Zobrazeno 1 - 10
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pro vyhledávání: '"Noll S"'
Autor:
Manjankattil, S. *, Dewi, G. *, Peichel, C. *, Creek, M. *, Bina, P. *, Lerohl, K. *, Deniz, K. *, Akhtar, L. *, Porter, R., Jr., Johnson, T.J., Noll, S. *, Kollanoor Johny, A.
Publikováno v:
In Journal of Applied Poultry Research September 2024 33(3)
Publikováno v:
EPJ Web of Conferences, Vol 89, p 01001 (2015)
Ground-based astronomical observations are influenced by scattering and absorption by molecules and aerosols in the Earth's atmosphere. They are additionally affected by background emission from scattered moonlight, zodiacal light, scattered starligh
Externí odkaz:
https://doaj.org/article/9efa9d5fafe3459093c221b13a9f7779
Akademický článek
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Autor:
Hayashino, T., Inoue, A. K., Kousai, K., Kashikawa, N., Mawatari, K., Matsuda, Y., Tejos, N., Prochaska, J. X., Iwata, I., Noll, S., Burgarella, D., Yamada, T., Akiyama, M.
In the SSA22 field which exhibits a large-scale proto-cluster at $z=3.1$, we carried out a spectroscopic survey for Lyman Break Galaxies (LBGs) with the VLT/VIMOS and identified 78 confident LBGs at $z=2.5$--4. We stacked their spectra in the observe
Externí odkaz:
http://arxiv.org/abs/1901.11242
Akademický článek
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Rotational temperatures Trot derived from lines of the same OH band are an important method to study the mesopause region near 87 km. To measure realistic temperatures, the rotational level populations have to be in local thermodynamic equilibrium (L
Externí odkaz:
http://arxiv.org/abs/1604.03961
Autor:
Smette, A., Sana, H., Noll, S., Horst, H., Kausch, W., Kimeswenger, S., Barden, M., Szyszka, C., Jones, A. M., Gallenne, A., Vinther, J., Ballester, P., Taylor, J.
Publikováno v:
A&A 576, A77 (2015)
Context: The interaction of the light from astronomical objects with the constituents of the Earth's atmosphere leads to the formation of telluric absorption lines in ground-based collected spectra. Correcting for these lines, mostly affecting the re
Externí odkaz:
http://arxiv.org/abs/1501.07239
Autor:
Moehler, S., Modigliani, A., Freudling, W., Giammichele, N., Gianninas, A., Gonneau, A., Kausch, W., Lancon, A., Noll, S., Rauch, T., Vinther, J.
While the near-infrared wavelength regime is becoming more and more important for astrophysics there is a marked lack of spectrophotometric standard star data that would allow the flux calibration of such data. Furthermore, flux calibrating medium- t
Externí odkaz:
http://arxiv.org/abs/1408.1797
Autor:
Noll, S., Kausch, W., Kimeswenger, S., Barden, M., Jones, A. M., Modigliani, A., Szyszka, C., Taylor, J.
Airglow emission lines, which dominate the optical-to-near-IR sky radiation, show strong, line-dependent variability on various time scales. Therefore, the subtraction of the sky background in the affected wavelength regime becomes a problem if plain
Externí odkaz:
http://arxiv.org/abs/1405.3679
Autor:
Kausch, W., Noll, S., Smette, A., Kimeswenger, S., Horst, H., Sana, H., Jones, A., Barden, M., Szyszka, C., Vinther, J.
Correcting for the sky signature usually requires supplementary calibration data which are very expensive in terms of telescope time. In addition, the scheduling flexibility is restricted as these data have to be taken usually directly before/after t
Externí odkaz:
http://arxiv.org/abs/1401.7768