A. Malizia

4.0k total citations
123 papers, 2.1k citations indexed

About

A. Malizia is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, A. Malizia has authored 123 papers receiving a total of 2.1k indexed citations (citations by other indexed papers that have themselves been cited), including 110 papers in Astronomy and Astrophysics, 77 papers in Nuclear and High Energy Physics and 16 papers in Computational Mechanics. Recurrent topics in A. Malizia's work include Astrophysical Phenomena and Observations (99 papers), Astrophysics and Cosmic Phenomena (75 papers) and Galaxies: Formation, Evolution, Phenomena (52 papers). A. Malizia is often cited by papers focused on Astrophysical Phenomena and Observations (99 papers), Astrophysics and Cosmic Phenomena (75 papers) and Galaxies: Formation, Evolution, Phenomena (52 papers). A. Malizia collaborates with scholars based in Italy, United Kingdom and United States. A. Malizia's co-authors include L. Bassani, P. Ubertini, A. Bazzano, A. J. Bird, J. B. Stephen, R. Landi, N. Masetti, A. J. Dean, M. Molina and V. Sguera and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

A. Malizia

116 papers receiving 2.0k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
A. Malizia Italy 26 2.0k 1.1k 138 78 59 123 2.1k
A. J. Dean United Kingdom 22 1.8k 0.9× 889 0.8× 125 0.9× 138 1.8× 33 0.6× 48 1.9k
E. M. Schlegel United States 23 2.0k 1.0× 755 0.7× 77 0.6× 142 1.8× 85 1.4× 132 2.0k
R. Landi Italy 21 1.3k 0.6× 646 0.6× 88 0.6× 51 0.7× 82 1.4× 73 1.4k
A. M. Read United Kingdom 24 1.6k 0.8× 611 0.5× 49 0.4× 63 0.8× 66 1.1× 50 1.6k
M. Ribó Spain 22 1.5k 0.7× 777 0.7× 49 0.4× 78 1.0× 43 0.7× 92 1.5k
P. D’Avanzo Italy 26 2.1k 1.0× 550 0.5× 42 0.3× 182 2.3× 109 1.8× 146 2.1k
R. S. Warwick United Kingdom 15 1.1k 0.5× 640 0.6× 42 0.3× 69 0.9× 35 0.6× 43 1.2k
C. Guidorzi Italy 23 2.5k 1.2× 740 0.7× 36 0.3× 80 1.0× 213 3.6× 151 2.5k
I. R. Tuohy Australia 21 1.5k 0.7× 691 0.6× 100 0.7× 169 2.2× 52 0.9× 93 1.6k
M. R. Garcia United States 20 1.4k 0.7× 410 0.4× 63 0.5× 180 2.3× 39 0.7× 66 1.4k

Countries citing papers authored by A. Malizia

Since Specialization
Citations

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

Fields of papers citing papers by A. Malizia

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of A. Malizia

This figure shows the co-authorship network connecting the top 25 collaborators of A. Malizia. A scholar is included among the top collaborators of A. Malizia 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 A. Malizia. A. Malizia 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.
Feruglio, C., M. Massardi, Andrea Lapi, et al.. (2023). NGC 2992: Interplay between the multiphase disc, wind, and radio bubbles. Astronomy and Astrophysics. 679. A88–A88. 8 indexed citations
2.
Hernández-García, L., P. Arévalo, Cláudio Ricci, et al.. (2022). Constraining the X-ray reflection in low accretion-rate active galactic nuclei using XMM-Newton, NuSTAR, and Swift. Astronomy and Astrophysics. 669. A114–A114. 5 indexed citations
3.
Feruglio, C., M. Bischetti, A. Malizia, et al.. (2021). The IBISCO survey. Astronomy and Astrophysics. 655. A25–A25. 8 indexed citations
4.
Malizia, A., L. Bassani, J. B. Stephen, A. Bazzano, & P. Ubertini. (2020). X-ray absorption in INTEGRAL active galactic nuclei. Springer Link (Chiba Institute of Technology). 6 indexed citations
5.
Ursini, F., L. Bassani, A. Malizia, et al.. (2019). The coronal temperature of NGC 4388 and NGC 2110 measured with INTEGRAL. Springer Link (Chiba Institute of Technology). 6 indexed citations
6.
Molina, M., L. Bassani, A. Malizia, et al.. (2014). IGR J17488–2338: a newly discovered giant radio galaxy. Springer Link (Chiba Institute of Technology). 12 indexed citations
7.
Masetti, N., A. Malizia, R. Landi, et al.. (2012). IGR J12319-0749: Evidence for Another Extreme Blazar Found with INTEGRAL. Springer Link (Chiba Institute of Technology). 4 indexed citations
8.
Masetti, N., P. Parisi, E. Jiménez‐Bailón, et al.. (2012). Unveiling the nature of INTEGRAL objects through optical spectroscopy IX. Twenty two more identifications, and a glance into the far hard X-ray Universe. Americanae (AECID Library). 23 indexed citations
9.
Molina, M., R. Landi, L. Bassani, et al.. (2012). Flat-spectrum radio sources as likely counterparts of unidentified INTEGRAL sources. Springer Link (Chiba Institute of Technology). 4 indexed citations
10.
Masetti, N., R. Landi, V. Sguera, et al.. (2010). The peculiar high-mass X-ray binary 1ES 1210-646. Springer Link (Chiba Institute of Technology). 4 indexed citations
11.
Parisi, P., N. Masetti, E. Jiménez‐Bailón, et al.. (2009). Accurate classification of 17 AGNs detected with\nSwift/BAT. Springer Link (Chiba Institute of Technology). 16 indexed citations
12.
Masetti, N., E. Mason, R. Landi, et al.. (2008). High-redshift blazar identification for Swift J1656.3-3302. Springer Link (Chiba Institute of Technology). 9 indexed citations
13.
Sguera, V., A. Bazzano, A. J. Bird, et al.. (2007). INTEGRAL high energy detection of the transient IGR J11321–5311. Springer Link (Chiba Institute of Technology). 1 indexed citations
14.
Masetti, N., R. Landi, M. L. Pretorius, et al.. (2007). IGR J16194–2810: a new symbiotic X-ray binary. Springer Link (Chiba Institute of Technology). 49 indexed citations
15.
McBride, V. A., Anthony J. Dean, A. Bazzano, et al.. (2007). INTEGRAL detection of the pulsar wind nebula in PSR J1846–0258. Springer Link (Chiba Institute of Technology). 13 indexed citations
16.
Sguera, V., E. J. Barlow, A. J. Bird, et al.. (2005). INTEGRAL observations of recurrent fast X-ray transient sources. Springer Link (Chiba Institute of Technology). 97 indexed citations
17.
Sguera, V., A. Malizia, L. Bassani, J. B. Stephen, & G. Di Cocco. (2004). 3EG J2027+3429: Another blazar behind the Galactic Plane. Springer Link (Chiba Institute of Technology). 5 indexed citations
18.
Malizia, A., L. Bassani, M. Capalbi, et al.. (2003). A BeppoSAX observation of MKN6. Springer Link (Chiba Institute of Technology). 5 indexed citations
19.
Malizia, A., G. Malaguti, L. Bassani, et al.. (2002). BeppoSAX/PDS identification of the true counterpart of the Piccinotti source H0917-074. Springer Link (Chiba Institute of Technology). 8 indexed citations
20.
Parmar, A. N., T. Oosterbroek, A. Orr, et al.. (1999). BeppoSAXLECS background subtraction techniques. Springer Link (Chiba Institute of Technology). 1 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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