N. D’Amico

8.0k total citations · 2 hit papers
75 papers, 3.7k citations indexed

About

N. D’Amico is a scholar working on Astronomy and Astrophysics, Oceanography and Nuclear and High Energy Physics. According to data from OpenAlex, N. D’Amico has authored 75 papers receiving a total of 3.7k indexed citations (citations by other indexed papers that have themselves been cited), including 73 papers in Astronomy and Astrophysics, 26 papers in Oceanography and 15 papers in Nuclear and High Energy Physics. Recurrent topics in N. D’Amico's work include Pulsars and Gravitational Waves Research (67 papers), Geophysics and Gravity Measurements (26 papers) and Gamma-ray bursts and supernovae (21 papers). N. D’Amico is often cited by papers focused on Pulsars and Gravitational Waves Research (67 papers), Geophysics and Gravity Measurements (26 papers) and Gamma-ray bursts and supernovae (21 papers). N. D’Amico collaborates with scholars based in Italy, United Kingdom and Australia. N. D’Amico's co-authors include R. N. Manchester, Andrea Possenti, A. G. Lyne, F. Camilo, D. R. Lorimer, M. Krämer, M. Burgay, M. A. McLaughlin, I. H. Stairs and P. C. C. Freire and has published in prestigious journals such as Nature, Science and The Astrophysical Journal.

In The Last Decade

N. D’Amico

73 papers receiving 3.6k citations

Hit Papers

Tests of General Relativity from Timing the Double Pulsar 2004 2026 2011 2018 2006 2004 100 200 300 400 500

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
N. D’Amico Italy 32 3.6k 963 733 563 314 75 3.7k
M. Burgay Italy 31 4.9k 1.4× 1.3k 1.4× 839 1.1× 763 1.4× 339 1.1× 157 5.1k
S. E. Thorsett United States 28 2.6k 0.7× 580 0.6× 477 0.7× 428 0.8× 222 0.7× 63 2.7k
C. Bassa Netherlands 30 3.2k 0.9× 866 0.9× 373 0.5× 650 1.2× 197 0.6× 174 3.3k
R. M. Shannon Australia 38 3.9k 1.1× 838 0.9× 781 1.1× 393 0.7× 386 1.2× 154 4.0k
B. C. Joshi India 17 2.1k 0.6× 593 0.6× 478 0.7× 321 0.6× 200 0.6× 75 2.2k
N. D. R. Bhat Australia 31 2.9k 0.8× 853 0.9× 421 0.6× 265 0.5× 316 1.0× 114 3.0k
John Sarkissian Australia 17 2.1k 0.6× 505 0.5× 438 0.6× 334 0.6× 210 0.7× 49 2.1k
Koutarou Kyutoku Japan 41 5.1k 1.4× 1.4k 1.5× 492 0.7× 811 1.4× 215 0.7× 83 5.2k
Alberto Sesana Italy 48 6.5k 1.8× 1.4k 1.5× 522 0.7× 254 0.5× 317 1.0× 150 6.7k
R. Wielebinski Germany 30 3.1k 0.9× 1.4k 1.5× 224 0.3× 148 0.3× 203 0.6× 240 3.3k

Countries citing papers authored by N. D’Amico

Since Specialization
Citations

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

Fields of papers citing papers by N. D’Amico

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of N. D’Amico

This figure shows the co-authorship network connecting the top 25 collaborators of N. D’Amico. A scholar is included among the top collaborators of N. D’Amico 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 N. D’Amico. N. D’Amico 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.
Levin, L., M. Bailes, Benjamin R. Barsdell, et al.. (2013). The High Time Resolution Universe Pulsar Survey –VIII. The Galactic millisecond pulsar population. Monthly Notices of the Royal Astronomical Society. 434(2). 1387–1397. 43 indexed citations
2.
Buttu, Marco, N. D’Amico, E. Egron, et al.. (2013). Detection by Sardinia Radio Telescope of radio pulses at 7 GHz from the Magnetar PSR J1745-2900 in the Galactic center region. The astronomer's telegram. 5053. 1. 1 indexed citations
3.
Bailes, M., Andrea Possenti, S. Johnston, et al.. (2008). The High Time Resolution Universe. 630.
4.
Burderi, L., V. Testa, M. T. Menna, et al.. (2007). Possible IR counterpart of the newly discovered X-ray MSP SWIFT J1756.9-2508. UNICA IRIS Institutional Research Information System (University of Cagliari). 1132. 1. 1 indexed citations
5.
Burgay, M., N. Rea, G. L. Israel, et al.. (2007). Search for radio pulsations in four anomalous X-ray pulsars and discovery of two new pulsars. Astrophysics and Space Science. 308(1-4). 531–534. 1 indexed citations
6.
D’Amico, N.. (2006). The Sardinia Radio Telescope and the local context. 10. 25. 1 indexed citations
7.
McLaughlin, M. A., A. G. Lyne, D. R. Lorimer, et al.. (2006). Transient radio bursts from rotating neutron stars. Nature. 439(7078). 817–820. 314 indexed citations
8.
Corongiu, A., M. Krämer, B. W. Stappers, et al.. (2006). The binary pulsar PSR J1811-1736: evidence of a low amplitude supernova kick. Astronomy and Astrophysics. 462(2). 703–709. 44 indexed citations
9.
Possenti, Andrea, A. Corongiu, R. N. Manchester, et al.. (2006). The Timing of Globular Cluster Pulsars at Parkes. Chinese Journal of Astronomy and Astrophysics. 6(S2). 176–180. 1 indexed citations
10.
Grueff, G., Roberto Ambrosini, Pietro Bolli, et al.. (2004). The Sardinia Radio Telescope. 5. 351. 5 indexed citations
11.
Burgay, M., L. Burderi, Andrea Possenti, et al.. (2003). A Search for Pulsars in Quiescent Soft X‐Ray Transients. I.. The Astrophysical Journal. 589(2). 902–910. 20 indexed citations
12.
Possenti, Andrea, N. D’Amico, R. N. Manchester, et al.. (2003). Three Binary Millisecond Pulsars in NGC 6266. The Astrophysical Journal. 599(1). 475–484. 35 indexed citations
13.
Freire, P. C. C., F. Camilo, M. Krämer, et al.. (2003). Further results from the timing of the millisecond pulsars in 47 Tucanae. Monthly Notices of the Royal Astronomical Society. 340(4). 1359–1374. 72 indexed citations
14.
Ferraro, F. R., N. D’Amico, Andrea Possenti, R. Mignani, & B. Paltrinieri. (2001). Blue Stragglers, Young White Dwarfs, and UV‐Excess Stars in the Core of 47 Tucanae. The Astrophysical Journal. 561(1). 337–345. 52 indexed citations
15.
Burderi, L., Andrea Possenti, F. D’Antona, et al.. (2001). Where May Ultrafast Rotating Neutron Stars Be Hidden?. The Astrophysical Journal. 560(1). L71–L74. 64 indexed citations
16.
Possenti, Andrea, Monica Colpi, U. Geppert, L. Burderi, & N. D’Amico. (1999). Recycling Neutron Stars to Ultrashort Periods: A Statistical Analysis of Their Evolution in the μ‐ P Plane. The Astrophysical Journal Supplement Series. 125(2). 463–477. 11 indexed citations
17.
Crawford, F., V. M. Kaspi, R. N. Manchester, et al.. (1998). Upper limits on radio emission from the young X-ray pulsars in the supernova remnants G11.2-0.3 and N157B.. CERN Bulletin. 69. 951–954. 3 indexed citations
18.
Bailes, M., Paul Harrison, D. R. Lorimer, et al.. (1994). Discovery of three binary millisecond pulsars. The Astrophysical Journal. 425. L41–L41. 58 indexed citations
19.
Kawai, N., R. Okayasu, W. Brinkmann, et al.. (1991). X-ray and radio pulse phase comparison for PSR 1509 - 58. The Astrophysical Journal. 383. L65–L65. 5 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