Add to ORKGWe describe the design and performance of the near IR telescope experiment (NITE), a rocket-borne instrument designed to search for IR emission from baryonic dark matter in the halos of nearby edge-on spiral galaxies. A 256 X 256 InSb array at the focus of a 16.5 cm liquid-helium- cooled telescope achieves near-background-limited sensitivity in a 3.5-5.5 micrometers waveband where the local foreground from zodiacal emission is at a minimum. This experiment represents the first scientific application of a low-background IR InSb array, a precursor to the InSb arrays intended for SIRTF, in a space-borne observation. We describe the flight performance of the instrument and preliminary scientific result from an observation of NGC 4565
Fluctuations in the extragalactic background light trace emission from the history of galaxy formati...
We present a study of different aspects of the multi-phase interstellar medium (ISM) of nearby galax...
We summarize the scientific goals and observing strategy for our GO-1 Spitzer program to study IRAC ...
We describe the design and performance of the near IR telescope experiment (NITE), a rocket-borne in...
The extragalactic background, based on absolute measurements reported by DIRBE and IRTS at 1.2 and 2...
In external galaxies, near-infrared emission originates from stellar populations, hot dust, free-fre...
[EN]The cosmic infrared background (CIB) contains emissions accumulated over the entire history of t...
The objective of this grant was to construct a series of far infrared photometers, cameras, and supp...
The SPICA mid- and far-infrared telescope will address fundamental issues in our understanding of st...
The Infrared Telescope (IRT) experiment, flown on Spacelab-2, was used to make infrared measurements...
To study large-scale structure in the Universe a full census of the contents are required. This is e...
Contains research objectives and summary of research on two research projects and a report on one re...
We present new methodology to use cosmic infrared background (CIB) fluctuations to probe sources at ...
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
The environment above earth's atmosphere offers significant advantages in sensitivity and wavelength...
Fluctuations in the extragalactic background light trace emission from the history of galaxy formati...
We present a study of different aspects of the multi-phase interstellar medium (ISM) of nearby galax...
We summarize the scientific goals and observing strategy for our GO-1 Spitzer program to study IRAC ...
We describe the design and performance of the near IR telescope experiment (NITE), a rocket-borne in...
The extragalactic background, based on absolute measurements reported by DIRBE and IRTS at 1.2 and 2...
In external galaxies, near-infrared emission originates from stellar populations, hot dust, free-fre...
[EN]The cosmic infrared background (CIB) contains emissions accumulated over the entire history of t...
The objective of this grant was to construct a series of far infrared photometers, cameras, and supp...
The SPICA mid- and far-infrared telescope will address fundamental issues in our understanding of st...
The Infrared Telescope (IRT) experiment, flown on Spacelab-2, was used to make infrared measurements...
To study large-scale structure in the Universe a full census of the contents are required. This is e...
Contains research objectives and summary of research on two research projects and a report on one re...
We present new methodology to use cosmic infrared background (CIB) fluctuations to probe sources at ...
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
The environment above earth's atmosphere offers significant advantages in sensitivity and wavelength...
Fluctuations in the extragalactic background light trace emission from the history of galaxy formati...
We present a study of different aspects of the multi-phase interstellar medium (ISM) of nearby galax...
We summarize the scientific goals and observing strategy for our GO-1 Spitzer program to study IRAC ...