H. Pablo

1.7k total citations
36 papers, 720 citations indexed

About

H. Pablo is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, H. Pablo has authored 36 papers receiving a total of 720 indexed citations (citations by other indexed papers that have themselves been cited), including 36 papers in Astronomy and Astrophysics, 8 papers in Instrumentation and 5 papers in Computational Mechanics. Recurrent topics in H. Pablo's work include Stellar, planetary, and galactic studies (34 papers), Astrophysics and Star Formation Studies (27 papers) and Astro and Planetary Science (16 papers). H. Pablo is often cited by papers focused on Stellar, planetary, and galactic studies (34 papers), Astrophysics and Star Formation Studies (27 papers) and Astro and Planetary Science (16 papers). H. Pablo collaborates with scholars based in Canada, United States and Poland. H. Pablo's co-authors include A. F. J. Moffat, K. Hambleton, Kyle E. Conroy, P. Degroote, J. Giammarco, Martin Horvat, S. Bloemen, G. Handler, G. A. Wade and Adam Popowicz and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

H. Pablo

33 papers receiving 667 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. Pablo Canada 14 701 256 65 37 19 36 720
K. Zwintz Austria 16 707 1.0× 285 1.1× 60 0.9× 27 0.7× 21 1.1× 66 738
M.-A. Dupret Belgium 15 700 1.0× 333 1.3× 47 0.7× 37 1.0× 17 0.9× 26 719
Chun‐Hwey Kim South Korea 16 923 1.3× 290 1.1× 64 1.0× 32 0.9× 27 1.4× 65 950
Boonrucksar Soonthornthum Thailand 16 824 1.2× 232 0.9× 56 0.9× 41 1.1× 44 2.3× 68 848
M. E. Shultz United States 20 1.1k 1.6× 172 0.7× 118 1.8× 19 0.5× 10 0.5× 77 1.1k
K. A. Carroll Canada 6 344 0.5× 146 0.6× 24 0.4× 11 0.3× 17 0.9× 23 377
K. Hambleton United States 11 533 0.8× 228 0.9× 49 0.8× 24 0.6× 9 0.5× 25 556
A. F. Gulliver Canada 14 563 0.8× 232 0.9× 78 1.2× 15 0.4× 38 2.0× 44 590
C. Tycner United States 16 602 0.9× 178 0.7× 61 0.9× 26 0.7× 93 4.9× 49 635
Jeffrey W. Percival United States 5 293 0.4× 114 0.4× 36 0.6× 16 0.4× 36 1.9× 15 351

Countries citing papers authored by H. Pablo

Since Specialization
Citations

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

Fields of papers citing papers by H. Pablo

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of H. Pablo. A scholar is included among the top collaborators of H. Pablo 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. Pablo. H. Pablo 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.
Richardson, Noel D., et al.. (2025). An Investigation into the Variability of Luminous Blue Variable Stars with TESS. The Astronomical Journal. 169(3). 128–128. 2 indexed citations
2.
Richardson, Noel D., J. J. Eldridge, H. Pablo, et al.. (2023). A high-mass X-ray binary descended from an ultra-stripped supernova. Nature. 614(7946). 45–47. 11 indexed citations
3.
Pétit, V., Yaël Nazé, M. F. Corcoran, et al.. (2023). Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system ϵ Lupi. Monthly Notices of the Royal Astronomical Society. 522(4). 5805–5827. 5 indexed citations
4.
Richardson, Noel D., A. F. J. Moffat, André-Nicolas Chené, et al.. (2023). The orbital kinematics of η Carinae over three periastra with a possible detection of the elusive secondary’s motion. Monthly Notices of the Royal Astronomical Society. 519(4). 5882–5892. 4 indexed citations
5.
Mayer, P., P. Harmanec, M. Brož, et al.. (2023). Spectrum of the secondary component and new orbital elements of the massive triple star δ Ori A. Astronomy and Astrophysics. 672. A31–A31. 2 indexed citations
6.
David-Uraz, Alexandre, M. E. Shultz, V. Pétit, et al.. (2021). MOBSTER – IV. Detection of a new magnetic B-type star from follow-up spectropolarimetric observations of photometrically selected candidates★. Monthly Notices of the Royal Astronomical Society. 504(4). 4841–4849. 6 indexed citations
7.
St‐Louis, Nicole, et al.. (2020). Variability of Wolf-Rayet Stars through MOST(LY) BRITE Eyes. 191–192.
8.
Pablo, H., M. E. Shultz, Jim Fuller, et al.. (2019). ϵ Lupi: measuring the heartbeat of a doubly magnetic massive binary with BRITE Constellation. Monthly Notices of the Royal Astronomical Society. 488(1). 64–77. 16 indexed citations
9.
Baade, D., A. Pigulski, Th. Rivinius, et al.. (2018). Short-term variability and mass loss in Be stars. Astronomy and Astrophysics. 620. A145–A145. 16 indexed citations
10.
Baade, D., A. Pigulski, Th. Rivinius, et al.. (2018). Short-term variability and mass loss in Be stars. Astronomy and Astrophysics. 610. A70–A70. 19 indexed citations
11.
Richardson, Noel D., H. Pablo, C. Sterken, et al.. (2018). BRITE-Constellation reveals evidence for pulsations in the enigmatic binary η Carinae. Monthly Notices of the Royal Astronomical Society. 475(4). 5417–5423. 10 indexed citations
12.
Kallinger, T., W. W. Weiß, P. G. Beck, et al.. (2017). Triple system HD 201433 with a SPB star component seen by BRITE - Constellation: Pulsation, differential rotation, and angular momentum transfer. Astronomy and Astrophysics. 603. A13–A13. 28 indexed citations
13.
Pablo, H., Noel D. Richardson, Jim Fuller, et al.. (2017). The most massive heartbeat: an in-depth analysis of ι Orionis. Monthly Notices of the Royal Astronomical Society. 467(2). 2494–2503. 27 indexed citations
14.
Shenar, T., R. Hainich, H. Todt, et al.. (2016). Wolf-Rayet stars in the Small Magellanic Cloud. Astronomy and Astrophysics. 591. A22–A22. 67 indexed citations
15.
Pigulski, A., Adam Popowicz, R. Kuschnig, et al.. (2016). Massive pulsating stars observed by BRITE-Constellation. Astronomy and Astrophysics. 588. A55–A55. 26 indexed citations
16.
Baade, D., Th. Rivinius, A. Pigulski, et al.. (2016). Short-term variability and mass loss in Be stars. Astronomy and Astrophysics. 588. A56–A56. 48 indexed citations
17.
Pigulski, A., Adam Popowicz, R. Kuschnig, et al.. (2016). Massive pulsating stars observed by BRITE-Constellation - I. The triple system β Centauri (Agena). 588(55). 23 indexed citations
18.
Baade, D., Th. Rivinius, A. Pigulski, et al.. (2016). Short-term variability and mass loss in Be stars I. BRITE satellite photometry of $η$ and $μ$ Centauri. arXiv (Cornell University). 22 indexed citations
19.
Moffat, A. F. J., Grant M. Hill, T. Shenar, et al.. (2016). WR 148: Identifying the companion of an extreme runaway massive binary. Monthly Notices of the Royal Astronomical Society. stw2283–stw2283. 6 indexed citations
20.
Nichols, Joy S., M. F. Corcoran, W. L. Waldron, et al.. (2015). A COORDINATED X-RAY AND OPTICAL CAMPAIGN OF THE NEAREST MASSIVE ECLIPSING BINARY, δ ORIONIS Aa. II. X-RAY VARIABILITY. DSpace@MIT (Massachusetts Institute of Technology). 8 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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