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Primary transit of the planet HD189733b at 3.6 and 5.8 microns.pdf
The hot Jupiter HD 189733b was observed during its primary transit using the nInfrared Array Camera on the Spitzer Space Telescope. The transit depths were nmeasured simultaneously at 3.6 and 5.8 microns. Our analysis yields values of n2.356 +- 0.019 % and 2.436 +- 0.020 % at 3.6 and 5.8 microns respectively, for na uniform source. We estimated the contribution of the limb-darkening and ns..
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4 Weiner S 1992 Bone structure from angstroms to microns.pdf
4 Weiner S 1992 Bone structure from angstroms to microns4 Weiner S 1992 Bone structure from angstroms to microns4 Weiner S 1992 Bone structure from angstroms to microns
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Normalised flux + constant Wavelength (microns)归一化通量+恒波长(微米).pdf
Normalised flux + constant Wavelength (microns)归一化通量+恒波长(微米)
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resolving iras 09111-1007 at 350 microns - a different path to ulirg formation.pdf
resolving iras 09111-1007 at 350 microns - a different path to ulirg formation
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GRACE Millimeters and Microns in Orbit - GDGPS.pdf
GRACE Millimeters and Microns in Orbit - GDGPS
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Towards 13 microns breeding ultrafine Merino sheep..pdf
Towards 13 microns breeding ultrafine Merino sheep.
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diode-pumped continuous wave operation and passively q-switched performances of a ndsc2sio5 laser crystal at 1.08 microns.pdf
diode-pumped continuous wave operation and passively q-switched performances of a ndsc2sio5 laser crystal at 1.08 microns
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Microns are used as the UNITS for measuring very small things such.doc
Microns are used as the UNITS for measuring very small things such
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HD 172555 detection of 63 microns [OI] emission in a debris disc.pdf
HD 172555 detection of 63 microns [OI] emission in a debris discHD 172555 detection of 63 microns [OI] emission in a debris discHD 172555 detection of 63 microns [OI] emission in a debris disc

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