Zobrazeno 1 - 10
of 2 207
pro vyhledávání: '"Unger S"'
Novel prediction models for hyperketonemia using bovine milk Fourier-transform infrared spectroscopy
Autor:
Walleser, E., Reyes, J.F. Mandujano, Anklam, K., Pralle, R.S., White, H.M., Unger, S., Panne, N., Kammer, M., Plattner, S., Döpfer, D.
Publikováno v:
In Preventive Veterinary Medicine April 2023 213
Akademický článek
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Autor:
Unger, S. J., Clegg, P. E., Stacey, G. J., Cox, P., Fischer, J., Greenhouse, M., Lord, S. D., Luhman, M. L., Satyapal, S., Smith, H. A., Spinoglio, L., Wolfire, M.
We present the first full FIR spectrum of Centaurus A (NGC 5128) from 43 - 196.7 um. The data was obtained with the ISO Long Wavelength Spectrometer (LWS). We conclude that the FIR emission in a 70 arcsec beam centred on the nucleus is dominated by s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0002024
Autor:
Fischer, J., Luhman, M. L., Satyapal, S., Greenhouse, M. A., Stacey, G. J., Bradford, C. M., Lord, S. D., Brauher, J. R., Unger, S. J., Clegg, P. E., Smith, H. A., Melnick, G., Colbert, J. W., Malkan, M. A., Spinoglio, L., Cox, P., Harvey, V., Suter, J. -P., Strelnitski, V.
Publikováno v:
Astrophys.Space Sci. 266 (1999) 91-98
Based on far-infrared spectroscopy of a small sample of nearby infrared-bright and ultraluminous infrared galaxies (ULIRGs) with the ISO Long Wavelength Spectrometer, we find a dramatic progression in ionic/atomic fine-structure emission line and mol
Externí odkaz:
http://arxiv.org/abs/astro-ph/9911310
Akademický článek
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Autor:
Jiang, Shibin, Digonnet, Michel J. F., Unger, S., Reichert, A., Aichele, C., Lindner, F., Kuhn, S., Lorenz, A., Bierlich, J., Schwuchow, A., Eschrich, T., Schaarschmidt, K., Lorenz, M., Wondraczek, K., Habisreuther, T.
Publikováno v:
Proceedings of SPIE; March 2024, Vol. 12882 Issue: 1 p128820F-128820F-7, 1159388p
Autor:
Colbert, J. W., Malkan, M. A., Clegg, P. E., Cox, P., Fischer, J., Lord, S. D., Luhman, M., Satyapal, S., Smith, H. A., Spinoglio, L., Stacey, G., Unger, S. J.
We present the first complete far-infrared spectrum (43 to 197 um) of M82, the brightest infrared galaxy in the sky, taken with the Long Wavelength Spectrometer of the Infrared Space Observatory (ISO). We detected seven fine structure emission lines,
Externí odkaz:
http://arxiv.org/abs/astro-ph/9810188
V635 Cas is the optical counterpart of the X-ray binary system 4U 0115+63. It was previously tentatively identified as a Be star based on its optical colours and the presence of H alpha emission. Our observations indicate that it is an O9e star. This
Externí odkaz:
http://arxiv.org/abs/astro-ph/9802086
Autor:
Unger, S., Ferreira, C.R., Mortier, G.R., Ali, H., Bertola, D.R., Calder, A., Cohn, D.H., Cormier-Daire, V., Girisha, K.M., Hall, C., Krakow, D., Makitie, O., Mundlos, S., Nishimura, G., Robertson, S.P., Savarirayan, R., Sillence, D., Simon, M., Sutton, V.R., Warman, M.L., Superti-Furga, A.
Publikováno v:
American journal of medical genetics. Part A, vol. 191, no. 5, pp. 1164-1209
The "Nosology of genetic skeletal disorders" has undergone its 11th revision and now contains 771 entries associated with 552 genes reflecting advances in molecular delineation of new disorders thanks to advances in DNA sequencing technology. The mos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1900::84a4ea32d072f51c13fb162fb5c60607
https://serval.unil.ch/notice/serval:BIB_A5308577ECD7
https://serval.unil.ch/notice/serval:BIB_A5308577ECD7
Autor:
Paredes, J. M., Marziani, P., Marti, J., Fabregat, J., Coe, M. J., Everall, C., Figueras, F., Jordi, C., Norton, A. J., Prince, T., Reglero, V., Roche, P., Torra, J., Unger, S. J., Zamanov, R.
We present new optical and infrared photometric observations and high resolution H$\alpha$ spectra of the periodic radio star \lsi. The optical photometric data set covers the time interval 1985-1993 and amounts to about a hundred nights. A period of
Externí odkaz:
http://arxiv.org/abs/astro-ph/9402016