H. Dole

55.5k total citations
60 papers, 2.7k citations indexed

About

H. Dole is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, H. Dole has authored 60 papers receiving a total of 2.7k indexed citations (citations by other indexed papers that have themselves been cited), including 54 papers in Astronomy and Astrophysics, 31 papers in Instrumentation and 9 papers in Nuclear and High Energy Physics. Recurrent topics in H. Dole's work include Galaxies: Formation, Evolution, Phenomena (49 papers), Astronomy and Astrophysical Research (31 papers) and Astrophysics and Star Formation Studies (21 papers). H. Dole is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (49 papers), Astronomy and Astrophysical Research (31 papers) and Astrophysics and Star Formation Studies (21 papers). H. Dole collaborates with scholars based in France, United States and United Kingdom. H. Dole's co-authors include G. Lagache, J.‐L. Puget, G. H. Rieke, Pablo G. Pérez‐González, Casey Papovich, E. Le Floc’h, Myra Blaylock, Eiichi Egami, A. Alonso‐Herrero and K. I. Caputi and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

H. Dole

57 papers receiving 2.6k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
H. Dole France 24 2.6k 1.3k 538 80 66 60 2.7k
S. Savaglio Germany 31 2.8k 1.1× 1.1k 0.9× 357 0.7× 76 0.9× 40 0.6× 76 2.9k
M. Sargent United Kingdom 30 2.9k 1.1× 1.3k 1.0× 462 0.9× 64 0.8× 42 0.6× 90 3.0k
D. H. Hughes United States 28 2.8k 1.1× 937 0.7× 933 1.7× 84 1.1× 54 0.8× 83 2.8k
Alexandra Pope United States 26 3.2k 1.2× 1.5k 1.2× 449 0.8× 61 0.8× 58 0.9× 75 3.2k
Eric Gawiser United States 33 3.0k 1.2× 1.2k 0.9× 572 1.1× 97 1.2× 112 1.7× 90 3.1k
C. Gronwall United States 27 2.5k 1.0× 1.3k 1.0× 410 0.8× 125 1.6× 120 1.8× 129 2.5k
G. Rodighiero Italy 30 2.9k 1.1× 1.4k 1.1× 830 1.5× 97 1.2× 62 0.9× 91 3.0k
D. T. Frayer United States 31 3.7k 1.4× 1.6k 1.2× 555 1.0× 75 0.9× 74 1.1× 89 3.8k
Helmut Jerjen Australia 36 3.7k 1.4× 2.0k 1.5× 459 0.9× 94 1.2× 35 0.5× 112 3.8k
P. Barmby United States 30 2.9k 1.1× 1.3k 1.0× 361 0.7× 68 0.8× 39 0.6× 94 2.9k

Countries citing papers authored by H. Dole

Since Specialization
Citations

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

Fields of papers citing papers by H. Dole

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of H. Dole

This figure shows the co-authorship network connecting the top 25 collaborators of H. Dole. A scholar is included among the top collaborators of H. Dole 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 H. Dole. H. Dole 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.
Li, Qiong, Christopher J. Conselice, Florian Sarron, et al.. (2025). EPOCHS paper – X. Environmental effects on Galaxy formation and protocluster Galaxy candidates at 4.5 < z < 10 from JWST observations. Monthly Notices of the Royal Astronomical Society. 539(2). 1796–1819. 3 indexed citations
2.
Polletta, M., et al.. (2022). Molecular gas properties of Planck-selected protocluster candidates at z ≃ 1.3–3. Astronomy and Astrophysics. 662. A85–A85. 6 indexed citations
3.
Pascale, Massimo, Brenda Frye, Liang Dai, et al.. (2022). Possible Ongoing Merger Discovered by Photometry and Spectroscopy in the Field of the Galaxy Cluster PLCK G165.7+67.0. arXiv (Cornell University). 6 indexed citations
4.
Aghanim, N., et al.. (2022). Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate. Astronomy and Astrophysics. 664. A155–A155. 7 indexed citations
5.
Polletta, M., G. Soucail, H. Dole, et al.. (2021). Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field. Astronomy and Astrophysics. 654. A121–A121. 29 indexed citations
6.
Boucaud, A., Caroline Heneka, Émille E. O. Ishida, et al.. (2019). Photometry of high-redshift blended galaxies using deep learning. Monthly Notices of the Royal Astronomical Society. 491(2). 2481–2495. 40 indexed citations
7.
Flores-Cacho, I., D. Pierini, G. Soucail, et al.. (2015). Multi-wavelength characterisation ofz~ 2 clustered, dusty star-forming galaxies discovered byPlanck. Astronomy and Astrophysics. 585. A54–A54. 15 indexed citations
8.
Béthermin, M., et al.. (2013). FASTPHOT: A simple and quick IDL PSF-fitting routine. Astrophysics Source Code Library. 1 indexed citations
9.
Béthermin, M., H. Dole, G. Lagache, D. Le Borgne, & Aurélie Pénin. (2011). Modeling the evolution of infrared galaxies: a parametric backward evolution model. Astronomy and Astrophysics. 529. A4–A4. 57 indexed citations
10.
Kneiske, T. & H. Dole. (2010). A lower-limit flux for the extragalactic background light. Springer Link (Chiba Institute of Technology). 74 indexed citations
11.
Jauzac, Mathilde, H. Dole, E. Le Floc’h, et al.. (2010). The cosmic far-infrared background buildup since redshift 2 at 70 and 160 microns in the COSMOS and GOODS fields. Astronomy and Astrophysics. 525. A52–A52. 20 indexed citations
12.
Fernández-Conde, N., G. Lagache, J.‐L. Puget, & H. Dole. (2010). Simulations of the cosmic infrared and submillimeter background for future large surveys. Astronomy and Astrophysics. 515. A48–A48. 4 indexed citations
13.
Béthermin, M., et al.. (2010). Submillimeter number counts at 250 μm, 350 μm and 500 μm in BLAST data. Astronomy and Astrophysics. 516. A43–A43. 27 indexed citations
14.
Sirothia, S. K., et al.. (2009). 325-MHz Observations of the ELAIS-N1 Field. ASPC. 407. 27. 1 indexed citations
15.
Beelen, A., A. Omont, N. Bavouzet, et al.. (2008). Submillimeter observations of the J2142-4423 Ly$\sf \alpha$ protocluster at z = 2.38. Astronomy and Astrophysics. 485(3). 645–655. 15 indexed citations
16.
Bavouzet, N., H. Dole, E. Le Floc’h, et al.. (2007). Estimating the total infrared luminosity of galaxies up toz$\mathsf{\sim 2}$ from mid- and far-infrared observations. Astronomy and Astrophysics. 479(1). 83–96. 45 indexed citations
17.
Takeuchi, Tsutomu T., Takako T. Ishii, H. Dole, et al.. (2006). TheISO170 μm luminosity function of galaxies. Astronomy and Astrophysics. 448(2). 525–534. 18 indexed citations
18.
Caputi, K. I., H. Dole, G. Lagache, et al.. (2006). The role of the LIRG and ULIRG phases in the evolution of K$\mathsf{_{s}}$-selected galaxies. Astronomy and Astrophysics. 454(1). 143–150. 20 indexed citations
19.
Elbaz, D., E. Le Floc’h, H. Dole, & D. Marcillac. (2005). Observational evidence for the presence of PAHs in distant Luminous Infrared Galaxies using ISO and Spitzer. Astronomy and Astrophysics. 434(1). L1–L4. 16 indexed citations
20.
Dennefeld, M., et al.. (2003). Spectroscopic follow-up of FIRBACK-South bright galaxies. Astronomy and Astrophysics. 412(2). 349–371. 11 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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