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18
Aerosol-Jet Printing - 5 microns to 5 millimeters.pdf
M3DAerosol-JetPrinting millimetersMichaelRenn, Ph.DDirector, M3D Applications LaboratoryAbout Optome
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112
atmospheric transmittance from 0.25 to 28.5 microns computer code lowtran 3(4.18mb).pdf
atmospheric transmittance from 0.25 to 28.5 microns computer code lowtran 3(4.18mb)
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151
GaAsAlGaAs based Intensity and Phase Modulators 1.55 Microns Directly Grown on Silicon.pdf
CALIFORNIASANTA BARBARA GaAs/AlGaAs based Intensity PhaseModulators 1.55Microns Directly Grown Silic
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51
the hubble space telescope wide field camera 3 early release science data panchromatic faint object counts for 0.2-2 microns wavelength.pdf
AstrophysicalJournal Supplement Series, December, 2010Preprint typeset using LATEX style emulateapj
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269
mid-infrared galaxy morphology from the spitzer survey of stellar structure in galaxies (s 4g) the imprint of the de vaucouleurs revised hubble-sandage classification system at 3.6 microns.pdf
arXiv:1008.0805v1[astro-ph.CO] Aug2010Mid-Infrared Galaxy Morphology from SpitzerSurvey Galaxies(S4G
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58
the structure of ir luminous galaxies at 100 microns.pdf
arXiv:astro-ph/0003439v129 Mar 2000The Structure IRLuminous Galaxies 100MicronsEric C. Zink, Dan F.
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44
BEPTHS BESS THAN TEN MICRONS Bavid L S tyx is.pdf
diffusioncoefficient metalsforpenetration depths less than ten microns Item type text; Thesis-Reprod
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43
Detection of a Far IR Excess with DIRBE at 60 and 100 Microns.pdf
arXiv:astro-ph/0004175v112 Apr 2000Detection FarIR Excess 100MicronsDouglas P. Finkbeiner MarcDavisU
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44
the nature of star formation at 24 microns in the group environment at 0.3 z 0.55.pdf
arXiv:1107.2431v1[astro-ph.CO] 12 Jul 2011The Nature StarFormation 0.55K.D. Tyler1, G. H. Rieke1, D.
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44
large area mapping at 850 microns. v. analysis of the clump distribution in the orion a sou.pdf
Sep2006Large Area Mapping 850Microns. V. Analysis SouthMolecular CloudDoug Johnstone1,2& John Bally3
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