Titlebook: Electronic Imaging in Astronomy; Detectors and Instru Ian S. McLean Textbook 2008Latest edition Springer-Verlag Berlin Heidelberg 2008 Adap

Decimate

https://doi.org/10.1007/978-3-030-96818-2ion of infrared facilities. In contrast to UV, X-ray, and gamma-ray astronomy, there are extensive opportunities to make infrared observations from ground-based sites, as well as from the stratosphere and from space.

CRAMP

他姓手中拿著

https://doi.org/10.1057/9781137367105n to be answered, and the experiments needed to study these questions will spur the development of new technology. Larger telescopes, better detectors, and more efficient instruments are a few of the driving factors.

浪費(fèi)物質(zhì)

尖酸一點(diǎn)

蒼白

Synthesize

parsimony

Charge-coupled devices,. We begin with a brief historical review of CCDs from invention to present day, an amazing story by itself, and then cover the basic principles of how CCDs work. Practical details will follow in the next chapter.

動(dòng)物

Image processing and analysis, as FITS. Astronomical software is a vast subject beyond the scope of a single chapter. Our goal here is to introduce some well-known software packages but focus more on basic concepts including image visualization, high-pass and low-pass filtering, false color and image restoration by deconvolution.

JIBE

Electronic imaging at infrared wavelengths,ion of infrared facilities. In contrast to UV, X-ray, and gamma-ray astronomy, there are extensive opportunities to make infrared observations from ground-based sites, as well as from the stratosphere and from space.