Zobrazeno 1 - 10
of 236
pro vyhledávání: '"Solheim J. E."'
Autor:
Solheim J. E.
Publikováno v:
Open Astronomy, Vol 12, Iss 4, Pp 463-470 (2003)
The Whole Earth Telescope (WET) saw first light in 1988. It was invented by scientists from the Astronomy Department, University of Texas at Austin. The idea was to generate a world-wide network of cooperating astronomical observatories to obtain uni
Externí odkaz:
https://doaj.org/article/0250a674708d47019e9b2659f7ae0765
Autor:
Pakštienė E., Solheim J. E.
Publikováno v:
Open Astronomy, Vol 12, Iss 2, Pp 221-242 (2003)
Account of the extinction in the Earth’s atmosphere is an important part of the WET light curve reduction procedures. Usually, WET observations are not corrected for the second order extinction effects: the dependence of the extinction coefficient
Externí odkaz:
https://doaj.org/article/31c9cea117db45eb812828e909ea9cab
Autor:
Solheim J. E., Sullivan D. J.
Publikováno v:
Open Astronomy, Vol 12, Iss 2, Pp 211-220 (2003)
The goal of the WET collaboration is to produce a photometric light curve as continuous and accurate as possible, given the weather and technical constraints. In order to join light curves from different observers, it is important that all observer
Externí odkaz:
https://doaj.org/article/79200364d2304af9b630dda30555024a
Publikováno v:
Open Astronomy, Vol 9, Iss 2, Pp 205-210 (2000)
Externí odkaz:
https://doaj.org/article/4fedee20570b40f481b458c4fc20c6ef
Autor:
Reed M. D., Kilkenny D., Kawaler S. D., Mukadam A., Kleinman S. J., Nitta-Kleinman A., Provencal J. L., Watson T., Sullivan D., Sullivan T., Shobbrook B., Jiang X. J., Ashoka B. N., Seetha S., Leibowitz E., Ibbetson P., Mendelson H., Meistas E. G., Kalytis R., Alisauskas D., O'Donoghue D., Martinez P., Wyk F. van, Stobie R., Marang F., Zola S., Krzesinski J., Ogloza W., Mosaklik P., Silvotti R., Piccioni A., Vauclair G., Dolez N., Rene-Fremy J., Chevreton M., Ulla A., Dreizler S., Schuh S., Deetjen J., Solheim J. E., Perez J., Suarez O., Manteiga M., Burleigh M., Barstow M., Kepler S. O., Kanaan A., Giovannini O., Metcalfe T., Ostensen R.
Publikováno v:
Open Astronomy, Vol 9, Iss 2, Pp 183-196 (2000)
Externí odkaz:
https://doaj.org/article/f42f34d7ff6d4a258bcb3310c4f4ac0d
Autor:
Solheim J. E., Provencal J. L.
Publikováno v:
Open Astronomy, Vol 7, Iss 2, Pp 277-286 (1998)
Externí odkaz:
https://doaj.org/article/39d2ff82054c4543a50ed11b737e9742
Autor:
Solheim J. E.
Publikováno v:
Open Astronomy, Vol 7, Iss 2, Pp 319-328 (1998)
Externí odkaz:
https://doaj.org/article/43a13bc5259d4125a581006098bd47c5
Autor:
Marar Τ. Μ. K., Seetha S., Ashoka B. N., Kasturirangan K., Mahra H. S., Bhattacharyya J. C., Leibowitz Ε. M., Hemar S., Mendelson H., Ibbetson P. A., O’Donoghue D., Buckley D. A. H., Βreger M., Handler G., Sperl M., Serkowitsch E., Reegen P., Moskalik P., Zola S., Pajdosz G., Krzesinski J., Silvotti R., Vauclair G., Dolez N., Solheim J. E., Pfeiffer B., Kepler S. O., Kanaan A., Provencal J., Kawaler S. D., O'Brien M. S., Nather R. E., Winget D. E., Kleinman S., Nitta A., Bradley P. A., Guzik J. A., Clemens C., Sullivan D. J., Jiang X.
Publikováno v:
Open Astronomy, Vol 7, Iss 2, Pp 287-292 (1998)
Externí odkaz:
https://doaj.org/article/f0267597886441339ee2f98870c6d1c7
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics, (2013)
Callebaut et al. (2012)'s claim that Scafetta (2010)'s results about a correlation between 20-year and 60-year temperature cycles and the orbital motion of Jupiter and Saturn were not confirmed by Humlum et al. (2011) is erroneous and severely mislea
Externí odkaz:
http://arxiv.org/abs/1304.2023
Autor:
Reed, M. D., Harms, S. L., Poindexter, S., Zhou, A. -Y., Eggen, J. R., Morris, M. A., Quint, A. C., McDaniel, S., Baran, A., Dolez, N., Kawaler, S. D., Kurtz, D. W., Moskalik, P., Riddle, R., Zola, S., Ostensen, R. H., Solheim, J. -E., Kepler, S. O., Costa, A. F. M., Provencal, J. L., Mullally, F., Winget, D. W., Vuckovic, M., Crowe, R., Terry, D., Avila, R., Berkey, B., Stewart, S., Bodnarik, J., Bolton, D., Binder, P. -M., Sekiguchi, K., Sullivan, D. J., Kim, S. -L., Chen, W. -P., Chen, C. -W., Lin, H. -C., Jian, X. -J., Wu, H., Gou, J. -P., Liu, Z., Leibowitz, E., Lipkin, Y., Akan, C., Cakirli, O., Janulis, R., Pretorius, R., Ogloza, W., Stachowski, G., Paparo, M., Szabo, R., Csubry, Z., Zsuffa, D., Silvotti, R., Marinoni, S., Bruni, I., Vauclair, G., Chevreton, M., Matthews, J. M., Cameron, C., Pablo, H.
KPD 1930+2752 is a short-period pulsating subdwarf B (sdB) star. It is also an ellipsoidal variable with a known binary period just over two hours. The companion is most likely a white dwarf and the total mass of the system is close to the Chandresak
Externí odkaz:
http://arxiv.org/abs/1011.0387