The Multiband Imaging Photometer for SIRTF (MIPS) is to be designed to reach as closely as possible the fundamental sensitivity and angular resolution limits for SIRTF over the 3 to 700μm spectral region. It will use high performance photoconductive detectors from 3 to 200μm with integrating JFET amplifiers. From 200 to 700μm, the MIPS will use a bolometer cooled by an adiabatic demagnetization refrigerator. Over much of its operating range, the MIPS will make possible observations at and beyond the conventional Rayleigh diffraction limit of angular resolution
A Cryogenic Scan Mirror Mechanism (CSMM) has been developed for the Multi-band Imaging Photometer fo...
The Space Infrared Telescope Facility (SIRTF) is planned for launch by NASA in the mid-1990's. It wi...
The Space Infrared Facility (SIRTF) Guaranteed Time Observers will be executing deep surveys of the ...
The Multiband Imaging Photometer for SIRTF (MIPS) is to be designed to reach as closely as possible ...
The Multiband Imaging Photometer for SIRTF (MIPS) is to be designed to reach as closely as possible ...
We describe the test approaches and results for the Multiband Imaging Photometer for SIRTF. To verif...
The Multiband Imaging Photometer for SIRTF (MIPS) will be one of the three instruments on the Space ...
Traditional photoconductive detectors are used at 70 and 160 microns in the Multiband Imaging Photom...
The Multiband Imaging Photometer for Spitzer (MIPS) provides long wavelength capability for the miss...
The GTO program for the MIPS team is concentrated in two areas. First, the evolution of planetary de...
SIRTF, the Space Infrared Telescope Facility, is a NASA mission to provide a long lifetime, sensitiv...
The Cosmic Infrared Background is the focus of many observations, since its understanding is a key f...
The Space Infrared Telescope Facility (SIRTF), the fourth of the Great Observatories, will look thro...
A conceptual design for an infrared spectrometer capable of both low resolution (λ/Δ-λ = 50; 2.5-200...
The first six months of flight data from the Multiband Imaging Photometer for Spitzer (MIPS) were us...
A Cryogenic Scan Mirror Mechanism (CSMM) has been developed for the Multi-band Imaging Photometer fo...
The Space Infrared Telescope Facility (SIRTF) is planned for launch by NASA in the mid-1990's. It wi...
The Space Infrared Facility (SIRTF) Guaranteed Time Observers will be executing deep surveys of the ...
The Multiband Imaging Photometer for SIRTF (MIPS) is to be designed to reach as closely as possible ...
The Multiband Imaging Photometer for SIRTF (MIPS) is to be designed to reach as closely as possible ...
We describe the test approaches and results for the Multiband Imaging Photometer for SIRTF. To verif...
The Multiband Imaging Photometer for SIRTF (MIPS) will be one of the three instruments on the Space ...
Traditional photoconductive detectors are used at 70 and 160 microns in the Multiband Imaging Photom...
The Multiband Imaging Photometer for Spitzer (MIPS) provides long wavelength capability for the miss...
The GTO program for the MIPS team is concentrated in two areas. First, the evolution of planetary de...
SIRTF, the Space Infrared Telescope Facility, is a NASA mission to provide a long lifetime, sensitiv...
The Cosmic Infrared Background is the focus of many observations, since its understanding is a key f...
The Space Infrared Telescope Facility (SIRTF), the fourth of the Great Observatories, will look thro...
A conceptual design for an infrared spectrometer capable of both low resolution (λ/Δ-λ = 50; 2.5-200...
The first six months of flight data from the Multiband Imaging Photometer for Spitzer (MIPS) were us...
A Cryogenic Scan Mirror Mechanism (CSMM) has been developed for the Multi-band Imaging Photometer fo...
The Space Infrared Telescope Facility (SIRTF) is planned for launch by NASA in the mid-1990's. It wi...
The Space Infrared Facility (SIRTF) Guaranteed Time Observers will be executing deep surveys of the ...