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|a Wynn-Williams, Gareth.
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|a Surveying the Skies :
|b How Astronomers Map the Universe.
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|a Cham :
|b Springer International Publishing,
|c 2016.
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|a 1 online resource (190 pages)
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|a Astronomers' Universe
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|a Preface; Contents; 1 Introduction; 1.1 The Five Eras of Astronomy; 1.2 Defining a Survey; 2 The Naked Eye Era; 2.1 The Babylonians and the Mul. Apin Tablets; 2.2 The Greeks: Aristotle, Hipparchus, and Ptolemy; 2.3 Islamic Astronomy; 2.4 Chinese Astronomy; 2.5 Tycho Brahe; 3 The Telescope Era; 3.1 Surveying the Solar System; 3.2 Halley, Flamsteed and Navigation; 3.3 Messier, Herschel, and Nebulae; 3.4 Variable Stars and Photometry; 3.5 Moving Stars; 3.6 The BD Catalog; 4 The Photography Era; 4.1 Carte du Ciel; 4.2 Harvard Plate Collection; 4.3 Schmidt Camera Surveys.
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|a 4.4 Harvard Spectroscopic Survey5 Radio Surveys; 5.1 Jansky and Reber; 5.2 Post World War II Radio Astronomy; 5.3 The Big Bang Controversy; 5.4 Recent Radio Surveys; 5.5 The Pulsar Discovery Survey; 5.6 The 21-cm Spectral Line; 5.7 Molecules in the Milky Way; 5.8 Searching for ET; 6 Infrared Surveys; 6.1 The Caltech TMSS Survey; 6.2 2MASS and DENIS; 6.3 The AFGL survey; 6.4 IRAS; 6.5 AKARI and WISE; 6.6 UKIDSS and VISTA; 6.7 SCUBA-2; 7 The Cosmic Microwave Background; 7.1 Discovery of the CMB; 7.2 COBE; 7.3 Mapping the Fluctuations in the CMB; 7.4 The Planck Spacecraft; 8 Ultraviolet Surveys.
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|a 8.1 TD-1A8.2 GALEX; 8.3 Extreme Ultraviolet Surveys; 9 X-ray Surveys; 9.1 Early Discoveries; 9.2 UHURU and HEAO-A; 9.3 Neutron Stars and Black Holes; 9.4 ROSAT; 10 Gamma Ray Surveys; 10.1 Early Surveys; 10.2 COS-B; 10.3 Compton and Fermi Satellites; 10.4 Gamma Ray Bursts; 10.5 Very High Energy Gamma Rays; 11 Space Astrometry; 11.1 Hipparcos; 11.2 Gaia; 12 The CCD Era; 12.1 Sloan Digital Sky Survey; 12.2 Pan-STARRS; 12.3 Asteroid Searches; 12.4 LSST; 13 Microsurveys; 13.1 Hubble Deep Fields; 13.2 The COSMOS Survey; 13.3 The MACHO Survey; 13.4 The Kepler Exoplanet Survey.
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|a 14 Accessing Astronomy SurveysAppendices; A.1 Further Reading; A.2 Units; A.3 Wavelength and Energy; A.4 Diffraction Limit; A.5 Precession; A.6 Stellar Magnitudes; A.7 Coordinate Systems; A.8 Interstellar Extinction and Reddening; A.9 Radiation, Temperature, and Wavelength; A.10 Redshift-Age Relationship; A.11 Determining the Properties of an Exoplanet; Index.
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|a Since the time of Galileo, astronomy has been driven by technological innovation. With each major advance has come the opportunity and enthusiasm to survey the sky in a way that was not possible before. It is these surveys of discovery that are the subject of this book. In the first few chapters the author discusses what astronomers learned from visible-light surveys, first with the naked eye, then using telescopes in the seventeenth century, and photography in the nineteenth century. He then moves to the second half of the twentieth century when the skies started to be swept by radio, infrared, ultraviolet, x-ray and gamma ray telescopes, many of which had to be flown in satellites above the Earth's atmosphere. These surveys led to the discovery of pulsars, quasars, molecular clouds, protostars, bursters, and black holes. He then returns to Earth to describe several currently active large-scale projects that methodically collect images, photometry and spectra that are then stored in vast publicly-accessible databases. Dr. Wynn-Williams also describes several recent "microsurveys"--Detailed studies of small patches of sky that have led to major advances in our understanding of cosmology and exoplanets.
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|i has work:
|a Surveying the skies (Text)
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|i Print version:
|a Wynn-Williams, Gareth.
|t Surveying the Skies : How Astronomers Map the Universe.
|d Cham : Springer International Publishing, ©2016
|z 9783319285085
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|a Astronomers' universe.
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