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Neutron Stars and Pulsars

Overview of attention for book
Cover of 'Neutron Stars and Pulsars'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 0 Neutron Star Interiors and the Equation of State of Superdense Matter
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    Chapter 1 Radio Pulsar Statistics
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    Chapter 2 Radio Emission Properties of Pulsars
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    Chapter 3 Rotating Radio Transients
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    Chapter 4 Intermittent Pulsars
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    Chapter 5 The Double Pulsar: A Unique Lab for Relativistic Plasma Physics and Tests of General Relativity
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    Chapter 6 X-Ray Emission from Pulsars and Neutron Stars
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    Chapter 7 Isolated Neutron Stars: The Challenge of Simplicity
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    Chapter 8 Millisecond Pulsars in Globular Clusters and the Field
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    Chapter 9 Theory of Radiative Transfer in Neutron Star Atmospheres and Its Applications
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    Chapter 11 Neutron Star Cooling: I
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    Chapter 12 Neutron Star Cooling: II
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    Chapter 13 Turning Points in the Evolution of Isolated Neutron Stars'Magnetic Fields
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    Chapter 14 Pulsar Spin, Magnetic Fields, and Glitches
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    Chapter 15 Pulsar Emission: Where to Go
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    Chapter 16 The Theory of Pulsar Winds and Nebulae
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    Chapter 17 Implications of HESS Observations of Pulsar
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    Chapter 18 High Energy Emission from Pulsars and Pulsar Wind Nebulae
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    Chapter 19 High-energy Emission from the Polar Cap and Slot Gap
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    Chapter 20 Physics of Drifting Sub-pulses in Radio Pulsars
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    Chapter 21 Soft Gamma-Ray Repeaters and Magnetars
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    Chapter 22 X-Ray Polarimetry and Its Potential Use for Understanding Neutron Stars
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    Chapter 23 GeV Gamma-Ray Pulsar Detection
  25. Altmetric Badge
    Chapter 24 Gravitational Waves from Spinning Neutron Stars
Attention for Chapter 4: Intermittent Pulsars
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About this Attention Score

  • In the top 25% of all research outputs scored by Altmetric
  • High Attention Score compared to outputs of the same age (85th percentile)
  • High Attention Score compared to outputs of the same age and source (95th percentile)

Mentioned by

1 news outlet


94 Dimensions

Readers on

6 Mendeley
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Chapter title
Intermittent Pulsars
Chapter number 4
Book title
Neutron Stars and Pulsars
Published in
ADS, November 2015
DOI 10.1007/978-3-540-76965-1_4
Book ISBNs
978-3-54-076964-4, 978-3-54-076965-1

Andrew G. Lyne

Mendeley readers

The data shown below were compiled from readership statistics for 6 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Italy 1 17%
Unknown 5 83%

Demographic breakdown

Readers by professional status Count As %
Student > Master 2 33%
Student > Ph. D. Student 1 17%
Student > Postgraduate 1 17%
Professor 1 17%
Unknown 1 17%
Readers by discipline Count As %
Physics and Astronomy 5 83%
Unknown 1 17%

Attention Score in Context

This research output has an Altmetric Attention Score of 10. 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 29 June 2015.
All research outputs
of 13,454,351 outputs
Outputs from ADS
of 23,544 outputs
Outputs of similar age
of 231,976 outputs
Outputs of similar age from ADS
of 113 outputs
Altmetric has tracked 13,454,351 research outputs across all sources so far. Compared to these this one has done well and is in the 88th percentile: it's in the top 25% of all research outputs ever tracked by Altmetric.
So far Altmetric has tracked 23,544 research outputs from this source. They receive a mean Attention Score of 4.4. This one has done particularly well, scoring higher than 94% 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 231,976 tracked outputs that were published within six weeks on either side of this one in any source. This one has done well, scoring higher than 85% of its contemporaries.
We're also able to compare this research output to 113 others from the same source and published within six weeks on either side of this one. This one has done particularly well, scoring higher than 95% of its contemporaries.