Claire Halliday

782 total citations
9 papers, 446 citations indexed

About

Claire Halliday is a scholar working on Astronomy and Astrophysics, Instrumentation and Computer Vision and Pattern Recognition. According to data from OpenAlex, Claire Halliday has authored 9 papers receiving a total of 446 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 9 papers in Instrumentation and 1 paper in Computer Vision and Pattern Recognition. Recurrent topics in Claire Halliday's work include Astronomy and Astrophysical Research (9 papers), Galaxies: Formation, Evolution, Phenomena (8 papers) and Stellar, planetary, and galactic studies (5 papers). Claire Halliday is often cited by papers focused on Astronomy and Astrophysical Research (9 papers), Galaxies: Formation, Evolution, Phenomena (8 papers) and Stellar, planetary, and galactic studies (5 papers). Claire Halliday collaborates with scholars based in United States, Italy and Germany. Claire Halliday's co-authors include Dennis Zaritsky, Bianca M. Poggianti, B. Milvang‐Jensen, Gregory Rudnick, Luc Simard, R. Pelló, G. De Lucia, Alfonso Aragón‐Salamanca, Rose Finn and Douglas Clowe 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

Claire Halliday

9 papers receiving 440 citations

Peers

Claire Halliday

AA

INSTR

NHEP

ECOLO

CVPR

Jenica E. Nelan United States

E. Pignatelli Italy

Hyunjin Jeong South Korea

Jerome J. Fang United States

David T. Maltby United Kingdom

G. Consolandi Italy

Y. Peng United Kingdom

M. Balogh Canada

T. Moutard France

Mark Seibert United States

Jenica E. Nelan United States

Claire Halliday

446 ×1.0

AA

320 ×1.0

INSTR

32 ×1.0

NHEP

25 ×0.8

ECOLO

24 ×0.8

CVPR

Citations per year, relative to Claire Halliday Claire Halliday (= 1×) peers Jenica E. Nelan

Countries citing papers authored by Claire Halliday

Since Specialization

Citations

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

Fields of papers citing papers by Claire Halliday

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Claire Halliday

This figure shows the co-authorship network connecting the top 25 collaborators of Claire Halliday. A scholar is included among the top collaborators of Claire Halliday 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 Claire Halliday. Claire Halliday 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:

9 of 9 papers shown

1.

Just, Dennis W., Dennis Zaritsky, Gregory Rudnick, et al.. (2019). Preprocessing among the Infalling Galaxy Population of EDisCS Clusters. The Astrophysical Journal. 885(1). 6–6. 18 indexed citations

2.

Rudnick, Gregory, P. Jablonka, John Moustakas, et al.. (2017). Determining the Halo Mass Scale Where Galaxies Lose Their Gas^*. The Astrophysical Journal. 850(2). 181–181. 14 indexed citations

3.

Martinet, N., F. Durret, L. Guennou, et al.. (2015). The evolution of the cluster optical galaxy luminosity function betweenz= 0.4 and 0.9 in the DAFT/FADA survey. Astronomy and Astrophysics. 575. A116–A116. 14 indexed citations

4.

Jaffé, Yara L., Alfonso Aragón‐Salamanca, B. Ziegler, et al.. (2014). Ionized gas discs in elliptical and S0 galaxies at z < 1. Monthly Notices of the Royal Astronomical Society. 440(4). 3491–3502. 15 indexed citations

5.

Cimatti, A., E. Daddi, M. Mignoli, et al.. (2009). A VLT Large Programme to Study Galaxies at z ~ 2: GMASS — the Galaxy Mass Assembly Ultra-deep Spectroscopic Survey. Max Planck Institute for Plasma Physics. 135(135). 40–44. 1 indexed citations

6.

Lucia, G. De, Bianca M. Poggianti, Claire Halliday, et al.. (2009). On the role of the post-starburst phase in the buildup of the red sequence of intermediate-redshift clusters. Monthly Notices of the Royal Astronomical Society. 400(1). 68–77. 19 indexed citations

7.

Poggianti, Bianca M., Vandana Desai, Rose Finn, et al.. (2008). The Relation between Star Formation, Morphology, and Local Density in High‐Redshift Clusters and Groups. The Astrophysical Journal. 684(2). 888–904. 89 indexed citations

8.

Poggianti, Bianca M., Anja von der Linden, G. De Lucia, et al.. (2006). The Evolution of the Star Formation Activity in Galaxies and Its Dependence on Environment. The Astrophysical Journal. 642(1). 188–215. 174 indexed citations

9.

Finn, Rose, Dennis Zaritsky, Bianca M. Poggianti, et al.. (2005). Hα‐derived Star Formation Rates for Threez≃0.75 EDisCS Galaxy Clusters. The Astrophysical Journal. 630(1). 206–227. 102 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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