Free Access
Table 2
Overview of the instruments involved in the spectroscopic observations during the three last eclipses at epochs E = 8, E = 9, and E = 10.
| Observatory | Country | Telescope type | Diameter [m] | Spectrograph | Res. power | Spectral reg. | Epoch | N |
|
|
||||||||
| NOT, La Palma | Canary Isl. | Ritchey-Chrétien | 2.56 | FIES-Echelle | 48 000 | 3680–7280 Å | 10 | 4 |
| Rozhen | Bulgaria | Ritchey-Chrétien | 2.0 | Coude | 15 000, 30 000 | Hα, Hβ, Na i | 8, 9, 10 | 38 |
| Asiago | Italy | Cassegrain | 1.82 | Echelle | 20 000 | 4600–9200 Å | 9 | 5 |
| SPM | Mexico | Ritchey-Chrétien | 2.12 | Echelle | 18 000 | 3700–6800 Å | 9 | 1 |
| DDO | Canada | Cassegrain | 1.88 | Cassegrain | 16 000 | Hα, Na i | 9 | 16 |
| Terskol | Russia | Ritchey-Chrétien | 2.0 | Echelle | 13 500 | 4200–6700 Å | 9 | 7 |
| Asiago | Italy | Cassegrain | 1.82 | AFOSC/echelle | 3600 | 3600–8800 Å | 9 | 3 |
| Piwnice | Poland | Schmidt-Cassegrain | 0.9 | CCS | 2000–4000 | 3500–10 500 Å | 9, 10 | 26 |
Notes. N is the number of spectra.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.