Zobrazeno 1 - 10
of 123
pro vyhledávání: '"Bauwens E"'
Autor:
Bouchet, P., Garcia-Marin, M., Lagage, P. -O., Amiaux, J., Augueres, J. -L., Bauwens, E., Blommaert, J. A. D. L., Chen, C. H., Detre, O. H., Dicken, D., Dubreuil, D., Galdemard, Ph., Gastaud, R., Glasse, A., Gordon, K. D., Gougnaud, F., Guillard, P., Justtanont, K., Krause, O., Leboeuf, D., Longval, Y., Martin, L., Mazy, E., Moreau, V., Olofsson, G., Ray, T. P., Reess, J. -M., Renotte, E., Ressler, M. E., Ronayette, S., Salasca, S., Scheithauer, S., Sykes, J., Thelen, M. P., Wells, M., Wright, D., Wright, G. S.
Publikováno v:
2015 Publications of the Astronomical Society of the Pacific, Volume 127, issue 953, pp.612-622
In this article, we describe the MIRI Imager module (MIRIM), which provides broad-band imaging in the 5 - 27 microns wavelength range for the James Webb Space Telescope. The imager has a 0"11 pixel scale and a total unobstructed view of 74"x113". The
Externí odkaz:
http://arxiv.org/abs/1508.02488
Autor:
Glasse, Alistair, Rieke, G. H., Bauwens, E., Garcıa-Marın, Macarena, Ressler, M. E., Rost, Steffen, Tikkanen, T. V., Vandenbussche, B., Wright, G. S.
Publikováno v:
PASP, 127, 686, 2015
We present an estimate of the performance that will be achieved during on orbit operations of the JWST Mid Infrared Instrument, MIRI. The efficiency of the main imager and spectrometer systems in detecting photons from an astronomical target are pres
Externí odkaz:
http://arxiv.org/abs/1508.02427
Autor:
Jacobs, V. A., Østensen, R. H., Van Winckel, H., Bloemen, S., Pápics, P. I., Raskin, G., Debosscher, J., Uttenthaler, S., Van Aarle, E., Waelkens, C., Bauwens, E., Verhoelst, T., Gielen, C., Lehmann, H., Oreiro, R.
A close substellar companion has been claimed to orbit the bright sdB star HD 149382 with a period of 2.391d. In order to check this important discovery we gathered 26 high resolution spectra over 55 days with the HERMES spectrograph on the 1.2m Merc
Externí odkaz:
http://arxiv.org/abs/1101.4158
Autor:
Saesen, S., Pigulski, A., Carrier, F., Michalska, G., Aerts, C., De Ridder, J., Briquet, M., Handler, G., Kolaczkowski, Z., Acke, B., Bauwens, E., Beck, P. G., Blom, Y., Blommaert, J., Broeders, E., Cherix, M., Davignon, G., Debosscher, J., Degroote, P., Decin, L., Dehaes, S., De Meester, W., Deroo, P., Desmet, M., Drummond, R., Eggen, J. R., Fu, J., Gazeas, K., Gelven, G. A., Gielen, C., Huygen, R., Jiang, X., Kalomeni, B., Kim, S. -L., Kim, D. H., Kopacki, G., Kwon, J. -H., Ladjal, D., Lee, C. -U., Lee, Y. -J., Lefever, K., Leitner, A., Lenz, P., Liakos, A., Lorenz, D., Narwid, A., Niarchos, P., Oestensen, R., Poretti, E., Prins, S., Provencal, J., Antolin, E. Puga, Puschnig, J., Raskin, G., Reed, M. D., Reyniers, M., Schmidt, E., Schmitzberger, L., Spano, M., Steininger, B., Steslicki, M., Uytterhoeven, K., Vanautgaerden, J., Vandenbussche, B., Van Helshoecht, V., Vanhollebeke, E., Van Winckel, H., Verhoelst, T., Vuckovic, M., Waelkens, C., Wolf, G. W., Yakut, K., Zhang, C., Zima, W.
Publikováno v:
Astronomische Nachrichten 331, No. 9/10, 1080 - 1083 (2010)
As a result of the variability survey in Chi Persei and NGC6910, the number of Beta Cep stars that are members of these two open clusters is increased to twenty stars, nine in NGC6910 and eleven in Chi Persei. We compare pulsational properties, in pa
Externí odkaz:
http://arxiv.org/abs/1004.2853
Autor:
Yakut, K., Zima, W., Kalomeni, B., Van Winckel, H., Waelkens, C., De Cat, P., Bauwens, E., Vuckovic, M., Saesen, S., Guillou, L. Le, Parmaksizoglu, M., Uluc, K., Khamitov, I., Raskin, G., Aerts, C.
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M67 (NGC 2682). About 3600 frames spread over 28 nights were obtained with the 1.5 m Russian-Turkish and 1.2 m Mercator telescopes. High-precision observations
Externí odkaz:
http://arxiv.org/abs/0906.4908
Autor:
Dehaes, S., Bauwens, E., Decin, L., Eriksson, K., Raskin, G., Butler, B., Dowell, C. D., Ali, B., Blommaert, J. A. D. L.
Context: Among late-type red giants, an interesting change occurs in the structure of the outer atmospheric layers as one moves to later spectral types in the Hertzsprung-Russell diagram: a chromosphere is always present, but the coronal emission dim
Externí odkaz:
http://arxiv.org/abs/0905.1240
Autor:
Gorlé, N., Blaecher, C., Bauwens, E., Vandendriessche, C., Balusu, S., Vandewalle, J., Van Cauwenberghe, C., Van Wonterghem, E., Van Imschoot, G., Liu, C., Ducatelle, R., Libert, C., Haesebrouck, F., Smet, A., Vandenbroucke, R.E.
Publikováno v:
In Brain Behavior and Immunity March 2018 69:35-47
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Akademický článek
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