Handbook of X-ray astronomy (Record no. 196599)
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000 -LEADER | |
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fixed length control field | 03522nam a2200361 a 4500 |
001 - CONTROL NUMBER | |
control field | ebr10514141 |
003 - CONTROL NUMBER IDENTIFIER | |
control field | CaPaEBR |
006 - FIXED-LENGTH DATA ELEMENTS--ADDITIONAL MATERIAL CHARACTERISTICS | |
fixed length control field | m u |
007 - PHYSICAL DESCRIPTION FIXED FIELD--GENERAL INFORMATION | |
fixed length control field | cr cn||||||||| |
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION | |
fixed length control field | 110706s2011 enka sb 001 0 eng d |
010 ## - LIBRARY OF CONGRESS CONTROL NUMBER | |
Canceled/invalid LC control number | 2011023034 |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
Canceled/invalid ISBN | 9780521883733 (hardback) |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
Canceled/invalid ISBN | 9781139157087 (e-book) |
040 ## - CATALOGING SOURCE | |
Original cataloging agency | CaPaEBR |
Transcribing agency | CaPaEBR |
035 ## - SYSTEM CONTROL NUMBER | |
System control number | (OCoLC)773036123 |
050 14 - LIBRARY OF CONGRESS CALL NUMBER | |
Classification number | QB472 |
Item number | .H36 2011eb |
082 04 - DEWEY DECIMAL CLASSIFICATION NUMBER | |
Classification number | 522/.6863 |
Edition number | 23 |
245 00 - TITLE STATEMENT | |
Title | Handbook of X-ray astronomy |
Medium | [electronic resource] / |
Statement of responsibility, etc. | edited by Keith A. Arnaud, Randall K. Smith, and Aneta Siemiginowska. |
260 ## - PUBLICATION, DISTRIBUTION, ETC. | |
Place of publication, distribution, etc. | Cambridge ; |
-- | New York : |
Name of publisher, distributor, etc. | Cambridge University Press, |
Date of publication, distribution, etc. | 2011. |
300 ## - PHYSICAL DESCRIPTION | |
Extent | viii, 197 p. : |
Other physical details | ill. |
490 1# - SERIES STATEMENT | |
Series statement | Cambridge observing handbooks for research astronomers ; |
Volume/sequential designation | 7 |
504 ## - BIBLIOGRAPHY, ETC. NOTE | |
Bibliography, etc. note | Includes bibliographical references and index. |
505 8# - FORMATTED CONTENTS NOTE | |
Formatted contents note | Machine generated contents note: 1. X-ray astronomy optics Daniel A. Schwartz; 2. Proportional counters and other detector techniques Richard J. Edgar; 3. CCDs for x-ray astronomy Catherine E. Grant; 4. Data reduction and calibration Keith A. Arnaud and Randall K. Smith; 5. Data analysis Randall K. Smith, Keith A. Arnaud and Aneta Siemiginowska; 6. Archives, surveys, catalogues and software Keith Arnaud; 7. Statistics Aneta Siemiginowska; 8. Analysis of extended emission K. D. Kuntz; Appendices; Index. |
520 ## - SUMMARY, ETC. | |
Summary, etc. | "It may be obvious why visible astronomy utilizes images, but it is illustrative to consider the value of focusing to X-ray astronomy. A list of advantages offered by the best possible two-dimensional angular resolution would include: (i) Resolving sources with small angular separation and distinguishing different regions of the same source. (ii) Using the image morphology to apply intuition in choosing specific models for quantitative fits to the data. (iii) Using as a "collector" to gather photons. This is necessary because X-ray-source fluxes are so low that individual X-ray photons are detected; the weakest sources give less than one photon per day. (iv) Using as a "concentrator," so that the photons from individual sources interact in such a small region of the detector that residual non-X-ray background counts are negligible. (v) Measuring sources of interest and simultaneously determining the contaminating background using other regions of the detector. (vi) Using with dispersive spectrometers such as transmission or reflection gratings to provide high spectral resolution. The Earth's atmosphere completely absorbs cosmic X-rays. Consequently, X-ray observatories must be launched into space; so size, weight, and cost are always important constraints on the design. In practice this leads to a trade-off between the best possible angular resolution and the largest possible collecting area. Realizing an X-ray telescope involves two key issues: reflection of X-rays, and formation of an image"-- |
Assigning source | Provided by publisher. |
533 ## - REPRODUCTION NOTE | |
Type of reproduction | Electronic reproduction. |
Place of reproduction | Palo Alto, Calif. : |
Agency responsible for reproduction | ebrary, |
Date of reproduction | 2013. |
Note about reproduction | Available via World Wide Web. |
-- | Access may be limited to ebrary affiliated libraries. |
650 #0 - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical term or geographic name entry element | X-ray astronomy. |
655 #7 - INDEX TERM--GENRE/FORM | |
Genre/form data or focus term | Electronic books. |
Source of term | local |
700 1# - ADDED ENTRY--PERSONAL NAME | |
Personal name | Arnaud, Keith A., |
Dates associated with a name | 1959- |
700 1# - ADDED ENTRY--PERSONAL NAME | |
Personal name | Smith, Randall K. |
Fuller form of name | (Randall Knowles), |
Dates associated with a name | 1969- |
700 1# - ADDED ENTRY--PERSONAL NAME | |
Personal name | Siemiginowska, Aneta. |
710 2# - ADDED ENTRY--CORPORATE NAME | |
Corporate name or jurisdiction name as entry element | ebrary, Inc. |
830 #0 - SERIES ADDED ENTRY--UNIFORM TITLE | |
Uniform title | Cambridge observing handbooks for research astronomers ; |
Volume/sequential designation | 7. |
856 40 - ELECTRONIC LOCATION AND ACCESS | |
Uniform Resource Identifier | <a href="http://site.ebrary.com/lib/daystar/Doc?id=10514141">http://site.ebrary.com/lib/daystar/Doc?id=10514141</a> |
Public note | An electronic book accessible through the World Wide Web; click to view |
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