W. Pych

1.7k total citations
50 papers, 864 citations indexed

About

W. Pych is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, W. Pych has authored 50 papers receiving a total of 864 indexed citations (citations by other indexed papers that have themselves been cited), including 45 papers in Astronomy and Astrophysics, 25 papers in Instrumentation and 7 papers in Computational Mechanics. Recurrent topics in W. Pych's work include Stellar, planetary, and galactic studies (34 papers), Astronomy and Astrophysical Research (25 papers) and Astrophysics and Star Formation Studies (22 papers). W. Pych is often cited by papers focused on Stellar, planetary, and galactic studies (34 papers), Astronomy and Astrophysical Research (25 papers) and Astrophysics and Star Formation Studies (22 papers). W. Pych collaborates with scholars based in Poland, United States and Chile. W. Pych's co-authors include J. Kałużny, W. Krzemiński, I. B. Thompson, P. García-Lario, S. R. Pottasch, A. Manchado, A. Schwarzenberg‐Czerny, A. Olech, S. M. Ruciński and Greg Burley and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

W. Pych

45 papers receiving 826 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
W. Pych Poland 17 815 317 52 37 25 50 864
R. Andrae Germany 12 784 1.0× 386 1.2× 47 0.9× 54 1.5× 18 0.7× 26 822
D. E. Mkrtichian Ukraine 18 838 1.0× 341 1.1× 21 0.4× 65 1.8× 29 1.2× 94 888
L. Molnár Hungary 18 895 1.1× 333 1.1× 40 0.8× 86 2.3× 17 0.7× 85 943
Geert Barentsen United States 14 781 1.0× 316 1.0× 24 0.5× 54 1.5× 20 0.8× 52 799
D. Pelat France 12 507 0.6× 220 0.7× 53 1.0× 18 0.5× 74 3.0× 36 557
Demitri Muna United States 5 613 0.8× 348 1.1× 42 0.8× 24 0.6× 20 0.8× 11 652
Patrick Dowler Canada 4 562 0.7× 227 0.7× 47 0.9× 27 0.7× 20 0.8× 15 614
Chelsea X. Huang United States 15 792 1.0× 343 1.1× 17 0.3× 52 1.4× 16 0.6× 44 848
R. Cosentino Italy 14 374 0.5× 139 0.4× 26 0.5× 24 0.6× 33 1.3× 52 444
François Mignard France 8 496 0.6× 130 0.4× 26 0.5× 22 0.6× 39 1.6× 20 571

Countries citing papers authored by W. Pych

Since Specialization
Citations

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

Fields of papers citing papers by W. Pych

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of W. Pych

This figure shows the co-authorship network connecting the top 25 collaborators of W. Pych. A scholar is included among the top collaborators of W. Pych 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 W. Pych. W. Pych 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.
Wielgórski, Piotr, G. Pietrzyński, W. Gieren, et al.. (2024). Projection factor and radii of Type II Cepheids. Astronomy and Astrophysics. 689. A241–A241. 2 indexed citations
2.
Różyczka, M., I. B. Thompson, Aaron Dotter, et al.. (2022). The Cluster Ages Experiment (CASE) – IX. Analysis of four detached eclipsing binaries in the globular cluster NGC 3201. Monthly Notices of the Royal Astronomical Society. 517(2). 2485–2501. 2 indexed citations
3.
Pietrzyński, G., W. Gieren, Andrés E. Piatti, et al.. (2022). Metallicities and ages for star clusters and their surrounding fields in the Large Magellanic Cloud. Astronomy and Astrophysics. 666. A80–A80. 15 indexed citations
4.
Pietrzyński, G., W. Gieren, Andrés E. Piatti, et al.. (2021). Metallicities and ages for 35 star clusters and their surrounding fields in the Small Magellanic Cloud. Astronomy and Astrophysics. 647. A135–A135. 17 indexed citations
5.
Zajaček, Michal, B. Czerny, Mary Loli Martínez‐Aldama, et al.. (2020). Time-delay Measurement of Mg ii Broad-line Response for the Highly Accreting Quasar HE 0413-4031: Implications for the Mg ii–based Radius–Luminosity Relation. The Astrophysical Journal. 896(2). 146–146. 25 indexed citations
6.
Szczerba, R., M. Hajduk, Ya. V. Pavlenko, et al.. (2020). Validating post-AGB candidates in the LMC and SMC using SALT spectra. Springer Link (Chiba Institute of Technology). 2 indexed citations
7.
Czerny, B., K. Hryniewicz, P. Marziani, et al.. (2017). SALT long-slit spectroscopy of quasar HE 0435-4312: fast displacement of the Mg II emission line. Springer Link (Chiba Institute of Technology). 2 indexed citations
8.
Hryniewicz, K., et al.. (2014). SALT long-slit spectroscopy of LBQS 2113-4538: variability of the Mg II and Fe II component. Springer Link (Chiba Institute of Technology). 9 indexed citations
9.
Kałużny, J., I. B. Thompson, Aaron Dotter, et al.. (2014). The Clusters AgeS Experiment (CASE). VI. Analysis of Two Detached Eclipsing Binaries in the Globular Cluster M55. Acta Astronomica. 64(1). 11–26. 1 indexed citations
10.
Różyczka, M., et al.. (2014). The Clusters AgeS Experiment (CASE). Analysis of the detached eclipsing binary V15 in the metal-rich open cluster NGC 6253. Acta Astronomica. 64. 233. 1 indexed citations
11.
Niemczura, E., B. Smalley, & W. Pych. (2014). Determination of atmospheric parameters of B-, A-, F- and G-type stars : lectures from the school of spectroscopic data analyses. DIAL (Catholic University of Leuven). 6 indexed citations
12.
Kałużny, J., W. Krzemiński, W. Pych, et al.. (2014). New Observations of the Old Magnetic Nova GQ Muscae. Open Astronomy. 23(1). 1–7. 2 indexed citations
13.
Różyczka, M., J. Kałużny, P. Pietrukowicz, et al.. (2009). A New Lower Main Sequence Eclipsing Binary with Detached Components. Acta Astronomica. 59. 385.
14.
Pietrukowicz, P., Tadeusz Michałowski, W. Pych, J. Kałużny, & Ian B. Thompson. (2006). Brightness variation of the asteroid (35690) 1999 CT21. ˜The œMinor planet bulletin. 33(4). 80–81.
15.
Torres, M. A. P., et al.. (2005). Optical counterpart candidate to XTE J1818-245. ATel. 585. 1. 3 indexed citations
16.
Pych, W. & S. M. Ruciński. (2004). TU UMi: A Contact Binary in a Triple System. IBVS. 5524. 1. 3 indexed citations
17.
Michałowski, Tadeusz, T. Kwiatkowski, M. Kaasalainen, et al.. (2004). Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona. Astronomy and Astrophysics. 416(1). 353–366. 20 indexed citations
18.
Michałowski, Tadeusz, W. Pych, T. Kwiatkowski, et al.. (2001). CCD photometry, spin and shape model of the asteroid 1572 Posnania. Astronomy and Astrophysics. 371(2). 748–752. 2 indexed citations
19.
Pych, W., J. Kałużny, W. Krzemiński, A. Schwarzenberg‐Czerny, & I. B. Thompson. (2001). Cluster AgeS Experiment. CCD photometry of SX Phoenicis variables in the globular cluster M 55. Astronomy and Astrophysics. 367(1). 148–158. 34 indexed citations
20.
Michałowski, Tadeusz, T. Kwiatkowski, W. Borczyk, & W. Pych. (1994). CCD Photometry of the Asteroid 1620 Geographos. 44. 223–226. 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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