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Reputation and impact in 
academic careers 
Santo Fortunato
Acknowledgement s 
Francesco Beca7ini Arnab Cha7erjee 
Marija Mitrović 
Pietro Parolo 
Raj K. Pan 
Kimmo Kaski 
Orion Penner 
Alex Petersen 
Fabio Pammolli 
Massimo Riccaboni 
Gene Stanley
The role of reputation … 
Question: what is the role of author’s reputation on 
citation dynamics? 
A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, 
M. Riccaboni, H. E. Stanley, F. Pammolli, 
Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
Reputation variabl e 
Measure of reputation of author i at time t: cumulative 
number of citation Ci(t), from the beginning of i’s career until 
year t 
Issues: 
1. H-­‐‑index? 
Ci(t) ⇠ hi(t)1+i 
2. It does not account for quality: high values of Ci(t) can be 
achieved with many low-­‐‑impact papers 
3. Effect of reputation of coauthors? 
4. It can only grow in time, while reputation may also 
decrease (misconduct, fraud) 
A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, 
M. Riccaboni, H. E. Stanley, F. Pammolli, 
Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
Other variable s 
t = Career age, number of years since first publication 
⌧ = Paper age, number of years since first citation 
Ni(t) = Total number of papers published by i until year t 
⌧ c 
1/2 = Half-life of paper c 
ci,p(t) = Citations of paper p and author i until time t 
ci,p(t) = Citations received by paper p of author i in year t 
A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, 
M. Riccaboni, H. E. Stanley, F. Pammolli, 
Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
Our data 
A. Prolific authors of Physical Review Le0ers (PRL) (1958-­‐‑2008) 
B. Highly productive physicists 
C. Young assistant professors from US Top 50 physics and 
astronomy departments 
D. Prolific authors of Cell 
E. Prolific authors of Annals of Mathematics 
Summary 
1. 300 physicists 
2. 100 biologists 
3. 50 mathematicians 
A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, 
M. Riccaboni, H. E. Stanley, F. Pammolli, 
Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
Reputation and citation 
dynamics: cumulativ e 
hN0(t)i ⇠ t¯↵, hC0(t)i ⇠ t¯⇣ 
¯↵  1, ¯⇣ 
 ¯↵ 
Superlinear algebraic growth!
Reputation and citation 
dynamics: individual career s 
Rank-­‐‑citation profile: discrete generalized β-­‐‑distribution: 
c(r) / r!(N + 1 − r)
Citation life-­‐‑cycl e 
• Citation peak before publication age τ ≈ 5 years 
• Slower decay for highly cited papers 
• Long half-­‐‑life for papers in math
Citation life-­‐‑cycle: half-­‐‑life 
versus number of citation s 
¯⌦ 
⌧1/2 ⇠ c¯⌦p 
ranges from 0.3 for Biology to 1 for Mathematics 
(uniformly distributed impact across time)
The reputation mode l 
ci,p(t + 1) vs cp(t) ? 
Preferential a7achment? 
For cp(t) lower than a threshold cx the number of cites 
exceeds that predicted by preferential a7achment: why?
The reputation mode l 
!ci,p(t + 1) ⌘⌘ ⇥ ⇧p(t) ⇥ A⇢(⌧ ) ⇥ Ri(t) = 
=⌘ [cp(t)]⇡ exp(−⌧p/¯⌧) [Ci(t)]⇢ 
noise 
preferential 
a7achment 
life cycle 
reputation 
Regression model 
Main result: 
⇢(c  cx)  ⇢(c  cx), ⇡(c  cx)  ⇡(c  cx) 
⇢(c ! cx) ⇡ 0
The reputation mode l 
Citations are initially boosted by author reputation up to a 
tipping point cx above which the citation rate is sustained 
mostly by publication reputation 
Example (aggregated dataset A/B) 
⇢(c  cx = 40) ⇡ 0.2, ⇢(c  cx = 40) ⇡ 0 
⇡(c  cx = 40) ⇡ 0.4, ⇡(c  cx = 40) ⇡ 1 
For two scientists such that C1(t)=10 C2(t): 
c1(t)/c2(t) = 10⇢ ⇡ 1.66 (c  cx = 40) 
66 % increase for each 10-­‐‑fold increase in Ci(t) !
The Nobel Prize Delay 
60 
50 
40 
30 
20 
10 
0 
Physics 
Data 
Average 
Model 
1900 
1925 
1950 
1975 
2000 
Time between discovery  prize 
Chemistry 
Physiology or Medicine 
1900 
1925 
1950 
1975 
2000 
1900 
1925 
1950 
1975 
2000 
Year of nobel award 
F. Beca7ini, A. Cha7erjee, S. F, M. Mitrović, R. K. Pan, P. 
Della Brio7a Parolo, Natur e 508, 186 (2014) 
h7p://scitation.aip.org/content/aip/magazine/physicstoday/ 
news/10.1063/PT.5.2012
The Nobel Prize Delay 
F. Beca7ini, A. Cha7erjee, S. F, M. Mitrović, R. K. Pan, P. 
Della Brio7a Parolo, Natur e 508, 186 (2014) 
h7p://scitation.aip.org/content/aip/magazine/physicstoday/ 
news/10.1063/PT.5.2012
The Nobel Prize Delay 
F. Beca7ini, A. Cha7erjee, S. F, M. Mitrović, R. K. Pan, P. 
Della Brio7a Parolo, Natur e 508, 186 (2014) 
h7p://scitation.aip.org/content/aip/magazine/physicstoday/ 
news/10.1063/PT.5.2012
Outlook 
• Author reputation drives the initial phase of the 
citation dynamics of papers 
• After a tipping point, citation accumulation is driven by 
the paper’s own reputation 
• Tip: look for quality! 
• The lag between discovery and the Nobel prize is 
growing rapidly 
• Extinction of worthy winners? 
• Decay of (fundamental) science?
Organizing commi7ee: S. Fortunato (Aalto), A. Gionis (Aalto), H. Hämmäinen (Aalto), 
K. Kaski (Aalto), W. Quahrociocchi (IMT), J. Saramäki (Aalto), J. Valimäki (Aalto)
Lada Adamic 
Facebook 
Sinan Aral 
MIT 
László Barabási 
Northeastern U. 
Nicholas Christakis 
Yale 
Robin Dunbar 
Oxford 
Andreas Flache 
Gröningen 
Dirk Helbing 
ETH Zürich 
Ma7hew Jackson 
Stanford 
Jure Leskovec 
Stanford 
Alex Pentland 
MIT 
David Lazer 
Northeastern U. 
Alex Vespignani 
Northeastern U. 
Duncan Wa7s 
Microsoft 
Michael Macy 
Cornell
www.iccss2015.eu 
#ICCSS2015 @ICCSS2015

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Reputation and Impact in Academic Careers

  • 1. Reputation and impact in academic careers Santo Fortunato
  • 2. Acknowledgement s Francesco Beca7ini Arnab Cha7erjee Marija Mitrović Pietro Parolo Raj K. Pan Kimmo Kaski Orion Penner Alex Petersen Fabio Pammolli Massimo Riccaboni Gene Stanley
  • 3. The role of reputation … Question: what is the role of author’s reputation on citation dynamics? A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, M. Riccaboni, H. E. Stanley, F. Pammolli, Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
  • 4. Reputation variabl e Measure of reputation of author i at time t: cumulative number of citation Ci(t), from the beginning of i’s career until year t Issues: 1. H-­‐‑index? Ci(t) ⇠ hi(t)1+i 2. It does not account for quality: high values of Ci(t) can be achieved with many low-­‐‑impact papers 3. Effect of reputation of coauthors? 4. It can only grow in time, while reputation may also decrease (misconduct, fraud) A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, M. Riccaboni, H. E. Stanley, F. Pammolli, Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
  • 5. Other variable s t = Career age, number of years since first publication ⌧ = Paper age, number of years since first citation Ni(t) = Total number of papers published by i until year t ⌧ c 1/2 = Half-life of paper c ci,p(t) = Citations of paper p and author i until time t ci,p(t) = Citations received by paper p of author i in year t A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, M. Riccaboni, H. E. Stanley, F. Pammolli, Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
  • 6. Our data A. Prolific authors of Physical Review Le0ers (PRL) (1958-­‐‑2008) B. Highly productive physicists C. Young assistant professors from US Top 50 physics and astronomy departments D. Prolific authors of Cell E. Prolific authors of Annals of Mathematics Summary 1. 300 physicists 2. 100 biologists 3. 50 mathematicians A. M. Petersen, S. F., R. K. Pan, K. Kaski, O. Penner, A. Rungi, M. Riccaboni, H. E. Stanley, F. Pammolli, Proc. Natl. Acad. Sci. USA 111, 15316-­‐‑15321 (2014 )
  • 7. Reputation and citation dynamics: cumulativ e hN0(t)i ⇠ t¯↵, hC0(t)i ⇠ t¯⇣ ¯↵ 1, ¯⇣ ¯↵ Superlinear algebraic growth!
  • 8. Reputation and citation dynamics: individual career s Rank-­‐‑citation profile: discrete generalized β-­‐‑distribution: c(r) / r!(N + 1 − r)
  • 9. Citation life-­‐‑cycl e • Citation peak before publication age τ ≈ 5 years • Slower decay for highly cited papers • Long half-­‐‑life for papers in math
  • 10. Citation life-­‐‑cycle: half-­‐‑life versus number of citation s ¯⌦ ⌧1/2 ⇠ c¯⌦p ranges from 0.3 for Biology to 1 for Mathematics (uniformly distributed impact across time)
  • 11. The reputation mode l ci,p(t + 1) vs cp(t) ? Preferential a7achment? For cp(t) lower than a threshold cx the number of cites exceeds that predicted by preferential a7achment: why?
  • 12. The reputation mode l !ci,p(t + 1) ⌘⌘ ⇥ ⇧p(t) ⇥ A⇢(⌧ ) ⇥ Ri(t) = =⌘ [cp(t)]⇡ exp(−⌧p/¯⌧) [Ci(t)]⇢ noise preferential a7achment life cycle reputation Regression model Main result: ⇢(c cx) ⇢(c cx), ⇡(c cx) ⇡(c cx) ⇢(c ! cx) ⇡ 0
  • 13. The reputation mode l Citations are initially boosted by author reputation up to a tipping point cx above which the citation rate is sustained mostly by publication reputation Example (aggregated dataset A/B) ⇢(c cx = 40) ⇡ 0.2, ⇢(c cx = 40) ⇡ 0 ⇡(c cx = 40) ⇡ 0.4, ⇡(c cx = 40) ⇡ 1 For two scientists such that C1(t)=10 C2(t): c1(t)/c2(t) = 10⇢ ⇡ 1.66 (c cx = 40) 66 % increase for each 10-­‐‑fold increase in Ci(t) !
  • 14.
  • 15. The Nobel Prize Delay 60 50 40 30 20 10 0 Physics Data Average Model 1900 1925 1950 1975 2000 Time between discovery prize Chemistry Physiology or Medicine 1900 1925 1950 1975 2000 1900 1925 1950 1975 2000 Year of nobel award F. Beca7ini, A. Cha7erjee, S. F, M. Mitrović, R. K. Pan, P. Della Brio7a Parolo, Natur e 508, 186 (2014) h7p://scitation.aip.org/content/aip/magazine/physicstoday/ news/10.1063/PT.5.2012
  • 16. The Nobel Prize Delay F. Beca7ini, A. Cha7erjee, S. F, M. Mitrović, R. K. Pan, P. Della Brio7a Parolo, Natur e 508, 186 (2014) h7p://scitation.aip.org/content/aip/magazine/physicstoday/ news/10.1063/PT.5.2012
  • 17. The Nobel Prize Delay F. Beca7ini, A. Cha7erjee, S. F, M. Mitrović, R. K. Pan, P. Della Brio7a Parolo, Natur e 508, 186 (2014) h7p://scitation.aip.org/content/aip/magazine/physicstoday/ news/10.1063/PT.5.2012
  • 18.
  • 19.
  • 20. Outlook • Author reputation drives the initial phase of the citation dynamics of papers • After a tipping point, citation accumulation is driven by the paper’s own reputation • Tip: look for quality! • The lag between discovery and the Nobel prize is growing rapidly • Extinction of worthy winners? • Decay of (fundamental) science?
  • 21. Organizing commi7ee: S. Fortunato (Aalto), A. Gionis (Aalto), H. Hämmäinen (Aalto), K. Kaski (Aalto), W. Quahrociocchi (IMT), J. Saramäki (Aalto), J. Valimäki (Aalto)
  • 22. Lada Adamic Facebook Sinan Aral MIT László Barabási Northeastern U. Nicholas Christakis Yale Robin Dunbar Oxford Andreas Flache Gröningen Dirk Helbing ETH Zürich Ma7hew Jackson Stanford Jure Leskovec Stanford Alex Pentland MIT David Lazer Northeastern U. Alex Vespignani Northeastern U. Duncan Wa7s Microsoft Michael Macy Cornell