S. Khan

79.6k citations
143 papers · 56.7k · 38 hit papers · h-index 77

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 139
    • Gamma-ray bursts and supernovae 86
    • Astrophysical Phenomena and Observations 49
    • Cosmology and Gravitation Theories 30
    • Geophysics and Gravity Measurements 26

S. Khan

140 papers receiving 54.7k citations

S. Khan's Hit Papers

Tests of general relativity with GWTC-3 2025 · 60 citations
600+2+4Years since publication50010001.5k2.0k2.5k

Peers

S. Khan
Comparison fields: 5 of 159
  • Astronomy and Astrophysics 52.4k
  • Nuclear and High Energy Physics 18.3k
  • Geophysics 6.4k
  • Oceanography 5.9k
  • Ocean Engineering 2.7k
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Citations per field
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Citations per year

Countries citing papers authored by S. Khan

Since Specialization
Citations

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

Fields of papers citing papers by S. Khan

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authors

The 25 scholars most cited alongside S. Khan, 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 S. Khan Line = papers co-authored together S. Khan links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown

Showing the 20 most-cited of 143 papers — load more, or switch the sort, to bring in the rest.

#Work
1
Observation of Gravitational Waves from a Binary Black Hole Merger
Hit paper breakdown →
20169808
2
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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20176925
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
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
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20172443
6
GW170817: Measurements of Neutron Star Radii and Equation of State
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20181847
7
GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
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20171776
8
GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
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20171499
9
Tests of General Relativity with GW150914
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20161320
10
GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M ⊙
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20201268
11
GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run
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20231246
12
GW190521: A Binary Black Hole Merger with a Total Mass of 150 M ⊙
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20201022
13
Properties of the Binary Neutron Star Merger GW170817
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2019990
14
Exploring the sensitivity of next generation gravitational wave detectors
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2017920
15
A gravitational-wave standard siren measurement of the Hubble constant
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2017894
16
GW170608: Observation of a 19 Solar-mass Binary Black Hole Coalescence
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2017881
17
Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA
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2018865
18
Frequency-domain gravitational waves from nonprecessing black-hole binaries. II. A phenomenological model for the advanced detector era
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2016844
19
Properties of the Binary Black Hole Merger GW150914
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2016733
20
Population Properties of Compact Objects from the Second LIGO–Virgo Gravitational-Wave Transient Catalog
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2021730

About S. Khan

S. Khan is a scholar working on Astronomy and Astrophysics, Oceanography, Geophysics, Nuclear and High Energy Physics and Ocean Engineering, having authored 143 papers that have together received 56.7k indexed citations. Recurring topics across this work include Pulsars and Gravitational Waves Research (139 papers), Gamma-ray bursts and supernovae (86 papers), Astrophysical Phenomena and Observations (49 papers), Cosmology and Gravitation Theories (30 papers), Geophysics and Gravity Measurements (26 papers), Astrophysics and Cosmic Phenomena (15 papers), High-pressure geophysics and materials (13 papers) and Geophysics and Sensor Technology (10 papers). The work is most often cited by research in Astronomy and Astrophysics (52.4k citations), Nuclear and High Energy Physics (18.3k citations), Geophysics (6.4k citations), Oceanography (5.9k citations) and Ocean Engineering (2.7k citations). S. Khan has collaborated with scholars based in United States, Germany and France. Frequent co-authors include Mark Hannam, Frank Ohme, Sascha Husa, Michael Pürrer, Xisco Jiménez Forteza, A. Bohé, Katerina Chatziioannou, Tim Dietrich, Francesco Pannarale and Reetika Dudi. Their work appears in journals such as Physical review. D, Physical Review Letters, The Astrophysical Journal, The Astrophysical Journal 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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