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Gamma rays, observing universe

Interrogating the light from stars and the absorption features of atoms and molecules in-between requires some fairly complicated optics in the form of a telescope. However, the telescopes are not restricted to the parts of the electromagnetic spectrum that you can see but use radiation from microwaves to gamma rays to observe the Universe. There is too much to learn about the optics or even adaptive optics of telescopes to be discussed here but there are some properties of telescopes that we must know because they are important for the identification of atoms and molecules. We shall discuss three telescope considerations the atmosphere, the spatial resolution and the spectral resolution. [Pg.52]

The selected samples were sent to the University of Maryland. They were opened in a Class 100 clean room and half of each filter was cut from the holder with a stainless steel scalpel, folded and transferred to an acid-washed polyethylene bag. The bags were placed into pneumatic tube sample carriers ("rabbits") along with standards and flux monitors, and irradiated in the National Bureau of Standards (NBS) reactor at a flux of 5 x 10 n/cm -sec. Gamma-ray spectra of the irradiation products were observed with Ge r-ray detectors using procedures discussed by... [Pg.71]


See other pages where Gamma rays, observing universe is mentioned: [Pg.311]    [Pg.353]    [Pg.554]    [Pg.11]    [Pg.224]    [Pg.2191]    [Pg.1]    [Pg.78]    [Pg.261]    [Pg.275]    [Pg.122]    [Pg.85]    [Pg.357]    [Pg.384]    [Pg.359]    [Pg.34]    [Pg.59]    [Pg.65]    [Pg.78]    [Pg.93]   
See also in sourсe #XX -- [ Pg.350 ]




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Gamma ray

Observable universe

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