This map shows the geographic impact of J. Krautter'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 J. Krautter with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. Krautter more than expected).
This network shows the impact of papers produced by J. Krautter. 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 J. Krautter. The network helps show where J. Krautter may publish in the future.
Co-authorship network of co-authors of J. Krautter
This figure shows the co-authorship network connecting the top 25 collaborators of J. Krautter.
A scholar is included among the top collaborators of J. Krautter 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 J. Krautter. J. Krautter is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Balman, Ş., S. Starrfield, J. J. Drake, et al.. (2012). The X-ray Nebula around the Recurrent Nova T Pyxidis. ATel. 3915. 1.3 indexed citations
4.
Bode, M. F., J. P. Osborne, K. L. Page, et al.. (2010). Emergence of a Bright and Highly Variable Super-soft Source Phase in Nova KT Eri (2009). The astronomer's telegram. 2392. 1.1 indexed citations
5.
Bode, M. F., J. P. Osborne, K. L. Page, et al.. (2009). Detection of Super-Soft X-ray emission in Nova LMC 2009. The astronomer's telegram. 2025. 1.1 indexed citations
6.
Ness, Jan‐Uwe, S. Starrfield, R. Gonzàlez, et al.. (2008). XMM-Newton RGS observation of V2491 Cyg. ATel. 1561. 1.1 indexed citations
7.
Osborne, J. P., K. L. Page, S. Starrfield, et al.. (2007). Swift X-ray flux limits for the recent novae V1280 and V1281 Sco. ATel. 1011. 1.1 indexed citations
8.
Osborne, J. P., K. L. Page, A. P. Beardmore, et al.. (2006). RS Oph: Swift X-ray observations find short period modulation and highly variable low energy flux. The astronomer's telegram. 770. 1.2 indexed citations
9.
Osborne, J. P., K. L. Page, A. P. Beardmore, et al.. (2006). The decline and rise of the X-ray flux of RS Oph. The astronomer's telegram. 764. 1.2 indexed citations
10.
Mamajek, Eric E., et al.. (1997). Radio Emission from ROSAT Discovered Young Stars in and Around Taurus-Auriga. MmSAI. 154. 1001–1068.1 indexed citations
Krautter, J.. (1996). The impact of ROSAT observations on our understanding of star forming regions. 109. 395.1 indexed citations
14.
Alcalá, J. M., J. Krautter, J. H. M. M. Schmitt, et al.. (1995). A study of the Chamaeleon star forming region from the ROSAT all-sky survey. I. X-ray observations and optical identifications.. Astronomy & Astrophysics Supplement Series. 114. 109.2 indexed citations
15.
Krautter, J., et al.. (1994). Meyers Handbuch Weltall.1 indexed citations
16.
Appenzeller, I., I. Jankovics, & J. Krautter. (1983). Spectroscopy and infrared photometry of southern T Tauri stars.. Astronomy & Astrophysics Supplement Series. 53. 291–309.1 indexed citations
17.
Ruciński, S. M. & J. Krautter. (1983). TW Hya : a T Tauri star far from any dark cloud.. 121. 200–225.1 indexed citations
18.
Appenzeller, I., Carlos Chavarría, J. Krautter, R. Mundt, & B. Wolf. (1980). UV spectrograms of T Tau stars.. A&A. 90. 184–191.2 indexed citations
Gaida, G., et al.. (1979). A Computer Readable Catalogue. Astronomy & Astrophysics Supplement Series. 37. 465.2 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.