V. A. McBride

3.4k total citations
89 papers, 1.6k citations indexed

About

V. A. McBride is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, V. A. McBride has authored 89 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 78 papers in Astronomy and Astrophysics, 23 papers in Nuclear and High Energy Physics and 16 papers in Computational Mechanics. Recurrent topics in V. A. McBride's work include Astrophysical Phenomena and Observations (65 papers), Pulsars and Gravitational Waves Research (38 papers) and Gamma-ray bursts and supernovae (24 papers). V. A. McBride is often cited by papers focused on Astrophysical Phenomena and Observations (65 papers), Pulsars and Gravitational Waves Research (38 papers) and Gamma-ray bursts and supernovae (24 papers). V. A. McBride collaborates with scholars based in United Kingdom, South Africa and United States. V. A. McBride's co-authors include M. J. Coe, A. J. Bird, J. L. Galache, A. Bazzano, A. B. Hill, A. Udalski, L. J. Townsend, R. H. D. Corbet, M. P. E. Schurch and P. Kretschmar and has published in prestigious journals such as Science, The Astrophysical Journal and Cancer.

In The Last Decade

V. A. McBride

80 papers receiving 1.5k citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
V. A. McBride United Kingdom	24	1.4k	434	235	177	134	89	1.6k
J. Fabregat Spain	24	1.6k 1.1×	162 0.4×	212 0.9×	146 0.8×	73 0.5×	117	1.7k
M. Tashiro Japan	22	1.4k 1.0×	982 2.3×	105 0.4×	23 0.1×	96 0.7×	135	1.7k
Kiyoshi Hayashida Japan	18	944 0.7×	457 1.1×	59 0.3×	22 0.1×	95 0.7×	93	1.2k
W. Steffen Mexico	22	1.2k 0.8×	305 0.7×	10 0.0×	47 0.3×	244 1.8×	98	1.6k
R. D. Saxton Spain	25	1.8k 1.3×	646 1.5×	90 0.4×	51 0.3×	75 0.6×	88	1.9k
P. D’Avanzo Italy	26	2.1k 1.5×	550 1.3×	182 0.8×	42 0.2×	98 0.7×	146	2.1k
Yuichiro Sekiguchi Japan	32	3.4k 2.4×	1.1k 2.6×	408 1.7×	51 0.3×	116 0.9×	76	3.7k
M. Giustini Spain	20	1.1k 0.8×	387 0.9×	87 0.4×	27 0.2×	80 0.6×	40	1.2k
F. Nicastro United States	30	2.8k 1.9×	1.2k 2.7×	48 0.2×	38 0.2×	34 0.3×	102	2.9k
K. Matthews United States	20	1.4k 1.0×	87 0.2×	16 0.1×	27 0.2×	39 0.3×	83	1.7k

Countries citing papers authored by V. A. McBride

Since Specialization

Citations

This map shows the geographic impact of V. A. McBride'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 V. A. McBride with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites V. A. McBride more than expected).

Fields of papers citing papers by V. A. McBride

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by V. A. McBride. 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 V. A. McBride. The network helps show where V. A. McBride may publish in the future.

Co-authorship network of co-authors of V. A. McBride

This figure shows the co-authorship network connecting the top 25 collaborators of V. A. McBride. A scholar is included among the top collaborators of V. A. McBride 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 V. A. McBride. V. A. McBride is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Monageng, I. M., V. A. McBride, J. Alfonso-Garzón, et al.. (2023). 4U 1210−64: a new member of the rare intermediate-mass X-ray binary subclass. Monthly Notices of the Royal Astronomical Society. 527(3). 5293–5301. 1 indexed citations

Corbet, R. H. D., Laura Chomiuk, G. Dubus, et al.. (2022). Gamma-Ray Eclipses and Orbital Modulation Transitions in the Candidate Redback 4FGL J1702.7–5655. The Astrophysical Journal. 935(1). 2–2. 9 indexed citations

Bloemen, S., P. Groot, R. J. P. Lyon, et al.. (2021). MeerCRAB: MeerLICHT classification of real and bogus transients using deep learning. Experimental Astronomy. 51(2). 319–344. 15 indexed citations

Lyon, R. J. P., et al.. (2020). Imbalance learning for variable star classification. Monthly Notices of the Royal Astronomical Society. 493(4). 6050–6059. 26 indexed citations

Alonso-Santiago, J., A. Marco, I. Negueruela, et al.. (2018). NGC 3105: a young open cluster with low metallicity. Springer Link (Chiba Institute of Technology). 10 indexed citations

Malacaria, Christian, W. Kollatschny, E. T. Whelan, et al.. (2017). Optical spectroscopy of the Be/X-ray binary V850 Centauri/GX 304-1 during faint X-ray periodical activity. Springer Link (Chiba Institute of Technology). 6 indexed citations

Townsend, L. J., J. A. Kennea, M. J. Coe, et al.. (2017). The 2016 super-Eddington outburst of SMC X-3: X-ray and optical properties and system parameters. Monthly Notices of the Royal Astronomical Society. 471(4). 3878–3887. 40 indexed citations

Coe, M. J., A. J. Bird, V. A. McBride, et al.. (2014). Detection of an X-ray outburst by INTEGRAL from a previously unknown SMC source IGR J01217-7257. ATel. 5806. 1. 1 indexed citations

Niccolai, Linda M., et al.. (2014). Sources of information for assessing human papillomavirus vaccination history among young women. Vaccine. 32(25). 2945–2947. 9 indexed citations

10.

Coe, M. J., A. J. Bird, V. A. McBride, E. S. Bartlett, & F. Haberl. (2013). Detection of a new, bright X-ray source in the Small Magellanic Cloud. The astronomer's telegram. 5547. 1.

11.

Parisi, P., N. Masetti, E. Jiménez‐Bailón, et al.. (2012). Accurate classification of 29 objects detected in the 39 month Palermo Swift /BAT hard X-ray catalogue. Open University of Cape Town (University of Cape Town). 15 indexed citations

12.

Corbet, R. H. D., E. S. Bartlett, M. J. Coe, et al.. (2010). RXTE Detection of an 85.4 s X-ray Pulsar in the Direction of the SMC (SXP 85.4). ATel. 2813. 1. 1 indexed citations

13.

Townsend, L. J., R. H. D. Corbet, M. J. Coe, et al.. (2009). Detection of a 36.3 day orbital period from the HMXB system IGR J01054-7253 with RXTE. ATel. 2202. 1. 1 indexed citations

14.

Coe, M. J., A. J. Bird, V. A. McBride, et al.. (2009). Optical counterpart and a probable pulse period in IGR J01054-7253. The astronomer's telegram. 2088. 1.

15.

Coe, M. J., et al.. (2008). Discovery of a new HMXB in the Magellanic Bridge. ATel. 1882. 1.

16.

McBride, V. A., Anthony J. Dean, A. Bazzano, et al.. (2007). INTEGRAL detection of the pulsar wind nebula in PSR J1846–0258. Springer Link (Chiba Institute of Technology). 13 indexed citations

17.

Negueruela, I., J. M. Torrejón, & V. A. McBride. (2007). The correct optical counterpart to IGR J11435-6109. The astronomer's telegram. 1239. 1. 1 indexed citations

18.

Coburn, W., P. Kretschmar, I. Kreykenbohm, et al.. (2005). Multiple Cyclotron Lines in V0332+53. ATel. 381. 1. 7 indexed citations

19.

Coe, M. J., et al.. (2004). Two new X-ray pulsars detected in the SMC using archive Chandra data (CXOU J005527.9-721058 and CXOU J005455.6-724510).. ATel. 217. 1. 2 indexed citations

20.

Coe, M. J., et al.. (2004). A new X-ray pulsar has been detected in the SMC using archive Chandra data (CXOU J005323.8-722715).. ATel. 220. 1.

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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