Publication data of Di Stefano, R.:
Link to Inspire
Created with Highcharts 9.0.1
Citations
Citations
w/o self-citaion
self-citaion
1985
1990
1995
2000
2005
2010
2015
2020
2025
0
500
1000
1500
2000
Created with Highcharts 9.0.1
Publications
publications per year
Publications
Publications per year
Cumulative publications
1990
2000
2010
2020
0
25
50
75
100
125
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
1985
1990
1995
2000
2005
2010
2015
2020
2025
0
5
10
15
20
25
30
Created with Highcharts 9.0.1
Citations
Breakdown of Most Cited Papers
rest
A luminous recurrent supersoft x-ray source in ngc 300
Chandra studies of the x-ray point source luminosity functions of M31
The Absence of Ex-Companions in Type Ia Supernova Remnants
Spikey: Self-Lensing Flares from Eccentric SMBH Binaries
The absence of radio emission from the globular cluster G1
Blending of light in gravitational microlensing events
Evidence for an intermediate-mass black hole: Chandra and XMM-Newton observations of the ultraluminous supersoft x-ray source in M101 during its 2004 outburst
Evidence for an intermediate-mass black hole: Chandra and XMM-Newton ob…
The Discovery of quasisoft and supersoft sources in external galaxies
The Progenitors of Type Ia Supernovae: II. Are they Double-Degenerate Binaries? The Symbiotic Channel
The Progenitors of Type Ia Supernovae: II. Are they Double-Degenerate Binari…
Interpretation of gravitational microlensing by binary systems
The Ultraluminous x-ray source NGC 1313 X-2 (MS 0317.7-6647) and its environment
The Ultraluminous x-ray source NGC 1313 X-2 (MS 0317.7-6647) and its envi…
Supersoft X-ray Sources in M31: I. A Chandra Survey and an Extension to Quasisoft Sources
Supersoft X-ray Sources in M31: I. A Chandra Survey and an Extension to Qu…
Bright x-ray sources in m31 globular clusters
The Optical gravitational lensing experiment. OGLE 7: Binary microlens or a new unusual variable?
The Optical gravitational lensing experiment. OGLE 7: Binary microlens or a n…
Luminous supersoft x-ray sources in external galaxies
The Progenitors of Type Ia Supernovae: Are They Supersoft Sources?
Periodic self-lensing from accreting massive black hole binaries
X-ray point sources in the central region of m31 as seen by chandra
Spin-Up/Spin-Down models for Type Ia Supernovae
1985
1990
1995
2000
2005
2010
2015
2020
2025
0
500
1000
1500
2000
Created with Highcharts 9.0.1
Fraction [%]
Breakdown of Most Cited Papers (Fraction)
A luminous recurrent supersoft x-ray source in ngc 300
Chandra studies of the x-ray point source luminosity functions of M31
The Absence of Ex-Companions in Type Ia Supernova Remnants
Spikey: Self-Lensing Flares from Eccentric SMBH Binaries
The absence of radio emission from the globular cluster G1
Blending of light in gravitational microlensing events
Evidence for an intermediate-mass black hole: Chandra and XMM-Newton observations of the ultraluminous supersoft x-ray source in M101 during its 2004 outburst
Evidence for an intermediate-mass black hole: Chandra and XMM-Newton ob…
The Discovery of quasisoft and supersoft sources in external galaxies
The Progenitors of Type Ia Supernovae: II. Are they Double-Degenerate Binaries? The Symbiotic Channel
The Progenitors of Type Ia Supernovae: II. Are they Double-Degenerate Binari…
Interpretation of gravitational microlensing by binary systems
The Ultraluminous x-ray source NGC 1313 X-2 (MS 0317.7-6647) and its environment
The Ultraluminous x-ray source NGC 1313 X-2 (MS 0317.7-6647) and its envi…
Supersoft X-ray Sources in M31: I. A Chandra Survey and an Extension to Quasisoft Sources
Supersoft X-ray Sources in M31: I. A Chandra Survey and an Extension to Qu…
Bright x-ray sources in m31 globular clusters
The Optical gravitational lensing experiment. OGLE 7: Binary microlens or a new unusual variable?
The Optical gravitational lensing experiment. OGLE 7: Binary microlens or a n…
Luminous supersoft x-ray sources in external galaxies
The Progenitors of Type Ia Supernovae: Are They Supersoft Sources?
Periodic self-lensing from accreting massive black hole binaries
X-ray point sources in the central region of m31 as seen by chandra
Spin-Up/Spin-Down models for Type Ia Supernovae
1985
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
1985
1990
1995
2000
2005
2010
2015
2020
2025
0
25
50
75
100
125
150
1 Month
3 Months
6 Months
12 Months