E. Puga

996 total citations
32 papers, 431 citations indexed

About

E. Puga is a scholar working on Astronomy and Astrophysics, Instrumentation and Spectroscopy. According to data from OpenAlex, E. Puga has authored 32 papers receiving a total of 431 indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 8 papers in Instrumentation and 6 papers in Spectroscopy. Recurrent topics in E. Puga's work include Stellar, planetary, and galactic studies (27 papers), Astrophysics and Star Formation Studies (23 papers) and Astronomy and Astrophysical Research (8 papers). E. Puga is often cited by papers focused on Stellar, planetary, and galactic studies (27 papers), Astrophysics and Star Formation Studies (23 papers) and Astronomy and Astrophysical Research (8 papers). E. Puga collaborates with scholars based in Germany, Spain and Belgium. E. Puga's co-authors include Arjan Bik, M. Feldt, Th. Henning, Donald F. Figer, F. Najarro, B. Stecklum, Catarina Alves de Oliveira, S. Hony, C. Neiner and F. Cusano 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

E. Puga

31 papers receiving 412 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
E. Puga Germany 15 396 105 51 38 31 32 431
Joana Ascenso Portugal 12 392 1.0× 65 0.6× 74 1.5× 21 0.6× 30 1.0× 23 416
F. Vitali Italy 10 249 0.6× 61 0.6× 33 0.6× 27 0.7× 22 0.7× 46 280
A. Meilland France 16 592 1.5× 62 0.6× 137 2.7× 67 1.8× 16 0.5× 45 629
Masuo Tanaka Japan 12 310 0.8× 94 0.9× 43 0.8× 49 1.3× 74 2.4× 35 349
R. Vavrek Netherlands 11 335 0.8× 74 0.7× 32 0.6× 14 0.4× 39 1.3× 27 354
A. M. Di Giorgio Italy 8 326 0.8× 90 0.9× 25 0.5× 16 0.4× 49 1.6× 33 346
Mitsuyoshi Yamagishi Japan 9 219 0.6× 31 0.3× 28 0.5× 37 1.0× 9 0.3× 30 237
D. Maier France 8 270 0.7× 62 0.6× 13 0.3× 22 0.6× 27 0.9× 21 287
M. Horrobin Germany 10 366 0.9× 22 0.2× 81 1.6× 41 1.1× 15 0.5× 30 394
C. Kasemann Germany 8 293 0.7× 123 1.2× 15 0.3× 36 0.9× 49 1.6× 19 320

Countries citing papers authored by E. Puga

Since Specialization
Citations

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

Fields of papers citing papers by E. Puga

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of E. Puga

This figure shows the co-authorship network connecting the top 25 collaborators of E. Puga. A scholar is included among the top collaborators of E. Puga 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 E. Puga. E. Puga 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.
Ferruit, Pierre, Nora Lützgendorf, Maurice te Plate, et al.. (2018). Preparing the NIRSpec/JWST science data calibration: from ground testing to sky. 28–28. 12 indexed citations
2.
Birkmann, Stephan M., M. Sirianni, Pierre Ferruit, et al.. (2018). Noise performance of the JWST/NIRSpec detector system. 5904. 116–116. 2 indexed citations
3.
Hopwood, R., E. T. Polehampton, I. Valtchanov, et al.. (2015). Systematic characterization of the Herschel SPIRE Fourier Transform Spectrometer★. Monthly Notices of the Royal Astronomical Society. 449(3). 2274–2303. 17 indexed citations
4.
Oliveira, Catarina Alves de, N. Schneider, B. Merín, et al.. (2014). Herschelview of the large-scale structure in the Chamaeleon dark clouds. Astronomy and Astrophysics. 568. A98–A98. 41 indexed citations
5.
Ribas, Álvaro, B. Merín, H. Bouy, et al.. (2013). Identification of transitional disks in Chamaeleon withHerschel. Astronomy and Astrophysics. 552. A115–A115. 10 indexed citations
6.
Winston, Elaine, N. L. J. Cox, T. Prusti, et al.. (2012). Herschelfar-IR observations of the Chamaeleon molecular cloud complex. Astronomy and Astrophysics. 545. A145–A145. 21 indexed citations
7.
Wang, Y., H. Beuther, Arjan Bik, et al.. (2011). Different evolutionary stages in the massive star-forming region S255 complex. Springer Link (Chiba Institute of Technology). 26 indexed citations
8.
Alegría, S. Ramírez, A. Herrero, A. Marín-Franch, et al.. (2011). Near-infrared study of the stellar population of Sh2-152. Astronomy and Astrophysics. 535. A8–A8. 7 indexed citations
9.
Maaskant, K. M., Arjan Bik, L. B. F. M. Waters, et al.. (2011). Sequential star formation in IRAS 06084-0611 (GGD 12-15). Astronomy and Astrophysics. 531. A27–A27. 9 indexed citations
10.
Puga, E., A. Marín-Franch, F. Najarro, et al.. (2010). Near-infrared spectroscopy in NGC 7538. Springer Link (Chiba Institute of Technology). 21 indexed citations
11.
Bik, Arjan, E. Puga, L. B. F. M. Waters, et al.. (2010). SEQUENTIAL STAR FORMATION IN RCW 34: A SPECTROSCOPIC CENSUS OF THE STELLAR CONTENT OF HIGH-MASS STAR-FORMING REGIONS. The Astrophysical Journal. 713(2). 883–899. 35 indexed citations
12.
Cusano, F., V. Ripepi, J. M. Alcalá, et al.. (2010). Pre-main-sequence stars in the star-forming complex Sh 2-284. Monthly Notices of the Royal Astronomical Society. 410(1). 227–240. 15 indexed citations
13.
Puga, E., S. Hony, C. Neiner, et al.. (2009). Spitzer/IRAC view of Sh 2-284. Astronomy and Astrophysics. 503(1). 107–119. 18 indexed citations
14.
Puga, E., S. Hony, C. Neiner, et al.. (2009). Spitzer/IRAC view of Sh 2-284: Searching for evidence of triggered star formation in an isolated region in the outer Milky Way. UvA-DARE (University of Amsterdam). 16 indexed citations
15.
Martín-Hernández, N. L., Arjan Bik, E. Puga, D. Nürnberger, & L. Bronfman. (2008). Spatially resolved near-infrared spectroscopy of the massive star-forming region IRAS 19410+2336. Astronomy and Astrophysics. 489(1). 229–243. 18 indexed citations
16.
Martín-Hernández, N. L., C. Esteban, A. Mesa‐Delgado, Arjan Bik, & E. Puga. (2008). M1–78: a nitrogen-rich Galactic compact H II region beyond the Perseus arm. Astronomy and Astrophysics. 482(1). 215–227. 3 indexed citations
17.
Puga, E., C. Álvarez, M. Feldt, Th. Henning, & S. Wolf. (2004). AO-assisted observations of G61.48+0.09. Astronomy and Astrophysics. 425(2). 543–552. 2 indexed citations
18.
Feldt, M., Thomas Henning, B. Stecklum, & E. Puga. (2003). Observing Massive Star Formation - the Story of G5.89-0.39. 221. 71.
19.
Feldt, M., E. Puga, R. Lenzen, et al.. (2003). Discovery of a Candidate for the Central Star of the Ultracompact H ii Region G5.89-0.39. The Astrophysical Journal. 599(2). L91–L94. 24 indexed citations
20.
Feldt, M., S. Hippler, Robert Weiß, et al.. (2003). Can we really go for direct exo-planet detection from the ground?. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 4860. 149–149. 2 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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