Publication data of Kochanek, Christopher S.:
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
5000
10000
15000
20000
25000
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
80
160
240
320
400
0
6
12
18
24
30
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
20
40
60
80
100
Created with Highcharts 9.0.1
Citations
Breakdown of Most Cited Papers
rest
Quantifying Quasar Variability As Part of a General Approach To Classifying Continuously Varying Sources
Quantifying Quasar Variability As Part of a General Approach To Classifying Co…
The Mass of the Milky Way galaxy
The Quasar Accretion Disk Size -- Black Hole Mass Relation
The Cosmic Core-collapse Supernova Rate does not match the Massive-Star Formation Rate
The Cosmic Core-collapse Supernova Rate does not match the Massive-Star F…
A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernovae
A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernov…
ASASSN-14ae: A Tidal Disruption Event at 200 Mpc
Shear and ellipticity in gravitational lenses
Observing the Next Galactic Supernova
Probing the coevolution of supermassive black holes and galaxies using gravitationally lensed quasar hosts
Probing the coevolution of supermassive black holes and galaxies using gravi…
Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs
Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and …
Black hole masses and eddington ratios at 0.3 < z < 4
Coalescing binary neutron stars
Is there a cosmological constant?
The k-band galaxy luminosity function
Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk
Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Rando…
The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0
The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server …
The tidal disruption of a star by a massive black hole
Direct detection of CDM substructure
Mid-infrared selection of active galaxies
1990
1995
2000
2005
2010
2015
2020
2025
0
5000
10000
15000
20000
25000
Created with Highcharts 9.0.1
Fraction [%]
Breakdown of Most Cited Papers (Fraction)
Quantifying Quasar Variability As Part of a General Approach To Classifying Continuously Varying Sources
Quantifying Quasar Variability As Part of a General Approach To Classifying Co…
The Mass of the Milky Way galaxy
The Quasar Accretion Disk Size -- Black Hole Mass Relation
The Cosmic Core-collapse Supernova Rate does not match the Massive-Star Formation Rate
The Cosmic Core-collapse Supernova Rate does not match the Massive-Star F…
A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernovae
A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernov…
ASASSN-14ae: A Tidal Disruption Event at 200 Mpc
Shear and ellipticity in gravitational lenses
Observing the Next Galactic Supernova
Probing the coevolution of supermassive black holes and galaxies using gravitationally lensed quasar hosts
Probing the coevolution of supermassive black holes and galaxies using gravi…
Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs
Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and …
Black hole masses and eddington ratios at 0.3 < z < 4
Coalescing binary neutron stars
Is there a cosmological constant?
The k-band galaxy luminosity function
Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk
Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Rando…
The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0
The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server …
The tidal disruption of a star by a massive black hole
Direct detection of CDM substructure
Mid-infrared selection of active galaxies
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
250
500
750
1000
1250
1500
1750
1 Month
3 Months
6 Months
12 Months