S. Galleti

12.2k total citations
37 papers, 966 citations indexed

About

S. Galleti is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, S. Galleti has authored 37 papers receiving a total of 966 indexed citations (citations by other indexed papers that have themselves been cited), including 37 papers in Astronomy and Astrophysics, 21 papers in Instrumentation and 4 papers in Computational Mechanics. Recurrent topics in S. Galleti's work include Stellar, planetary, and galactic studies (36 papers), Galaxies: Formation, Evolution, Phenomena (22 papers) and Astronomy and Astrophysical Research (21 papers). S. Galleti is often cited by papers focused on Stellar, planetary, and galactic studies (36 papers), Galaxies: Formation, Evolution, Phenomena (22 papers) and Astronomy and Astrophysical Research (21 papers). S. Galleti collaborates with scholars based in Italy, Spain and Germany. S. Galleti's co-authors include M. Bellazzini, F. Fusi Pecci, L. Federici, A. Buzzoni, V. Caloi, Robert T. Rood, F. R. Ferraro, S. Perina, Tom Oosterloo and C. Cacciari and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

S. Galleti

36 papers receiving 948 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
S. Galleti Italy 17 955 460 36 22 19 37 966
L. Federici Italy 17 885 0.9× 442 1.0× 15 0.4× 23 1.0× 21 1.1× 41 898
K. Pilkington United States 11 799 0.8× 282 0.6× 46 1.3× 28 1.3× 9 0.5× 14 803
Alexa Villaume United States 15 697 0.7× 458 1.0× 56 1.6× 24 1.1× 23 1.2× 22 711
C. G. Few United Kingdom 14 639 0.7× 228 0.5× 33 0.9× 27 1.2× 7 0.4× 20 641
Peter A. Bergbusch Canada 9 632 0.7× 328 0.7× 41 1.1× 16 0.7× 10 0.5× 10 638
M. Tripicco United States 10 567 0.6× 298 0.6× 56 1.6× 9 0.4× 19 1.0× 18 583
Alice Concas Germany 13 622 0.7× 324 0.7× 57 1.6× 23 1.0× 12 0.6× 19 647
Florian Niederhofer Germany 21 955 1.0× 578 1.3× 25 0.7× 9 0.4× 14 0.7× 43 982
Miguel A. Urbaneja United States 19 1.0k 1.1× 526 1.1× 34 0.9× 9 0.4× 30 1.6× 48 1.1k
Dana I. Dinescu United States 15 858 0.9× 390 0.8× 42 1.2× 10 0.5× 27 1.4× 25 864

Countries citing papers authored by S. Galleti

Since Specialization
Citations

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

Fields of papers citing papers by S. Galleti

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by S. Galleti. 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 S. Galleti. The network helps show where S. Galleti may publish in the future.

Co-authorship network of co-authors of S. Galleti

This figure shows the co-authorship network connecting the top 25 collaborators of S. Galleti. A scholar is included among the top collaborators of S. Galleti 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 S. Galleti. S. Galleti 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.
Pancino, E., N. Sanna, G. Altavilla, et al.. (2021). The Gaia spectrophotometric standard stars survey – V. Preliminary flux tables for the calibration of Gaia DR2 and (E)DR3. Monthly Notices of the Royal Astronomical Society. 503(3). 3660–3676. 7 indexed citations
2.
Beccari, G., M. Bellazzini, Filippo Fraternali, et al.. (2014). The extended structure of the dwarf irregular galaxy Sagittarius. Springer Link (Chiba Institute of Technology). 9 indexed citations
3.
Bellazzini, M., G. Beccari, Filippo Fraternali, et al.. (2014). The extended structure of the dwarf irregular galaxies Sextans A and Sextans B. Astronomy and Astrophysics. 566. A44–A44. 27 indexed citations
4.
Federici, L., C. Cacciari, M. Bellazzini, et al.. (2012). The horizontal branch luminosity vs. metallicity in M 31 globular clusters. Astronomy and Astrophysics. 544. A155–A155. 19 indexed citations
5.
Perina, S., S. Galleti, F. Fusi Pecci, et al.. (2011). HST/ACS color-magnitude diagrams of candidate intermediate-age M 31 globular clusters. Springer Link (Chiba Institute of Technology). 16 indexed citations
6.
Bellazzini, M., S. Perina, S. Galleti, & Tom Oosterloo. (2011). HST-ACS photometry of the isolated dwarf galaxy VV124=UGC 4879. Astronomy and Astrophysics. 533. A37–A37. 8 indexed citations
7.
Perina, S., Judith G. Cohen, P. Barmby, et al.. (2010). An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates. CaltechAUTHORS (California Institute of Technology). 10 indexed citations
8.
Bellazzini, M., G. Beccari, Tom Oosterloo, et al.. (2010). An optical and H i study of the dwarf Local Group galaxy VV124 = UGC4879. Astronomy and Astrophysics. 527. A58–A58. 19 indexed citations
9.
Perina, S., L. Federici, M. Bellazzini, et al.. (2009). HST/ACS colour–magnitude diagrams of M 31 globular clusters. Springer Link (Chiba Institute of Technology). 20 indexed citations
10.
Perina, S., P. Barmby, Michael A. Beasley, et al.. (2009). An HST/WFPC2 survey of bright young clusters in M31 I. VdB0, a massive star cluster seen at t ≃ a 25 Myr. CaltechAUTHORS (California Institute of Technology). 16 indexed citations
11.
Monaco, L., I. Saviane, S. Perina, et al.. (2009). The young stellar population at the center of NGC 205. Astronomy and Astrophysics. 502(2). L9–L12. 21 indexed citations
12.
Perina, S., P. Barmby, M. Bellazzini, et al.. (2008). An HST/WFPC2 survey of bright young clusters in M31. Astronomy and Astrophysics. 494(3). 933–948. 16 indexed citations
13.
Viotti, Roberto, S. Galleti, R. Gualandi, et al.. (2007). The 2006 hot phase of Romano's star (GR 290) in M 33. Springer Link (Chiba Institute of Technology). 6 indexed citations
14.
Federici, L., M. Bellazzini, S. Galleti, et al.. (2007). The extended structure of the remote cluster B514 in M 31. Astronomy and Astrophysics. 473(2). 429–436. 17 indexed citations
15.
Galleti, S., M. Bellazzini, L. Federici, A. Buzzoni, & F. Fusi Pecci. (2007). An updated survey of globular clusters in M 31. Astronomy and Astrophysics. 471(1). 127–136. 44 indexed citations
16.
Galleti, S., L. Federici, M. Bellazzini, A. Buzzoni, & F. Fusi Pecci. (2006). An updated survey of globular clusters in M 31. Astronomy and Astrophysics. 456(3). 985–999. 48 indexed citations
17.
Bellazzini, M., V. Caloi, F. Fusi Pecci, S. Galleti, & Robert T. Rood. (2005). A helium spread among the main sequence stars in NGC 2808. 184 indexed citations
18.
Galleti, S., M. Bellazzini, L. Federici, & F. Fusi Pecci. (2005). The outermost cluster of M 31. Astronomy and Astrophysics. 436(2). 535–540. 15 indexed citations
19.
Galleti, S., et al.. (2004). 2MASS NIR photometry for 693 candidate globular clusters in M 31 and the Revised Bologna Catalogue. Astronomy and Astrophysics. 416(3). 917–924. 138 indexed citations
20.
Galleti, S., M. Bellazzini, & F. R. Ferraro. (2004). The distance of M 33 and the stellar population in its outskirts. Astronomy and Astrophysics. 423(3). 925–934. 65 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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026