Publication data of Laskar, Jacques:
Link to Inspire
Created with Highcharts 9.0.1
Citations
Citations
w/o self-citaion
self-citaion
1990
1995
2000
2005
2010
2015
2020
2025
0
250
500
750
1000
1250
1500
1750
Created with Highcharts 9.0.1
Publications
publications per year
Publications
Publications per year
Cumulative publications
1990
1995
2000
2005
2010
2015
2020
2025
0
20
40
60
80
100
0
2.5
5
7.5
10
12.5
Created with Highcharts 9.0.1
h-index
h-index
h-index
h-index w/o self-citaion
1990
1995
2000
2005
2010
2015
2020
2025
0
5
10
15
20
25
Created with Highcharts 9.0.1
Citations
Breakdown of Most Cited Papers
rest
Constraint on the Yukawa suppression of the Newtonian potential from the planetary ephemeris INPOP19a
Constraint on the Yukawa suppression of the Newtonian potential from the pl…
HD45364, a pair of planets in a 3:2 mean motion resonance
The HARPS search for southern extra-solar planets. XXVII. Up to seven planets orbiting HD 10180: probing the architecture of low-mass planetary systems
The HARPS search for southern extra-solar planets. XXVII. Up to seven planet…
Global Dynamics of the Advanced Light Source Revealed through Experimental Frequency Map Analysis
Global Dynamics of the Advanced Light Source Revealed through Experimen…
On the Spacing of Planetary Systems
Measuring and optimizing the momentum aperture in a particle accelerator
Constraining the mass of the graviton with the planetary ephemeris INPOP
Review of single particle dynamics for third generation light sources through frequency map analysis
Review of single particle dynamics for third generation light sources through …
Tidal dissipation within hot Jupiters: A new appraisal
INPOP08, a 4-D planetary ephemeris: From asteroid and time-scale computations to ESA Mars Express and Venus Express contributions
INPOP08, a 4-D planetary ephemeris: From asteroid and time-scale computat…
The HARPS search for southern extra-solar planets. IX. mu Ara, a system with four planets
The HARPS search for southern extra-solar planets. IX. mu Ara, a system with…
The new lunar ephemeris INPOP17a and its application to fundamental physics
The new lunar ephemeris INPOP17a and its application to fundamental physi…
The CORALIE survey for southern extra-solar planets. 13. A Pair of planets around HD 202206 or a circumbinary planet?
The CORALIE survey for southern extra-solar planets. 13. A Pair of planets aro…
Numerical estimation of the sensitivity of INPOP planetary ephemerides to general relativity parameters
Numerical estimation of the sensitivity of INPOP planetary ephemerides to ge…
Use of MESSENGER radioscience data to improve planetary ephemeris and to test general relativity
Use of MESSENGER radioscience data to improve planetary ephemeris and to…
The measure of chaos by the numerical analysis of the fundamental frequencies. Application to the standard mapping
The measure of chaos by the numerical analysis of the fundamental frequen…
The INPOP10a planetary ephemeris and its applications in fundamental physics
The INPOP10a planetary ephemeris and its applications in fundamental physi…
The chaotic motion of the solar system: A numerical estimate of the size of the chaotic zones
The chaotic motion of the solar system: A numerical estimate of the size of th…
An extrasolar planetary system with three Neptune-mass planets
1990
1995
2000
2005
2010
2015
2020
2025
0
250
500
750
1000
1250
1500
1750
Created with Highcharts 9.0.1
Fraction [%]
Breakdown of Most Cited Papers (Fraction)
Constraint on the Yukawa suppression of the Newtonian potential from the planetary ephemeris INPOP19a
Constraint on the Yukawa suppression of the Newtonian potential from the pl…
HD45364, a pair of planets in a 3:2 mean motion resonance
The HARPS search for southern extra-solar planets. XXVII. Up to seven planets orbiting HD 10180: probing the architecture of low-mass planetary systems
The HARPS search for southern extra-solar planets. XXVII. Up to seven planet…
Global Dynamics of the Advanced Light Source Revealed through Experimental Frequency Map Analysis
Global Dynamics of the Advanced Light Source Revealed through Experimen…
On the Spacing of Planetary Systems
Measuring and optimizing the momentum aperture in a particle accelerator
Constraining the mass of the graviton with the planetary ephemeris INPOP
Review of single particle dynamics for third generation light sources through frequency map analysis
Review of single particle dynamics for third generation light sources through …
Tidal dissipation within hot Jupiters: A new appraisal
INPOP08, a 4-D planetary ephemeris: From asteroid and time-scale computations to ESA Mars Express and Venus Express contributions
INPOP08, a 4-D planetary ephemeris: From asteroid and time-scale computat…
The HARPS search for southern extra-solar planets. IX. mu Ara, a system with four planets
The HARPS search for southern extra-solar planets. IX. mu Ara, a system with…
The new lunar ephemeris INPOP17a and its application to fundamental physics
The new lunar ephemeris INPOP17a and its application to fundamental physi…
The CORALIE survey for southern extra-solar planets. 13. A Pair of planets around HD 202206 or a circumbinary planet?
The CORALIE survey for southern extra-solar planets. 13. A Pair of planets aro…
Numerical estimation of the sensitivity of INPOP planetary ephemerides to general relativity parameters
Numerical estimation of the sensitivity of INPOP planetary ephemerides to ge…
Use of MESSENGER radioscience data to improve planetary ephemeris and to test general relativity
Use of MESSENGER radioscience data to improve planetary ephemeris and to…
The measure of chaos by the numerical analysis of the fundamental frequencies. Application to the standard mapping
The measure of chaos by the numerical analysis of the fundamental frequen…
The INPOP10a planetary ephemeris and its applications in fundamental physics
The INPOP10a planetary ephemeris and its applications in fundamental physi…
The chaotic motion of the solar system: A numerical estimate of the size of the chaotic zones
The chaotic motion of the solar system: A numerical estimate of the size of th…
An extrasolar planetary system with three Neptune-mass planets
1990
1995
2000
2005
2010
2015
2020
2025
0
25
50
75
100
Created with Highcharts 9.0.1
Citations/1 Year
Citations/Period
Citations / 1 Year
Moving average
1990
1995
2000
2005
2010
2015
2020
2025
0
25
50
75
100
125
150
175
1 Month
3 Months
6 Months
12 Months