L. Angelini

8.3k total citations
80 papers, 987 citations indexed

About

L. Angelini is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, L. Angelini has authored 80 papers receiving a total of 987 indexed citations (citations by other indexed papers that have themselves been cited), including 72 papers in Astronomy and Astrophysics, 20 papers in Nuclear and High Energy Physics and 13 papers in Computational Mechanics. Recurrent topics in L. Angelini's work include Astrophysical Phenomena and Observations (59 papers), Gamma-ray bursts and supernovae (23 papers) and Pulsars and Gravitational Waves Research (20 papers). L. Angelini is often cited by papers focused on Astrophysical Phenomena and Observations (59 papers), Gamma-ray bursts and supernovae (23 papers) and Pulsars and Gravitational Waves Research (20 papers). L. Angelini collaborates with scholars based in United States, Italy and United Kingdom. L. Angelini's co-authors include N. E. White, L. Stella, A. N. Parmar, S. H. Pravdo, Pranab Ghosh, P. Giommi, T. R. Kallman, G. L. Israel, G. Trinchieri and Stephen E. Zepf 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

L. Angelini

69 papers receiving 954 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
L. Angelini United States 20 962 257 199 46 42 80 987
N. La Palombara Italy 15 685 0.7× 253 1.0× 79 0.4× 39 0.8× 53 1.3× 73 733
M. W. Pakull France 21 1.1k 1.2× 335 1.3× 92 0.5× 77 1.7× 63 1.5× 72 1.2k
Chandreyee Maitra Germany 15 747 0.8× 217 0.8× 201 1.0× 70 1.5× 70 1.7× 76 770
S. D. Vrtilek United States 17 1.0k 1.1× 249 1.0× 171 0.9× 98 2.1× 62 1.5× 63 1.1k
G. C. Dewangan India 17 1.1k 1.2× 498 1.9× 93 0.5× 76 1.7× 38 0.9× 101 1.1k
O. Vilhu Finland 17 791 0.8× 206 0.8× 76 0.4× 50 1.1× 41 1.0× 93 831
M. R. Garcia United States 20 1.4k 1.5× 410 1.6× 180 0.9× 177 3.8× 63 1.5× 66 1.4k
M. Orlandini Italy 20 1.2k 1.2× 448 1.7× 225 1.1× 96 2.1× 61 1.5× 85 1.2k
J. E. McClintock United States 18 744 0.8× 188 0.7× 204 1.0× 65 1.4× 56 1.3× 52 798
M. L. Pretorius United Kingdom 19 965 1.0× 249 1.0× 62 0.3× 37 0.8× 92 2.2× 41 1.0k

Countries citing papers authored by L. Angelini

Since Specialization
Citations

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

Fields of papers citing papers by L. Angelini

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of L. Angelini

This figure shows the co-authorship network connecting the top 25 collaborators of L. Angelini. A scholar is included among the top collaborators of L. Angelini 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 L. Angelini. L. Angelini 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.
Mitsuishi, Ikuyuki, et al.. (2024). Soft X-Ray Energy Spectra in the Wide-field Galactic Disk Area Revealed with HaloSat. The Astrophysical Journal. 962(2). 153–153.
2.
Loewenstein, Michael, L. Angelini, M. Dutka, et al.. (2018). Heasim and skyback simulation tools and their application to the Hitomi mission. Journal of Astronomical Telescopes Instruments and Systems. 4(4). 1–1. 1 indexed citations
3.
Mereghetti, S., A. Tiengo, P. Esposito, et al.. (2010). The discovery of a massive white dwarf in the peculiar binary system HD 49798∕RX J0648.0–4418. AIP conference proceedings. 85–88. 1 indexed citations
4.
Reis, R. C., A. C. Fabian, J. M. Mïller, et al.. (2010). Stellar mass black holes accretion disks in the low-hard state. AIP conference proceedings. 115–118.
5.
Gilli, R., A. Comastri, C. Vignali, et al.. (2010). The evolution of obscured accretion. AIP conference proceedings. 359–364. 2 indexed citations
6.
Massaro, F., M. Chiaberge, P. Grandi, et al.. (2010). Extended X-ray emission in radio galaxies: 3C 305. AIP conference proceedings. 473–474. 1 indexed citations
7.
Richards, J. L., W. Max-Moerbeck, V. Pavlidou, et al.. (2010). 15 GHz Monitoring of Gamma-ray Blazars with the OVRO 40 Meter Telescope in Support of Fermi. AIP conference proceedings. 503–504.
8.
Fragos, Tassos, V. Kalogera, B. Willems, et al.. (2009). TRANSIENT LOW-MASS X-RAY BINARY POPULATIONS IN ELLIPTICAL GALAXIES NGC 3379 AND NGC 4278. The Astrophysical Journal. 702(2). L143–L147. 20 indexed citations
9.
Slane, Patrick, Suzanne Romaine, S. S. Murray, et al.. (2008). Simbol-X: A New Generation Soft/Hard X-ray Telescope. 1 indexed citations
10.
Hill, J. E., M. McConnell, Peter F. Bloser, et al.. (2008). POET: POlarimeters for Energetic Transients. AIP conference proceedings. 331–337. 13 indexed citations
11.
Fragos, Tassos, V. Kalogera, Krzysztof Belczyński, et al.. (2008). Models for Low‐Mass X‐Ray Binaries in the Elliptical Galaxies NGC 3379 and NGC 4278: Comparison with Observations. The Astrophysical Journal. 683(1). 346–356. 41 indexed citations
12.
Kim, D.‐W., G. Fabbiano, V. Kalogera, et al.. (2006). Probing the Low‐Luminosity X‐Ray Luminosity Function in Normal Elliptical Galaxies. The Astrophysical Journal. 652(2). 1090–1096. 18 indexed citations
13.
Fox, D. B., C. Pagani, L. Angelini, et al.. (2005). GRB 050906: possible X-ray counterpart.. GRB Coordinates Network. 3956. 1. 1 indexed citations
14.
Bocchino, F., A. N. Parmar, S. Mereghetti, et al.. (2001). X-ray emission in the direction of the SNR G318.2+0.1. Astronomy and Astrophysics. 367(2). 629–634. 2 indexed citations
15.
Buckley, D. A. H., M. J. Coe, J. Stevens, et al.. (2001). Multiwaveband studies of the hard ROSAT SMC transient 1WGA J0053.8-7226: a new X-ray pulsar. Monthly Notices of the Royal Astronomical Society. 320(2). 281–288. 13 indexed citations
16.
Israel, G. L., et al.. (1999). SAX and XTE observations of GX 1+4, SMCX-1, RX J0146.9+6121 and 4U 0142+614, a sample of X-ray pulsators with extreme properties. UNICA IRIS Institutional Research Information System (University of Cagliari). 1 indexed citations
17.
Mihara, T., T. Takeshima, F. Nagase, et al.. (1997). An ASCA Observation of the X-Ray Binary GX301-2. Tokyo Tech Research Repository (Tokyo Institute of Technology). 491. 1 indexed citations
18.
Ghosh, Pranab, L. Angelini, & N. E. White. (1997). The Nature of the “6 Second” and Related X‐Ray Pulsars: Evolutionary and Dynamical Considerations. The Astrophysical Journal. 478(2). 713–722. 33 indexed citations
19.
Angelini, L., N. E. White, F. Nagase, et al.. (1995). Neon Line Emission in the X-Ray Spectrum of the Pulsar 4U 1626−67. The Astrophysical Journal. 449(1). 47 indexed citations
20.
Osborne, J. P., P. Giommi, L. Angelini, G. Tagliaferri, & L. Stella. (1988). The discovery of the 2 hour modulated X-ray source EXO 033319-2554.2, an AM Herculis system. The Astrophysical Journal. 328. L45–L45. 10 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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