises a feedhorn that couples the incoming radiation
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Hubble Science Briefing 30 Doradus: Birthplace of giants and dwarfs Elena Sabbi June 7, 2012
Hubble Science Briefing 30 Doradus: Birthplace of giants and dwarfs Elena Sabbi June 7, 2012
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Galaxy Formation and Evolution Dr. Pimol Moth Astronomy Instructor Hartnell College
Galaxy Formation and Evolution Dr. Pimol Moth Astronomy Instructor Hartnell College
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Albert Stebbins Theoretical Astrophysics Group Fermi National Laboratory stebbins@fnal.gov Theoretical Astrophysics Group @ Fermilab Annual DOE Review
Albert Stebbins Theoretical Astrophysics Group Fermi National Laboratory [email protected] Theoretical Astrophysics Group @ Fermilab Annual DOE Review
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