C. Morossi

842 total citations
38 papers, 201 citations indexed

About

C. Morossi is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, C. Morossi has authored 38 papers receiving a total of 201 indexed citations (citations by other indexed papers that have themselves been cited), including 33 papers in Astronomy and Astrophysics, 16 papers in Instrumentation and 8 papers in Computational Mechanics. Recurrent topics in C. Morossi's work include Stellar, planetary, and galactic studies (31 papers), Astronomy and Astrophysical Research (16 papers) and Astro and Planetary Science (8 papers). C. Morossi is often cited by papers focused on Stellar, planetary, and galactic studies (31 papers), Astronomy and Astrophysical Research (16 papers) and Astro and Planetary Science (8 papers). C. Morossi collaborates with scholars based in Italy, Mexico and United Kingdom. C. Morossi's co-authors include M. Franchini, M. Chávez, P. Di Marcantonio, A. Buzzoni, E. Spitoni, V. Grisoni, M. Chávez, D. Romano, F. Matteuccí and G. S. Vaiana 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

C. Morossi

34 papers receiving 194 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
C. Morossi Italy 9 195 79 12 9 8 38 201
Luiz Paulo R. Vaz Brazil 8 270 1.4× 92 1.2× 12 1.0× 10 1.1× 11 1.4× 14 272
N. Reid United States 10 202 1.0× 84 1.1× 17 1.4× 4 0.4× 9 1.1× 14 206
P. Guterman France 5 156 0.8× 64 0.8× 13 1.1× 7 0.8× 5 0.6× 8 157
G. Wuchterl Germany 7 249 1.3× 60 0.8× 7 0.6× 14 1.6× 4 0.5× 18 250
Sebastian Schröter Germany 8 201 1.0× 97 1.2× 12 1.0× 9 1.0× 7 0.9× 9 204
Е. Л. Ченцов Russia 11 319 1.6× 124 1.6× 13 1.1× 7 0.8× 14 1.8× 43 330
Y. Katherina Feng United States 6 194 1.0× 62 0.8× 6 0.5× 6 0.7× 10 1.3× 9 202
Paul Butler United States 8 187 1.0× 67 0.8× 6 0.5× 6 0.7× 11 1.4× 11 193
A. Künstler Germany 5 240 1.2× 78 1.0× 7 0.6× 9 1.0× 5 0.6× 5 244
В. П. Архипова Russia 10 298 1.5× 124 1.6× 19 1.6× 10 1.1× 5 0.6× 64 308

Countries citing papers authored by C. Morossi

Since Specialization
Citations

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

Fields of papers citing papers by C. Morossi

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of C. Morossi

This figure shows the co-authorship network connecting the top 25 collaborators of C. Morossi. A scholar is included among the top collaborators of C. Morossi 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 C. Morossi. C. Morossi 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.
Cescutti, G., C. Morossi, M. Franchini, et al.. (2021). Barium lines in high-quality spectra of two metal-poor giants in the Galactic halo. ArTS Archivio della ricerca di Trieste (University of Trieste https://www.units.it/). 4 indexed citations
2.
Romano, D., M. Franchini, V. Grisoni, et al.. (2020). The variation of carbon abundance in galaxies and its implications. Springer Link (Chiba Institute of Technology). 27 indexed citations
3.
Morossi, C., et al.. (2007). Age-Metallicity Relation, [Fe/H] and [α/Fe] vertical gradients in the Milky Way from the SDSS–DR5 spectroscopic database. Proceedings of the International Astronomical Union. 3(S248). 504–505. 1 indexed citations
4.
Chávez, M., E. Bertone, A. Buzzoni, et al.. (2007). Synthetic Mid‐UV Spectroscopic Indices of Stars. The Astrophysical Journal. 657(2). 1046–1057. 12 indexed citations
5.
Franchini, M., et al.. (2007). Simultaneous Bayesian estimation of distances and ages from isochrones: SDSS and solar neighborhood FGK stars. Proceedings of the International Astronomical Union. 3(S248). 494–495. 1 indexed citations
6.
Franchini, M., et al.. (2005). Synthetic Lick Indices and Detection of α‐enhanced Stars. III. F, G, and K Stars with [Fe/H] > 0.00. The Astrophysical Journal. 634(2). 1319–1335. 2 indexed citations
7.
Franchini, M., et al.. (2004). Synthetic Lick Indices and Detection of α‐Enhanced Stars. The Astrophysical Journal. 601(1). 485–499. 10 indexed citations
8.
Morossi, C., et al.. (2000). Observations and Atmospheric Parameters of Super–Metal‐rich Candidates1. Publications of the Astronomical Society of the Pacific. 112(777). 1455–1466. 9 indexed citations
9.
Morossi, C., et al.. (1997). Accuracy of effective temperatures of solar chemical composition stars derived from the flux fitting method.. 326(2). 736–740. 1 indexed citations
10.
Chávez, M., et al.. (1997). An Atlas of high resolution synthetic spectra in the wavelength region $\bf 4850-5400 \AA$. Astronomy and Astrophysics Supplement Series. 126(2). 267–272. 9 indexed citations
11.
Chávez, M., et al.. (1996). Synthesis of Stellar Mg and Fe Absorption Indices for Stellar Population Studies. II. The Extended and Up‐to‐Date Collection. The Astrophysical Journal. 471(2). 726–736. 8 indexed citations
12.
Chávez, M., et al.. (1995). New synthetic Mg2 indices. The Astrophysical Journal. 440. 210–210. 7 indexed citations
13.
Morossi, C., et al.. (1990). Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars. Astronomy & Astrophysics Supplement Series. 85(3). 1015–1019. 3 indexed citations
14.
Sciortino, S., G. S. Vaiana, Jr. Harnden F. R., et al.. (1990). Relationship between optical and X-ray properties of O-type stars surveyed with the Einstein Observatory. The Astrophysical Journal. 361. 621–621. 28 indexed citations
15.
Gulati, R. K., et al.. (1989). Empirical temperature calibrations for early-type stars.. Astronomy & Astrophysics Supplement Series. 80(1). 73–88. 1 indexed citations
16.
Marlborough, J. M., C. Morossi, Godefridus J. Peters, et al.. (1986). Ultraviolet and visual variability of Theta CrB during a normal B-phase following a shell phase (1980-1985). 158. 1–13. 3 indexed citations
17.
Morossi, C., et al.. (1985). Observed and computed spectral flux distribution of non-supergiant 09-G8 stars. III. Determination of Teff for the stars in the Breger Catalogue.. Astronomy & Astrophysics Supplement Series. 60(3). 365–372. 1 indexed citations
18.
Franco, Maximilien, L. Crivellari, P. Molaro, et al.. (1984). The spectra of late-type dwarfs and sub-dwarfs in the near ultraviolet. III: An atlas of Mg II h and k profiles. Astronomy & Astrophysics Supplement Series. 58(3). 693–704.
19.
Faraggiana, R., et al.. (1983). Observed and computed spectral distribution of early-type stars. II: Determination of Te for B5-A0 stars. 128(2). 375–383. 1 indexed citations
20.
Crivellari, L., F. Mardirossian, & C. Morossi. (1978). A criterion for the measurement of equivalent widths.. 72. 256–260.

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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