Jan‐Uwe Ness

4.5k total citations
167 papers, 2.3k citations indexed

About

Jan‐Uwe Ness is a scholar working on Astronomy and Astrophysics, Computational Mechanics and Nuclear and High Energy Physics. According to data from OpenAlex, Jan‐Uwe Ness has authored 167 papers receiving a total of 2.3k indexed citations (citations by other indexed papers that have themselves been cited), including 155 papers in Astronomy and Astrophysics, 36 papers in Computational Mechanics and 36 papers in Nuclear and High Energy Physics. Recurrent topics in Jan‐Uwe Ness's work include Astrophysical Phenomena and Observations (126 papers), Gamma-ray bursts and supernovae (67 papers) and Stellar, planetary, and galactic studies (40 papers). Jan‐Uwe Ness is often cited by papers focused on Astrophysical Phenomena and Observations (126 papers), Gamma-ray bursts and supernovae (67 papers) and Stellar, planetary, and galactic studies (40 papers). Jan‐Uwe Ness collaborates with scholars based in United States, Spain and United Kingdom. Jan‐Uwe Ness's co-authors include J. H. M. M. Schmitt, M. Güdel, M. Audard, R. Mewe, J. J. Drake, J. P. Osborne, K. L. Page, J. Robrade, A. J. J. Raassen and R. L. J. van der Meer and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

Jan‐Uwe Ness

165 papers receiving 2.2k citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
Jan‐Uwe Ness United States	28	2.1k	513	215	210	158	167	2.3k
David P. Huenemoerder United States	25	1.8k 0.8×	209 0.4×	105 0.5×	186 0.9×	107 0.7×	93	1.9k
J. P. Pye United Kingdom	22	1.4k 0.6×	330 0.6×	74 0.3×	216 1.0×	90 0.6×	84	1.6k
Bradford J. Wargelin United States	18	884 0.4×	296 0.6×	72 0.3×	374 1.8×	58 0.4×	43	1.2k
J. A. M. Bleeker Netherlands	18	1.6k 0.7×	742 1.4×	95 0.4×	124 0.6×	55 0.3×	80	1.8k
F. Jansen Netherlands	11	1.8k 0.8×	619 1.2×	241 1.1×	122 0.6×	51 0.3×	31	1.9k
Allyn F. Tennant United States	26	1.8k 0.8×	775 1.5×	227 1.1×	78 0.4×	90 0.6×	99	1.9k
K. Beuermann Germany	29	2.1k 1.0×	394 0.8×	172 0.8×	89 0.4×	146 0.9×	148	2.2k
S. H. Pravdo United States	23	1.7k 0.8×	322 0.6×	291 1.4×	125 0.6×	101 0.6×	105	1.8k
B. J. Kellett United Kingdom	21	986 0.5×	284 0.6×	71 0.3×	246 1.2×	35 0.2×	93	1.2k
F. Paerels United States	13	788 0.4×	203 0.4×	179 0.8×	146 0.7×	30 0.2×	22	878

Countries citing papers authored by Jan‐Uwe Ness

Since Specialization

Citations

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

Fields of papers citing papers by Jan‐Uwe Ness

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Jan‐Uwe Ness. 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 Jan‐Uwe Ness. The network helps show where Jan‐Uwe Ness may publish in the future.

Co-authorship network of co-authors of Jan‐Uwe Ness

This figure shows the co-authorship network connecting the top 25 collaborators of Jan‐Uwe Ness. A scholar is included among the top collaborators of Jan‐Uwe Ness 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 Jan‐Uwe Ness. Jan‐Uwe Ness is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

Orio, Marina, S. Ciroi, E. Aydi, et al.. (2024). V407 Lup, an intermediate polar nova. Monthly Notices of the Royal Astronomical Society. 533(2). 1541–1549. 1 indexed citations

Beardmore, A. P., et al.. (2017). Detection of a 9.4 min periodicity in the XMM-Newton and Chandra X-ray light curves of V407 Lup (Nova Lup 2016). ATel. 10749. 1. 1 indexed citations

Ness, Jan‐Uwe, A. P. Beardmore, J. P. Osborne, et al.. (2015). Short-period X-ray oscillations in super-soft novae and persistent super-soft sources. Springer Link (Chiba Institute of Technology). 21 indexed citations

Ness, Jan‐Uwe, et al.. (2015). Nova V723 Cas off in X-rays. ATel. 8053. 1. 2 indexed citations

Shore, S. N., Frederick M. Walter, P. A. Woudt, et al.. (2014). First high resolution ultraviolet (HST/STIS) and supporting optical spectroscopy (CHIRON/SMARTS, HRS/SALT) of V1369 Cen = Nova Cen 2013. ATel. 6413. 1. 1 indexed citations

Darnley, M. J., M. F. Bode, A. W. Shafter, et al.. (2014). Recurrent Nova M31N 2008-12a: Additional observations, pre-detection limit, and erratum to ATel #6527. ATel. 6535. 1. 1 indexed citations

Ness, Jan‐Uwe, J. P. Osborne, M. Henze, et al.. (2013). Obscuration effects in super-soft-source X-ray spectra. Springer Link (Chiba Institute of Technology). 27 indexed citations

Pinto, C., et al.. (2012). A phenomenological model for the X-ray spectrum of nova V2491\n Cygni. Springer Link (Chiba Institute of Technology). 10 indexed citations

Osborne, J. P., K. L. Page, A. A. Henden, et al.. (2011). Swift observations of the March 2011 outburst of the cataclysmic variable NSV 1436: a probable dwarf nova. Springer Link (Chiba Institute of Technology).

10.

Fuhrmeister, B., S. Lalitha, Katja Poppenhaeger, et al.. (2011). Multi-wavelength observations of Proxima Centauri. Springer Link (Chiba Institute of Technology). 33 indexed citations

11.

Schwarz, G. J., J. P. Osborne, K. L. Page, et al.. (2011). Swift detection of super soft X-ray emission in Nova V2468 Cygni. The astronomer's telegram. 3754. 1. 1 indexed citations

12.

Schwarz, G. J., J. P. Osborne, K. L. Page, et al.. (2010). Swift super soft X-ray detection in Nova V1213 Centauri. The astronomer's telegram. 2904. 1. 2 indexed citations

13.

Ness, Jan‐Uwe, J. J. Drake, S. Starrfield, et al.. (2010). A Chandra High-Resolution X-ray spectrum of KT Eri. ATel. 2418. 1. 2 indexed citations

14.

Schaefer, Bradley E., Ashley Pagnotta, J. P. Osborne, et al.. (2010). Recurrent Nova U Sco Has Sharp Decline in X-ray/UV/Optical/IR. ATel. 2477. 1. 3 indexed citations

15.

Page, K. L., J. P. Osborne, A. M. Read, et al.. (2009). X-ray and UV observations of nova V598 Puppis between 147 and 255 days after outburst. Springer Link (Chiba Institute of Technology). 3 indexed citations

16.

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

17.

Günther, Hans Moritz, C. Liefke, J. H. M. M. Schmitt, J. Robrade, & Jan‐Uwe Ness. (2006). X-ray accretion signatures in the close CTTS binary V4046 Sagittarii. Springer Link (Chiba Institute of Technology). 54 indexed citations

18.

Ness, Jan‐Uwe, M. Güdel, J. H. M. M. Schmitt, M. Audard, & A. Telleschi. (2004). On the sizes of stellar X-ray coronae. Springer Link (Chiba Institute of Technology). 77 indexed citations

19.

Schmitt, J. H. M. M. & Jan‐Uwe Ness. (2004). Coronal abundances from high-resolution X-ray data: The case of Algol. Springer Link (Chiba Institute of Technology). 13 indexed citations

20.

Ness, Jan‐Uwe & J. H. M. M. Schmitt. (2000). A Search for X-ray emission from Saturn, Uranus and Neptune. CERN Bulletin. 355. 394–397. 4 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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