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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 103 1499 1421 789 736 317 37366

Kartik Sheth publications per year

The chart shows the history of publications by Kartik Sheth between 1998 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Kartik Sheth published across 28 years, from 1998 to 2025, averaging 12.1 papers a year. Output peaked at 47 publications in 2015. 13 of the 339 publications appeared in the last two years.

No. of publications
10 20 30 40
Bar chart. Horizontal axis: year, 1998 to 2025. Vertical axis: number of publications, 0 to 47. Peak 47 publications in 2015. 1998: 2 publications 1999: 7 publications 2000: 4 publications 2001: 6 publications 2002: 4 publications 2003: 6 publications 2004: 7 publications 2005: 13 publications 2006: 18 publications 2007: 21 publications 2008: 14 publications 2009: 15 publications 2010: 9 publications 2011: 7 publications 2012: 23 publications 2013: 21 publications 2014: 23 publications 2015: 47 publications 2016: 13 publications 2017: 13 publications 2018: 12 publications 2019: 9 publications 2020: 12 publications 2021: 11 publications 2022: 6 publications 2023: 3 publications 2024: 8 publications 2025: 5 publications
1998 2025

339 publications in total across all disciplines

View publications per year as a table
Kartik Sheth: publications per year, 1998 to 2025
Year Publications
1998 2
1999 7
2000 4
2001 6
2002 4
2003 6
2004 7
2005 13
2006 18
2007 21
2008 14
2009 15
2010 9
2011 7
2012 23
2013 21
2014 23
2015 47
2016 13
2017 13
2018 12
2019 9
2020 12
2021 11
2022 6
2023 3
2024 8
2025 5
Total 339
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Kartik Sheth publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Kartik Sheth sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 303–322 publications, is where this scientist sits. 103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103–122 publications 1,469+

This scientist: 317 publications — 21st percentile

21% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31
163–182 35
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136 317
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
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Kartik Sheth D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Kartik Sheth sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 102–103 D-Index, is where this scientist sits. 70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70–71 D-Index 185+

This scientist: 103 D-Index — 60th percentile

60% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153
78–79 144
80–81 167
82–83 167
84–85 166
86–87 132
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97 103
104–105 103
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60
122–123 59
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
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Overview

Kartik Sheth is affiliated with the National Aeronautics and Space Administration in the United States, contributing research primarily in the fields of Physics and Astronomy. Their work spans various subfields including Astronomy and Astrophysics, Instrumentation, General Health Professions, Computational Mechanics, and Philosophy.

The scientist's research covers a range of topics related to galaxies, star formation, and astrophysical phenomena. Key topics of study include:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Gamma-ray bursts and supernovae
  • Astronomical Observations and Instrumentation
  • Hermeneutics and Narrative Identity

Kartik Sheth has published extensively in respected journals and venues. Frequent publication venues include:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Astronomy and Astrophysics
  • Monthly Notices of the Royal Astronomical Society
  • Journal of Astronomical Telescopes Instruments and Systems

Recent papers by the scientist span from 2022 through 2024 and demonstrate a focus on observational astronomy and galaxy characterization. Notable recent publications are:

  • "COSMOS-Web: An Overview of the JWST Cosmic Origins Survey" (2023) in The Astrophysical Journal
  • "Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies" (2022) in The Astrophysical Journal
  • "MHONGOOSE: A MeerKAT nearby galaxy H I survey" (2024) in Astronomy and Astrophysics
  • "Stellar masses, sizes, and radial profiles for 465 nearby early-type galaxies: An extension to the Spitzer survey of stellar structure in Galaxies (S4G)" (2022) in Astronomy and Astrophysics
  • "Unveiling the Distant Universe: Characterizing z ≥ 9 Galaxies in the First Epoch of COSMOS-Web" (2024) in The Astrophysical Journal

Kartik Sheth frequently collaborates with various scientists, including:

  • O. Ilbert
  • Caitlin M. Casey
  • Andreas L. Faisst
  • G. Magdis
  • D. B. Sanders

Best Publications

  • The First Release COSMOS Optical and Near-IR Data and Catalog

    P. Capak;H. Aussel;M. Ajiki;H. J. McCracken

  • Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

    B. T. Draine;D. A. Dale;G. Bendo;K. D. Gordon

  • The Calibration of Mid-Infrared Star Formation Rate Indicators

    D. Calzetti;D. Calzetti;R. C. Kennicutt;C. W. Engelbracht;C. Leitherer

  • The mid-infrared spectrum of star-forming galaxies: Global properties of polycyclic aromatic hydrocarbon emission

    J. D.T. Smith;Bruce T. Draine;D. A. Dale;J. Moustakas

  • The First Release COSMOS Optical and Near-IR Data and Catalog

    P. Capak;H. Aussel;H. Aussel;M. Ajiki;H. J. McCracken;H. J. McCracken

  • The spitzer survey of stellar structure in galaxies (s^4g)

    Kartik Sheth;Kartik Sheth;Michael Regan;Joannah L. Hinz;Armando Gil de Paz

  • S-COSMOS: The Spitzer Legacy Survey of the Hubble Space Telescope ACS 2 deg^2 COSMOS Field I: Survey Strategy and First Analysis

    D. B. Sanders;M. Salvato;H. Aussel;H. Aussel;O. Ilbert

  • COSMOS : Hubble Space Telescope Observations

    N. Scoville;A. Benson;A. W. Blain;D. Calzetti

  • Star Formation in NGC5194 (M51a): The Panchromatic View from GALEX to Spitzer

    D. Calzetti;R. C. Kennicutt;L. Bianchi;D. A. Thilker

  • Star Formation in NGC 5194 (M51a). II. The Spatially Resolved Star Formation Law

    Robert C. Kennicutt;Robert C. Kennicutt;Robert C. Kennicutt;Daniela Calzetti;Daniela Calzetti;Daniela Calzetti;Fabian Walter;George Helou

  • COSMOS: Hubble Space Telescope Observations

    N. Scoville;N. Scoville;R. G. Abraham;H. Aussel;J. E. Barnes

  • The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang

    P.L. Capak;C. Carilli;G. Jones;C. M. Casey

  • Star formation in NGC 5194 (M51a): The Panchromatic view from GALEX to Spitzer

    D. Calzetti;R. C. Kennicutt;L. Bianchi;D. A. Thilker

  • The BIMA Survey of Nearby Galaxies (BIMA SONG). II. The CO Data

    Tamara T. Helfer;Michele D. Thornley;Michael W. Regan;Tony Wong;Tony Wong

  • ISM MASSES AND THE STAR FORMATION LAW AT Z = 1 TO 6: ALMA OBSERVATIONS OF DUST CONTINUUM IN 145 GALAXIES IN THE COSMOS SURVEY FIELD

    N. Scoville;K. Sheth;H. Aussel;P. Vanden Bout

  • Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission

    Peter L. Capak;C. Carilli;C. Carilli;G. Jones;C. M. Casey

  • Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence

    Kartik Sheth;Debra Meloy Elmegreen;Bruce G. Elmegreen;Peter Capak

  • The Bulk of the Black Hole Growth Since z ~ 1 Occurs in a Secular Universe: No Major Merger-AGN Connection

    Mauricio Cisternas;Mauricio Cisternas;Knud Jahnke;Katherine J. Inskip;Jeyhan Kartaltepe

  • THE EVOLUTION OF ISM MASS PROBED BY DUST EMISSION - ALMA OBSERVATIONS AT Z = 0.3 TO 2

    N. Scoville;H. Aussel;K. Sheth;K. S. Scott

  • The BIMA Survey of Nearby Galaxies (BIMA SONG)

    Tamara T. Helfer;Michael W. Regan;Michele D. Thornley;Tony Wong

Frequent Co-Authors

Peter Capak
Peter Capak California Institute of Technology
Nick Scoville
Nick Scoville California Institute of Technology
Eva Schinnerer
Eva Schinnerer Max Planck Society
Luis C. Ho
Luis C. Ho Peking University
E. Athanassoula
E. Athanassoula Aix-Marseille University
Dennis Zaritsky
Dennis Zaritsky University of Arizona
H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
Mark Seibert
Mark Seibert Carnegie Institution for Science
Heikki Salo
Heikki Salo University of Oulu
George Helou
George Helou California Institute of Technology

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