I. Puerari

1.7k total citations
56 papers, 1.1k citations indexed

About

I. Puerari is a scholar working on Astronomy and Astrophysics, Instrumentation and Statistical and Nonlinear Physics. According to data from OpenAlex, I. Puerari has authored 56 papers receiving a total of 1.1k indexed citations (citations by other indexed papers that have themselves been cited), including 50 papers in Astronomy and Astrophysics, 28 papers in Instrumentation and 5 papers in Statistical and Nonlinear Physics. Recurrent topics in I. Puerari's work include Galaxies: Formation, Evolution, Phenomena (39 papers), Stellar, planetary, and galactic studies (34 papers) and Astronomy and Astrophysical Research (28 papers). I. Puerari is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (39 papers), Stellar, planetary, and galactic studies (34 papers) and Astronomy and Astrophysical Research (28 papers). I. Puerari collaborates with scholars based in Mexico, United States and South Africa. I. Puerari's co-authors include David L. Block, Bruce G. Elmegreen, F. Bournaud, K. C. Freeman, H. Dottori, Romain Teyssier, R. Buta, F. Combes, D. M. Elmegreen and J. H. Knapen 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

I. Puerari

54 papers receiving 1.0k citations

Peers

I. Puerari

INSTR

NHEP

CVPR

SNP

Bau-Ching Hsieh Taiwan

Ivana Damjanov United States

Seppo Laine United States

Marc S. Seigar United States

Habib G. Khosroshahi Iran

A. Burkert Germany

B. Épinat France

Mireia Montes Spain

Sirio Belli United States

Johnny P. Greco United States

Bau-Ching Hsieh Taiwan

I. Puerari

852 ×0.8

485 ×1.1

INSTR

66 ×1.1

NHEP

61 ×1.2

CVPR

33 ×0.8

SNP

Citations per year, relative to I. Puerari I. Puerari (= 1×) peers Bau-Ching Hsieh

Countries citing papers authored by I. Puerari

Since Specialization

Citations

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

Fields of papers citing papers by I. Puerari

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of I. Puerari

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

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Zamora-Avilés, Manuel, et al.. (2025). Peculiar galaxies – I. A catalogue of polar-ring galaxies from the TNG50 simulation. Monthly Notices of the Royal Astronomical Society. 545(2).

Puerari, I., et al.. (2023). Orbital structure evolution in self-consistent N-body simulations. Monthly Notices of the Royal Astronomical Society. 525(2). 3162–3180. 2 indexed citations

Longinotti, A. L., Y. Krongold, C. Feruglio, et al.. (2020). Evidence of galaxy interaction in the narrow-line Seyfert 1 galaxy IRAS 17020+4544 seen by NOEMA. Monthly Notices of the Royal Astronomical Society. 501(1). 219–228. 5 indexed citations

Mayya, Y. D., et al.. (2020). Mass–radius relation of intermediate-age disc super star clusters of M82. Monthly Notices of the Royal Astronomical Society. 500(4). 4422–4438. 7 indexed citations

Puerari, I., et al.. (2017). Detecting the growth of structures in Pure Stellar Disk Models. Redalyc (Universidad Autónoma del Estado de México). 53. 257–273. 1 indexed citations

Viaene, S., M. Sarzi, M. Baes, & I. Puerari. (2017). NGC 5626: a massive fast rotator with a twist. Monthly Notices of the Royal Astronomical Society Letters. 474(1). L47–L51. 1 indexed citations

Davis, Benjamin L., Joel C. Berrier, Julia Kennefick, et al.. (2016). 2DFFT: Measuring Galactic Spiral Arm Pitch Angle. Astrophysics Source Code Library. 3 indexed citations

Wall, W. F., I. Puerari, R. P. J. Tilanus, et al.. (2016). Continuum observations of M 51 and M 83 at 1.1 mm with AzTEC. Monthly Notices of the Royal Astronomical Society. 459(2). 1440–1467. 9 indexed citations

Bournaud, F., Bruce G. Elmegreen, Romain Teyssier, David L. Block, & I. Puerari. (2010). ISM properties in hydrodynamic galaxy simulations: turbulence cascades, cloud formation, role of gravity and feedback. Zurich Open Repository and Archive (University of Zurich). 152 indexed citations

10.

Allam, S., D. L. Tucker, Perry M. Gee, et al.. (2007). Chapter 25: Finding and Exploring Merging Pairs of Galaxies in 2MASS Using the NVO. ASPC. 382. 261. 1 indexed citations

11.

Block, David L., F. Combes, I. Puerari, et al.. (2007). Keck spectroscopy and Spitzer space telescope analysis of the outer disk of the Triangulum spiral galaxy M 33. Astronomy and Astrophysics. 471(2). 467–474. 4 indexed citations

12.

Bournaud, F., F. Combes, Chanda J. Jog, & I. Puerari. (2005). Lopsided spiral galaxies: evidence for gas accretion. Springer Link (Chiba Institute of Technology). 71 indexed citations

13.

Block, David L., K. C. Freeman, T. H. Jarrett, et al.. (2004). Very luminous carbon stars in the outer disk of the Triangulum spiral galaxy. Astronomy and Astrophysics. 425(3). L37–L40. 15 indexed citations

14.

Puerari, I., et al.. (2003). Fourier Analysis of a Spiral Galaxies Sample: Determination of Kinematic and Morphological Parameters. 17. 201–202. 1 indexed citations

15.

Block, David L., et al.. (2002). Gravitational torques in spiral galaxies: Gas accretion as a driving mechanism of galactic evolution. Springer Link (Chiba Institute of Technology). 38 indexed citations

16.

Block, David L., I. Puerari, M. Takamiya, et al.. (2001). Dust-penetrated morphology in the high-redshift universe: Clues from NGC 922. Astronomy and Astrophysics. 371(2). 393–403. 10 indexed citations

17.

Block, David L., I. Puerari, J. H. Knapen, et al.. (2001). The gravitational torque of bars in opticallyunbarred and barred galaxies. Astronomy and Astrophysics. 375(3). 761–769. 37 indexed citations

18.

Block, David L., et al.. (2000). Toward a new millennium in galaxy morphology : proceedings of an International Conference 'Toward a New Millennium in Galaxy Morphology: from z=0 to the Lyman Break' held at the Eskom Conference Centre, Midrand, South Africa, September 13-18, 1999. Kluwer Academic Publishers eBooks. 3 indexed citations

19.

Mayya, Y. D., I. Puerari, & O. Kuhn. (1998). Supernova 1998bu in NGC 3368. IAUC. 6907. 2. 1 indexed citations

20.

Pastoriza, M. G., et al.. (1994). The distribution of light in the spiral galaxy NGC 7412.. Astronomy & Astrophysics Supplement Series. 108. 41–54. 4 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