- Added "Calculate" check box in FocusCraft for easy enabling/disabling the HFD/FWHM calculation- Added support for PrimaLuceLab EAGLE EYE ( in Sky & T settings tab)- Added support for PrimaLuceLab EAGLE GPS (in Extra Devices) - Added remembering the selected button in Graphs between the ...
3. The differential micro-lensing of the BELs confirms that the size of an emission line region is anti-correlated with the FWHM of the corresponding ... D Sluse,Claeskens, J.-F.,Hutsemékers, D.,... - 《Astronomy & Astrophysics》 被引量: 35发表: 2006年 New algebraic models of soc...
There ya go - as far as planetary is concerned. Back to long exposure imaging. I'll briefly go over what is involved, and why Astronomy.tools calculation is wrong. In long exposure imaging there are several factors that contribute to total FWHM of the stars in the image - that is seeing...
A bandpass filter is a combination of a longpass and a shortpass filter. The center wavelength of this filter is deduced as the arithmetic mean of the wavelengths measured at 50% of peak transmission and the value of FWHM is calculated as the bandwidth at 50% of peak transmission....
I've loaded in your Eskimo frames and experimented. Still experimenting -- lots of variables affect picture quality. That stack has a few images that can be weeded out using the FWHM filter. Play around with it. The less tolerance you have for subpar frames, the better your final image wi...
As QE max is only about 30% in this region I had to use max gain and 8-12 sec images to get sufficient stars to plate solve; There was surprisingly little sensor noise at these frequencies; A Bahtinov mask did not work in this frequency band, so I went back to FWHM ...
[87]. The FWHM of the restoring beam is 0″.15×0″.150″.15×0″.15. Figure 1. Observational evidence of radio jets in RQ AGN. (a) 6 cm continuum images of NGC 1068, taken from Gallimore et al. [86]. Left panel: VLA 6 cm radio continuum image of NGC 1068. The restoring...
Meanwhile, Raman spectroscopy, applied to 16 Ryugu particles, indicated that MOM/IOM was distributed ubiquitously throughout the matrix and revealed a slight difference between the particles in terms of their G-band FWHM and peak center positions. The G-band arises from the in-plane stretching of...
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[87]. The FWHM of the restoring beam is 0″.15×0″.150″.15×0″.15. 2.2. Evidence That the Linear Radio Structures Are Jets Here, we discuss the evidence that the linear radio structures seen in about 50% of RQ AGN represent jets, i.e., collimated outflows of radio-emitting ...