G. Östlin

409 total citations
8 papers, 202 citations indexed

About

G. Östlin is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, G. Östlin has authored 8 papers receiving a total of 202 indexed citations (citations by other indexed papers that have themselves been cited), including 8 papers in Astronomy and Astrophysics, 4 papers in Instrumentation and 3 papers in Nuclear and High Energy Physics. Recurrent topics in G. Östlin's work include Galaxies: Formation, Evolution, Phenomena (7 papers), Stellar, planetary, and galactic studies (6 papers) and Astronomy and Astrophysical Research (4 papers). G. Östlin is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (7 papers), Stellar, planetary, and galactic studies (6 papers) and Astronomy and Astrophysical Research (4 papers). G. Östlin collaborates with scholars based in Sweden, France and United States. G. Östlin's co-authors include D. Schaerer, Peter Laursen, Florent Duval, Erik Zackrisson, Angela Adamo, Robert Cumming, Rachael Livermore, N. Bastian, L. Guaita and Aida Wofford 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

G. Östlin

8 papers receiving 201 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
G. Östlin Sweden	6	200	80	15	13	5	8	202
Leo Y. Alcorn United States	7	146 0.7×	84 1.1×	13 0.9×	8 0.6×	6 1.2×	15	151
Stephen Gwyn Canada	4	160 0.8×	67 0.8×	33 2.2×	15 1.2×	4 0.8×	6	166
Stephen Pardy United States	4	116 0.6×	53 0.7×	14 0.9×	8 0.6×	4 0.8×	5	122
Chen-Fatt Lim Taiwan	6	179 0.9×	84 1.1×	33 2.2×	13 1.0×	4 0.8×	7	185
Adrien Guérou Germany	5	142 0.7×	72 0.9×	16 1.1×	14 1.1×	2 0.4×	5	142
S. Parsa United Kingdom	4	201 1.0×	90 1.1×	36 2.4×	12 0.9×	8 1.6×	4	204
Eduard Westra Australia	7	130 0.7×	76 0.9×	20 1.3×	11 0.8×	3 0.6×	7	134
Madeline A. Marshall Australia	7	175 0.9×	100 1.3×	16 1.1×	10 0.8×	3 0.6×	12	182
A. Molino Spain	6	182 0.9×	102 1.3×	20 1.3×	13 1.0×	2 0.4×	10	186
Sidney Lower United States	7	159 0.8×	91 1.1×	7 0.5×	7 0.5×	4 0.8×	10	171

Countries citing papers authored by G. Östlin

Since Specialization

Citations

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

Fields of papers citing papers by G. Östlin

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of G. Östlin

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

All Works

Sort: Min cites: Since: Top N: Style:

8 of 8 papers shown

1.

Herenz, E. C., Peter Laursen, Axel Runnholm, et al.. (2024). The Lyman alpha reference sample. XV. Relating ionised gas kinematics with Lyman-alpha observables. Astronomy and Astrophysics. 1 indexed citations

2.

Wofford, Aida, S. Charlot, Gustavo Bruzual, et al.. (2016). A comprehensive comparative test of seven widely used spectral synthesis models against multi-band photometry of young massive-star clusters. Monthly Notices of the Royal Astronomical Society. 457(4). 4296–4322. 45 indexed citations

3.

Duval, Florent, D. Schaerer, G. Östlin, & Peter Laursen. (2013). Lymanαline and continuum radiative transfer in a clumpy interstellar medium. Astronomy and Astrophysics. 562. A52–A52. 50 indexed citations

4.

Adamo, Angela, et al.. (2013). HIGH-RESOLUTION STUDY OF THE CLUSTER COMPLEXES IN A LENSED SPIRAL AT REDSHIFT 1.5: CONSTRAINTS ON THE BULGE FORMATION AND DISK EVOLUTION. The Astrophysical Journal. 766(2). 105–105. 31 indexed citations

5.

Otí-Floranes, H., J. M. Más-Hesse, E. Jiménez‐Bailón, et al.. (2012). Multiwavelength analysis of the Lyman-αemitting galaxy Haro 2: relation between the diffuse Lyman-αand soft X-ray emissions. Astronomy and Astrophysics. 546. A65–A65. 16 indexed citations

6.

Micheva, Genoveva, et al.. (2009). How the extinction of extragalactic background light affects surface photometry of galaxies, groups and clusters. Monthly Notices of the Royal Astronomical Society. 397(4). 2057–2069. 2 indexed citations

7.

Östlin, G., et al.. (2006). Dynamical masses of two young globular clusters in the blue compact galaxy ESO 338–IG04. Astronomy and Astrophysics. 461(2). 471–483. 23 indexed citations

8.

Östlin, G., et al.. (2003). The temporal and spatial evolution of the starburst in ESO 338-IG04 as probed by its star clusters. Astronomy and Astrophysics. 408(3). 887–903. 34 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.

Explore authors with similar magnitude of impact