K. Haris

52.3k citations
125 papers · 37.5k · 27 hit papers · h-index 60

Impact in

    • Pulsars and Gravitational Waves Research
    • Gamma-ray bursts and supernovae
    • Cosmology and Gravitation Theories
    • Astrophysical Phenomena and Observations
    • Black Holes and Theoretical Physics
    • Astrophysics and Cosmic Phenomena

Papers in

    • Pulsars and Gravitational Waves Research 125
    • Gamma-ray bursts and supernovae 67
    • Astrophysical Phenomena and Observations 37
    • Cosmology and Gravitation Theories 24
    • Geophysics and Gravity Measurements 22

K. Haris

124 papers receiving 36.0k citations

K. Haris's Hit Papers

GW231123: A Binary Black Hole Merger with Total Mass 190–265 M ⊙ 2025 · 78 citations
780+2+4Years since publication4008001.2k

Peers

K. Haris
Comparison fields: 5 of 140
  • Astronomy and Astrophysics 33.5k
  • Nuclear and High Energy Physics 11.3k
  • Geophysics 4.0k
  • Oceanography 3.6k
  • Ocean Engineering 2.2k
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Citations per field
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M. Tse · 1×
Citations per year

Countries citing papers authored by K. Haris

Since Specialization
Citations

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

Fields of papers citing papers by K. Haris

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authors

The 23 scholars most cited alongside K. Haris, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with K. Haris Line = papers co-authored together K. Haris links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown

Showing the 20 most-cited of 125 papers — load more, or switch the sort, to bring in the rest.

#Work
1
Observation of Gravitational Waves from a Binary Black Hole Merger
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20169808
2
Advanced LIGO
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20152689
3
GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
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20192661
4
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
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20162488
5
GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M ⊙
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20201268
6
GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run
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20231246
7
GW190521: A Binary Black Hole Merger with a Total Mass of 150 M ⊙
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20201022
8
Characterization of the LIGO detectors during their sixth science run
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2015968
9
Exploring the sensitivity of next generation gravitational wave detectors
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2017920
10
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light
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2013843
11
Properties of the Binary Black Hole Merger GW150914
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2016733
12
Population Properties of Compact Objects from the Second LIGO–Virgo Gravitational-Wave Transient Catalog
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2021730
13
Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3
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2023729
14
Tests of general relativity with the binary black hole signals from the LIGO-Virgo catalog GWTC-1
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2019637
15
Binary Black Hole Mergers in the first Advanced LIGO Observing Run
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2016629
16
Tests of general relativity with binary black holes from the second LIGO-Virgo gravitational-wave transient catalog
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2021604
17
ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914
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2016576
18
GW150914: The Advanced LIGO Detectors in the Era of First Discoveries
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2016540
19
Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences
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2021538
20
GW190412: Observation of a binary-black-hole coalescence with asymmetric masses
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2020508

About K. Haris

K. Haris is a scholar working on Astronomy and Astrophysics, Oceanography, Nuclear and High Energy Physics, Geophysics and Atomic and Molecular Physics, and Optics, having authored 125 papers that have together received 37.5k indexed citations. Recurring topics across this work include Pulsars and Gravitational Waves Research (125 papers), Gamma-ray bursts and supernovae (67 papers), Astrophysical Phenomena and Observations (37 papers), Cosmology and Gravitation Theories (24 papers), Geophysics and Gravity Measurements (22 papers), Astrophysics and Cosmic Phenomena (14 papers), Geophysics and Sensor Technology (10 papers) and Seismic Waves and Analysis (8 papers). The work is most often cited by research in Astronomy and Astrophysics (33.5k citations), Nuclear and High Energy Physics (11.3k citations), Geophysics (4.0k citations), Oceanography (3.6k citations) and Ocean Engineering (2.2k citations). K. Haris has collaborated with scholars based in United States, Germany and France. Frequent co-authors include Ajit Kumar Mehta, Parameswaran Ajith, Otto Akseli Hannuksela, Justin Janquart, David Keitel, Ken K. Y. Ng, Sumit Kumar, Tjonnie Guang Feng Li, Srashti Gopal Goyal and Chris Van Den Broeck. Their work appears in journals such as Physical review. D, The Astrophysical Journal, The Astrophysical Journal Letters, Physical Review Letters and Classical and Quantum Gravity.

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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