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time development of recurrent nova ci aquilaes 2000 outburst between 0.8 and 2.5 microns.pdf
time development of recurrent nova ci aquilaes 2000 outburst between 0.8 and 2.5 microns
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a simple method to incorporate water vapor absorption in the 15 microns remote temperature sounding(499.28kb).pdf
a simple method to incorporate water vapor absorption in the 15 microns remote temperature sounding(499.28kb)
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new experimental limits on macroscopic forces below 100 microns.pdf
arXiv:hep-ph/0210004v311 Mar 2003New Experimental Limits onMacroscopic Forces Below 100 MicronsJoshu
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towards high-efficiency mid-infrared diode lasers operating from 3-5 microns(474.06kb).pdf
towards high-efficiency mid-infrared diode lasers operating from 3-5 microns(474.06kb)
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Adaptive Optics Imaging at 1-5 Microns on Large ....pdf
Adaptive Optics Imaging at 1–5 Microns on Large …
8
The Zeeman-sensitive Emission Lines of Mg I at 12 Microns in....pdf
The Zeeman-sensitive Emission Lines of Mg I at 12 Microns in…
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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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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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