@conference {28485,
	title = {A test of the Kryonerion {\textquoteleft}{\textquoteleft}seeing{\textquoteright}{\textquoteright} with DIMM equipment},
	volume = {848},
	year = {2006},
	month = {2006/08/1},
	pages = {901 - 905},
	abstract = {We present a test-study of the {\textquoteleft}{\textquoteleft}seeing{\textquoteright}{\textquoteright} at the Kryonerion Station of the National Observatory of Athens. We used a Differential Image Motion Monitor (DIMM) during July and October 2002 and found a median {\textquoteleft}{\textquoteleft}seeing{\textquoteright}{\textquoteright} of 0.68 arcseconds and 1.42 arcseconds, respectively. We also compared the technique against the Hartmann-version of the ESO-type DIMM method and found similar results within 0.05 arcseconds. For some reason, which is under investigation by international teams, the measurements of our ESO-type DIMM are underestimated by ~ 10\% compared to ESO-standard DIMM measurements. Simultaneous ESO-type DIMM measurements and standard gauss-fitting-technique measurements, taken with the Kryonerion 1.2m telescope (inside the dome) indicate that the {\textquoteleft}{\textquoteleft}seeing{\textquoteright}{\textquoteright}, as measured by the telescope is by 1 arcsecond larger. The above tests were performed in order to calibrate, test and make a brief sampling of the {\textquoteleft}{\textquoteleft}seeing{\textquoteright}{\textquoteright} at the Kryonerion Station with the aim to move eventually the equipment to the Emilios Harlaftis Astronomical Station the site of the new 2.3m ARISTARCHOS telescope - for a long-term {\textquoteleft}{\textquoteleft}seeing{\textquoteright}{\textquoteright} monitoring. As a by-product of this project, a new DIMM Station became operational at Mt. Holomon, in the premises of the University of Thessaloniki, in 2004.},
	keywords = {95.45.+i, 95.55.-n, Astronomical and space-research instrumentation, Observatories and site testing},
	isbn = {0094-243X},
	url = {https://ui.adsabs.harvard.edu/abs/2006AIPC..848..901M},
	author = {Mislis, D. and Harlaftis, E. T. and Buckley, D. and Gazeas, K. and Stathoulis, K. and Dimou, G. and Seiradakis, J. H.}
}
