The simplest way to measure the luminosity of a star is to observe its radiated output at all wavelengths ( the spectral energy distribution or SED ) and sum them together.
12.
That colour has nothing to do with the redshift, it is due to the fact that these galaxies contain lots of young stars which have a spectral energy distribution that increases towards the ultraviolet.
13.
The most consistent outcomes from such experiments are that brightness or spectral energy distribution, and the " bite ", or rate and synchronicity and rise time, of the attack are important factors.
14.
The power spectral density ( PSD ) then refers to the spectral energy distribution that would be found per unit time, since the total energy of such a signal over all time would generally be infinite.
15.
This interaction is dependent on the spectral energy distribution ( SED ) of the EBL . Therefore, it is necessary to know the SED of the EBL in order to study intrinsic properties of the emission in the VHE sources.
16.
Non-tidal factors, such as extreme stellar variation, spectral energy distributions shifted to the infrared relative to the Sun, and small circumstellar habitable zones due to low light output, further reduce the prospects for life in red-dwarf systems.
17.
This involved the development of several key technical innovations to better determine the galaxies spectral energy distributions, especially the world's first optical fibre multi-object spectrograph on the AAT, which simultaneously gathered high quality spectra for large numbers of these faint galaxies in distant clusters.
18.
Addressing fluctuating partially coherent light emitters with a tailored spectral energy distribution in the optical range, this establishes the link between stochastic electrodynamics and coherence theory; henceforth putting forward a way to optically create and control both such zero-point fields as well as Lifshitz forces of thermal fluctuations.
19.
Temperature estimates for the star range from around 18, 000K to well over 30, 000K . The hotter temperatures found from fitting the spectral energy distribution ( SED ) are consistent with the calculated luminosity of an LBV in the quiescent stage, but the spectrum is that of a cooler star.
20.
The hotspots that are usually seen in FRII sources are interpreted as being the visible manifestations of shocks formed when the fast, and therefore supersonic, jet ( the speed of sound cannot exceed c / " 3 ) abruptly terminates at the end of the source, and their spectral energy distributions are consistent with this picture.
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