Results 121 to 130 of about 5,123 (230)

Asteroids as far-infrared photometric standards for ISOPHOT

open access: yes, 1998
Asteroids are used as far-IR calibrators for the imaging photopolarimeter ISOPHOT on board the Infrared Space Observatory ISO. For the 10 selected objects we compiled a large uniform database(1) of 678 individual observations, ranging from 7-2 000 mu m ...
Muller, TG,, Lagerros, JSV,
core  

Nereid as a regular satellite of Neptune. [PDF]

open access: yesSci Adv
Belyakov M   +4 more
europepmc   +1 more source

The Far-Infrared Spectral Energy Distributions of Quasars

open access: yes, 2001
The origin of the infrared emission in Active Galactic Nuclei (AGN), whose strength is comparable to the optical/ultraviolet (OUV) emission, is generally thought to be a combination of thermal emission from dust and non-thermal, synchrotron emission ...
Wilkes, Belinda J., West, Donald K.
core  

Far infrared astronomy

open access: yes, 1973
The research to develop a spectrometer to be used with a ground based telescope is described. Two liquid helium cooled infrared spectrometers were designed and built.
Houck, J. R.
core  

A tidal disruption event from an intermediate-mass black hole revealed by comprehensive multi-wavelength observations. [PDF]

open access: yesNat Commun
Wang J   +14 more
europepmc   +1 more source

Frequency-dependent topological polaritons in carbon nanotube array/hBN heterostructures. [PDF]

open access: yesNat Commun
Xie Y   +13 more
europepmc   +1 more source

Mid- and far-infrared astronomy mission SPICA

open access: yesMid- and far-infrared astronomy mission SPICA
Accepted: 2007-05-01 資料番号 ...
openaire  

Analysis of Quasi-Optical Components for Far-Infrared Astronomy

open access: yes, 2014
This thesis is concerned with the development and analysis of quasi-optical components used in experiments to measure of the CMB in the terahertz and submillimetre wavebands. I have concentrated on corrugated horn structures in the Planck and QUBIC experiments.
openaire   +1 more source

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