B. J. Maughan

3.5k total citations
38 papers, 970 citations indexed

About

B. J. Maughan is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, B. J. Maughan has authored 38 papers receiving a total of 970 indexed citations (citations by other indexed papers that have themselves been cited), including 38 papers in Astronomy and Astrophysics, 8 papers in Instrumentation and 8 papers in Nuclear and High Energy Physics. Recurrent topics in B. J. Maughan's work include Galaxies: Formation, Evolution, Phenomena (37 papers), Astrophysical Phenomena and Observations (27 papers) and Stellar, planetary, and galactic studies (14 papers). B. J. Maughan is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (37 papers), Astrophysical Phenomena and Observations (27 papers) and Stellar, planetary, and galactic studies (14 papers). B. J. Maughan collaborates with scholars based in United Kingdom, United States and France. B. J. Maughan's co-authors include C. Jones, L. van Speybroeck, W. Forman, H. Ebeling, Paul Giles, Caleb Scharf, Massimiliano Bonamente, G. Trinchieri, S. Andreon and J. Kurk and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

B. J. Maughan

38 papers receiving 929 citations

Peers

B. J. Maughan
Emmanouil Papastergis Netherlands
S. I. Loubser South Africa
I. Delvecchio Italy
S. Maurogordato France
Allison Merritt United States
Joe Wolf United States
Lamiya Mowla United States
Louis E. Abramson United States
Chiara Tonini Australia
Camilla Penzo Germany
Emmanouil Papastergis Netherlands
B. J. Maughan
Citations per year, relative to B. J. Maughan B. J. Maughan (= 1×) peers Emmanouil Papastergis

Countries citing papers authored by B. J. Maughan

Since Specialization
Citations

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

Fields of papers citing papers by B. J. Maughan

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by B. J. Maughan. 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 B. J. Maughan. The network helps show where B. J. Maughan may publish in the future.

Co-authorship network of co-authors of B. J. Maughan

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

All Works

20 of 20 papers shown
1.
Bourdin, H., Federico De Luca, P. Mazzotta, et al.. (2023). CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters. Astronomy and Astrophysics. 678. A181–A181. 1 indexed citations
2.
Oppizzi, F., Federico De Luca, H. Bourdin, et al.. (2023). CHEX-MATE: Pressure profiles of six galaxy clusters as seen by SPT and Planck. Astronomy and Astrophysics. 672. A156–A156. 3 indexed citations
3.
Bhargava, S, C. Garrel, E. Koulouridis, et al.. (2023). The XXL Survey. Astronomy and Astrophysics. 673. A92–A92. 3 indexed citations
4.
Wik, Daniel R., et al.. (2023). The Hydrostatic Mass of A478: Discrepant Results from Chandra, NuSTAR, and XMM-Newton. The Astrophysical Journal. 958(2). 112–112. 1 indexed citations
5.
McGee, Sean, T. J. Ponman, M. E. Ramos-Ceja, et al.. (2022). The XXL Survey. Astronomy and Astrophysics. 663. A2–A2. 5 indexed citations
6.
Maughan, B. J., et al.. (2022). Chandrafollow-up of the Hectospec Cluster Survey: Comparison of caustic and hydrostatic masses and constraints on the hydrostatic bias. Astronomy and Astrophysics. 665. A124–A124. 6 indexed citations
7.
Pratt, G. W., M. Arnaud, B. J. Maughan, & J.-B. Mélin. (2022). Linking a universal gas density profile to the core-excised X-ray luminosity in galaxy clusters up to z ∼ 1.1. Astronomy and Astrophysics. 665. A24–A24. 10 indexed citations
8.
Sereno, M., Keiichi Umetsu, S. Ettori, et al.. (2019). XXL Survey groups and clusters in the Hyper Suprime-Cam Survey. Scaling relations between X-ray properties and weak lensing mass. Monthly Notices of the Royal Astronomical Society. 492(3). 4528–4545. 16 indexed citations
9.
Maughan, B. J., Paul Giles, Kenneth J. Rines, et al.. (2016). Hydrostatic and caustic mass profiles of galaxy clusters. Monthly Notices of the Royal Astronomical Society. 461(4). 4182–4191. 27 indexed citations
10.
Clerc, N., C. Adami, Maggie Lieu, et al.. (2014). The XMM-LSS survey: the Class 1 cluster sample over the extended 11 deg2 and its spatial distribution. Monthly Notices of the Royal Astronomical Society. 444(3). 2723–2753. 27 indexed citations
11.
Mantz, A., J. E. Carlstrom, Christopher H. Greer, et al.. (2014). THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1–034536 WITH CARMA. The Astrophysical Journal. 794(2). 157–157. 27 indexed citations
12.
Laganá, T. F., et al.. (2013). A comprehensive picture of baryons in groups and clusters of galaxies. Springer Link (Chiba Institute of Technology). 33 indexed citations
13.
Sayers, Jack, Nicole G. Czakon, A. Mantz, et al.. (2013). SUNYAEV-ZEL'DOVICH-MEASURED PRESSURE PROFILES FROM THE BOLOCAM X-RAY/SZ GALAXY CLUSTER SAMPLE. The Astrophysical Journal. 768(2). 177–177. 59 indexed citations
14.
Pierre, M., et al.. (2012). AChandraview of thez = 1.62 galaxy cluster IRC-0218A. Astronomy and Astrophysics. 540. A4–A4. 20 indexed citations
15.
Andreon, S., B. J. Maughan, G. Trinchieri, & J. Kurk. (2009). JKCS 041: a colour-detected galaxy cluster at $z_{\mathrm{phot}}$ ~ 1.9 with deep potential well as confirmed by X-ray data. Astronomy and Astrophysics. 507(1). 147–157. 59 indexed citations
16.
Mroczkowski, Tony, Massimiliano Bonamente, J. E. Carlstrom, et al.. (2009). APPLICATION OF A SELF-SIMILAR PRESSURE PROFILE TO SUNYAEV-ZEL'DOVICH EFFECT DATA FROM GALAXY CLUSTERS. The Astrophysical Journal. 694(2). 1034–1044. 41 indexed citations
17.
Maughan, B. J., C. Jones, W. Forman, & L. van Speybroeck. (2008). Images, Structural Properties, and Metal Abundances of Galaxy Clusters Observed withChandraACIS‐I at 0.1 <z< 1.3. The Astrophysical Journal Supplement Series. 174(1). 117–135. 169 indexed citations
18.
Horner, D., Eric S. Perlman, H. Ebeling, et al.. (2008). The WARPS Survey. VII. The WARPS‐II Cluster Catalog. The Astrophysical Journal Supplement Series. 176(2). 374–413. 27 indexed citations
19.
Maughan, B. J.. (2007). TheLX‐YXRelation: Using Galaxy Cluster X‐Ray Luminosity as a Robust, Low‐Scatter Mass Proxy. The Astrophysical Journal. 668(2). 772–780. 85 indexed citations
20.
Maughan, B. J., L. R. Jones, H. Ebeling, et al.. (2003). ChandraX‐Ray Analysis of the Massive High‐Redshift Galaxy Clusters Cl J1113.1−2615 and Cl J0152.7−1357. The Astrophysical Journal. 587(2). 589–604. 50 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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