S. Sciortino

6.8k total citations · 1 hit paper
181 papers, 3.7k citations indexed

About

S. Sciortino is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, S. Sciortino has authored 181 papers receiving a total of 3.7k indexed citations (citations by other indexed papers that have themselves been cited), including 162 papers in Astronomy and Astrophysics, 47 papers in Instrumentation and 27 papers in Computational Mechanics. Recurrent topics in S. Sciortino's work include Stellar, planetary, and galactic studies (142 papers), Astrophysics and Star Formation Studies (93 papers) and Astrophysical Phenomena and Observations (62 papers). S. Sciortino is often cited by papers focused on Stellar, planetary, and galactic studies (142 papers), Astrophysics and Star Formation Studies (93 papers) and Astrophysical Phenomena and Observations (62 papers). S. Sciortino collaborates with scholars based in Italy, United States and Netherlands. S. Sciortino's co-authors include G. Micela, A. Maggio, E. Flaccomio, F. Damiani, F. Favata, Jr. Harnden F. R., Nicola Pizzolato, P. Ventura, L. Prisinzano and G. S. Vaiana and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Computer Physics Communications.

In The Last Decade

S. Sciortino

174 papers receiving 3.6k citations

Hit Papers

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What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

The stellar activity-rotation relationship revisited: Dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfs

2002 501 citations A. Maggio, G. Micela et al. profile →

Peers

Countries citing papers authored by S. Sciortino

Since Specialization

Citations

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

Fields of papers citing papers by S. Sciortino

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. Sciortino

This figure shows the co-authorship network connecting the top 25 collaborators of S. Sciortino. A scholar is included among the top collaborators of S. Sciortino 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 S. Sciortino. S. Sciortino is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

#	Work	Indexed citations
1	Dispersal timescale of protoplanetary disks in the low-metallicity young cluster Dolidze 25 2021 ·Springer Link (Chiba Institute of Technology) ·M. G. Guarcello, K. Biazzo, J. J. Drake, G. Micela, L. Prisinzano, S. Sciortino, F. Damiani, E. Flaccomio, C. Neiner, N. J. Wright	9
2	A multi-wavelength view of magnetic flaring from PMS stars 2018 ·Springer Link (Chiba Institute of Technology) ·E. Flaccomio, G. Micela, S. Sciortino, Ann Marie Cody, M. G. Guarcello, M. Morales‐Calderón, L. M. Rebull, J. R. Stauffer	6
3	Sull'assenza dell'imputato nel processo criminale romano 2017 ·SPIRE - Sciences Po Institutional REpository ·S. Sciortino	0
4	Supersaturation and activity-rotation relation in PMS stars: the young cluster h Persei 2016 ·Springer Link (Chiba Institute of Technology) ·C. Argiroffi, M. Caramazza, G. Micela, S. Sciortino, E. Moraux, J. Bouvier, E. Flaccomio	27
5	COORDINATED X-RAY AND OPTICAL OBSERVATIONS OF STAR–PLANET INTERACTION IN HD 17156 2015 ·The Astrophysical Journal Letters ·A. Maggio, I. Pillitteri, G. Scandariato, A. F. Lanza, S. Sciortino, F. Borsa, A. S. Bonomo, R. Claudi, E. Covino, S. Desidera, R. Gratton, G. Micela, I. Pagano, G. Piotto, A. Sozzetti, R. Cosentino, J. Maldonado	20
6	SPATIAL DISTRIBUTION OF X-RAY EMITTING EJECTA IN TYCHO’S SNR: INDICATIONS OF SHOCKED TITANIUM 2015 ·The Astrophysical Journal ·M. Miceli, S. Sciortino, E. Troja, S. Orlando	14
7	Spectral classification and HR diagram of pre-main sequence stars in NGC 6530 2012 ·Springer Link (Chiba Institute of Technology) ·L. Prisinzano, G. Micela, S. Sciortino, L. Affer, F. Damiani	12
8	Star formation in the outer Galaxy: membership and fundamental\n parameters of the young open cluster NGC 1893 2011 ·Springer Link (Chiba Institute of Technology) ·L. Prisinzano, J. Sanz‐Forcada, G. Micela, M. Caramazza, M. G. Guarcello, S. Sciortino, L. Testi	17
9	Chronology of star formation and disk evolution in the Eagle Nebula 2010 ·Springer Link (Chiba Institute of Technology) ·M. G. Guarcello, G. Micela, G. Pérès, L. Prisinzano, S. Sciortino	18
10	Correlation between the spatial distribution of circumstellar disks and massive stars in the young open cluster NGC 6611 2009 ·Springer Link (Chiba Institute of Technology) ·M. G. Guarcello, G. Micela, F. Damiani, G. Pérès, L. Prisinzano, S. Sciortino	22
11	X-ray optical depth diagnostics of T Tauri accretion shocks 2009 ·Springer Link (Chiba Institute of Technology) ·C. Argiroffi, A. Maggio, G. Pérès, J. J. Drake, J. López‐Santiago, S. Sciortino, B. Stelzer	16
12	ACIS-I observations of NGC 2264. Membership and X-ray\nproperties of PMS stars 2006 ·Springer Link (Chiba Institute of Technology) ·E. Flaccomio, G. Micela, S. Sciortino	63
13	X-ray spectral and timing characteristics of the stars in the young open cluster IC2391 2005 ·Springer Link (Chiba Institute of Technology) ·A. Marino, G. Micela, G. Pérès, I. Pillitteri, S. Sciortino	11
14	The star formation\n region NGC 6530: Distance, ages and initial mass function 2005 ·Springer Link (Chiba Institute of Technology) ·L. Prisinzano, F. Damiani, G. Micela, S. Sciortino	45
15	XMM-Newton observations of the young open cluster Blanco 1. I. X-ray spectroscopy and photometry. 2004 ·Nova Science Publishers (Nova Science Publishers, Inc.) ·I. Pillitteri, G. Micela, S. Sciortino, F. Damiani, F. R. Harnden	10
16	Parameter properties and stellar population of the old open cluster\n NGC 3960 \n 2004 ·Springer Link (Chiba Institute of Technology) ·L. Prisinzano, G. Micela, S. Sciortino, F. Favata	11
17	X-Ray Rotational Modulation in VXR45 2003 ·IBVS ·Alberto M. Marino, G. Micela, G. Pérès, S. Sciortino	1
18	Observational clues for a role of circumstellar accretion in PMS X-ray activity 2002 ·Springer Link (Chiba Institute of Technology) ·E. Flaccomio, G. Micela, S. Sciortino	29
19	XMM-Newton survey of the low-metallicity open cluster NGC 2516 2001 ·Springer Link (Chiba Institute of Technology) ·S. Sciortino, G. Micela, F. Damiani, E. Flaccomio, K. R. Briggs, M. Denby, J. P. Pye, N. Grosso, A. M. Read, P. Gondoin, R. D. Jeffries	18
20	Multi-wavelength observations and modelling of shock-cloud interaction regions in the Vela Supernova Remnant 2000 ·A&A ·F. Bocchino, A. Maggio, S. Sciortino, J. C. Raymond	1

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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