Nine additional radiation sources, above a 3-sigma confidence level of 1300 Jy, were identified at 100 microns by far infrared photometry of the galactic plane using a 0.4 meter aperture, liquid helium cooled, multichannel far infrared balloon-borne telescope. The instrument is described, including its electronics, pointing and suspension systems, and ground support equipment. Testing procedures and flight staging are discussed along with the reduction and analysis of the data acquired. The history of infrared astronomy is reviewed. General infrared techniques and the concerns of balloon astronomers are explored
The use of balloon vehicles to observe the solar corona with an infrared coronagraph is reviewed. Th...
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
Over the last 10 years infrared astronomy from 2 µm to 1000 µm has blossomed into a major field of o...
A 0.4-meter aperture, liquid helium cooled multichannel far-infrared balloon-borne telescope was con...
Localized sources of far infrared radiation (approximately 50 microns) have been detected during a h...
The characteristics of a 16 inch liquid helium cooled Cassegrain telescope with vibrating secondary ...
The flight of a balloon-borne one-meter telescope for infrared astronomy in the wavelength interval ...
The characteristics of a telescope system which was developed for high altitude balloon astronomy ar...
The development of a balloon gondola and pointing system are discussed which can be used with the lo...
The research to develop a spectrometer to be used with a ground based telescope is described. Two li...
Contains research objectives and summary of research on two research projects and a report on one re...
The objective of this grant was to construct a series of far infrared photometers, cameras, and supp...
The objective of this grant is to develop the Far IR Photometer (FIRP), one of four focal plane inst...
An all-sky survey at submillimeter waves is examined. Far-infrared all-sky surveys were performed us...
The scientific objectives, engineering analysis and design, results of technology development, and f...
The use of balloon vehicles to observe the solar corona with an infrared coronagraph is reviewed. Th...
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
Over the last 10 years infrared astronomy from 2 µm to 1000 µm has blossomed into a major field of o...
A 0.4-meter aperture, liquid helium cooled multichannel far-infrared balloon-borne telescope was con...
Localized sources of far infrared radiation (approximately 50 microns) have been detected during a h...
The characteristics of a 16 inch liquid helium cooled Cassegrain telescope with vibrating secondary ...
The flight of a balloon-borne one-meter telescope for infrared astronomy in the wavelength interval ...
The characteristics of a telescope system which was developed for high altitude balloon astronomy ar...
The development of a balloon gondola and pointing system are discussed which can be used with the lo...
The research to develop a spectrometer to be used with a ground based telescope is described. Two li...
Contains research objectives and summary of research on two research projects and a report on one re...
The objective of this grant was to construct a series of far infrared photometers, cameras, and supp...
The objective of this grant is to develop the Far IR Photometer (FIRP), one of four focal plane inst...
An all-sky survey at submillimeter waves is examined. Far-infrared all-sky surveys were performed us...
The scientific objectives, engineering analysis and design, results of technology development, and f...
The use of balloon vehicles to observe the solar corona with an infrared coronagraph is reviewed. Th...
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
Over the last 10 years infrared astronomy from 2 µm to 1000 µm has blossomed into a major field of o...