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Peter M. Garnavich

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 124 676 643 371 347 789 118829

Peter M. Garnavich publications per year

The chart shows the history of publications by Peter M. Garnavich between 1975 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Peter M. Garnavich published across 47 years, from 1975 to 2021, averaging 17.1 papers a year. Output peaked at 52 publications in 2006. 37 of the 806 publications appeared in the last two years.

No. of publications
10 20 30 40 50
Bar chart. Horizontal axis: year, 1975 to 2021. Vertical axis: number of publications, 0 to 52. Peak 52 publications in 2006. 1975: 1 publication 1976: 0 publications 1977: 0 publications 1978: 0 publications 1979: 0 publications 1980: 0 publications 1981: 2 publications 1982: 2 publications 1983: 0 publications 1984: 1 publication 1985: 1 publication 1986: 2 publications 1987: 2 publications 1988: 5 publications 1989: 4 publications 1990: 4 publications 1991: 2 publications 1992: 5 publications 1993: 7 publications 1994: 10 publications 1995: 16 publications 1996: 14 publications 1997: 27 publications 1998: 26 publications 1999: 17 publications 2000: 27 publications 2001: 28 publications 2002: 40 publications 2003: 37 publications 2004: 24 publications 2005: 47 publications 2006: 52 publications 2007: 45 publications 2008: 35 publications 2009: 20 publications 2010: 21 publications 2011: 30 publications 2012: 20 publications 2013: 22 publications 2014: 19 publications 2015: 30 publications 2016: 21 publications 2017: 35 publications 2018: 49 publications 2019: 19 publications 2020: 17 publications 2021: 20 publications
1975 2021

806 publications in total across all disciplines

View publications per year as a table
Peter M. Garnavich: publications per year, 1975 to 2021
Year Publications
1975 1
1976 0
1977 0
1978 0
1979 0
1980 0
1981 2
1982 2
1983 0
1984 1
1985 1
1986 2
1987 2
1988 5
1989 4
1990 4
1991 2
1992 5
1993 7
1994 10
1995 16
1996 14
1997 27
1998 26
1999 17
2000 27
2001 28
2002 40
2003 37
2004 24
2005 47
2006 52
2007 45
2008 35
2009 20
2010 21
2011 30
2012 20
2013 22
2014 19
2015 30
2016 21
2017 35
2018 49
2019 19
2020 17
2021 20
Total 806
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Peter M. Garnavich 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 Peter M. Garnavich 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, 783–802 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: 789 publications — 84th percentile

84% 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
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 43 789
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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Peter M. Garnavich 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 Peter M. Garnavich 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, 124–125 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: 124 D-Index — 82nd percentile

82% 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
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 53 124
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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Research.com Recognitions

  • 2012 - Fellow of the American Association for the Advancement of Science (AAAS)
  • 2007 - Fellow of American Physical Society (APS) Citation For pioneering work on the discovery of dark energy and the cosmic equation of state, along with important observvational discoveries regarding the nature of gamma ray bursts and the physics of supernova light curves

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Astrophysics
  • Galaxy

His primary scientific interests are in Astrophysics, Supernova, Astronomy, Light curve and Redshift. Astrophysics is often connected to Cosmological constant in his work. Peter M. Garnavich has researched Cosmological constant in several fields, including Metric expansion of space, Dark energy and Universe.

His research integrates issues of Gamma-ray burst, Shape of the universe, Spectral line and Baryon acoustic oscillations in his study of Supernova. Peter M. Garnavich combines subjects such as Variable star, Center and Sky with his study of Light curve. Peter M. Garnavich works mostly in the field of Redshift, limiting it down to concerns involving Star formation and, occasionally, Hubble Deep Field and Limiting magnitude.

His most cited work include:

  • Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant (14054 citations)
  • Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant (12314 citations)
  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (1588 citations)

What are the main themes of his work throughout his whole career to date?

His scientific interests lie mostly in Astrophysics, Supernova, Astronomy, Light curve and Redshift. His Astrophysics research focuses on subjects like Spectral line, which are linked to Line. His studies deal with areas such as Cosmology, Dark energy, Luminosity and Sky as well as Supernova.

His Light curve study combines topics in areas such as Cataclysmic variable star, White dwarf, Brightness, Radius and Orbital period. His Orbital period study combines topics from a wide range of disciplines, such as Amplitude and Dwarf nova. He studies Supernova Legacy Survey, a branch of Redshift.

He most often published in these fields:

  • Astrophysics (93.09%)
  • Supernova (56.36%)
  • Astronomy (39.56%)

What were the highlights of his more recent work (between 2015-2021)?

  • Astrophysics (93.09%)
  • Light curve (31.55%)
  • Supernova (56.36%)

In recent papers he was focusing on the following fields of study:

The scientist’s investigation covers issues in Astrophysics, Light curve, Supernova, White dwarf and Orbital period. The Astrophysics study combines topics in areas such as Brightness and Astronomy. His Light curve research is multidisciplinary, incorporating elements of Stars, Accretion, Radius and Mass ratio.

His study in Supernova is interdisciplinary in nature, drawing from both Galaxy, Redshift and Sky. His work deals with themes such as Dark energy and Photometric system, which intersect with Redshift. His work carried out in the field of White dwarf brings together such families of science as Accretion, Spectral line, Pulsar and Polar.

Between 2015 and 2021, his most popular works were:

  • Type Ia Supernova Distances at Redshift > 1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate (117 citations)
  • Type Ia Supernova Distances at z > 1.5 from the Hubble Space Telescope Multi-Cycle Treasury Programs: The Early Expansion Rate (105 citations)
  • SHOCK BREAKOUT AND EARLY LIGHT CURVES OF TYPE II-P SUPERNOVAE OBSERVED WITH KEPLER (83 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Astrophysics
  • Galaxy

Peter M. Garnavich spends much of his time researching Astrophysics, Light curve, Supernova, White dwarf and Astronomy. His work investigates the relationship between Astrophysics and topics such as Brightness that intersect with problems in Emission spectrum. His Light curve study incorporates themes from Accretion, Cataclysmic variable star, Stars, Orbital period and Mass ratio.

His Supernova study incorporates themes from Wavelength, Redshift, Telescope and Shock wave. Peter M. Garnavich has included themes like Dark energy and Photometric system in his Redshift study. His White dwarf research is multidisciplinary, incorporating perspectives in Pulsar and Beat.

Best Publications

  • Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

    Adam G. Riess;Alexei V. Filippenko;Peter Challis;Alejandro Clocchiatti

  • Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

    Adam G. Riess;Alexei V. Filippenko;Peter Challis;Alejandro Clocchiattia

  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics

    Anton M. Koekemoer;S. M. Faber;Henry C. Ferguson;Norman A. Grogin

  • Cosmological Results from High-z Supernovae* **

    John L. Tonry;Brian P. Schmidt;Brian Barris;Pablo Candia

  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

    Norman A. Grogin;Dale D. Kocevski;S. M. Faber;Henry C. Ferguson

  • The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Curvature of the Universe Using Type Ia Supernovae*

    Brian P. Schmidt;Nicholas B. Suntzeff;M. M. Phillips;Robert A. Schommer

  • Candels: The cosmic assembly near-infrared deep extragalactic legacy survey - The hubble space telescope observations, imaging data products, and mosaics

    Anton M. Koekemoer;S. M. Faber;Henry C. Ferguson;Norman A. Grogin

  • The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Cur vature of the Universe Using Type Ia Supernovae

    Brian P. Schmidt;Nicholas B. Suntzeff;M. M. Phillips;Robert A. Schommer

  • Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329

    K. Z. Stanek;T. Matheson;P. M. Garnavich;P. Martini

  • Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey

    W. M. Wood-Vasey;G. Miknaitis;C. W. Stubbs;S. Jha

  • LSST Science Book, Version 2.0

    Paul A. Abell;Julius Allison;Scott F. Anderson

  • Supernova limits on the cosmic equation of state

    Peter M. Garnavich;Saurabh Jha;Peter Challis;Alejandro Clocchiatti

  • Observational Constraints on the Nature of Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey

    W. M. Wood-Vasey;G. Miknaitis;C. W. Stubbs;Saurabh Jha;Saurabh Jha

  • Long γ-ray bursts and core-collapse supernovae have different environments

    A. S. Fruchter;A. J. Levan;A. J. Levan;A. J. Levan;L. Strolger;L. Strolger;P. M. Vreeswijk

  • Constraints on Cosmological Models from Hubble Space Telescope Observations of High-z Supernovae

    P. M. Garnavich;R. P. Kirshner;P. Challis;J. Tonry

  • First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters

    Richard Kessler;Andrew Becker;David Cinabro;Jake Vanderplas

  • BVRI Light Curves for 22 Type Ia Supernovae

    Adam G. Riess;Robert P. Kirshner;Brian P. Schmidt;Saurabh Jha

  • BVRI Light Curves for 22 Type Ia Supernovae

    Adam G. Riess;Robert P. Kirshner;Brian P. Schmidt;Saurabh Jha

  • Supernova Limits on the Cosmic Equation of State

    P. M. Garnavich;S. Jha;P. M. Challis;A. Clocchiatti

  • Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes

    T. M. Davis;E. Mortsell;J. Sollerman;A. C. Becker

Frequent Co-Authors

Saurabh Jha
Saurabh Jha Rutgers, The State University of New Jersey
Adam G. Riess
Adam G. Riess Johns Hopkins University
Robert P. Kirshner
Robert P. Kirshner Harvard University
Jesper Sollerman
Jesper Sollerman Stockholm University
Joshua A. Frieman
Joshua A. Frieman University of Chicago
Thomas Matheson
Thomas Matheson National Optical-Infrared Astronomy Research Lab
Alexei V. Filippenko
Alexei V. Filippenko University of California, Berkeley
Peter Challis
Peter Challis Harvard University
Bruno Leibundgut
Bruno Leibundgut European Southern Observatory
Brian P. Schmidt
Brian P. Schmidt Australian National University

External Links

Wikipedia of Peter M. Garnavich Personal website of Peter M. Garnavich

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