E. V. Held

2.8k total citations
81 papers, 1.4k citations indexed

About

E. V. Held is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, E. V. Held has authored 81 papers receiving a total of 1.4k indexed citations (citations by other indexed papers that have themselves been cited), including 75 papers in Astronomy and Astrophysics, 59 papers in Instrumentation and 12 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in E. V. Held's work include Stellar, planetary, and galactic studies (66 papers), Astronomy and Astrophysical Research (59 papers) and Galaxies: Formation, Evolution, Phenomena (40 papers). E. V. Held is often cited by papers focused on Stellar, planetary, and galactic studies (66 papers), Astronomy and Astrophysical Research (59 papers) and Galaxies: Formation, Evolution, Phenomena (40 papers). E. V. Held collaborates with scholars based in Italy, United States and Chile. E. V. Held's co-authors include I. Saviane, Marco Gullieuszik, L. Rizzi, G. S. Da Costa, Y. Momany, S. Ortolani, G. Clementini, B. Barbuy, M. Vietri and S. Zaggia and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Annals of the New York Academy of Sciences.

In The Last Decade

E. V. Held

78 papers receiving 1.3k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
E. V. Held Italy 24 1.4k 722 110 44 19 81 1.4k
L. M. Buson Italy 19 1.2k 0.9× 569 0.8× 93 0.8× 28 0.6× 14 0.7× 57 1.2k
Themiya Nanayakkara Australia 19 1.1k 0.8× 600 0.8× 131 1.2× 39 0.9× 22 1.2× 61 1.2k
I. Zolotukhin Russia 9 818 0.6× 355 0.5× 89 0.8× 36 0.8× 20 1.1× 17 835
Kuenley Chiu United States 13 1.0k 0.8× 460 0.6× 124 1.1× 67 1.5× 30 1.6× 17 1.1k
E. M. Malumuth United States 18 842 0.6× 373 0.5× 87 0.8× 64 1.5× 22 1.2× 50 883
K. Boutsia Italy 18 1.1k 0.8× 521 0.7× 167 1.5× 65 1.5× 21 1.1× 49 1.1k
J. Graciá‐Carpio Spain 23 1.9k 1.4× 436 0.6× 205 1.9× 33 0.8× 14 0.7× 33 2.0k
Georges Meylan United States 12 1.0k 0.7× 428 0.6× 62 0.6× 45 1.0× 14 0.7× 21 1.0k
C. Balkowski France 14 1.2k 0.9× 456 0.6× 156 1.4× 26 0.6× 26 1.4× 41 1.2k
J. E. Hibbard United States 19 1.6k 1.2× 662 0.9× 135 1.2× 61 1.4× 23 1.2× 36 1.6k

Countries citing papers authored by E. V. Held

Since Specialization
Citations

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

Fields of papers citing papers by E. V. Held

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of E. V. Held

This figure shows the co-authorship network connecting the top 25 collaborators of E. V. Held. A scholar is included among the top collaborators of E. V. Held 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 E. V. Held. E. V. Held 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.
Ortolani, S., E. V. Held, D. Nardiello, et al.. (2019). Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2). Springer Link (Chiba Institute of Technology). 12 indexed citations
2.
Spavone, Marilena, E. Iodice, R. Rampazzo, et al.. (2019). VEGAS: A VST Early-type GAlaxy Survey. IV. NGC 1533, IC 2038, and IC 2039: An Interacting Triplet in the Dorado Group. The Astrophysical Journal. 874(2). 130–130. 19 indexed citations
3.
Vásquez, S., I. Saviane, E. V. Held, et al.. (2018). Homogeneous metallicities and radial velocities for Galactic globular clusters. Astronomy and Astrophysics. 619. A13–A13. 22 indexed citations
4.
Dias, Bruno, B. Barbuy, I. Saviane, et al.. (2016). FORS2/VLT survey of Milky Way globular clusters. Astronomy and Astrophysics. 590. A9–A9. 58 indexed citations
5.
Momany, Y., S. Ortolani, E. V. Held, et al.. (2015). V, J, H and K imaging of the metal rich globular cluster NGC 6528 : reddening, metallicity, and distance based on cleaned colour-magnitude diagrams. Americanae (AECID Library). 4 indexed citations
6.
Saviane, I., et al.. (2014). Homogeneous Metallicities and Radial Velocities for Galactic Globular Clusters⋆ First CaT metallicities for twenty clusters. ANU Open Research (Australian National University). 36 indexed citations
7.
Costa, G. S. Da, E. V. Held, & I. Saviane. (2014). NGC 5824: a luminous outer halo globular cluster with an intrinsic abundance spread. Monthly Notices of the Royal Astronomical Society. 438(4). 3507–3520. 30 indexed citations
8.
Dias, Bruno, B. Barbuy, I. Saviane, et al.. (2014). FORS2/VLT survey of Milky Way globular clusters. Astronomy and Astrophysics. 573. A13–A13. 21 indexed citations
9.
Saviane, I., E. V. Held, G. S. Da Costa, et al.. (2012). New Surprises in Old Stellar Clusters. ˜The œMessenger. 149. 23–27.
10.
Saviane, I., V. D. Ivanov, E. V. Held, et al.. (2008). Luminosity-metallicity relation for dIrr galaxies in the near-infrared. Astronomy and Astrophysics. 487(3). 901–920. 20 indexed citations
11.
Gullieuszik, Marco, E. V. Held, L. Rizzi, et al.. (2007). Near-infrared observations of the Fornax dwarf galaxy. Springer Link (Chiba Institute of Technology). 25 indexed citations
12.
Momany, Y., E. V. Held, I. Saviane, et al.. (2007). The blue plume population in dwarf spheroidal galaxies. Astronomy and Astrophysics. 468(3). 973–978. 52 indexed citations
13.
Salaris, M., E. V. Held, S. Ortolani, Marco Gullieuszik, & Y. Momany. (2007). Deep near-infrared photometry of the globular cluster 47 Tucanae. Reconciling theory and observations. Astronomy and Astrophysics. 476(1). 243–253. 38 indexed citations
14.
Vallenari, A., et al.. (2006). Age distribution of young clusters and field stars in the Small Magellanic Cloud. Springer Link (Chiba Institute of Technology). 53 indexed citations
15.
Berta, S., Stefano Rubele, A. Franceschini, et al.. (2006). The ESO-Spitzer Imaging extragalactic Survey (ESIS). Astronomy and Astrophysics. 451(3). 881–900. 33 indexed citations
16.
Clementini, G., V. Ripepi, A. Bragaglia, et al.. (2005). The metal abundance distribution of the oldest stellar component in the Sculptor dwarf spheroidal galaxy★. Monthly Notices of the Royal Astronomical Society. 363(3). 734–748. 24 indexed citations
17.
Held, E. V., et al.. (2005). The stellar populations of local dwarfs. 2 indexed citations
18.
Saviane, I., E. V. Held, Y. Momany, & L. Rizzi. (2001). Population gradients in nearby dwarf galaxies. CERN Bulletin. 72. 773–778. 1 indexed citations
19.
Richtler, T., et al.. (1993). NGC 4636 - a rich globular cluster system in a normal elliptical galaxy.. ˜The œMessenger. 73. 183–34. 1 indexed citations
20.
Capaccioli, M., et al.. (1988). Application of an adaptive filtering technique to surface photometry of galaxies. I. The method tested on NGC 3379. Astronomische Nachrichten. 309(2). 69–80. 7 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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