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The top documents tagged [continuum sources]

High Resolution Observations of Orion-KL: Insight into its Chemical Complexity D. N. Friedel S. L. Widicus Weaver
High Resolution Observations of Orion-KL: Insight into its Chemical Complexity D. N. Friedel S. L. Widicus Weaver
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Chapter 25 Instruments for Optical Spectroscopy INSTRUMENT COMPONENTS Most spectroscopic instruments in the UV/visible and IR regions are made up of five
Chapter 25 Instruments for Optical Spectroscopy INSTRUMENT COMPONENTS Most spectroscopic instruments in the UV/visible and IR regions are made up of five
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Sources Usually electrical to optical converters 1.Continuum sources a. Incandescent sources Blackbody sources Tungsten filament sources b. ASE (EDFAs)
Sources Usually electrical to optical converters 1.Continuum sources a. Incandescent sources Blackbody sources Tungsten filament sources b. ASE (EDFAs)
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UV instrumentation Abu Yousuf, PhD Associate Professor Department of Chemical Engineering & Polymer Science Shahjalal University of Science & Technology
UV instrumentation Abu Yousuf, PhD Associate Professor Department of Chemical Engineering & Polymer Science Shahjalal University of Science & Technology
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CHM260 - UV-VIS
CHM260 - UV-VIS
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Spectral and VLBI-structure monitoring of OH-maser flare in W75N: preliminary results Alexey Alakoz & Vyacheslav Slysh Astro Space Center Moscow, Russia
Spectral and VLBI-structure monitoring of OH-maser flare in W75N: preliminary results Alexey Alakoz & Vyacheslav Slysh Astro Space Center Moscow, Russia
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Neutral Hydrogen Gas in Star Forming Galaxies at z=0.24 Philip Lah Frank Briggs (ANU) Jayaram Chengalur (NCRA) Matthew Colless (AAO) Roberto De Propris
Neutral Hydrogen Gas in Star Forming Galaxies at z=0.24 Philip Lah Frank Briggs (ANU) Jayaram Chengalur (NCRA) Matthew Colless (AAO) Roberto De Propris
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Chapter 7 Components of Optical Instruments. Instruments for the ultraViolet (UV),ViSible, and infrared (IR) regions have enough features in common
Chapter 7 Components of Optical Instruments. Instruments for the ultraViolet (UV),ViSible, and infrared (IR) regions have enough features in common
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Z > 6 Surveys Represent the Current Frontier Motivation: - census of earliest galaxies (z=6, =0.95 Gyr) - contribution of SF to cosmic reionization -
Z > 6 Surveys Represent the Current Frontier Motivation: - census of earliest galaxies (z=6, =0.95 Gyr) - contribution of SF to cosmic reionization -
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Astrometry from VERA to SKA
Astrometry from VERA to SKA
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1962 Lederman,Schwartz,Steinberger Brookhaven National Laboratory
1962 Lederman,Schwartz,Steinberger Brookhaven National Laboratory
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Sanjay K. Pandey L.B.S.P.G.College, Gonda (India). Statistical Analysis of Redshifted Neutral Hydrogen
Sanjay K. Pandey L.B.S.P.G.College, Gonda (India). Statistical Analysis of Redshifted Neutral Hydrogen
218 views