by Louis Bell
Publisher: McGraw-Hill 1922
Number of pages: 294
This book is written for the many observers, who use telescopes for study or pleasure and desire more information about their construction and properties. It attempts neither exhaustive technicalities nor popular descriptions of great observatories and their work.
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by Matthew Pitkin, Stuart Reid, Sheila Rowan, Jim Hough - arXiv
The main theme of this review is a discussion of the mechanical and optical principles used in the various long baseline systems in operation around the world - LIGO, Virgo, TAMA300, LCGT, GEO600 - and in LISA, a proposed space-borne interferometer.
by F. Brünnow - Van Nostrand
The celestial sphere and its diurnal motion; On the changes of the fundamental planes to which the places of the stars are referred; Corrections of the observations arising from the position of the observer on the surface of the Earth; and more.
by Frederick Hanley Seares - Stephens
The main purpose of the volume is an exposition of the principal methods of determining latitude, azimuth, and time. Generally speaking, the limit of precision is that corresponding to the engineer's transit or the sextant.
by T. L. Wilson - arXiv
An overview of the techniques of radio astronomy. It contains a short history, details of calibration procedures, coherent/heterodyne and incoherent/bolometer receiver systems, observing methods for single apertures and interferometers, etc.