O. L. Creevey

32.6k total citations · 1 hit paper
31 papers, 771 citations indexed

About

O. L. Creevey is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, O. L. Creevey has authored 31 papers receiving a total of 771 indexed citations (citations by other indexed papers that have themselves been cited), including 29 papers in Astronomy and Astrophysics, 16 papers in Instrumentation and 5 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in O. L. Creevey's work include Stellar, planetary, and galactic studies (29 papers), Astronomy and Astrophysical Research (16 papers) and Astrophysics and Star Formation Studies (11 papers). O. L. Creevey is often cited by papers focused on Stellar, planetary, and galactic studies (29 papers), Astronomy and Astrophysical Research (16 papers) and Astrophysics and Star Formation Studies (11 papers). O. L. Creevey collaborates with scholars based in France, United States and Spain. O. L. Creevey's co-authors include Τ. S. Metcalfe, Y. Lebreton, M. Fouesneau, Alexandru Burlacu, G. Kordopatis, A. Jean-Antoine-Piccolo, Bernard Pichon, A. J. Korn, Coryn A. L. Bailer‐Jones and Nicolas Mary and has published in prestigious journals such as SHILAP Revista de lepidopterología, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

O. L. Creevey

29 papers receiving 722 citations

Hit Papers

Gaia Data Release 2 2018 2026 2020 2023 2018 50 100 150 200 250

Peers

O. L. Creevey
Leigh C. Smith United Kingdom
Meridith Joyce United States
Jamie Tayar United States
K. Brogaard Denmark
Sara Bladh Sweden
Leigh C. Smith United Kingdom
O. L. Creevey
Citations per year, relative to O. L. Creevey O. L. Creevey (= 1×) peers Leigh C. Smith

Countries citing papers authored by O. L. Creevey

Since Specialization
Citations

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

Fields of papers citing papers by O. L. Creevey

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by O. L. Creevey. 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 O. L. Creevey. The network helps show where O. L. Creevey may publish in the future.

Co-authorship network of co-authors of O. L. Creevey

This figure shows the co-authorship network connecting the top 25 collaborators of O. L. Creevey. A scholar is included among the top collaborators of O. L. Creevey 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 O. L. Creevey. O. L. Creevey 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.
Creevey, O. L., S. Cassisi, F. Thévenin, M. Salaris, & A. Pietrinferni. (2024). Benchmarking the effective temperature scale of red giant branch stellar models: The case of the metal-poor halo giant HD 122563. Astronomy and Astrophysics. 689. A243–A243. 4 indexed citations
2.
Soubiran, C., O. L. Creevey, N. Lagarde, et al.. (2023). Gaia FGK benchmark stars: Fundamental Teff and log g of the third version. Astronomy and Astrophysics. 682. A145–A145. 12 indexed citations
3.
Creevey, O. L., et al.. (2023). Asteroseismic age constraints on the open cluster NGC 2477 using oscillating stars identified with TESS FFI. Astronomy and Astrophysics. 674. A146–A146. 6 indexed citations
4.
Nardetto, N., D. Mourard, O. L. Creevey, et al.. (2020). Precise calibration of the dependence of surface brightness–colour relations on colour and class for late-type stars. Astronomy and Astrophysics. 640. A2–A2. 6 indexed citations
5.
Nardetto, N., D. Mourard, O. L. Creevey, et al.. (2020). Precise calibration of the dependence of surface brightness–colour relations on colour and class for late-type stars (Corrigendum). Astronomy and Astrophysics. 641. C3–C3. 1 indexed citations
6.
Creevey, O. L., F. Grundahl, F. Thévenin, et al.. (2019). First detection of oscillations in the Halo giant HD 122563: Validation of seismic scaling relations and new parameters. Springer Link (Chiba Institute of Technology). 9 indexed citations
7.
Ligi, R., Caroline Dorn, A. Crida, et al.. (2019). From the stellar properties of HD 219134 to the internal compositions of its transiting exoplanets. Springer Link (Chiba Institute of Technology). 9 indexed citations
8.
Bazot, M., O. L. Creevey, J. Christensen‐Dalsgaard, & J. Meléndez. (2018). Modelling the solar twin 18 Scorpii. Springer Link (Chiba Institute of Technology). 11 indexed citations
9.
Andrae, R., M. Fouesneau, O. L. Creevey, et al.. (2018). Gaia Data Release 2. Astronomy and Astrophysics. 616. A8–A8. 283 indexed citations breakdown →
10.
Beck, P. G., J.-D. do Nascimento, D. Salabert, et al.. (2017). Lithium abundance and rotation of seismic solar analogues. Astronomy and Astrophysics. 602. A63–A63. 20 indexed citations
11.
Mourard, D., P. Bério, K. Perraut, et al.. (2017). SPICA, Stellar Parameters and Images with a Cophased Array: a 6T visible combiner for the CHARA array. Journal of the Optical Society of America A. 34(5). A37–A37. 11 indexed citations
12.
Salabert, D., C. Régulo, R. A. García, et al.. (2016). Magnetic variability in the young solar analog KIC 10644253. Astronomy and Astrophysics. 589. A118–A118. 29 indexed citations
13.
Ceillier, T., Jennifer L. van Saders, R. A. García, et al.. (2015). Rotation periods and seismic ages of KOIs – comparison with stars without detected planets fromKeplerobservations. Monthly Notices of the Royal Astronomical Society. 456(1). 119–125. 30 indexed citations
14.
Metcalfe, Τ. S., O. L. Creevey, & G. R. Davies. (2015). ASTEROSEISMIC MODELING OF 16 Cyg A & B USING THE COMPLETE KEPLER DATA SET. The Astrophysical Journal Letters. 811(2). L37–L37. 25 indexed citations
15.
Ligi, R., O. L. Creevey, D. Mourard, et al.. (2015). Radii, masses, and ages of 18 bright stars using interferometry and new estimations of exoplanetary parameters. Astronomy and Astrophysics. 586. A94–A94. 47 indexed citations
16.
Rodler, F., R. Deshpande, M. R. Zapatero Osorio, et al.. (2012). Search for radial velocity variations in eight M-dwarfs with NIRSPEC/Keck II. Astronomy and Astrophysics. 538. A141–A141. 10 indexed citations
17.
Creevey, O. L., Tabetha S. Boyajian, P. Kervella, et al.. (2012). Fundamental properties of the Population II fiducial stars HD 122563 and Gmb 1830 from CHARA interferometric observations. Astronomy and Astrophysics. 545. A17–A17. 43 indexed citations
18.
Mathur, S., R. A. García, C. Régulo, et al.. (2010). Determining global parameters of the oscillations of solar-like stars. Astronomy and Astrophysics. 511. A46–A46. 81 indexed citations
19.
Michel, E., O. L. Creevey, Juan Antonio Belmonte, et al.. (2007). Pulsational frequencies of the eclipsing δ Scuti star HD 172189. Results of the STEPHI XIII campaign. Astronomy and Astrophysics. 468(2). 637–642. 8 indexed citations
20.
Creevey, O. L., M. J. P. F. G. Monteiro, Τ. S. Metcalfe, et al.. (2007). The Complementary Roles of Interferometry and Asteroseismology in Determining the Mass of Solar‐Type Stars. The Astrophysical Journal. 659(1). 616–625. 30 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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