Cargando…

Big data in astronomy : scientific data processing for advanced radio telescopes /

Detalles Bibliográficos
Clasificación:Libro Electrónico
Otros Autores: Kong, Linghe (Computer scientist) (Editor ), Huang, Tian (Computer scientist) (Editor ), Zhu, Yongxin (Computer scientist) (Editor ), Yu, Shenghua (Editor )
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Amsterdam, Netherlands : Elsevier, [2020]
Temas:
Acceso en línea:Texto completo

MARC

LEADER 00000cam a2200000 i 4500
001 SCIDIR_on1159164401
003 OCoLC
005 20231120010457.0
006 m o d
007 cr un|---aucuu
008 200620t20202020ne a ob 001 0 eng d
040 |a EBLCP  |b eng  |e rda  |e pn  |c EBLCP  |d YDX  |d OPELS  |d EBLCP  |d UKMGB  |d N$T  |d OCLCF  |d WAU  |d OCLCO  |d UKAHL  |d AUD  |d DKU  |d OCLCO  |d OCLCQ  |d SFB  |d OCLCQ  |d OCLCO 
015 |a GBC072192  |2 bnb 
016 7 |a 019811075  |2 Uk 
019 |a 1158708560  |a 1162184862 
020 |a 9780128190852  |q (electronic bk.) 
020 |a 012819085X  |q (electronic bk.) 
020 |z 9780128190845 
020 |z 0128190841 
035 |a (OCoLC)1159164401  |z (OCoLC)1158708560  |z (OCoLC)1162184862 
050 4 |a QB475 
082 0 4 |a 522/.682  |2 23 
245 0 0 |a Big data in astronomy :  |b scientific data processing for advanced radio telescopes /  |c edited by Linghe Kong, Tian Huang, Yongxin Zhu, Shenghua Yu. 
264 1 |a Amsterdam, Netherlands :  |b Elsevier,  |c [2020] 
264 4 |c �2020 
300 |a 1 online resource (xv, 422 pages) :  |b illustrations 
336 |a text  |b txt  |2 rdacontent 
336 |a still image  |b sti  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
504 |a Includes bibliographical references and index. 
505 0 |a Intro -- Big Data in Astronomy: Scientific Data Processing for Advanced Radio Telescopes -- Copyright -- Contents -- Contributors -- Preface -- Acknowledgments -- Part A: Fundamentals -- Chapter 1: Introduction to radio astronomy -- 1. The history of astronomy -- 1.1. Ancient astronomy -- 1.2. Astronomy from the mid-16th century to the mid-19th century -- 1.3. Astronomy since the mid-19th century -- 2. What is radio astronomy -- 2.1. How does radio astronomy occur -- 2.2. The radio stars, quasars, and black holes -- 2.2.1. The strongest radio source, Cygnus A, in the sky 
505 8 |a 2.2.2. The discovery of cliff allergens and radio galaxies -- 2.2.3. Nonthermal radiation -- 2.2.4. Synchronous radiation -- 2.2.5. Synchrotron radiation pattern -- 2.2.6. Connect nonthermal radiation and cosmic rays -- 2.2.7. Astrophysics of cosmic rays -- 2.2.8. Discovery of quasars -- 2.3. The radio astronomy instrument: Radio telescope -- 2.4. Some achievements of radio astronomy -- 2.5. Astronomical research nowadays -- 3. Advanced radio telescope -- 3.1. The square kilometer array (SKA) -- 3.2. Fast -- 4. The challenge of radio astronomy -- 4.1. System noise 
505 8 |a 4.2. Antennas and collecting area -- 4.3. Data transmission -- 5. The development tendency of radio astronomy -- 5.1. Mid-frequency aperture arrays -- 5.2. Entering a near future -- References -- Chapter 2: Fundamentals of big data in radio astronomy -- 1. Big data and astronomy -- 1.1. Background of big data -- 1.2. Definitions and features of big data -- 1.3. Development of big data -- 1.4. Big data in astronomy -- 1.5. Statistical challenges in astronomy -- 2. Increasing data volumes of telescopes -- 2.1. Sloan digital sky survey -- 2.2. Visible and infrared survey telescope for astronomy 
505 8 |a 2.3. Large synoptic survey telescope -- 2.4. Thirty meter telescope -- 3. Existing methods for the value chain of big data -- 3.1. Data generation -- 3.2. Data acquisition -- 3.3. Data storage -- 3.4. Data analysis -- 3.4.1. Traditional data analysis methods -- 3.4.2. Big data analytic methods -- 3.4.3. Architecture for big data analysis -- 4. Current statistical methods for astronomical data analysis -- 4.1. Nonparametric statistics -- 4.2. Data smoothing -- 4.3. Multivariate clustering and classification -- 4.4. Nondetections and truncation -- 4.5. Spatial point processes 
505 8 |a 5. Platforms for big data processing -- 5.1. Horizontal scaling platforms -- 5.2. Vertical scaling platforms -- 5.2.1. High performance computing (HPC) clusters -- 5.2.2. Multicore CPU -- 5.2.3. Graphics processing unit (GPU) -- 5.2.4. Field programmable gate arrays (FPGA) -- References -- Part B: Big data processing -- Chapter 3: Preprocessing pipeline on FPGA -- 1. FPGA interface for ADC -- 1.1. ADC interleaving -- 1.2. Bit alignment -- 1.3. Stream deserialization -- 2. FIR filtering -- 2.1. Leakage -- 2.2. Scalloping loss -- 2.3. Polyphase filter -- 3. Time-frequency domain transposing -- 3.1. Real-valued FFT. 
588 0 |a Online resource; title from PDF title page (viewed August 30, 2021). 
650 0 |a Radio astronomy  |x Data processing. 
650 0 |a Big data. 
650 6 |a Radioastronomie  |0 (CaQQLa)201-0016455  |x Informatique.  |0 (CaQQLa)201-0380011 
650 6 |a Donn�ees volumineuses.  |0 (CaQQLa)000284673 
650 7 |a Big data  |2 fast  |0 (OCoLC)fst01892965 
700 1 |a Kong, Linghe  |c (Computer scientist)  |e editor. 
700 1 |a Huang, Tian  |c (Computer scientist)  |e editor. 
700 1 |a Zhu, Yongxin  |c (Computer scientist)  |e editor. 
700 1 |a Yu, Shenghua,  |e editor. 
776 0 8 |i Print version:  |a Kong, Linghe.  |t Big Data in Astronomy : Scientific Data Processing for Advanced Radio Telescopes.  |d San Diego : Elsevier, �2020 
856 4 0 |u https://sciencedirect.uam.elogim.com/science/book/9780128190845  |z Texto completo