S. Feltzing

13.9k total citations · 7 hit papers
99 papers, 5.6k citations indexed

About

S. Feltzing is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, S. Feltzing has authored 99 papers receiving a total of 5.6k indexed citations (citations by other indexed papers that have themselves been cited), including 93 papers in Astronomy and Astrophysics, 52 papers in Instrumentation and 7 papers in Nuclear and High Energy Physics. Recurrent topics in S. Feltzing's work include Stellar, planetary, and galactic studies (90 papers), Astrophysics and Star Formation Studies (55 papers) and Astronomy and Astrophysical Research (52 papers). S. Feltzing is often cited by papers focused on Stellar, planetary, and galactic studies (90 papers), Astrophysics and Star Formation Studies (55 papers) and Astronomy and Astrophysical Research (52 papers). S. Feltzing collaborates with scholars based in Sweden, United States and Germany. S. Feltzing's co-authors include T. Bensby, Ingemar Lundström, M. S. Oey, M. Asplund, L. Casagrande, T. Bensby, J. Meléndez, S. Cassisi, Ralph Schönrich and I. Ramírez 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

S. Feltzing

94 papers receiving 5.4k citations

Hit Papers

Exploring the Milky Way stellar disk 2003 2026 2010 2018 2014 2003 2011 2011 2013 200 400 600
What are hit papers?

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.

  1. Exploring the Milky Way stellar disk
    2014 604 citations T. Bensby, S. Feltzing et al. profile →
  2. Elemental abundance trends in the Galactic thin and thick disks as traced by nearby F and G dwarf stars
    2003 496 citations T. Bensby, S. Feltzing et al. profile →
  3. New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s)
    2011 487 citations L. Casagrande, Ralph Schönrich et al. profile →
  4. New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey
    2011 349 citations L. Casagrande, Ralph Schönrich et al. profile →
  5. Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood
    2013 342 citations T. Bensby, S. Feltzing et al. profile →
  6. The Gaia-ESO Public Spectroscopic Survey
    2012 328 citations G. Gilmore, M. Asplund et al. profile →
  7. VINTERGATAN – I. The origins of chemically, kinematically, and structurally distinct discs in a simulated Milky Way-mass galaxy
    2021 121 citations Oscar Agertz, Florent Renaud et al. Monthly Notices of the Royal Astronomical Society profile →

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
S. Feltzing Sweden 36 5.5k 2.5k 402 140 103 99 5.6k
C. Chiappini Germany 40 5.2k 1.0× 2.1k 0.9× 419 1.0× 97 0.7× 78 0.8× 158 5.4k
M. Marconi Italy 36 4.3k 0.8× 2.1k 0.8× 377 0.9× 175 1.3× 159 1.5× 228 4.5k
Matthew Shetrone United States 46 5.6k 1.0× 2.8k 1.1× 455 1.1× 126 0.9× 125 1.2× 130 5.8k
Rolf‐Peter Kudritzki United States 39 4.9k 0.9× 1.9k 0.8× 361 0.9× 205 1.5× 166 1.6× 130 5.0k
P. E. Nissen Denmark 38 3.7k 0.7× 1.5k 0.6× 481 1.2× 116 0.8× 116 1.1× 106 3.9k
A. Pietrinferni Italy 32 4.3k 0.8× 2.5k 1.0× 271 0.7× 115 0.8× 161 1.6× 81 4.4k
D. Geisler Chile 48 6.7k 1.2× 3.4k 1.4× 394 1.0× 124 0.9× 137 1.3× 256 6.8k
S. G. Sousa Portugal 37 4.6k 0.8× 1.9k 0.8× 333 0.8× 119 0.8× 123 1.2× 133 4.7k
Kátia Cunha United States 37 3.8k 0.7× 1.6k 0.6× 351 0.9× 96 0.7× 142 1.4× 151 4.0k
David Yong Australia 50 6.8k 1.2× 3.0k 1.2× 817 2.0× 108 0.8× 153 1.5× 157 7.0k

Countries citing papers authored by S. Feltzing

Since Specialization
Citations

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

Fields of papers citing papers by S. Feltzing

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. Feltzing

This figure shows the co-authorship network connecting the top 25 collaborators of S. Feltzing. A scholar is included among the top collaborators of S. Feltzing 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. Feltzing. S. Feltzing 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.
Sahlholdt, C., S. Feltzing, & Diane Feuillet. (2021). Characterizing epochs of star formation across the Milky Way disc using age–metallicity distributions of GALAH stars. Monthly Notices of the Royal Astronomical Society. 510(4). 4669–4688. 44 indexed citations
2.
Agertz, Oscar, Florent Renaud, S. Feltzing, et al.. (2021). VINTERGATAN – I. The origins of chemically, kinematically, and structurally distinct discs in a simulated Milky Way-mass galaxy. Monthly Notices of the Royal Astronomical Society. 503(4). 5826–5845. 121 indexed citations breakdown →
3.
Feuillet, Diane, C. Sahlholdt, S. Feltzing, & L. Casagrande. (2021). Selecting accreted populations: metallicity, elemental abundances, and ages of the Gaia-Sausage-Enceladus and Sequoia populations. Monthly Notices of the Royal Astronomical Society. 508(1). 1489–1508. 63 indexed citations
4.
Bensby, T., et al.. (2020). The HR 1614 moving group is not a dissolving cluster. Springer Link (Chiba Institute of Technology). 12 indexed citations
5.
Feuillet, Diane, S. Feltzing, C. Sahlholdt, & L. Casagrande. (2020). The SkyMapper-Gaia RVS view of the Gaia–Enceladus–Sausage  – an investigation of the metallicity and mass of the Milky Way’s last major merger. Monthly Notices of the Royal Astronomical Society. 497(1). 109–124. 76 indexed citations
6.
Sahlholdt, C. & S. Feltzing. (2019). A Benchmark Age for μ Herculis. Research Notes of the AAS. 3(4). 65–65. 1 indexed citations
7.
Sahlholdt, C., L. Casagrande, & S. Feltzing. (2019). Characteristics of the Two Sequences Seen in the High-velocity Hertzsprung–Russell Diagram in Gaia DR2*. The Astrophysical Journal Letters. 881(1). L10–L10. 23 indexed citations
8.
Gruyters, Pieter, L. Casagrande, A. P. Milone, et al.. (2017). First evidence of multiple populations along the AGB from Strömgren photometry. Springer Link (Chiba Institute of Technology). 12 indexed citations
9.
Liu, Cheng, S. Feltzing, & G. Ruchti. (2015). The nature of the KFR08 stellar stream. Springer Link (Chiba Institute of Technology). 3 indexed citations
10.
Casagrande, L., V. Silva Aguirre, Katharine J. Schlesinger, et al.. (2015). Measuring the vertical age structure of the Galactic disc using asteroseismology and SAGA★. Monthly Notices of the Royal Astronomical Society. 455(1). 987–1007. 88 indexed citations
11.
Koch, Andreas, et al.. (2013). Neutron-capture element deficiency of the Hercules dwarf spheroidal galaxy. Springer Link (Chiba Institute of Technology). 31 indexed citations
12.
Bensby, T. & S. Feltzing. (2012). Chemical constraints on the formation of the Galactic thick disk. Springer Link (Chiba Institute of Technology). 2 indexed citations
13.
Church, Ross P., Jennifer A. Johnson, & S. Feltzing. (2011). Coordinates and 2MASS and OGLE identifications for all stars in Arp’s 1965 finding chart for Baade’s Window. Springer Link (Chiba Institute of Technology).
14.
Árnadóttir, Anna, S. Feltzing, & Ingemar Lundström. (2010). The ability of intermediate-band Strömgren photometry to correctly identify dwarf, subgiant, and giant stars and provide stellar metallicities and surface gravities. Springer Link (Chiba Institute of Technology). 26 indexed citations
15.
16.
Bensby, T., S. Feltzing, & Ingemar Lundström. (2004). Oxygen trends in the Galactic thin and thick disks. Springer Link (Chiba Institute of Technology). 130 indexed citations
17.
Feltzing, S., T. Bensby, & Ingemar Lundström. (2003). Signatures of SN Ia in the galactic thick disk. Observational evidence from alpha -elements in 67 dwarf stars in the solar neighbourhood. Lund University Publications (Lund University). 66 indexed citations
18.
Feltzing, S., Johan Holmberg, & Jarrod R. Hurley. (2001). The solar neighbourhood age-metallicity relation -Does it exist?. Springer Link (Chiba Institute of Technology). 92 indexed citations
19.
Feltzing, S. & Johan Holmberg. (2000). The reality of old moving groups - the case of HR 1614 - Age, metallicity, and a new extended sample. Lund University Publications (Lund University). 7 indexed citations
20.
Feltzing, S.. (2000). Disentangling the Bulge and NGC 6528 - a proper motion study. 8696.

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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