C. E. Corsi

995 total citations
26 papers, 505 citations indexed

About

C. E. Corsi is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, C. E. Corsi has authored 26 papers receiving a total of 505 indexed citations (citations by other indexed papers that have themselves been cited), including 24 papers in Astronomy and Astrophysics, 11 papers in Instrumentation and 4 papers in Computational Mechanics. Recurrent topics in C. E. Corsi's work include Stellar, planetary, and galactic studies (23 papers), Astronomy and Astrophysical Research (11 papers) and Astrophysics and Star Formation Studies (10 papers). C. E. Corsi is often cited by papers focused on Stellar, planetary, and galactic studies (23 papers), Astronomy and Astrophysical Research (11 papers) and Astrophysics and Star Formation Studies (10 papers). C. E. Corsi collaborates with scholars based in Italy, Chile and Germany. C. E. Corsi's co-authors include R. Buonanno, F. Fusi Pecci, R. Zinn, Harvey B. Richer, M. Castellani, L. Pulone, G. Marconi, Eduardo Hardy, M. Monelli and G. Bono and has published in prestigious journals such as The Astrophysical Journal, The Astronomical Journal and Symposium - International Astronomical Union.

In The Last Decade

C. E. Corsi

24 papers receiving 491 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
C. E. Corsi Italy	13	496	257	24	13	13	26	505
E. Nasi Italy	8	570 1.1×	321 1.2×	28 1.2×	12 0.9×	15 1.2×	18	582
A. M. Piersimoni Italy	14	496 1.0×	265 1.0×	27 1.1×	12 0.9×	13 1.0×	19	501
A. Recio-Blanco Italy	9	591 1.2×	328 1.3×	47 2.0×	7 0.5×	6 0.5×	9	603
F. Matteucci Italy	8	522 1.1×	206 0.8×	30 1.3×	7 0.5×	6 0.5×	8	531
X. W. Liu China	7	351 0.7×	163 0.6×	18 0.8×	17 1.3×	22 1.7×	9	357
C. Bonatto Brazil	16	873 1.8×	489 1.9×	10 0.4×	13 1.0×	11 0.8×	34	881
N. Krumm United States	10	413 0.8×	229 0.9×	24 1.0×	10 0.8×	11 0.8×	22	424
P. François France	6	459 0.9×	240 0.9×	35 1.5×	24 1.8×	18 1.4×	8	464
D. R. H. Johnson United Kingdom	6	763 1.5×	358 1.4×	39 1.6×	9 0.7×	34 2.6×	8	774
E. D. Friel United States	8	429 0.9×	244 0.9×	15 0.6×	25 1.9×	23 1.8×	15	433

Countries citing papers authored by C. E. Corsi

Since Specialization

Citations

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

Fields of papers citing papers by C. E. Corsi

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by C. E. Corsi. 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. E. Corsi. The network helps show where C. E. Corsi may publish in the future.

Co-authorship network of co-authors of C. E. Corsi

This figure shows the co-authorship network connecting the top 25 collaborators of C. E. Corsi. A scholar is included among the top collaborators of C. E. Corsi 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. E. Corsi. C. E. Corsi 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

Sanna, N., G. Bono, P. B. Stetson, et al.. (2008). On the Distance and Reddening of the Starburst Galaxy IC 10. The Astrophysical Journal. 688(2). L69–L73. 18 indexed citations

Principe, M., A. M. Piersimoni, J. Storm, et al.. (2006). A Pulsational Distance to ω Centauri Based on Near‐Infrared Period‐Luminosity Relations of RR Lyrae Stars. The Astrophysical Journal. 652(1). 362–369. 44 indexed citations

Freyhammer, L. M., M. Monelli, G. Bono, et al.. (2005). On the Anomalous Red Giant Branch of the Globular Cluster ω Centauri. The Astrophysical Journal. 623(2). 860–865. 9 indexed citations

Calamida, A., P. B. Stetson, G. Bono, et al.. (2005). Reddening Distribution across the Center of the Globular Cluster ω Centauri. The Astrophysical Journal. 634(1). L69–L72. 32 indexed citations

Monelli, M., A. R. Walker, G. Bono, et al.. (2004). Short and long period variable stars in the Carina dwarf Spheroidal galaxy. International Astronomical Union Colloquium. 193. 133–137. 2 indexed citations

Dall’Ora, M., J. Storm, G. Bono, et al.. (2004). The Distance to the Large Magellanic Cloud Cluster Reticulum from theK‐Band Period‐Luminosity‐Metallicity Relation of RR Lyrae Stars. The Astrophysical Journal. 610(1). 269–274. 38 indexed citations

Dall’Ora, M., G. Bono, J. Storm, et al.. (2004). Near-Infrared photometry of the LMC cluster Reticulum. International Astronomical Union Colloquium. 193. 189–192.

Ripepi, V., F. Caputo, V. Castellani, et al.. (2003). The Carina Project: I. Bright Variable Stars 1. 35 indexed citations

Marconi, G., R. Buonanno, M. Castellani, C. E. Corsi, & R. Zinn. (1999). Star Formation History in the Fornax Dwarf Galaxy from HST data. Symposium - International Astronomical Union. 192. 174–178. 3 indexed citations

10.

Buonanno, R., C. E. Corsi, L. Pulone, F. Fusi Pecci, & M. Bellazzini. (1998). On the relative ages of galactic globular clusters. A new observable, a semi-empirical calibration and problems with the theoretical isochrones. 333(2). 505–523. 1 indexed citations

11.

Buonanno, R., et al.. (1995). Terzan 7: A young metal-rich globular cluster in the Milky Way. The Astronomical Journal. 109. 663–663. 25 indexed citations

12.

Buonanno, R., C. E. Corsi, F. Fusi Pecci, Harvey B. Richer, & Gregory G. Fahlman. (1995). Young globular clusters in the Milky Way: ARP 2. The Astronomical Journal. 109. 650–650. 18 indexed citations

13.

Ferraro, F. R., F. Fusi Pecci, C. Cacciari, et al.. (1993). Blue Stragglers in the Galactic globular clusters M3: Evidence for two populations. The Astronomical Journal. 106. 2324–2324. 62 indexed citations

14.

Buonanno, R., C. Cacciari, C. E. Corsi, & F. Fusi Pecci. (1990). The ZAHB luminosity-metallicity relationship as derived from main sequence fitting. 230(2). 315–325. 1 indexed citations

15.

Buonanno, R., A. Buzzoni, C. E. Corsi, F. Fusi Pecci, & Allan Sandage. (1988). High Precision Photometry of 10,000 Stars in M 3. Symposium - International Astronomical Union. 126. 621–622. 1 indexed citations

16.

Alcaíno, G., R. Buonanno, V. Caloi, et al.. (1987). The CM diagram of the nearby globular cluster NGC 6397. The Astronomical Journal. 94. 917–917. 9 indexed citations

17.

Renzini, A., et al.. (1985). Asymptotic giant branch stars in the Large Magellanic Cloud Results from a deep BV survey and theoretical implications. The Astrophysical Journal. 294. L7–L7. 2 indexed citations

18.

Hardy, Eduardo, et al.. (1984). The population structure of the large Magellanic Cloud bar. The Astrophysical Journal. 278. 592–592. 19 indexed citations

19.

Buonanno, R., et al.. (1984). On the suggested peculiarity of the galactic globular cluster NGC 288. The Astrophysical Journal. 277. 220–220. 4 indexed citations

20.

Buzzoni, A., F. Fusi Pecci, R. Buonanno, & C. E. Corsi. (1983). Helium abundance in globular clusters: the R-method. 128(1). 94–101. 15 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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