|
|
|
|
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
|