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Featured researches published by Jochen M. M. Horn.


Astronomical Telescopes and Instrumentation | 1998

Heterodyne instrument for FIRST (HIFI): preliminary design

Thijs de Graauw; N. Whyborn; Hermann van de Stadt; Gerard Beaudin; D. A. Beintema; Victor Belitsky; Phillipe Cais; E. Caux; Maurice Gheudin; A. Cros; P. de Groene; Anders Emrich; Neil A. Erickson; Todd Gaier; Juan Daniel Gallego-Puyol; J. R. Gao; Paul Hartogh; N. Honingh; Jochen M. M. Horn; Karl Jacobs; R. Kruisinga; F. Lura; Alain Lecacheux; Vincento Natale; R. Orfei; John C. Pearson; T. G. Phillips; Peter Roelfsema; Carlo Rosolen; Morvan Salez

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 - 1910 GHz and 2400 - 2700 GHz. The first five bands will use SIS mixers and varactor frequency multipliers while in the sixth band a laser photomixer local oscillator will pump HEB mixers. HIFI will have an instantaneous bandwidth of 4 GHz, analyzed in parallel by two types of spectrometers: a pair of wide-band spectrometers (WBS), and a pair of high- resolution spectrometer (HRS). The wide-band spectrometer will use acousto-optic technology with a frequency resolution of 1 MHz and a bandwidth of 4 GHz for each of the two polarizations. The HRS will provide two combinations of bandwidth and resolution: 1 GHz bandwidth at 200 kHz resolution, and at least 500 MHz at 100 kHz resolution. The HRS will be divided into 4 or 5 sub-bands, each of which can be placed anywhere within the full 4 GHz IF band. The instrument will be able to perform rapid and complete spectral line surveys with resolving powers from 103 up to 107 (300 - 0.03 km/s) and deep line observations.


Archive | 2007

Spectral domain optical coherence tomography system

Matthew J. Everett; Scott A. Meyer; Martin Hacker; Jochen M. M. Horn; Christopher J. R. V. Baker; Kabir M. Arianta; James P. Foley; Jochen Straub; Yue Qiu; David Landhuis; Claus Flachenecker; Clement Louis-rene Viard


Archive | 2005

Littrow spectrometer and a spectral domain optical coherence tomography system with a littrow spectrometer

Matthew J. Everett; Yan Zhou; Jochen M. M. Horn; Keith E. O'Hara; James P. Foley


Archive | 2012

Ultra wide-field optical coherence tomography

Jochen M. M. Horn; Andre Malz; Christopher J. R. V. Baker; Oliver Wirth


Archive | 2002

Method and apparatus for measuring optical aberration of eye

James P. Foley; Jochen M. M. Horn; Ming Lai; Scott A. Meyer; Jay Wei; ウェイ ジェイ; ピー フォーリー ジェームス; エイ マイアー スコット; ライ ミン; エム ホルン ヨヘン


Astronomical Telescopes and Instrumentation | 2003

Toward very large bandwidth with acousto-optical spectrometers

R. Schieder; Oliver Siebertz; Csaba Gal; Michael Olbrich; Frank Schloeder; R. Bieber; Frank Schmuelling; Volker Tolls; Jochen M. M. Horn


Archive | 1996

Acousto-Optical Spectrometers in Space

R. Schieder; Jochen M. M. Horn; Oliver Siebertz; Markus Klumb; Johannes Frerick; Volker Tolls


Archive | 2012

Tomographie de cohérence optique à champ ultralarge

Jochen M. M. Horn; Andre Malz; Christopher J. R. V. Baker; Oliver Wirth


Archive | 2009

Chirurgisches mikroskopiesystem mit optischer kohärenz-tomografieeinrichtung

Christoph Hauger; Markus Seesselberg; Keith E. O'Hara; Yue Qiu; Xing Wei; Jochen M. M. Horn; Peter Reimer


Archive | 2009

Chirurgisches Mikroskopsystem mit optischer Kohärenz-Tomographieeinrichtung

Christoph Hauger; Jochen M. M. Horn; Keith E. O'Hara; Yue Qiu; Peter Reimer; Markus Seesselberg; Xing Wei

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