C.‐Y. Ng

4.4k total citations
56 papers, 1.2k citations indexed

About

C.‐Y. Ng is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Oceanography. According to data from OpenAlex, C.‐Y. Ng has authored 56 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 53 papers in Astronomy and Astrophysics, 27 papers in Nuclear and High Energy Physics and 4 papers in Oceanography. Recurrent topics in C.‐Y. Ng's work include Pulsars and Gravitational Waves Research (40 papers), Astrophysical Phenomena and Observations (33 papers) and Astrophysics and Cosmic Phenomena (26 papers). C.‐Y. Ng is often cited by papers focused on Pulsars and Gravitational Waves Research (40 papers), Astrophysical Phenomena and Observations (33 papers) and Astrophysics and Cosmic Phenomena (26 papers). C.‐Y. Ng collaborates with scholars based in United States, Hong Kong and Canada. C.‐Y. Ng's co-authors include Roger W. Romani, V. M. Kaspi, B. M. Gaensler, John Whalley, Patrick Slane, George G. Pavlov, Margaret A. Livingstone, L. Staveley‐Smith, Paul Scholz and R. F. Archibald and has published in prestigious journals such as Nature, Physical review. B, Condensed matter and The Astrophysical Journal.

In The Last Decade

C.‐Y. Ng

52 papers receiving 1.1k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name	h						Papers	Cites
C.‐Y. Ng United States	22	1.1k	550	173	100	49	56	1.2k
F. De Paolis Italy	17	1.0k 1.0×	468 0.9×	28 0.2×	37 0.4×	31 0.6×	108	1.1k
Paul Harrison United Kingdom	14	662 0.6×	149 0.3×	102 0.6×	162 1.6×	8 0.2×	27	833
Ersin Göğüş Türkiye	20	1.2k 1.2×	184 0.3×	427 2.5×	59 0.6×	4 0.1×	110	1.3k
Francis Graham-Smith United Kingdom	10	625 0.6×	142 0.3×	157 0.9×	206 2.1×	9 0.2×	23	683
Peter Seymour Australia	5	544 0.5×	226 0.4×	111 0.6×	56 0.6×	11 0.2×	9	638
Christian Fendt Germany	22	1.2k 1.2×	600 1.1×	108 0.6×	43 0.4×	2 0.0×	59	1.3k
Rachid Ouyed Canada	20	1.1k 1.1×	379 0.7×	135 0.8×	18 0.2×	22 0.4×	81	1.2k
Ben Anderson United Kingdom	13	385 0.4×	134 0.2×	20 0.1×	76 0.8×	5 0.1×	34	578
G. Marklund Sweden	26	1.9k 1.8×	100 0.2×	757 4.4×	37 0.4×	11 0.2×	89	1.9k
Marc Freitag United States	13	1.1k 1.0×	203 0.4×	19 0.1×	28 0.3×	3 0.1×	22	1.2k

Countries citing papers authored by C.‐Y. Ng

Since Specialization

Citations

This map shows the geographic impact of C.‐Y. Ng's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by C.‐Y. Ng with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C.‐Y. Ng more than expected).

Fields of papers citing papers by C.‐Y. Ng

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by C.‐Y. Ng. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by C.‐Y. Ng. The network helps show where C.‐Y. Ng may publish in the future.

Co-authorship network of co-authors of C.‐Y. Ng

This figure shows the co-authorship network connecting the top 25 collaborators of C.‐Y. Ng. A scholar is included among the top collaborators of C.‐Y. Ng based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with C.‐Y. Ng. C.‐Y. Ng is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

Bucciantini, N., Josephine Wong, Roger W. Romani, et al.. (2025). A polarized view of the young pulsar wind nebula 3C 58 with IXPE. Astronomy and Astrophysics. 699. A33–A33.

Zhou, Ping, Patrick Slane, Jacco Vink, et al.. (2025). X-Ray Polarization in SN 1006 Southwest Shows Spatial Variations and Differences in the Radio Band. The Astrophysical Journal. 986(2). 210–210.

Ng, C.‐Y., et al.. (2023). High-resolution Radio Study of the Dragonfly Pulsar Wind Nebula Powered by PSR J2021+3651. The Astrophysical Journal. 942(2). 100–100. 2 indexed citations

Liu, Kuan, Fei Xie, Yihan Liu, et al.. (2023). A Spatially Resolved X-Ray Polarization Map of the Vela Pulsar Wind Nebula. The Astrophysical Journal Letters. 959(1). L2–L2. 6 indexed citations

Ng, C.‐Y., et al.. (2023). Radio Study of the Pulsar Wind Nebula Powered by PSR B1706-44. The Astrophysical Journal. 945(1). 82–82. 4 indexed citations

Hu, Chin‐Ping, et al.. (2022). A Comprehensive Study of the Spectral Variation and the Brightness Profile of Young Pulsar Wind Nebulae. The Astrophysical Journal. 927(1). 87–87. 7 indexed citations

Hu, Chin‐Ping, A. K. H. Kong, C.‐Y. Ng, & Kwan-Lok Li. (2018). NGC 7793 P9: An Ultraluminous X-Ray Source Evolved from a Canonical Black Hole X-Ray Binary. The Astrophysical Journal. 864(1). 64–64. 8 indexed citations

Cendes, Y., B. M. Gaensler, C.‐Y. Ng, et al.. (2018). The Reacceleration of the Shock Wave in the Radio Remnant of SN 1987A. The Astrophysical Journal. 867(1). 65–65. 11 indexed citations

Hu, Chin‐Ping, et al.. (2017). Evolution of Spin, Orbital, and Superorbital Modulations of 4U 0114+650. The Astrophysical Journal. 844(1). 16–16. 16 indexed citations

10.

Klingler, N. J., Blagoy Rangelov, Oleg Kargaltsev, et al.. (2016). DEEP CHANDRA OBSERVATIONS OF THE PULSAR WIND NEBULA CREATED BY PSR B0355+54. The Astrophysical Journal. 833(2). 253–253. 27 indexed citations

11.

Klingler, N. J., Oleg Kargaltsev, Blagoy Rangelov, et al.. (2016). CHANDRA OBSERVATIONS OF OUTFLOWS FROM PSR J1509–5850. The Astrophysical Journal. 828(2). 70–70. 26 indexed citations

12.

Potter, T. W., Giovanna Zanardo, B. M. Gaensler, et al.. (2013). IAU volume 9 issue S296 Cover and Front matter. Proceedings of the International Astronomical Union. 9(S296). f1–f22. 1 indexed citations

13.

Ng, C.‐Y., Giovanna Zanardo, L. Staveley‐Smith, et al.. (2013). EVOLUTION OF THE RADIO REMNANT OF SUPERNOVA 1987A: MORPHOLOGICAL CHANGES FROM DAY 7000. The Astrophysical Journal. 777(2). 131–131. 17 indexed citations

14.

Lakićević, Maša, Giovanna Zanardo, J. Th. van Loon, et al.. (2012). The remnant of supernova 1987A resolved at 3-mm wavelength. Astronomy and Astrophysics. 541. L2–L2. 10 indexed citations

15.

Ng, C.‐Y., V. M. Kaspi, Wynn C. G. Ho, et al.. (2012). DEEP X-RAY OBSERVATIONS OF THE YOUNG HIGH-MAGNETIC-FIELD RADIO PULSAR J1119–6127 AND SUPERNOVA REMNANT G292.2–0.5. The Astrophysical Journal. 761(1). 65–65. 21 indexed citations

16.

Lovchinsky, Igor, Patrick Slane, B. M. Gaensler, et al.. (2011). ACHANDRAOBSERVATION OF SUPERNOVA REMNANT G350.1–0.3 AND ITS CENTRAL COMPACT OBJECT. The Astrophysical Journal. 731(1). 70–70. 26 indexed citations

17.

Livingstone, Margaret A., C.‐Y. Ng, V. M. Kaspi, F. P. Gavriil, & E. V. Gotthelf. (2011). POST-OUTBURST OBSERVATIONS OF THE MAGNETICALLY ACTIVE PULSAR J1846–0258. A NEW BRAKING INDEX, INCREASED TIMING NOISE, AND RADIATIVE RECOVERY. The Astrophysical Journal. 730(2). 66–66. 58 indexed citations

18.

Zanardo, Giovanna, L. Staveley‐Smith, Lewis Ball, et al.. (2010). MULTIFREQUENCY RADIO MEASUREMENTS OF SUPERNOVA 1987A OVER 22 YEARS. The Astrophysical Journal. 710(2). 1515–1529. 33 indexed citations

19.

Ng, C.‐Y., B. M. Gaensler, L. Staveley‐Smith, et al.. (2008). Fourier Modeling of the Radio Torus Surrounding SN 1987A. The Astrophysical Journal. 684(1). 481–497. 25 indexed citations

20.

Romani, Roger W. & C.‐Y. Ng. (2003). The Pulsar Wind Nebula Torus of PSR J0538+2817 and the Origin of Pulsar Velocities. The Astrophysical Journal. 585(1). L41–L44. 40 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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