Low Frequency Radio Astronomy and the LOFAR Observatory (eBook)

Lectures from the Third LOFAR Data Processing School
eBook Download: PDF
2018 | 1st ed. 2018
XXIV, 251 Seiten
Springer International Publishing (Verlag)
978-3-319-23434-2 (ISBN)

Lese- und Medienproben

Low Frequency Radio Astronomy and the LOFAR Observatory -
Systemvoraussetzungen
128,39 inkl. MwSt
  • Download sofort lieferbar
  • Zahlungsarten anzeigen
This book presents lecture materials from the Third LOFAR Data School, transformed into a coherent and complete reference book describing the LOFAR design, along with descriptions of primary science cases, data processing techniques, and recipes for data handling. Together with hands-on exercises the chapters, based on the lecture notes, teach fundamentals and practical knowledge. LOFAR is a new and innovative radio telescope operating at low radio frequencies (10-250 MHz) and is the first of a new generation of radio interferometers that are leading the way to the ambitious Square Kilometre Array (SKA) to be built in the next decade. This unique reference guide serves as a primary information source for research groups around the world that seek to make the most of LOFAR data, as well as those who will push these topics forward to the next level with the design, construction, and realization of the SKA. This book will also be useful as supplementary reading material for any astrophysics overview or astrophysical techniques course, particularly those geared towards radio astronomy (and radio astronomy techniques).

About the Editors:

George Heald received his PhD in 2006 from the University of New Mexico, Albuquerque, USA. He has held several leadership roles within the LOFAR collaboration as well as other international radio astronomy projects such as the Murchison Widefield Array (MWA). He now holds the position of Science Leader at the Commonwealth Scientific and Industrial Research Organisation (CSIRO), Australia's science agency, where he leads a research team focused on the low-frequency component of the forthcoming Square Kilometre Array (SKA).

 

Roberto Pizzo received his PhD in Astronomy  in 2010 from the University of Groningen, The Netherlands. In his career, he has lead various LOFAR projects as well as several programs associated with other radio facilities, such as WSRT/APERTIF. Currently, he is the Head of Science Operations and Support for LOFAR and WSRT/APERTIF at the Radio Observatory of ASTRON. In this position, he leads a team of astronomers tackling the challenges which will be common to next generation radio facilities, such as the Square Kilometre Array (SKA).


John McKean received his PhD in Radio Astronomy from the University of Manchester, United Kingdom, in 2004. He has held various research positions at the University of California, the Max Planck Institute for Radio Astronomy and the Netherlands Institute for Radio Astronomy, with scientific interests in galaxy formation and testing models with dark matter using very long baseline interferometry. He is currently Professor for Radio Astronomy at the University of Groningen and a Staff Astronomer at the Netherlands Institute for Radio Astronomy. His work at low frequencies is focussed on studying particle energetics within radio galaxies and high resolution imaging of gravitational lenses with the International LOFAR Telescope.


About the Editors:George Heald received his PhD in 2006 from the University of New Mexico, Albuquerque, USA. He has held several leadership roles within the LOFAR collaboration as well as other international radio astronomy projects such as the Murchison Widefield Array (MWA). He now holds the position of Science Leader at the Commonwealth Scientific and Industrial Research Organisation (CSIRO), Australia's science agency, where he leads a research team focused on the low-frequency component of the forthcoming Square Kilometre Array (SKA).   Roberto Pizzo received his PhD in Astronomy  in 2010 from the University of Groningen, The Netherlands. In his career, he has lead various LOFAR projects as well as several programs associated with other radio facilities, such as WSRT/APERTIF. Currently, he is the Head of Science Operations and Support for LOFAR and WSRT/APERTIF at the Radio Observatory of ASTRON. In this position, he leads a team of astronomers tackling the challenges which will be common to next generation radio facilities, such as the Square Kilometre Array (SKA).John McKean received his PhD in Radio Astronomy from the University of Manchester, United Kingdom, in 2004. He has held various research positions at the University of California, the Max Planck Institute for Radio Astronomy and the Netherlands Institute for Radio Astronomy, with scientific interests in galaxy formation and testing models with dark matter using very long baseline interferometry. He is currently Professor for Radio Astronomy at the University of Groningen and a Staff Astronomer at the Netherlands Institute for Radio Astronomy. His work at low frequencies is focussed on studying particle energetics within radio galaxies and high resolution imaging of gravitational lenses with the International LOFAR Telescope.

Introduction to Low Frequency Radio Astronomy.- LOFAR Overview.- LOFAR station processing.- RFI flagging, Demixing and Visibilities Compression.- Correlator and Online Processing.- Introduction to Calibration.- Error Analysis in LOFAR Data.- Calibration of LOFAR interferometric data.- Ionospheric Effects.- Wide Field Imaging.- The Standard Imaging Pipeline.- Polarization Imaging with LOFAR.- Long Baseline Imaging with LOFAR.- Calibration of LOFAR Spectral Line data.- Beam-formed Data with LOFAR.- Particle Physics with LOFAR.- High Time Resolution with LOFAR.

Erscheint lt. Verlag 11.10.2018
Reihe/Serie Astrophysics and Space Science Library
Zusatzinfo XXIV, 251 p. 105 illus., 76 illus. in color.
Verlagsort Cham
Sprache englisch
Themenwelt Naturwissenschaften Physik / Astronomie Astronomie / Astrophysik
Technik Elektrotechnik / Energietechnik
Schlagworte Interferometric Data Calibration and Imaging • LOFAR Radio Telescope • Low Radio Frequencies Observations • Radio Astronomy Reference Guide • Radio Astronomy Techniques • Radio interferometers • Square Kilometer Array (SKA)
ISBN-10 3-319-23434-X / 331923434X
ISBN-13 978-3-319-23434-2 / 9783319234342
Haben Sie eine Frage zum Produkt?
PDFPDF (Wasserzeichen)
Größe: 11,9 MB

DRM: Digitales Wasserzeichen
Dieses eBook enthält ein digitales Wasser­zeichen und ist damit für Sie persona­lisiert. Bei einer missbräuch­lichen Weiter­gabe des eBooks an Dritte ist eine Rück­ver­folgung an die Quelle möglich.

Dateiformat: PDF (Portable Document Format)
Mit einem festen Seiten­layout eignet sich die PDF besonders für Fach­bücher mit Spalten, Tabellen und Abbild­ungen. Eine PDF kann auf fast allen Geräten ange­zeigt werden, ist aber für kleine Displays (Smart­phone, eReader) nur einge­schränkt geeignet.

Systemvoraussetzungen:
PC/Mac: Mit einem PC oder Mac können Sie dieses eBook lesen. Sie benötigen dafür einen PDF-Viewer - z.B. den Adobe Reader oder Adobe Digital Editions.
eReader: Dieses eBook kann mit (fast) allen eBook-Readern gelesen werden. Mit dem amazon-Kindle ist es aber nicht kompatibel.
Smartphone/Tablet: Egal ob Apple oder Android, dieses eBook können Sie lesen. Sie benötigen dafür einen PDF-Viewer - z.B. die kostenlose Adobe Digital Editions-App.

Buying eBooks from abroad
For tax law reasons we can sell eBooks just within Germany and Switzerland. Regrettably we cannot fulfill eBook-orders from other countries.

Mehr entdecken
aus dem Bereich
Der Wettstreit Dunkler Materie und Dunkler Energie: Ist das Universum …

von Adalbert W. A. Pauldrach; Tadziu Hoffmann

eBook Download (2022)
Springer-Verlag
39,99