Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Jochen M. M. Horn"'
Autor:
Eric E. Becklin, Jochen M. M. Horn
Publikováno v:
Publications of the Astronomical Society of the Pacific. 113:997-1008
We present the results of a study that offers an observing scenario that can significantly enhance the scientific return from the Stratospheric Observatory for Infrared Astronomy (SOFIA). By examining atmospheric data from a satellite mission, we fou
Autor:
Jochen M. M. Horn, Ian S. McLean
Publikováno v:
SPIE Proceedings.
FLITECAM is a facility class instrument on SOFIA, operating form 1-5 microns. A 1024 by 1024 InSb ALADDIN II array will be used in a fully refractive optics system that provides three optical modes; imaging at a plate scale of 0.47 inch by 0.47 inch
Autor:
Jochen M. M. Horn, Oddvar O. Bendiksen, Nick Magnone, Ian S. McLean, George Brims, N. Molayem, Harvey Moseley, Evan Kress, John Goulter, Eric E. Becklin, Michael Spencer, John Milburn
Publikováno v:
SPIE Proceedings.
As a facility class instrument on SOFIA, FLITECAM will be developed at the UCLA Infrared Imaging Detector Laboratory. Its primary purpose is to test the SOFIA telescope imaging quality from 1.0 to 5.5 microns, using a 1024 X 1024 InSb ALADDIN II arra
Autor:
Eric E. Becklin, Jochen M. M. Horn
Publikováno v:
SPIE Proceedings.
A study of the average upper atmospheric conditions has been carried out in order to optimize the scientific return from SOFIA. By examination of atmospheric data from satellite missions, we found that at typical SOFIA flight altitudes (between 37,00
Autor:
Eric E. Becklin, Jochen M. M. Horn
Publikováno v:
ISO Surveys of a Dusty Universe ISBN: 9783540674795
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::caf9177920b657f2ffb94297c20aa395
https://doi.org/10.1007/3-540-45553-1_52
https://doi.org/10.1007/3-540-45553-1_52
Autor:
Frank Schloeder, Frank Schmuelling, Rudolf Schieder, Jochen M. M. Horn, Oliver Siebertz, C. Macke, Cornelius Moeckel
Publikováno v:
SPIE Proceedings.
Large bandwidth acousto-optical spectrometers have now reached a very high level of maturity. They achieve very compatible results in comparison with other spectrometer types like filterbanks, autocorrelators, and chirp transform spectrometers. In ad
Autor:
Anders Emrich, Gerhard W. Schwaab, Hermann van de Stadt, Alain Cros, Rudolf Schieder, Gerard Beaudin, Phillipe Cais, Stafford Withington, Jian-Rong Gao, Jochen M. M. Horn, Alain Lecacheux, P. de Groene, J. P. Starsky, D. A. Beintema, C. Rosolen, Maurice Gheudin, F. Lura, Victor Belitsky, Netty Honingh, Karl Jacobs, Peter Roelfsema, Paul Hartogh, Vincento Natale, Jürgen Stutzki, R. Kruisinga, Thomas G. Phillips, Todd D. Gaier, N. Whyborn, Steve Torchinsky, Karl-Friedrich Schuster, Neil A. Erickson, Thijs de Graauw, John C. Pearson, K. Wildeman, Boris van Leeuwen, Emmanuel Caux, H. Visser, Juan D. Gallego-Puyol, Morvan Salez, Jonas Zmuidzinas, R. Orfei
Publikováno v:
SPIE Proceedings.
We describe the preliminary design of the proposed Heterodyne Instrument for FIRST (HIFI). The instrument will have a continuous frequency coverage over the range from 480 to 1250 GHz in five bands, while a sixth band will provide coverage for 1410 -
Publikováno v:
SPIE Proceedings.
Acousto optical spectrometers (AOS) have become an attractive alternative to filterbanks or autocorrelators for applications in radioastronomy and in heterodyne as well as in laboratory spectroscopy. Due to continuous improvements, AOSs have now achi