J. G. Bartlett

39.3k total citations · 1 hit paper
25 papers, 933 citations indexed

About

J. G. Bartlett is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, J. G. Bartlett has authored 25 papers receiving a total of 933 indexed citations (citations by other indexed papers that have themselves been cited), including 20 papers in Astronomy and Astrophysics, 8 papers in Nuclear and High Energy Physics and 3 papers in Computational Mechanics. Recurrent topics in J. G. Bartlett's work include Galaxies: Formation, Evolution, Phenomena (15 papers), Cosmology and Gravitation Theories (14 papers) and Astrophysical Phenomena and Observations (7 papers). J. G. Bartlett is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (15 papers), Cosmology and Gravitation Theories (14 papers) and Astrophysical Phenomena and Observations (7 papers). J. G. Bartlett collaborates with scholars based in France, United States and United Kingdom. J. G. Bartlett's co-authors include P. Fernique, F. Genova, D. Egret, Mireille Louys, M. Wenger, F. Bonnarel, O. Bienaymé, Alain Blanchard, Philippe Marty and David H. Lumb and has published in prestigious journals such as Physical Review Letters, Monthly Notices of the Royal Astronomical Society and The Journal of Infectious Diseases.

In The Last Decade

J. G. Bartlett

25 papers receiving 875 citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

The ALADIN interactive sky atlas

2000 495 citations F. Bonnarel, P. Fernique et al. profile →

Peers

J. G. Bartlett

AA

INSTR

NHEP

CM

SNP

J. E. Steiner Brazil

Steffen Heß Germany

Beth Reid United States

Nicholas Scott Australia

Kelsey E. Johnson United States

Alessandro B. Romeo Sweden

M. R. S. Hawkins United Kingdom

Chris Pearson United Kingdom

R. C. Kraan‐Korteweg South Africa

Y. Ascasíbar Spain

J. E. Steiner Brazil

J. G. Bartlett

1.3k ×1.6

AA

301 ×1.1

INSTR

182 ×0.8

NHEP

88 ×1.3

CM

33 ×1.1

SNP

Citations per year, relative to J. G. Bartlett J. G. Bartlett (= 1×) peers J. E. Steiner

Countries citing papers authored by J. G. Bartlett

Since Specialization

Citations

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

Fields of papers citing papers by J. G. Bartlett

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of J. G. Bartlett

This figure shows the co-authorship network connecting the top 25 collaborators of J. G. Bartlett. A scholar is included among the top collaborators of J. G. Bartlett 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 J. G. Bartlett. J. G. Bartlett 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

1.

Mélin, J.-B., et al.. (2020). PSZSPT: a joint Planck and SPT-SZ cluster catalogue. HAL (Le Centre pour la Communication Scientifique Directe). 13 indexed citations

2.

Bartlett, J. G., Eduardo Rozo, J.‐B. Melin, et al.. (2017). Calibrating thePlanckcluster mass scale with CLASH. Astronomy and Astrophysics. 604. A89–A89. 28 indexed citations

3.

Sartoris, B., A. Biviano, C. Fedeli, et al.. (2016). Next generation cosmology: constraints from theEuclidgalaxy cluster survey. Monthly Notices of the Royal Astronomical Society. 459(2). 1764–1780. 109 indexed citations

4.

Chamballu, A., J. G. Bartlett, & J.-B. Mélin. (2012). ThePlanckSZ Cluster Catalog: expected X-ray properties. Astronomy and Astrophysics. 544. A40–A40. 2 indexed citations

5.

Gaume, R. A., G. S. Hennessy, R. P. Dudik, et al.. (2009). The Joint Milli-Arcsecond Pathfinder Survey (J-MAPS) Mission: Introduction and Science Goals. AAS. 213. 1 indexed citations

6.

Baccigalupi, C., A. Balbi, J. G. Bartlett, et al.. (2007). Making maps from Planck LFI 30 GHz data. Astronomy and Astrophysics. 471(1). 361–380. 14 indexed citations

7.

Baccigalupi, C., A. Balbi, J. G. Bartlett, et al.. (2007). Making sky maps from Planck data. Astronomy and Astrophysics. 467(2). 761–775. 26 indexed citations

8.

Bartlett, J. G. & J.-B. Mélin. (2006). Point source confusion in SZ cluster surveys. Astronomy and Astrophysics. 447(2). 405–412. 3 indexed citations

9.

Sadat, R., S. Vauclair, David H. Lumb, et al.. (2005). TheXMM-Newton$\mathsf{\Omega}$ project. Astronomy and Astrophysics. 437(1). 31–38. 25 indexed citations

10.

Mei, S. & J. G. Bartlett. (2004). Cosmological constraints from a 2D SZ catalog. Springer Link (Chiba Institute of Technology). 6 indexed citations

11.

Mélin, J.-B., J. G. Bartlett, & G. de Zotti. (2004). The selection function of SZ cluster surveys. Astronomy and Astrophysics. 429(2). 417–426. 18 indexed citations

12.

Lumb, David H., J. G. Bartlett, A. K. Romer, et al.. (2004). The XMM-NEWTONΩproject. Astronomy and Astrophysics. 420(3). 853–872. 31 indexed citations

13.

Mei, S. & J. G. Bartlett. (2003). On the angular correlation function of SZ clusters: \n Extracting cosmological information from a 2D catalog. Springer Link (Chiba Institute of Technology). 7 indexed citations

14.

Vauclair, S., Alain Blanchard, R. Sadat, et al.. (2003). The XMM-Omega project. II. Cosmological implications from the high redshift L - T relation of X-ray clusters. HAL (Le Centre pour la Communication Scientifique Directe). 23 indexed citations

15.

Vauclair, S., Alain Blanchard, R. Sadat, et al.. (2003). The XMM-Ω project. Astronomy and Astrophysics. 412(2). L37–L41. 25 indexed citations

16.

Bartlett, J. G., et al.. (2002). The Victorian emergency department collaboration. International Journal for Quality in Health Care. 14(6). 463–470. 27 indexed citations

17.

Bartlett, J. G., et al.. (2000). Approximating the Likelihood Function of CMB Experiments. CERN Bulletin. 37. 321. 1 indexed citations

18.

Genova, F., J. G. Bartlett, O. Bienaymé, et al.. (1996). CDS as an astronomical information HUB. Vistas in Astronomy. 40(3). 429–437. 1 indexed citations

19.

Bartlett, J. G. & Lawrence J. Hall. (1991). Closed baryonic universe from photon cooling. Physical Review Letters. 66(5). 541–544. 16 indexed citations

20.

Laughon, Barbara E., Andrew Vernon, Daniel Druckman, et al.. (1988). Recovery of Campylobacter Species from Homosexual Men. The Journal of Infectious Diseases. 158(2). 464–467. 13 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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