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High-Energy Emission from Pulsars and their Systems

Overview of attention for book
Cover of 'High-Energy Emission from Pulsars and their Systems'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 Radio Pulsar Phenomenology
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    Chapter 2 Radio pulsar populations
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    Chapter 3 Pulsar Results with the Fermi Large Area Telescope
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    Chapter 4 Fermi view of the EGRET pulsars
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    Chapter 5 “Garden-variety” Gamma-ray Pulsars J0248+6021 & J2240+5832
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    Chapter 6 Extension studies of galactic sources with Fermi
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    Chapter 7 Advances in understanding double features in radio pulsar profiles
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    Chapter 8 Emission from the Polar Cap and Slot Gap
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    Chapter 9 Gamma-ray emission and pair creation of outer gap
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    Chapter 10 What Pulsar High-Energy Emission Model Survives?
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    Chapter 11 Current Models of Pulsar Magnetospheres
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    Chapter 12 Modeling of γ-ray Pulsar Light Curves from Force-Free Magnetosphere
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    Chapter 13 A Tale of Two Current Sheets
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    Chapter 14 The high-energy emission from the pulsar striped wind
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    Chapter 15 Gamma-rays from millisecond pulsars in Globular Clusters
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    Chapter 16 Modelling the Growing Population of γ-ray Millisecond Pulsars
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    Chapter 17 A Joint Radio Gamma-ray Variability Study of the Crab Pulsar
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    Chapter 18 AGILE observations of PSR B1509-58
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    Chapter 19 Understanding the fundamental parameters of millisecond pulsars
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    Chapter 20 Pulsars as gravitational wave detectors
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    Chapter 21 Magnetar outbursts: an observational review
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    Chapter 22 Wide-band X-ray Studies of Magnetars with Suzaku
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    Chapter 23 Bursts and Flares from Highly Magnetic Pulsars
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    Chapter 24 Activated Magnetospheres of Magnetars
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    Chapter 25 Suzaku Detection of Hard X-ray Emission in SGR 0501+4516 Short Burst Spectrum
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    Chapter 26 The magnetar emission in the IR band: the role of magnetospheric currents
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    Chapter 27 Double features in mean pulsar profiles and the nature of their radio emission
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    Chapter 28 Can the magnetic field of long-period X-ray pulsars be supercritical ?
  30. Altmetric Badge
    Chapter 29 High-Energy Emission from Pulsars and their Systems
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    Chapter 30 X-ray thermal radiation from hot polar cap in pulsars
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    Chapter 31 Radio polarization of RRAT J1819-1458
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    Chapter 32 Multiwavelength Observations of Pulsar Wind Nebulae
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    Chapter 33 Multi-wavelength Observations of Composite Supernova Remnants
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    Chapter 34 Fermi -LAT Results on Pulsar Wind Nebulae after 1.5 year of Observations
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    Chapter 35 Pulsar Wind Nebulae: The GeV to TeV Connection
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    Chapter 36 Extended hard X-ray emission from Vela X
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    Chapter 37 Cherenkov Telescopes Results on Pulsar Wind Nebulae and Pulsars
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    Chapter 38 Lepton Acceleration in Pulsar Wind Nebulae
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    Chapter 39 MHD models of Pulsar Wind Nebulae
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    Chapter 40 TeV Gamma Ray Survey on the Direction of Fermi -LAT Pulsars with the Tibet Air Shower Array
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    Chapter 41 Fermi results on γ-ray binaries
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    Chapter 42 Cherenkov Telescope results on gamma-ray binaries
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    Chapter 43 γ-ray binaries as non-accreting pulsar systems
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    Chapter 44 Relativistic motion and beamed radiation in gamma-ray binaries
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    Chapter 45 A leptonic One-Zone model of the X-Ray/VHE correlated emission in LS I +61 303
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    Chapter 46 New Optical Results on γ-ray Binaries
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    Chapter 47 The International X-ray Observatory and other X-ray missions, expectations for pulsar physics
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    Chapter 48 X-ray Polarimeters
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    Chapter 49 New results on high energy cosmic ray electrons observed with Fermi LAT
  51. Altmetric Badge
    Chapter 50 Positrons from pulsar winds
Overall attention for this book and its chapters
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About this Attention Score

  • Good Attention Score compared to outputs of the same age (70th percentile)
  • Good Attention Score compared to outputs of the same age and source (72nd percentile)

Mentioned by

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26 Mendeley
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Title
High-Energy Emission from Pulsars and their Systems
Published by
ADS, February 2011
DOI 10.1007/978-3-642-17251-9
ISBNs
978-3-64-217250-2, 978-3-64-217251-9
Editors

Torres, Diego F., Rea, Nanda

X Demographics

X Demographics

The data shown below were collected from the profile of 1 X user who shared this research output. Click here to find out more about how the information was compiled.
Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 26 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Germany 3 12%
Netherlands 1 4%
Chile 1 4%
Unknown 21 81%

Demographic breakdown

Readers by professional status Count As %
Researcher 8 31%
Student > Ph. D. Student 7 27%
Student > Master 4 15%
Student > Bachelor 2 8%
Professor 1 4%
Other 1 4%
Unknown 3 12%
Readers by discipline Count As %
Physics and Astronomy 23 88%
Materials Science 1 4%
Unknown 2 8%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 4. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 01 August 2023.
All research outputs
#7,041,349
of 23,041,514 outputs
Outputs from ADS
#8,731
of 37,451 outputs
Outputs of similar age
#52,248
of 184,267 outputs
Outputs of similar age from ADS
#217
of 812 outputs
Altmetric has tracked 23,041,514 research outputs across all sources so far. This one has received more attention than most of these and is in the 68th percentile.
So far Altmetric has tracked 37,451 research outputs from this source. They receive a mean Attention Score of 4.6. This one has done well, scoring higher than 75% of its peers.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 184,267 tracked outputs that were published within six weeks on either side of this one in any source. This one has gotten more attention than average, scoring higher than 70% of its contemporaries.
We're also able to compare this research output to 812 others from the same source and published within six weeks on either side of this one. This one has gotten more attention than average, scoring higher than 72% of its contemporaries.