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Experimental astrophysics /

We are now living in the multimessenger era in which often weak and elusive astrophysical phenomena need to be studied using different and orthogonal probes and information carriers in order to be fully understood. This book is designed to give advanced undergraduate students a description of the mo...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Battistelli, Elia Stefano (Autor)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) : IOP Publishing, [2021]
Colección:IOP (Series). Release 21.
AAS-IOP astronomy. 2021 collection.
Temas:
Acceso en línea:Texto completo

MARC

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100 1 |a Battistelli, Elia Stefano,  |e author. 
245 1 0 |a Experimental astrophysics /  |c Elia Stefano Battistelli. 
264 1 |a Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) :  |b IOP Publishing,  |c [2021] 
300 |a 1 online resource (various pagings) :  |b illustrations (some color). 
336 |a text  |2 rdacontent 
337 |a electronic  |2 isbdmedia 
338 |a online resource  |2 rdacarrier 
490 1 |a [IOP release $release] 
490 1 |a AAS-IOP astronomy. [2021 collection],  |x 2514-3433 
500 |a "Version: 202110"--Title page verso. 
504 |a Includes bibliographical references. 
505 0 |a 1. Astrophysical observables -- 1.1. Astrophysical information carriers -- 1.2. Cosmic rays -- 1.3. Meteorites -- 1.4. Cosmic dust -- 1.5. Gravitational waves -- 1.6. Neutrinos -- 1.7. Dark matter 
505 8 |a 2. Astronomical optics -- 2.1. Electromagnetic waves -- 2.2. Observables -- 2.3. Geometrical optics : Snell's law -- 2.4. Lenses and mirrors -- 2.5. Diffraction and interference 
505 8 |a 3. Telescopes -- 3.1. Diffraction-limited telescopes or not? -- 3.2. Refractive telescopes -- 3.3. Reflective telescopes -- 3.4. Telescope mounts -- 3.5. Telescopes construction -- 3.6. X-ray telescopes 
505 8 |a 4. Signal processing -- 4.1. Fourier transform -- 4.2. Transmission lines -- 4.3. Digital versus analog signals : ADC and DAC -- 4.4. Quantization -- 4.5. Sampling : Nyquist-Shannon theorem 
505 8 |a 5. Semiconductor Physics -- 5.1. Semiconductors and junctions -- 5.2. Diodes -- 5.3. Photomultipliers and their use in astrophysics -- 5.4. Junction-gate field-effect transistors -- 5.5. Transistors -- 5.6. Operational amplifier 
505 8 |a 6. Detectors in astronomy -- 6.1. Introduction -- 6.2. Coherent detectors -- 6.3. Thermal detectors -- 6.4. Quantum detectors -- 6.5. X-ray detectors -- 6.6. Detector characteristics 
505 8 |a 7. Read-out electronics -- 7.1. Read-out electronics -- 7.2. Multiplexing -- 7.3. Read-out of a CCD -- 7.4. Feedback loop 
505 8 |a 8. Noise and its origin -- 8.1. Autocorrelation function and power spectrum -- 8.2. Brownian noise -- 8.3. Kinds of noise 
505 8 |a 9. Cryogenics -- 9.1. Introduction -- 9.2. Cryogens (liquids) -- 9.3. Thermal inputs -- 9.4. Vacuum pumps -- 9.5. Cryostats and their cool down -- 9.6. Mechanical cryocoolers -- 9.7. Sub-kelvin refrigerators 
505 8 |a 10. Spectroscopy -- 10.1. The importance of spectroscopy -- 10.2. Broadband photometry -- 10.3. Prism -- 10.4. Grating -- 10.5. Fourier transform spectrometer 
505 8 |a 11. Polarization -- 11.1. The importance of polarization measurements -- 11.2. Stokes parameters -- 11.3. Polarization at radio frequencies -- 11.4. Polarization at millimeter and submillimeter wavelengths -- 11.5. Optical polarization -- 11.6. X-ray polarization -- 11.7. Martin-Pupplet interferometer 
505 8 |a 12. Signal extraction from noise and calibration -- 12.1. Signal extraction from noise : filters and amplifiers -- 12.2. Modulation -- 12.3. Lock-in amplifiers -- 12.4. Modulations in astrophysics -- 12.5. CCD calibration. 
520 3 |a We are now living in the multimessenger era in which often weak and elusive astrophysical phenomena need to be studied using different and orthogonal probes and information carriers in order to be fully understood. This book is designed to give advanced undergraduate students a description of the most popular techniques and instrumentation employed in modern astrophysics. 
521 |a University students in physics, astronomy and engineering. 
530 |a Also available in print. 
538 |a Mode of access: World Wide Web. 
538 |a System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader. 
545 |a Elia Battistelli is an experimental astrophysicist and cosmologist working on several aspects of astrophysics, including the study of the cosmic microwave background (CMB) radiation. Battistelli is currently Associate Professor in the Physics Department of the Sapienza University of Rome, where he teaches the Astrophysics Laboratory course for third-year bachelor physics students and the General Physics course for biotechnology students in the Medicine faculty. In Battistelli's research, he develops radio-frequency, microwave, and millimeter/submillimeter instrumentation for millimeter astronomy and CMB observations and data analysis. 
588 0 |a Title from PDF title page (viewed on November 8, 2021). 
650 0 |a Astrophysics  |x Technique. 
650 0 |a Astrophysics  |x Experiments. 
650 0 |a Astronomical instruments. 
650 7 |a Astronomical observation - observatories, equipment & methods.  |2 bicssc 
650 7 |a AAS: Instrumentation, Software, Laboratory Astrophysics, and Data.  |2 bisacsh 
710 2 |a Institute of Physics (Great Britain),  |e publisher. 
776 0 8 |i Print version:  |z 9780750331173  |z 9780750331203 
830 0 |a IOP (Series).  |p Release 21. 
830 0 |a AAS-IOP astronomy.  |p 2021 collection. 
856 4 0 |u https://iopscience.uam.elogim.com/book/978-0-7503-3119-7  |z Texto completo