Performance characteristics of doped-Ge photoconductors for the Infrared Space Observatory Long Wavelength Spectrometer

1993 ◽  
Author(s):  
Sarah E. Church ◽  
Matthew J. Griffin ◽  
Marc C. Price ◽  
Peter A. R. Ade ◽  
Roger J. Emery ◽  
...  
Keyword(s):  
Performance Characteristics ◽  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength

scholarly journals The Infrared Space Observatory

1990 ◽  
Vol 123 ◽  
pp. 205-214 ◽  
Author(s):  
C.J. Cesarsky ◽  
M.F. Kessler
Keyword(s):  
Optical Sensors ◽  
European Space Agency ◽  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength ◽  
Space Agency ◽  
Pointing Accuracy ◽  
Funded Project ◽  
Astronomical Satellite ◽  
The Universe

AbstractThe Infrared Space Observatory (ISO), a fully approved and funded project of the European Space Agency (ESA), is an astronomical satellite, which will operate at wavelengths from 3–200 μm. ISO will provide astronomers with a unique facility of unprecedented sensitivity for a detailed exploration of the universe ranging from objects in the solar system right out to distant extragalactic sources. The satellite essentially consists of a large cryostat containing at launch about 2300 litres of superfluid helium to maintain the Ritchey-Chrétien telescope, the scientific instruments and the optical baffles at temperatures between 2K and 8K. The telescope has a 60-cm diameter primary mirror and is diffraction-limited at a wavelength of 5μm. A pointing accuracy of a few arc seconds is provided by a three-axis-stabilisation system consisting of reaction wheels, gyros and optical sensors. ISO’s instrument complement consists of four instruments, namely: a photo-polarimeter (3–200μm), a camera (3–17μm), a short wavelength spectrometer (3–45μm) and a long wavelength spectrometer (45–180μm). These instruments are being built by international consortia of scientific institutes and will be delivered to ESA for in-orbit operations. ISO will be launched in 1993 by an Ariane 4 into an elliptical orbit (apogee 70000km and perigee 1000km) and will be operational for at least 18 months. In keeping with ISO’s role as an observatory, two-thirds of its observing time will be made available to the european and american astronomical community.

Measuring the performance of the Infrared Space Observatory long-wavelength spectrometer

1993 ◽  
Author(s):  
Roger J. Emery ◽  
Bruce M. Swinyard ◽  
Kenneth J. King ◽  
Sarah E. Church
Keyword(s):  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength

Detection of the 62 Micron Crystalline H[TINF]2[/TINF]O Ice Feature in Emission toward HH 7 with the [ITAL]Infrared Space Observatory[/ITAL] Long-Wavelength Spectrometer

1999 ◽  
Vol 521 (1) ◽  
pp. L71-L74 ◽  
Author(s):  
Sergio Molinari ◽  
Cecilia Ceccarelli ◽  
Glenn J. White ◽  
Paolo Saraceno ◽  
Brunella Nisini ◽  
...  
Keyword(s):  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength

[ITAL]Infrared Space Observatory[/ITAL]–Long Wavelength Spectrometer Detection of the 112 Micron HD [ITAL]J[/ITAL] = 1 → 0 Line toward the Orion Bar

1999 ◽  
Vol 515 (1) ◽  
pp. L29-L33 ◽  
Author(s):  
Christopher M. Wright ◽  
Ewine F. van Dishoeck ◽  
Pierre Cox ◽  
Sunil D. Sidher ◽  
Martin F. Kessler
Keyword(s):  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength

scholarly journals ISO results on AGB and post-AGB objects

1997 ◽  
Vol 180 ◽  
pp. 139-144
Author(s):  
P. Cox
Keyword(s):  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength

We present results obtained on well-known AGB and post-AGB sources with the Long Wavelength Spectrometer (LWS) and ISOCAM on board the Infrared Space Observatory (ISO). The main findings of these studies are briefly summarized.

First detection of thermal H2O Emission from a Herbig-Haro Object

1997 ◽  
Vol 178 ◽  
pp. 393-396
Author(s):  
R. Liseau ◽  
Keyword(s):  
Shock Waves ◽  
Shock Model ◽  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength

The first detection of thermal H2O emission from an Herbig-Haro flow was made with the LWS (Long Wavelength Spectrometer) aboard ISO (Infrared Space Observatory). In addition to H2O, rotational lines of CO and OH as well as lines from [O I] and [C II] were also recorded from HH 54. These observations are consistent with the concept of interstellar shock waves, but a quantitative unifying shock model, capable of explaining all observations, has yet to be developed.

scholarly journals A long-wavelength view on galaxy evolution from deep surveys by the Infrared Space Observatory

2001 ◽  
Vol 378 (1) ◽  
pp. 1-29 ◽  
Author(s):  
A. Franceschini ◽  
H. Aussel ◽  
C. J. Cesarsky ◽  
D. Elbaz ◽  
D. Fadda
Keyword(s):  
Galaxy Evolution ◽  
Space Observatory ◽  
Infrared Space Observatory ◽  
Long Wavelength
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