B. Holden

8.8k total citations · 2 hit papers
79 papers, 3.3k citations indexed

About

B. Holden is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, B. Holden has authored 79 papers receiving a total of 3.3k indexed citations (citations by other indexed papers that have themselves been cited), including 74 papers in Astronomy and Astrophysics, 43 papers in Instrumentation and 6 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in B. Holden's work include Galaxies: Formation, Evolution, Phenomena (57 papers), Astronomy and Astrophysical Research (43 papers) and Stellar, planetary, and galactic studies (32 papers). B. Holden is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (57 papers), Astronomy and Astrophysical Research (43 papers) and Stellar, planetary, and galactic studies (32 papers). B. Holden collaborates with scholars based in United States, Germany and Netherlands. B. Holden's co-authors include G. D. Illingworth, Marijn Franx, R. J. Bouwens, Pieter van Dokkum, D. Magee, P. Rosati, S. A. Stanford, Pascal A. Oesch, Ivo Labbé and Arjen van der Wel and has published in prestigious journals such as The Astrophysical Journal, ACS Applied Materials & Interfaces and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

B. Holden

70 papers receiving 3.2k citations

Hit Papers

Confirmation of the Remarkable Compactness of Massive Qui... 2008 2026 2014 2020 2008 2016 100 200 300

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
B. Holden United States 34 3.2k 1.8k 462 160 113 79 3.3k
Daniel D. Kelson United States 34 3.7k 1.2× 1.8k 1.0× 493 1.1× 149 0.9× 95 0.8× 77 3.7k
C. Lidman United States 32 2.8k 0.9× 1.3k 0.8× 522 1.1× 193 1.2× 78 0.7× 130 3.0k
O. Le Fèvre France 32 3.4k 1.1× 1.8k 1.0× 542 1.2× 194 1.2× 164 1.5× 90 3.5k
Michael D. Gladders United States 30 2.6k 0.8× 1.3k 0.7× 377 0.8× 208 1.3× 110 1.0× 102 2.7k
Pablo G. Pérez‐González Spain 35 4.6k 1.5× 2.4k 1.4× 723 1.6× 144 0.9× 111 1.0× 137 4.7k
Klaus Meisenheimer Germany 22 2.6k 0.8× 1.5k 0.9× 420 0.9× 122 0.8× 129 1.1× 43 2.7k
R. M. González Delgado Spain 40 4.4k 1.4× 1.8k 1.0× 501 1.1× 151 0.9× 127 1.1× 123 4.5k
D. Magee United States 30 3.2k 1.0× 1.9k 1.1× 417 0.9× 153 1.0× 55 0.5× 47 3.2k
D. Burgarella France 27 3.0k 0.9× 1.3k 0.8× 413 0.9× 117 0.7× 136 1.2× 89 3.1k
Norman A. Grogin United States 43 4.3k 1.4× 2.2k 1.2× 792 1.7× 182 1.1× 127 1.1× 107 4.4k

Countries citing papers authored by B. Holden

Since Specialization
Citations

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

Fields of papers citing papers by B. Holden

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of B. Holden

This figure shows the co-authorship network connecting the top 25 collaborators of B. Holden. A scholar is included among the top collaborators of B. Holden 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 B. Holden. B. Holden 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
3.
Lubin, Dan, et al.. (2024). Hamilton Echelle Spectrograph Observations of Solar Analog Field Stars: Lithium Abundance and Activity. The Astronomical Journal. 168(6). 240–240.
4.
Hinz, Philip M., B. Holden, Maureen L. Savage, et al.. (2024). Keck adaptive secondary mirror overview. eScholarship (California Digital Library). 97–97.
5.
Barrufet, Laia, Pascal A. Oesch, Andrea Weibel, et al.. (2023). Unveiling the nature of infrared bright, optically dark galaxies with early JWST data. Monthly Notices of the Royal Astronomical Society. 522(1). 449–456. 41 indexed citations
6.
Feng, Fabo, et al.. (2023). Revised orbits of the two nearest Jupiters. Monthly Notices of the Royal Astronomical Society. 525(1). 607–619. 12 indexed citations
7.
Wang, Songhu, Jennifer Burt, Malena Rice, et al.. (2022). Revisiting the Full Sets of Orbital Parameters for the XO-3 System: No Evidence for Temporal Variation of the Spin–Orbit Angle. The Astronomical Journal. 163(4). 158–158. 4 indexed citations
8.
Morselli, L., P. Popesso, A. Cibinel, et al.. (2019). Spatial distribution of stellar mass and star formation activity at 0.2 < z < 1.2 across and along the main sequence. Astronomy and Astrophysics. 626. A61–A61. 23 indexed citations
9.
Millholland, Sarah, Gregory Laughlin, Johanna Teske, et al.. (2018). New Constraints on Gliese 876—Exemplar of Mean-motion Resonance. The Astronomical Journal. 155(3). 106–106. 25 indexed citations
10.
Reddy, Naveen A., Pascal A. Oesch, R. J. Bouwens, et al.. (2018). The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies. The Astrophysical Journal. 853(1). 56–56. 125 indexed citations
11.
Naidu, Rohan P., Pascal A. Oesch, Naveen A. Reddy, et al.. (2017). The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ∼ 2 Revealed by HST UV Imaging*. The Astrophysical Journal. 847(1). 12–12. 26 indexed citations
12.
Vogt, Steven S., R. Paul Butler, Jennifer Burt, et al.. (2017). A Six-planet System around the Star HD 34445. The Astronomical Journal. 154(5). 181–181. 5 indexed citations
13.
Butler, R. Paul, Steven S. Vogt, Gregory Laughlin, et al.. (2017). The LCES HIRES/Keck Precision Radial Velocity Exoplanet Survey. The Astronomical Journal. 153(5). 208–208. 113 indexed citations
14.
Roberts-Borsani, Guido, R. J. Bouwens, Pascal A. Oesch, et al.. (2016). z? 7 galazies with red spitzer/IRAC [3.6]–[4.5] colors in the full CANDELS data set: the brightest-known galaxies at z~ 7–9 and a probable spectroscopic confirmation atz= 7.48. Figshare. 140 indexed citations
15.
Mei, S., S. A. Stanford, B. Holden, et al.. (2012). EARLY-TYPE GALAXIES ATz= 1.3. I. THE LYNX SUPERCLUSTER: CLUSTER AND GROUPS ATz= 1.3. MORPHOLOGY AND COLOR-MAGNITUDE RELATION. The Astrophysical Journal. 754(2). 141–141. 40 indexed citations
16.
Wel, Arjen van der, Hans‐Walter Rix, B. Holden, Eric F. Bell, & Aday R. Robaina. (2009). MAJOR MERGING: THE WAY TO MAKE A MASSIVE, PASSIVE GALAXY. The Astrophysical Journal. 706(1). L120–L123. 45 indexed citations
17.
Prochaska, J. X., et al.. (2008). GRB 080310: redshift from Keck/DEIMOS spectra.. GCN. 7397. 1. 1 indexed citations
18.
Adami, C., M. P. Ulmer, F. Durret, et al.. (2007). An extension of the SHARC survey. Astronomy and Astrophysics. 472(2). 373–381.
19.
Fosbury, R. A. E., M. Villar-Martı́n, A. Humphrey, et al.. (2003). Massive Star Formation in a Gravitationally Lensed HiiGalaxy atz= 3.357. The Astrophysical Journal. 596(2). 797–809. 70 indexed citations
20.
Stanford, S. A., B. Holden, P. Rosati, et al.. (2002). An X-Ray–Selected Galaxy Cluster at [ITAL][CLC]z[/CLC][/ITAL] = 1.11 in the [ITAL]ROSAT[/ITAL] Deep Cluster Survey. The Astronomical Journal. 123(2). 619–626. 37 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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