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Cited article:

RRAT-like behaviour of PSR B0656+14 observed with I-LOFAR

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Single-pulse analysis and average emission characteristics of PSR J1820−0427 from observations made with the MWA and uGMRT

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Low-frequency observations of giant pulses from ordinary pulsars

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Simultaneous 50 cm/10 cm Single-pulse Polarization Observations of PSR J0953+0755

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The Significance of Low-frequency Interferometric Observations for the GPS Pulsar Flux Estimation: The Case of J1740+1000

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Finding the Ionospheric Fluctuations Reflection in the Pulsar Signals’ Characteristics Observed with LOFAR

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High-cadence observations and variable spin behaviour of magnetar Swift J1818.0−1607 after its outburst

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Detection of Bursts from FRB 121102 with the Effelsberg 100 m Radio Telescope at 5 GHz and the Role of Scintillation

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WIDE-BAND SPECTRA OF GIANT RADIO PULSES FROM THE CRAB PULSAR

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LOFAR discovery of a quiet emission mode in PSR B0823+26

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Analysis of single pulse radio flux measurements of PSR B1133+16 at 4.85 and 8.35 GHz

K. Krzeszowski, O. Maron, A. Słowikowska, J. Dyks and A. Jessner
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Timing, polarimetry and physics of the bright, nearby millisecond pulsar PSR J0437−4715 – a single-pulse perspective

S. Osłowski, W. van Straten, M. Bailes, A. Jameson and G. Hobbs
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FREQUENCY INDEPENDENT QUENCHING OF PULSED EMISSION

Vishal Gajjar, Bhal Chandra Joshi, Michael Kramer, Ramesh Karuppusamy and Roy Smits
The Astrophysical Journal 797 (1) 18 (2014)
https://doi.org/10.1088/0004-637X/797/1/18

Short timescale intensity fluctuations of PSR B1133+16 and PSR B1237+25 due to interstellar scintillation at 1.54 GHz

H. B. Niu, A. Esamdin and N. Wang
Astrophysics and Space Science 347 (2) 327 (2013)
https://doi.org/10.1007/s10509-013-1518-y

A study of the strong pulses detected from PSR B0656+14 using the Urumqi 25-m radio telescope at 1540 MHz

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Research in Astronomy and Astrophysics 12 (12) 1649 (2012)
https://doi.org/10.1088/1674-4527/12/12/006

Simultaneous multifrequency single-pulse properties of AXP XTE J1810-197

M. Serylak, B. W. Stappers, P. Weltevrede, et al.
Monthly Notices of the Royal Astronomical Society 394 (1) 295 (2009)
https://doi.org/10.1111/j.1365-2966.2008.14260.x

Timing observations of Rotating Radio Transient J1819−1458 at Urumqi observatory

A. Esamdin, C. S. Zhao, Y. Yan, et al.
Monthly Notices of the Royal Astronomical Society 389 (3) 1399 (2008)
https://doi.org/10.1111/j.1365-2966.2008.13669.x

PuMa-II: A Wide Band Pulsar Machine for the Westerbork Synthesis Radio Telescope

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Radio Phase-Resolved Spectra of the Conal-Double Pulsar B1133+16

Jian-Ling Chen, Hong-Guang Wang, Wan-Hai Chen, Hui Zhang and Yi Liu
Chinese Journal of Astronomy and Astrophysics 7 (6) 789 (2007)
https://doi.org/10.1088/1009-9271/7/6/06

The Variable Radio–to–X‐Ray Spectrum of the Magnetar XTE J1810−197

F. Camilo, S. M. Ransom, J. Penalver, et al.
The Astrophysical Journal 669 (1) 561 (2007)
https://doi.org/10.1086/521548

Is Pulsar B0656+14 a Very Nearby Rotating Radio Transient?

P. Weltevrede, B. W. Stappers, J. M. Rankin and G. A. E. Wright
The Astrophysical Journal 645 (2) L149 (2006)
https://doi.org/10.1086/506346

Monitoring of Pulse Intensity and Mode Changing for PSR B0329+54

Z. Y Liu, N Wang, J. O Urama and R. N Manchester
Chinese Journal of Astronomy and Astrophysics 6 (S2) 64 (2006)
https://doi.org/10.1088/1009-9271/6/S2/14

Flux Monitoring Using the Toruń 32-m Radio Telescope

J. Kijak, Y. Gupta, W. Lewandowski, G. Hrynek and K. Krzeszowski
Symposium - International Astronomical Union 218 441 (2004)
https://doi.org/10.1017/S0074180900181616

Observing Single Pulses Over a Broad Frequency Range

A. Karastergiou, S. Johnston, M. Kramer, N. D. R. Bhat and Y. Gupta
Symposium - International Astronomical Union 218 337 (2004)
https://doi.org/10.1017/S0074180900181318

Giant Pulses from PSR B1937+21 with Widths ≤15 Nanoseconds and \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $T_{b}\geq 5\times 10^{39}$ \end{document} K, the Highest Brightness Temperature Observed in the Universe

V. A. Soglasnov, M. V. Popov, N. Bartel, et al.
The Astrophysical Journal 616 (1) 439 (2004)
https://doi.org/10.1086/424908