U. Haud

2.3k total citations · 1 hit paper
26 papers, 1.4k citations indexed

About

U. Haud is a scholar working on Astronomy and Astrophysics, Instrumentation and Oceanography. According to data from OpenAlex, U. Haud has authored 26 papers receiving a total of 1.4k indexed citations (citations by other indexed papers that have themselves been cited), including 23 papers in Astronomy and Astrophysics, 7 papers in Instrumentation and 4 papers in Oceanography. Recurrent topics in U. Haud's work include Stellar, planetary, and galactic studies (14 papers), Astrophysics and Star Formation Studies (12 papers) and Astronomy and Astrophysical Research (7 papers). U. Haud is often cited by papers focused on Stellar, planetary, and galactic studies (14 papers), Astrophysics and Star Formation Studies (12 papers) and Astronomy and Astrophysical Research (7 papers). U. Haud collaborates with scholars based in Estonia, Germany and Netherlands. U. Haud's co-authors include P. M. W. Kalberla, L. Dedes, J. Kerp, H. Alyson Ford, F. J. Lockman, M. R. Calabretta, N. Ben Bekhti, H. Nakanishi, Reinhard Keller and L. Flöer and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Astrophysics and Space Science.

In The Last Decade

U. Haud

23 papers receiving 1.3k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

HI4PI: a full-sky H i survey based on EBHIS and GASS

2016 853 citations N. Ben Bekhti, L. Flöer et al. Astronomy and Astrophysics profile →

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
U. Haud Estonia	11	1.3k	432	99	49	45	26	1.4k
L. Dedes Germany	8	1.5k 1.1×	492 1.1×	121 1.2×	43 0.9×	41 0.9×	12	1.5k
J. Kerp Germany	16	1.4k 1.0×	482 1.1×	113 1.1×	48 1.0×	32 0.7×	31	1.4k
F. J. Lockman Australia	3	917 0.7×	358 0.8×	54 0.5×	43 0.9×	23 0.5×	4	959
M. Kidger Spain	19	1.1k 0.8×	281 0.7×	114 1.2×	34 0.7×	42 0.9×	90	1.1k
V. Piirola Finland	19	874 0.7×	210 0.5×	83 0.8×	48 1.0×	12 0.3×	100	929
S. L. Snowden United States	20	1.3k 0.9×	471 1.1×	71 0.7×	32 0.7×	9 0.2×	44	1.3k
D. A. Grabelsky United States	16	794 0.6×	412 1.0×	43 0.4×	36 0.7×	25 0.6×	43	854
O. González-Martín Spain	24	1.8k 1.3×	524 1.2×	258 2.6×	24 0.5×	28 0.6×	94	1.8k
F. M. Walter United States	20	1.5k 1.1×	115 0.3×	291 2.9×	39 0.8×	86 1.9×	84	1.5k
V. D’Elia Italy	23	1.8k 1.3×	528 1.2×	172 1.7×	16 0.3×	125 2.8×	125	1.8k

Countries citing papers authored by U. Haud

Since Specialization

Citations

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

Fields of papers citing papers by U. Haud

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of U. Haud

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

20 of 20 papers shown

1.

Kalberla, P. M. W., J. Kerp, & U. Haud. (2020). H I filaments are cold and associated with dark molecular gas. Astronomy and Astrophysics. 639. A26–A26. 29 indexed citations

2.

Kalberla, P. M. W. & U. Haud. (2019). Turbulent power distribution in the local interstellar medium. Astronomy and Astrophysics. 627. A112–A112. 9 indexed citations

3.

Ghosh, T., F. Boulanger, P. G. Martin, et al.. (2017). Modelling and simulation of large-scale polarized dust emission over the southern Galactic cap using the GASS Hi data. Astronomy and Astrophysics. 601. A71–A71. 17 indexed citations

4.

Kalberla, P. M. W., J. Kerp, U. Haud, & M. Haverkorn. (2017). H i anisotropies associated with radio-polarimetric filaments. Astronomy and Astrophysics. 607. A15–A15. 18 indexed citations

5.

Kalberla, P. M. W., J. Kerp, U. Haud, & M. Haverkorn. (2017). HI anisotropies associated with radio-polarimetric filaments. Steep power spectra associated with cold gas. arXiv (Cornell University). 10 indexed citations

6.

Bekhti, N. Ben, L. Flöer, Reinhard Keller, et al.. (2016). HI4PI: a full-sky H i survey based on EBHIS and GASS. Astronomy and Astrophysics. 594. A116–A116. 853 indexed citations breakdown →

7.

Kalberla, P. M. W. & U. Haud. (2015). GASS: The Parkes Galactic All-Sky Survey. Astronomy and Astrophysics. 578. A78–A78. 98 indexed citations

8.

Kalberla, P. M. W. & U. Haud. (2015). GASS: The Parkes Galactic All-Sky Survey. Update: improved correction for instrumental effects and new data release. arXiv (Cornell University). 48 indexed citations

9.

Haud, U.. (2010). Gaussian decomposition of $\ion{H}{i}$ surveys. Astronomy and Astrophysics. 514. A27–A27. 15 indexed citations

10.

Haud, U.. (2008). Gaussian decomposition of H I surveys. Astronomy and Astrophysics. 483(2). 461–469. 8 indexed citations

11.

Kalberla, P. M. W., L. Dedes, J. Kerp, & U. Haud. (2007). Dark matter in the Milky Way. Astronomy and Astrophysics. 469(2). 511–527. 107 indexed citations

12.

Kalberla, P. M. W., L. Dedes, J. Kerp, & U. Haud. (2007). Dark matter in the Milky Way, II. the HI gas distribution as a tracer of the gravitational potential. ArXiv.org. 94 indexed citations

13.

Kalberla, P. M. W. & U. Haud. (2006). Global properties of the HI high velocity sky. Astronomy and Astrophysics. 455(2). 481–498. 5 indexed citations

14.

Kalberla, P. M. W. & U. Haud. (2006). Global properties of the HI high velocity sky, a statistical investigation based on the LAB survey. ArXiv.org. 30 indexed citations

15.

Haud, U.. (1992). Dynamics of the Outer Arm high-velocity cloud and the triaxiality of the Milky Way. Monthly Notices of the Royal Astronomical Society. 257(4). 707–714. 7 indexed citations

16.

Tenjes, P., J. Einasto, & U. Haud. (1991). Galactic models with massive coronae. III - Giant elliptical galaxy M 87. 248(2). 395–403.

17.

Einasto, J. & U. Haud. (1989). Galactic models with massive corona. I - Method. II - Galaxy. A&A. 223. 89–106. 8 indexed citations

18.

Haud, U.. (1986). Our Galaxy - A polar ring galaxy?. 198. 125–134. 2 indexed citations

19.

Haud, U.. (1984). Rotation curve of our Galaxy forR>R o. Astrophysics and Space Science. 104(2). 337–345. 1 indexed citations

20.

Einasto, J., U. Haud, M. Jõeveer, & Ants Kaasik. (1976). The Magellanic Stream and the mass of our Hypergalaxy. Monthly Notices of the Royal Astronomical Society. 177(2). 357–375. 12 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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