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.
Medium-resolution Isaac Newton Telescope library of empirical spectra
2006923 citationsS. O. Selam et al.Monthly Notices of the Royal Astronomical Societyprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of S. O. Selam'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. O. Selam with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. O. Selam more than expected).
This network shows the impact of papers produced by S. O. Selam. 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. O. Selam. The network helps show where S. O. Selam may publish in the future.
Co-authorship network of co-authors of S. O. Selam
This figure shows the co-authorship network connecting the top 25 collaborators of S. O. Selam.
A scholar is included among the top collaborators of S. O. Selam 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. O. Selam. S. O. Selam is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
ÖZTÜRK, Derya, H. V. Şenavcı, M. Yılmaz, et al.. (2017). Times of Minima of Some Eclipsing Binaries. Information Bulletin on Variable Stars. 63(6209).3 indexed citations
Baştürk, Özgür, H. V. Şenavcı, Artem Burdanov, et al.. (2014). Times of Minima of Eclipsing Binaries and Mid-Transit Times of Transiting Exoplanets. IBVS. 6125. 1.3 indexed citations
11.
Yılmaz, M., et al.. (2009). New Times of Minima of Some Eclipsing Binary Stars and Maxima of Pulsating Stars. IBVS. 5887. 1.13 indexed citations
12.
Demırcan, Osman, S. O. Selam, & B. Albayrak. (2007). Solar and stellar physics through eclipses : proceedings of a workshop held at Ankara University, ÖRSEM Campus, Side, Antalya, Turkey, 27-29 March 2006. Astronomical Society of the Pacific eBooks.
13.
Selam, S. O. & Osman Demırcan. (1999). Cyclic Nature of the Orbital Period Variations of some Algol-type Binaries. DergiPark (Istanbul University).1 indexed citations
14.
Selam, S. O., et al.. (1999). Photoelectric times of minima of some eclipsing binary systems. IBVS. 4670. 1.1 indexed citations
15.
Selam, S. O., et al.. (1996). Photoelectric Minima of Some Eclipsing Binaries. IBVS. 4380. 1.4 indexed citations
16.
Selam, S. O., et al.. (1995). A period study of XZ Andromedae.. Astronomy & Astrophysics Supplement Series. 114. 167.3 indexed citations
17.
Demırcan, Osman, et al.. (1995). The light and period variation of CV Cygni.. A&A. 297. 364.
18.
Selam, S. O. & Osman Demırcan. (1994). Some statistical results on contact and near contact binaries. MmSAI. 65. 405.2 indexed citations
19.
Demırcan, Osman, et al.. (1994). UBV photometry of the contact binary AB Andromedae.. Astronomy & Astrophysics Supplement Series. 106(3). 373–376.1 indexed citations
20.
Selam, S. O., et al.. (1993). Long-term behaviour of the orbital period of Algol-type binary ST Persei.. Astronomy & Astrophysics Supplement Series. 98(3). 513–521.1 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.