Results 201 to 210 of about 149,506 (246)
Some of the next articles are maybe not open access.
1971
Abstract : The report describes the work completed between 11 December 1970 and 10 May 1971, and is divided into seven sections; performance of the reassembled telescope system, the new optical system, results of December 2, 1970 flight: short wavelength detectors, results of December 2, 1970 flight: long wavelength detectors, ground based effort ...
Baruch T. Soifer +4 more
openaire +1 more source
Abstract : The report describes the work completed between 11 December 1970 and 10 May 1971, and is divided into seven sections; performance of the reassembled telescope system, the new optical system, results of December 2, 1970 flight: short wavelength detectors, results of December 2, 1970 flight: long wavelength detectors, ground based effort ...
Baruch T. Soifer +4 more
openaire +1 more source
Stellar infrared astronomy with EDISON
Space Science Reviews, 1992In this review the IR emission from circumstellar material is discussed, both of ionized gas and dust grains, and the astrophysical information that can be extracted from such observations. Some emphasis is placed on the possibilities of stellar IR astronomy using a large space-borne telescope, especially with respect to the much better spatial and ...
openaire +1 more source
1972
The extension of astronomy in the wavelength region of 1 μ to 1 mm has in the past been limited by lack of detectors of high sensitivity and by the obscuration of the Earth’s atmosphere. Ground-based near infrared astronomy could be carried out within certain partial windows: i.e. from 2.1 μ to 2.4 μ, 3.5 μ to 4.0 μ, 4.6 μ to 4.7 μ, 8–13 μ, and 20–25 μ.
openaire +1 more source
The extension of astronomy in the wavelength region of 1 μ to 1 mm has in the past been limited by lack of detectors of high sensitivity and by the obscuration of the Earth’s atmosphere. Ground-based near infrared astronomy could be carried out within certain partial windows: i.e. from 2.1 μ to 2.4 μ, 3.5 μ to 4.0 μ, 4.6 μ to 4.7 μ, 8–13 μ, and 20–25 μ.
openaire +1 more source
The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope
Astronomy and Astrophysics, 2022Pierre Ferruit +2 more
exaly

