This map shows the geographic impact of C. Schrijvers'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. Schrijvers with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. Schrijvers more than expected).
This network shows the impact of papers produced by C. Schrijvers. 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. Schrijvers. The network helps show where C. Schrijvers may publish in the future.
Co-authorship network of co-authors of C. Schrijvers
This figure shows the co-authorship network connecting the top 25 collaborators of C. Schrijvers.
A scholar is included among the top collaborators of C. Schrijvers 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. Schrijvers. C. Schrijvers is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
18 of 18 papers shown
1.
Holties, H. A., Guido Diepen, Fokke Dijkstra, et al.. (2012). Astronomical Data Analysis Software and Systems XXI.51 indexed citations
Ahlers, Berit, G. Bazalgette Courrèges-Lacoste, C. Schrijvers, & Hedser van Brug. (2004). In-orbit detection of spectral features in SCIAMACHY. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 5570. 401–401.5 indexed citations
Jong, J. A. de, H. F. Henrichs, C. Schrijvers, et al.. (1999). Non-radial pulsations in the O stars xi-Persei and lambda-Cephei. UvA-DARE (University of Amsterdam). 345(1). 172–180.6 indexed citations
12.
Schrijvers, C. & J. H. Telting. (1999). Line-profile variations due to adiabetic non-radial pulsations in rotating stars. IV The effects of intrinsic profile variations on the IPS diagnostics. UvA-DARE (University of Amsterdam). 342(2). 453–463.2 indexed citations
13.
Schrijvers, C.. (1999). Spectroscopic diagnostics of pulsation in rotating stars. UvA-DARE (University of Amsterdam).1 indexed citations
14.
Telting, J. H. & C. Schrijvers. (1998). A new bright beta Cephei star: line-profile variability in omega Sco. UvA-DARE (University of Amsterdam). 339(1). 150–158.2 indexed citations
15.
Aerts, C., et al.. (1997). The line-profile variable Lambda Scorpii os a spectroscopic triple system. UvA-DARE (University of Amsterdam). 324(3). 1096–1104.1 indexed citations
16.
Telting, J. H. & C. Schrijvers. (1997). Line-profile variations of non-radial adiabetic pulsations of rotating stars II. The diagnostic value of amplitude and phase diagrams derived from time series of spectra. UvA-DARE (University of Amsterdam). 317(3). 723–741.6 indexed citations
17.
Telting, J. H. & C. Schrijvers. (1997). LINE-PROFILE VARIATIONS OF NON-RADIAL ADIABATIC PULSATIONS OF ROTATING STARS. III. ON THE ALLEGED MISIDENTIFICATION OF TESSERAL MODES. 317(3). 742–748.1 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.