K. Nilsson

1.3k total citations
20 papers, 563 citations indexed

About

K. Nilsson is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, K. Nilsson has authored 20 papers receiving a total of 563 indexed citations (citations by other indexed papers that have themselves been cited), including 17 papers in Astronomy and Astrophysics, 11 papers in Instrumentation and 3 papers in Nuclear and High Energy Physics. Recurrent topics in K. Nilsson's work include Galaxies: Formation, Evolution, Phenomena (16 papers), Astronomy and Astrophysical Research (11 papers) and Gamma-ray bursts and supernovae (5 papers). K. Nilsson is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (16 papers), Astronomy and Astrophysical Research (11 papers) and Gamma-ray bursts and supernovae (5 papers). K. Nilsson collaborates with scholars based in Germany, Denmark and Chile. K. Nilsson's co-authors include J. P. U. Fynbo, P. Møller, C. Ledoux, Jesper Sommer‐Larsen, W. Freudling, K. Meisenheimer, Peter Laursen, C. Tapken, G. Östlin and M. J. Michałowski 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

K. Nilsson

19 papers receiving 553 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
K. Nilsson Germany 11 554 220 120 29 18 20 563
M. Ajiki Japan 11 714 1.3× 285 1.3× 178 1.5× 39 1.3× 18 1.0× 20 718
C. Tapken Germany 12 647 1.2× 279 1.3× 121 1.0× 51 1.8× 25 1.4× 16 655
Ali Ahmad Khostovan United States 11 465 0.8× 209 0.9× 95 0.8× 40 1.4× 16 0.9× 20 485
Mimi Song United States 11 502 0.9× 212 1.0× 95 0.8× 27 0.9× 22 1.2× 16 510
Jun Toshikawa Japan 11 481 0.9× 219 1.0× 108 0.9× 24 0.8× 17 0.9× 22 489
Amber N. Straughn United States 12 421 0.8× 211 1.0× 54 0.5× 25 0.9× 20 1.1× 15 435
Steve Dawson United States 14 876 1.6× 295 1.3× 228 1.9× 36 1.2× 23 1.3× 18 886
Silvio Lorenzoni United Kingdom 10 580 1.0× 321 1.5× 76 0.6× 38 1.3× 44 2.4× 13 589
Harold Francke Chile 5 433 0.8× 214 1.0× 106 0.9× 37 1.3× 21 1.2× 7 439
Moire K. M. Prescott United States 12 436 0.8× 163 0.7× 68 0.6× 9 0.3× 16 0.9× 22 440

Countries citing papers authored by K. Nilsson

Since Specialization
Citations

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

Fields of papers citing papers by K. Nilsson

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of K. Nilsson

This figure shows the co-authorship network connecting the top 25 collaborators of K. Nilsson. A scholar is included among the top collaborators of K. Nilsson 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 K. Nilsson. K. Nilsson 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.
Møller, P., J. P. U. Fynbo, C. Ledoux, & K. Nilsson. (2013). Mass–metallicity relation from z = 5 to the present: evidence for a transition in the mode of galaxy growth at z = 2.6 due to the end of sustained primordial gas infall. Monthly Notices of the Royal Astronomical Society. 430(4). 2680–2687. 84 indexed citations
2.
Pirzkal, Nor, Barry Rothberg, K. Nilsson, et al.. (2012). A LINK TO THE PAST: USING MARKOV CHAIN MONTE CARLO FITTING TO CONSTRAIN FUNDAMENTAL PARAMETERS OF HIGH-REDSHIFT GALAXIES. The Astrophysical Journal. 748(2). 122–122. 10 indexed citations
3.
Malhotra, Sangeeta, James E. Rhoads, Steven L. Finkelstein, et al.. (2012). SIZING UP Lyα AND LYMAN BREAK GALAXIES. The Astrophysical Journal Letters. 750(2). L36–L36. 44 indexed citations
4.
Zafar, Tayyaba, P. Møller, C. Ledoux, et al.. (2011). A Lyαblob andzabs ≈ zemdamped Lyαabsorber in the dark matter halo of the binary quasar Q 0151+048. Astronomy and Astrophysics. 532. A51–A51. 25 indexed citations
5.
Clément, B., Jean-Gabriel Cuby, F. Courbin, et al.. (2011). Evolution of the observed Lyαluminosity function fromz= 6.5 toz= 7.7: evidence for the epoch of reionization?. Astronomy and Astrophysics. 538. A66–A66. 26 indexed citations
6.
Kümmel, M., P. Rosati, R. A. E. Fosbury, et al.. (2011). TheHubbleLegacy Archive ACS grism data. Astronomy and Astrophysics. 530. A86–A86. 2 indexed citations
7.
Nilsson, K., O. Möller-Nilsson, P. Rosati, et al.. (2010). Stellar properties ofz ~ 1 Lyman-break galaxies from ACS slitless grism spectra. Astronomy and Astrophysics. 526. A10–A10. 4 indexed citations
8.
Nilsson, K. & P. Møller. (2009). Lyα emitters: blue dwarfs or supermassive ULIRGs? Evidence for a transition with redshift. Astronomy and Astrophysics. 508(2). L21–L25. 10 indexed citations
9.
Fynbo, J. P. U., C. Ledoux, Marceau Limousin, et al.. (2009). The Building the Bridge survey for z = 3 Lyα emitting galaxies. Astronomy and Astrophysics. 497(3). 689–702. 19 indexed citations
10.
Nilsson, K., C. Tapken, P. Møller, et al.. (2009). Evolution in the properties of Lyman-αemitters from redshiftsz~ 3 toz ~ 2. Astronomy and Astrophysics. 498(1). 13–23. 82 indexed citations
11.
Nilsson, K. & Klaus Meisenheimer. (2009). Understanding Lyα emitters. New Astronomy Reviews. 53(3). 37–39. 2 indexed citations
12.
Nilsson, K., et al.. (2009). On the dependence between UV luminosity and Ly�� equivalent width in high-redshift galaxies. Monthly Notices of the Royal Astronomical Society. 400(1). 232–237. 23 indexed citations
13.
Takalo, L. O., K. Nilsson, E. Lindfors, et al.. (2008). Tuorla Blazar Monitoring Program. AIP conference proceedings. 705–707. 6 indexed citations
14.
Nilsson, K., et al.. (2007). Narrow-band surveys for very high redshift Lyman-α emitters. Durham Research Online (Durham University). 22 indexed citations
15.
Nilsson, K., P. Møller, J. P. U. Fynbo, et al.. (2007). A multi-wavelength study ofz= 3.15 Lyman-$\mathsf{\alpha}$ emitters in the GOODS South Field. Astronomy and Astrophysics. 471(1). 71–82. 64 indexed citations
16.
Nilsson, K., J. P. U. Fynbo, P. Møller, Jesper Sommer‐Larsen, & C. Ledoux. (2006). A Lyman-α blob in the GOODSSouth field: evidence for cold accretion onto a dark matter halo. Astronomy and Astrophysics. 452(3). L23–L26. 81 indexed citations
17.
Gorosabel, J., D. Pérez-Ramírez, J. Sollerman, et al.. (2005). The GRB 030329 host: a blue low metallicity subluminous galaxy with intense star formation. Astronomy and Astrophysics. 444(3). 711–721. 45 indexed citations
18.
Nilsson, K., et al.. (2003). On the scalability of visualization in manufacturing. Lund University Publications (Lund University). 1. 43–51. 3 indexed citations
19.
Nilsson, K.. (2003). Increasing Quality with Pair Programming. KTH Publication Database DiVA (KTH Royal Institute of Technology). 1 indexed citations
20.
Pursimo, T., K. Nilsson, P. Teerikorpi, et al.. (1999). Optical morphology of distant RATAN-600 radio galaxiesfrom subarcsecond resolution NOT images. Astronomy and Astrophysics Supplement Series. 134(3). 505–521. 10 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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