D. Maccagni

10.0k total citations
35 papers, 698 citations indexed

About

D. Maccagni is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, D. Maccagni has authored 35 papers receiving a total of 698 indexed citations (citations by other indexed papers that have themselves been cited), including 24 papers in Astronomy and Astrophysics, 14 papers in Nuclear and High Energy Physics and 12 papers in Instrumentation. Recurrent topics in D. Maccagni's work include Astrophysics and Cosmic Phenomena (13 papers), Galaxies: Formation, Evolution, Phenomena (12 papers) and Astronomy and Astrophysical Research (12 papers). D. Maccagni is often cited by papers focused on Astrophysics and Cosmic Phenomena (13 papers), Galaxies: Formation, Evolution, Phenomena (12 papers) and Astronomy and Astrophysical Research (12 papers). D. Maccagni collaborates with scholars based in Italy, France and United Kingdom. D. Maccagni's co-authors include B. Garilli, P. Giommi, T. Maccacaro, I. M. Gioia, A. M. T. Pollock, P. Barr, Rudolph E. Schild, A. C. Fabian, W. R. Stoeger and M. J. Rees and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

D. Maccagni

34 papers receiving 671 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
D. Maccagni Italy 15 635 338 141 33 27 35 698
Larry Bradley United States 17 986 1.6× 153 0.5× 454 3.2× 31 0.9× 61 2.3× 41 1.1k
A. Cassatella Italy 18 807 1.3× 129 0.4× 120 0.9× 9 0.3× 43 1.6× 68 851
S. M. Adams United States 17 784 1.2× 261 0.8× 154 1.1× 4 0.1× 23 0.9× 31 975
Stefano Marchesi United States 18 985 1.6× 353 1.0× 291 2.1× 28 0.8× 37 1.4× 72 1.0k
E. L. Blanton United States 18 1.4k 2.2× 550 1.6× 199 1.4× 18 0.5× 30 1.1× 43 1.4k
R. D. Cohen United States 18 1.3k 2.0× 313 0.9× 200 1.4× 19 0.6× 50 1.9× 51 1.3k
P. Jakobsson Denmark 24 1.9k 3.0× 338 1.0× 225 1.6× 26 0.8× 24 0.9× 136 1.9k
D. Alloin France 21 1.2k 1.9× 168 0.5× 422 3.0× 18 0.5× 71 2.6× 94 1.3k
A. G. Pacholczyk United States 11 531 0.8× 380 1.1× 42 0.3× 21 0.6× 24 0.9× 50 582
Lukas Labhardt United States 12 734 1.2× 114 0.3× 165 1.2× 20 0.6× 28 1.0× 16 751

Countries citing papers authored by D. Maccagni

Since Specialization
Citations

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

Fields of papers citing papers by D. Maccagni

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. Maccagni

This figure shows the co-authorship network connecting the top 25 collaborators of D. Maccagni. A scholar is included among the top collaborators of D. Maccagni 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 D. Maccagni. D. Maccagni 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.
Vietri, G., B. Garilli, M. Polletta, et al.. (2021). The Type II AGN-host galaxy connection. Astronomy and Astrophysics. 659. A129–A129. 18 indexed citations
2.
Marchi, F., L. Pentericci, L. Guaita, et al.. (2018). Lyα-Lyman continuum connection in 3.5 ≤ z ≤ 4.3 star-forming galaxies from the VUDS survey. Astronomy and Astrophysics. 614. A11–A11. 45 indexed citations
3.
Cassata, P., O. Le Fèvre, S. Charlot, et al.. (2013). He II emitters in the VIMOS VLT Deep Survey: Population III star formation or peculiar stellar populations in galaxies at 2 <z< 4.6?. Astronomy and Astrophysics. 556. A68–A68. 45 indexed citations
4.
López-Sanjuán, C., O. Le Fèvre, L. de Ravel, et al.. (2011). The VIMOS VLT Deep Survey. Astronomy and Astrophysics. 530. A20–A20. 45 indexed citations
5.
Fèvre, O. Le, L. Hill, D. Le Mignant, et al.. (2010). OPTIMOS-DIORAMAS: A Wide-field Imaging and Multi-slit Spectrograph for the E-ELT. Msngr. 140. 34–35. 1 indexed citations
6.
Meneux, B., B. Garilli, D. Maccagni, et al.. (2007). VIMOS-VLT Deep Survey: Galaxy Structures in the Wide Sample. ASPC. 379. 320. 1 indexed citations
7.
Tajer, M., M. Polletta, L. Chiappetti, et al.. (2007). Obscured and unobscured AGN populations in a hard-X-ray selected sample of the XMDS survey. Astronomy and Astrophysics. 467(1). 73–91. 25 indexed citations
8.
Gandhi, P., O. Garcet, F. Pacaud, et al.. (2006). The XMM large scale structure survey: properties and two-point angular correlations of point-like sources. Astronomy and Astrophysics. 457(2). 393–404. 22 indexed citations
9.
Chiappetti, L., M. Tajer, G. Trinchieri, et al.. (2005). The XMM-LSS survey. Astronomy and Astrophysics. 439(1). 413–425. 26 indexed citations
10.
Bolzonella, M., R. Pelló, & D. Maccagni. (2002). Luminosity functions beyond the spectroscopic limit. Astronomy and Astrophysics. 395(2). 443–463. 12 indexed citations
11.
Bolzonella, M., R. Pelló, & D. Maccagni. (2002). Luminosity Functions beyond the spectroscopic limit. I. Method and near-infrared LFs in the HDF-N and HDF-S. ArXiv.org. 10 indexed citations
12.
Alloin, D., B. Altieri, M. N. Bremer, et al.. (2001). The XMM large scale structure survey and its multi-λ follow-up. Explore Bristol Research. 105. 32–36. 5 indexed citations
13.
Guzzo, L., James G. Bartlett, A. Cappi, et al.. (2000). The ESO Slice Project (ESP) galaxy redshift survey ? VII. The redshift and real-space correlation functions. A&A. 355. 1–16. 1 indexed citations
14.
Prieto, Éric, O. Le Fèvre, M. Saïsse, et al.. (1998). A Wide-Field Integral-Spectroscopy Unit for the VLT-VIRMOS. ASPC. 152. 229. 1 indexed citations
15.
Giommi, P., P. Barr, A. M. T. Pollock, B. Garilli, & D. Maccagni. (1990). A study of BL Lacertae-type objects with Exosat. I - Flux correlations, luminosity variability, and spectral variability. The Astrophysical Journal. 356. 432–432. 80 indexed citations
16.
Treves, A., Marco Morini, L. Chiappetti, et al.. (1989). Simultaneous X-ray, ultraviolet, and optical observations of the BL Lacertae object PKS 2155-304. The Astrophysical Journal. 341. 733–733. 14 indexed citations
17.
Maccagni, D., B. Garilli, I. M. Gioia, et al.. (1988). A red envelope around a dominant elliptical galaxy in an X-ray selected poor cluster. The Astrophysical Journal. 334. L1–L1. 7 indexed citations
18.
Maccagni, D., I. M. Gioia, T. Maccacaro, Rudolph E. Schild, & John T. Stocke. (1987). 1E 0116.3-0116 - A peculiar, X-ray-bright early-type galaxy. The Astrophysical Journal. 316. 132–132. 1 indexed citations
19.
Giommi, P., D. Maccagni, B. Garilli, et al.. (1985). X-ray and Optical Observations of Four X-ray Selected BL Lac Objects. Bulletin of the American Astronomical Society. 17. 608. 1 indexed citations
20.
Dilworth, C., D. Maccagni, F. Perotti, et al.. (1972). High energy electrons detected during solar flares. Solar Physics. 23(2). 487–500. 8 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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