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Eleonora Troja

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 102 1540 1462 809 756 307 41622

Eleonora Troja publications per year

The chart shows the history of publications by Eleonora Troja between 2006 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Eleonora Troja published across 16 years, from 2006 to 2021, averaging 19.2 papers a year. Output peaked at 33 publications in 2017. 41 of the 307 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 2006 to 2021. Vertical axis: number of publications, 0 to 33. Peak 33 publications in 2017. 2006: 15 publications 2007: 14 publications 2008: 6 publications 2009: 4 publications 2010: 8 publications 2011: 22 publications 2012: 25 publications 2013: 15 publications 2014: 20 publications 2015: 21 publications 2016: 27 publications 2017: 33 publications 2018: 24 publications 2019: 32 publications 2020: 14 publications 2021: 27 publications
2006 2021

307 publications in total across all disciplines

View publications per year as a table
Eleonora Troja: publications per year, 2006 to 2021
Year Publications
2006 15
2007 14
2008 6
2009 4
2010 8
2011 22
2012 25
2013 15
2014 20
2015 21
2016 27
2017 33
2018 24
2019 32
2020 14
2021 27
Total 307
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Eleonora Troja 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 Eleonora Troja 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: 307 publications — 19th percentile

19% 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
303–322 136 307
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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Eleonora Troja 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 Eleonora Troja 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: 102 D-Index — 59th percentile

59% 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 97 102
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

What is she best known for?

The fields of study she is best known for:

  • Astronomy
  • Astrophysics
  • Quantum mechanics

Her primary areas of investigation include Astrophysics, Astronomy, Fermi Gamma-ray Space Telescope, Telescope and Gamma ray. Her study in Galaxy, Cosmic ray, Gamma-ray burst, Dark matter and Galactic Center are all subfields of Astrophysics. Eleonora Troja interconnects Gamma-ray astronomy and Flux in the investigation of issues within Astronomy.

Her Fermi Gamma-ray Space Telescope study combines topics from a wide range of disciplines, such as Spectral line, Pulsar, Active galactic nucleus and Galactic halo. In her work, Molecular cloud and Photon is strongly intertwined with Supernova remnant, which is a subfield of Telescope. Her work carried out in the field of Gamma ray brings together such families of science as Stars, Radius, Synchrotron radiation and Supernova.

Her most cited work include:

  • Fermi Large Area Telescope Second Source Catalog (1327 citations)
  • Searching for dark matter annihilation from Milky Way dwarf spheroidal galaxies with six years of Fermi Large Area Telescope data (811 citations)
  • THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS (728 citations)

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

Her scientific interests lie mostly in Astrophysics, Gamma-ray burst, Astronomy, Fermi Gamma-ray Space Telescope and Telescope. All of her Astrophysics and Afterglow, Galaxy, Gamma ray, Light curve and Neutron star investigations are sub-components of the entire Astrophysics study. Her studies in Gamma ray integrate themes in fields like Astroparticle physics and Flux.

Her biological study spans a wide range of topics, including Black hole and Kilonova. Her Gamma-ray burst research includes themes of Swift, Gravitational wave and Redshift. In her study, Galactic Center is strongly linked to Cosmic ray, which falls under the umbrella field of Fermi Gamma-ray Space Telescope.

She most often published in these fields:

  • Astrophysics (148.87%)
  • Gamma-ray burst (78.60%)
  • Astronomy (75.23%)

What were the highlights of her more recent work (between 2018-2021)?

  • Astrophysics (148.87%)
  • Gamma-ray burst (78.60%)
  • Gravitational wave (27.70%)

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

Eleonora Troja spends much of her time researching Astrophysics, Gamma-ray burst, Gravitational wave, Neutron star and LIGO. In her study, she carries out multidisciplinary Astrophysics and Population research. Eleonora Troja combines subjects such as Galaxy, Redshift, Energy, Photometry and Light curve with her study of Gamma-ray burst.

As part of the same scientific family, she usually focuses on Neutron star, concentrating on Black hole and intersecting with Luminosity function, Spin-½ and Magnetic field. Her Telescope study incorporates themes from Fermi Gamma-ray Space Telescope, Gamma ray and Photon. Her work deals with themes such as Primary, Proton, Cosmic ray and Anisotropy, which intersect with Fermi Gamma-ray Space Telescope.

Between 2018 and 2021, her most popular works were:

  • A long-lived neutron star merger remnant in GW170817: Constraints and clues from X-ray observations (83 citations)
  • A long-lived neutron star merger remnant in GW170817: Constraints and clues from X-ray observations (83 citations)
  • A Decade of Gamma-Ray Bursts Observed by Fermi-LAT: The Second GRB Catalog (77 citations)

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

  • Astronomy
  • Quantum mechanics
  • Astrophysics

Her primary areas of study are Astrophysics, Gravitational wave, Afterglow, Gamma-ray burst and Neutron star. She connects Astrophysics with Population in her research. Shock, Photometry, Photon and Fermi Gamma-ray Space Telescope is closely connected to Redshift in her research, which is encompassed under the umbrella topic of Gamma-ray burst.

In her study, Luminosity and Telescope is inextricably linked to LIGO, which falls within the broad field of Neutron star. Her Galaxy research includes elements of Photosphere, Infrared, Opacity and White dwarf. The study incorporates disciplines such as Magnitude, Light curve and Observatory in addition to Kilonova.

Best Publications

  • Fermi Large Area Telescope Second Source Catalog

    P. L. Nolan;A. A. Abdo;A. A. Abdo;M. Ackermann;M. Ajello

  • Searching for dark matter annihilation from Milky Way dwarf spheroidal galaxies with six years of Fermi Large Area Telescope data

    M. Ackermann;A. Albert;B. Anderson;W. B. Atwood

  • The second catalog of active galactic nuclei detected by the Fermi Large Area Telescope

    Markus Ackermann;Marco Ajello;A. Allafort;E. Antolini;E. Antolini

  • Detection of the characteristic pion-decay signature in supernova remnants

    Markus Ackermann;Marco Ajello;A. Allafort;Luca Baldini

  • The Second Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

    M. Ackermann;M. Ajello;A. Allafort;E. Antolini

  • THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS

    A. A. Abdo;A. A. Abdo;M. Ajello;A. Allafort;L. Baldini

  • Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger

    E. Pian;P. D'Avanzo;S. Benetti;M. Branchesi

  • Fermi-LAT observations of the diffuse γ-ray emission: implications for cosmic rays and the interstellar medium

    M. Ackermann;M. Ajello;W. B. Atwood;L. Baldini

  • The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV

    M. Ackermann;M. Ajello;A. Albert

  • Measurement of Separate Cosmic-Ray Electron and Positron Spectra with the Fermi Large Area Telescope

    M. Ackermann;M. Ajello;A. Allafort;W. B. Atwood

  • The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV

    M. Ackermann;M. Ajello;A. Albert;W. B. Atwood

  • The Third Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

    M. Ackermann;M. Ajello;W. Atwood;L. Baldini

  • The X-ray counterpart to the gravitational-wave event GW170817

    E. Troja;E. Troja;L. Piro;H. van Eerten;R.T. Wollaeger

  • A limit on the variation of the speed of light arising from quantum gravity effects

    A. A. Abdo;M. Ackermann;M. Ajello;K. Asano

  • The Third Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

    M. Ackermann;M. Ajello;W. B. Atwood;L. Baldini

  • Constraining Dark Matter Models from a Combined Analysis of Milky Way Satellites with the Fermi Large Area Telescope

    M. Ackermann;M. Ajello;A. Albert;W. B. Atwood

  • The fermi large area telescope on orbit: Event classification, instrument response functions, and calibration

    Markus Ackermann;Marco Ajello;A. Albert;A. Allafort

  • Relativistic jet activity from the tidal disruption of a star by a massive black hole

    D. N. Burrows;J. A. Kennea;G. Ghisellini;V. Mangano

  • FERMI-LAT OBSERVATIONS of HIGH-ENERGY γ-RAY EMISSION TOWARD the GALACTIC CENTER

    M. Ajello;A. Albert;W.B. Atwood;G. Barbiellini;G. Barbiellini

  • Gamma-Ray Flares from the Crab Nebula

    A. A. Abdo;Markus Ackermann;Marco Ajello;A. Allafort

Frequent Co-Authors

Diego F. Torres
Diego F. Torres Institute of Space Sciences
Julie McEnery
Julie McEnery Goddard Space Flight Center
Olaf Reimer
Olaf Reimer University of Innsbruck
G. Tosti
G. Tosti University of Perugia
Peter F. Michelson
Peter F. Michelson Stanford University
P. A. Caraveo
P. A. Caraveo National Institute for Astrophysics
Marcello Giroletti
Marcello Giroletti National Institute for Astrophysics
A. Morselli
A. Morselli National Institute for Nuclear Physics
Marco Ajello
Marco Ajello Clemson University
Igor V. Moskalenko
Igor V. Moskalenko Stanford University

External Links

Wikipedia of Eleonora Troja Personal website of Eleonora Troja

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Best Scientists Citing Eleonora Troja

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Publications: 236

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Diego F. Torres

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Publications: 233

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Felix Aharonian

Dublin Institute For Advanced Studies

Publications: 222

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Publications: 198

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Publications: 134

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P. T. O'Brien

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Publications: 133

Kohta Murase

Kohta Murase

Pennsylvania State University

Publications: 125

Jochen Greiner

Jochen Greiner

Max Planck Society

Publications: 121

Fabrizio Tavecchio

Fabrizio Tavecchio

National Institute for Astrophysics

Publications: 120

Marcello Giroletti

Marcello Giroletti

National Institute for Astrophysics

Publications: 119

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Olaf Reimer

University of Innsbruck

Publications: 117

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Marco Ajello

Clemson University

Publications: 117

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Liverpool John Moores University

Publications: 117

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