M. Asplund

44.5k citations

292 papers · 23.7k indexed · 11 hit papers · h-index 73

Impact in

Instrumentation top 0.02%
- Astronomy and Astrophysical Research
Astronomy and Astrophysics top 0.01%
- Stellar, planetary, and galactic studies
- Astrophysics and Star Formation Studies
- Astro and Planetary Science
- Gamma-ray bursts and supernovae
- Galaxies: Formation, Evolution, Phenomena
- Solar and Space Plasma Dynamics
- Astrophysical Phenomena and Observations

Papers in

Instrumentation 100
- Astronomy and Astrophysical Research 100
Astronomy and Astrophysics 284
- Stellar, planetary, and galactic studies 270
- Astro and Planetary Science 152
- Astrophysics and Star Formation Studies 149
- Solar and Space Plasma Dynamics 66
- Gamma-ray bursts and supernovae 27

Co-authors: N. Grevesse A. J. Sauval Pat Scott J. Meléndez R. Collet I. Ramírez K. Lind David L. Lambert
Journals: Astronomy and Astrophysics (66 papers)Monthly Notices of the Royal Astronomical Society (58 papers)The Astrophysical Journal (30 papers)Monthly Notices of the Royal Astronomical Society Letters (7 papers)The Astronomical Journal (4 papers)
Partner nations: Australia Germany United States

In The Last Decade

M. Asplund

284 papers receiving 22.7k citations

Hit Papers

11 papers align trajectories log scale

The chemical make-up of the Sun: A 2020 vision 2021 · 351 citations

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if any of the following hold:

it has ≥500 total citations;
it reaches ≥1.5× the top-1% citation threshold for papers in the same subfield and year (the threshold is the minimum needed to enter the top 1%, not the average within it);
it reaches the top citation threshold in at least one of its specific research topics.

2021 Springer Link (Chiba Institute of Technology)
2012 Nova Science Publishers (Nova Science Publishers, Inc.)
2011 Astronomy and Astrophysics
2011 Scientific Electronic Library Online (São Paulo Research Foundation, Latin American and Caribbean Center on Health Sciences Information, Conselho Nacional de Desenvolvimento Científico e Tecnológico)
2010 Astronomy and Astrophysics
2009 Annual Review of Astronomy and Astrophysics
2007 Space Science Reviews
2005 Annual Review of Astronomy and Astrophysics
2004 Astronomy and Astrophysics
2003 ArXiv.org
2001 The Astrophysical Journal

Peers

Countries citing papers authored by M. Asplund

Since Specialization

Citations

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

Fields of papers citing papers by M. Asplund

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network

The 25 scholars most cited alongside M. Asplund, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with M. Asplund Line = papers co-authored together M. Asplund links everyone, so they are left out of the graph.

All Works

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

20 of 20 papers shown

#	Work
1	The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations Monthly Notices of the Royal Astronomical Society ·Carl Poree, Thomas Nordlander, L. Casagrande, Meridith Joyce, Yaguang Li, A. M. Amarsi, Henrique Reggiani, M. Asplund	2021	4
2	The 3D non-LTE solar nitrogen abundance from atomic lines Springer Link (Chiba Institute of Technology) ·A. M. Amarsi, N. Grevesse, Jon Grumer, M. Asplund, P. S. Barklem, R. Collet	2020	22
3	The GALAH survey: chemodynamics of the solar neighbourhood Monthly Notices of the Royal Astronomical Society ·Michael Hayden, Joss Bland‐Hawthorn, Sanjib Sharma, K. C. Freeman, Janez Kos, Sven Buder, Borja Anguiano, M. Asplund, Boquan Chen, Gayandhi M De Silva, S. Khanna, Jane Lin, Jonathan Horner, Sarah L. Martell, Yuan-Sen Ting, Rosemary F. Ġ. Wyse, D. B. Zucker, T. Zwitter	2020	49
4	Keck HIRES spectroscopy of SkyMapper commissioning survey candidate extremely metal-poor stars Monthly Notices of the Royal Astronomical Society ·A. F. Marino, G. S. Da Costa, Andrew R. Casey, M. Asplund, M. S. Bessell, Anna Frebel, S. Keller, K. Lind, Dougal Mackey, Simon J. Murphy, Thomas Nordlander, John E. Norris, B. Schmidt, David Yong	2019	13
5	Effective temperature determinations of late-type stars based on 3D non-LTE Balmer line formation Springer Link (Chiba Institute of Technology) ·A. M. Amarsi, Thomas Nordlander, P. S. Barklem, M. Asplund, R. Collet, K. Lind	2018	61
6	HIGH-RESOLUTION SPECTROSCOPIC STUDY OF EXTREMELY METAL-POOR STAR CANDIDATES FROM THE SKYMAPPER SURVEY DSpace@MIT (Massachusetts Institute of Technology) ·Stefan Keller, Andrew R. Casey, M. Asplund, M. S. Bessell, (unknown), K. Lind, A. F. Marino, John E. Norris, B. Schmidt, P. Tisserand, 関根智子, David Yong, Heather R. Jacobson, Anna Frebel, José Martínez Peña, Qinqin Yu	2015	81
7	Line formation in solar granulation VI. [Cl], Cl, CH and C2 lines and the photospheric C abundance ANU Open Research (Australian National University) ·M. Asplund, N. Grevesse, A. J. Sauval, C. Allende Prieto, R. Blomme	2015	34
8	How realistic are solar model atmospheres? Springer Link (Chiba Institute of Technology) ·Tiago M. D. Pereira, M. Asplund, R. Collet, 美登利鈴木, Regner Trampedach, J. Leenaarts	2013	44
9	Springer Link (Chiba Institute of Technology) ·A. Chiavassa, Lionel Bigot, P. Kervella, A. Matter, B. López, R. Collet, Z. Magic, M. Asplund	2012	21
10	Sulphur abundances in halo giants from the [S ı] line at 1082 nm and the S ı triplet around 1045 nm Springer Link (Chiba Institute of Technology) ·Henrik Jönsson, N. Ryde, P. E. Nissen, R. Collet, Kimmo Eriksson, M. Asplund, B. Gustafsson	2011	14
11	Lithium depletion in solar-like stars: no planet connection Springer Link (Chiba Institute of Technology) ·Patrick Baumann, I. Ramírez, J. Meléndez, M. Asplund, K. Lind	2010	76
12	Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion Springer Link (Chiba Institute of Technology) ·J. Meléndez, L. Casagrande, I. Ramírez, M. Asplund, W. J. Schuster	2010	64
13	A possible signature of terrestrial planet formation in the chemical composition of solar analogs Springer Link (Chiba Institute of Technology) ·I. Ramírez, M. Asplund, Patrick Baumann, J. Meléndez, T. Bensby	2010	74
14	O and Na abundance patterns in open clusters of the Galactic disk Springer Link (Chiba Institute of Technology) ·Guichaud, B. K. Gibson, John C. Lattanzio, M. Asplund	2009	47
15	Sulphur and zinc abundances in Galactic halo stars revisited Springer Link (Chiba Institute of Technology) ·P. E. Nissen, Kathyl Faitel, M. Asplund, D. Fabbian, F. Kerber, H. U. Käufl, Max Pettini	2007	75
16	Chemical abundances in 43 metal-poor stars Springer Link (Chiba Institute of Technology) ·Xingyuan Xu, T Reca De Acosta, B. Gustafsson, P. Magain, Hansae Ju, M. Asplund	2005	51
17	The evolution of the C/O ratio in metal-poor halo stars Springer Link (Chiba Institute of Technology) ·Kathyl Faitel, Leticia Carigi, P. E. Nissen, Max Pettini, M. Asplund	2004	112
18	On OH line formation and oxygen abundances in metal-poor stars Springer Link (Chiba Institute of Technology) ·M. Asplund, A. E. García Pérez	2001	82
19	Chemical Abundances from Inversions of Stellar Spectra: Analysis of Solar-Type Stars with Homogeneous and Static Model Atmospheres ANU Open Research (Australian National University) ·Carlos Allende Prieto, P. S. Barklem, M. Asplund, B. Ruiz Cobo	2001	29
20	Commission 36: Theory of Stellar Atmospheres Transactions of the International Astronomical Union ·J. D. Landstreet, M. Asplund, M. Spite, José L. García Siñeriz Martínez, S. V. Berdyugina, P. H. Hauschildt, H.‐G. Ludwig, L. Mashonkina, Howard P. Colson, S. Randich	1991	1

About M. Asplund

M. Asplund is a scholar working on Instrumentation, Astronomy and Astrophysics, Nuclear and High Energy Physics, Atmospheric Science and Geophysics, having authored 292 papers that have together received 23.7k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (270 papers), Astro and Planetary Science (152 papers), Astrophysics and Star Formation Studies (149 papers), Astronomy and Astrophysical Research (100 papers), Solar and Space Plasma Dynamics (66 papers), Gamma-ray bursts and supernovae (27 papers), Atmospheric Ozone and Climate (16 papers) and Astronomical and nuclear sciences (14 papers). The work is most often cited by research in Instrumentation (7.5k citations), Astronomy and Astrophysics (22.7k citations), Nuclear and High Energy Physics (2.2k citations), Atmospheric Science (1.2k citations) and Geophysics (523 citations). M. Asplund has collaborated with scholars based in Australia, Germany and United States. Frequent co-authors include N. Grevesse, A. J. Sauval, Pat Scott, J. Meléndez, R. Collet, I. Ramírez, K. Lind, David L. Lambert, Carlos Allende Prieto and David Yong. Their work appears in journals such as Astronomy and Astrophysics, Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society Letters and The Astronomical Journal.

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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