dc.contributor.author |
Pearson, J. |
en_US |
dc.contributor.author |
Guesten, R. |
en_US |
dc.contributor.author |
Klein, T. |
en_US |
dc.contributor.author |
Whyborn, N. |
en_US |
dc.date.accessioned |
2004-09-23T17:41:49Z |
|
dc.date.available |
2004-09-23T17:41:49Z |
|
dc.date.issued |
2000-03-27 |
en_US |
dc.identifier.citation |
UV Optical and IR Space Telescopes and Instruments |
en_US |
dc.identifier.citation |
Munich, Germany |
en_US |
dc.identifier.clearanceno |
00-0417 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/14033 |
|
dc.description.abstract |
The Heterodyne Instrument for FIRST (HIFI) is comprised of five SIS receiver channels covering 480-1250 GHz and two HEB receiver channels covering parts of 1410-1910 GHz and 2400-2700 GHz. |
en_US |
dc.format.extent |
980990 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
sub-millimeter heterodyne far-infrared FIRST Instruments |
en_US |
dc.title |
The Local Oscillator System for the Heterodyne Instrument for FIRST (HIFI) |
en_US |