Abstract
We present a test-study of the "seeing" 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 "seeing" 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 "seeing", 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 "seeing" 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 "seeing" 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.
| Original language | English |
|---|---|
| Title of host publication | AIP Conference Proceedings |
| Pages | 901-905 |
| Number of pages | 5 |
| Volume | 848 |
| DOIs | |
| Publication status | Published - 2006 |
| Externally published | Yes |
| Event | 7th International Conference of the Hellenic Astronomical Society - Lixourion, Kefallinia Island Duration: 8 Sep 2005 → 11 Sep 2005 |
Other
| Other | 7th International Conference of the Hellenic Astronomical Society |
|---|---|
| City | Lixourion, Kefallinia Island |
| Period | 8/9/05 → 11/9/05 |
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Keywords
- Atmospheric effects
- Site testing
ASJC Scopus subject areas
- Physics and Astronomy(all)
Cite this
A test of the Kryonerion "seeing" with DIMM equipment. / Mislis, Dimitrios; Harlaftis, E. T.; Buckley, D.; Gazeas, K.; Stathoulis, K.; Dimou, G.; Seiradakis, J. H.
AIP Conference Proceedings. Vol. 848 2006. p. 901-905.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
TY - GEN
T1 - A test of the Kryonerion "seeing" with DIMM equipment
AU - Mislis, Dimitrios
AU - Harlaftis, E. T.
AU - Buckley, D.
AU - Gazeas, K.
AU - Stathoulis, K.
AU - Dimou, G.
AU - Seiradakis, J. H.
PY - 2006
Y1 - 2006
N2 - We present a test-study of the "seeing" 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 "seeing" 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 "seeing", 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 "seeing" 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 "seeing" 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.
AB - We present a test-study of the "seeing" 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 "seeing" 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 "seeing", 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 "seeing" 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 "seeing" 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.
KW - Atmospheric effects
KW - Site testing
UR - http://www.scopus.com/inward/record.url?scp=33846536181&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=33846536181&partnerID=8YFLogxK
U2 - 10.1063/1.2348076
DO - 10.1063/1.2348076
M3 - Conference contribution
AN - SCOPUS:33846536181
SN - 0735403430
SN - 9780735403437
VL - 848
SP - 901
EP - 905
BT - AIP Conference Proceedings
ER -