Publication data of Miceli, Marco:
Link to Inspire
Created with Highcharts 9.0.1
Citations
Citations
w/o self-citaion
self-citaion
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
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Created with Highcharts 9.0.1
Publications
publications per year
Publications
Publications per year
Cumulative publications
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
0
25
50
75
100
125
0
2
4
6
8
10
Created with Highcharts 9.0.1
h-index
h-index
h-index
h-index w/o self-citaion
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
0
5
10
15
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25
Created with Highcharts 9.0.1
Citations
Breakdown of Most Cited Papers
rest
Physical and chemical inhomogeneities inside the Vela SNR shell. Indications of ejecta shrapnels
Physical and chemical inhomogeneities inside the Vela SNR shell. Indications …
XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic acceleration
XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic ac…
Spatially resolved X-ray study of supernova remnants that host magnetars: Implication of their fossil field origin
Spatially resolved X-ray study of supernova remnants that host magnetars: I…
Indication of a Pulsar Wind Nebula in the hard X-ray emission from SN 1987A
Evidence for past interaction with an asymmetric circumstellar shell in the young SNR Cassiopeia A
Evidence for past interaction with an asymmetric circumstellar shell in the y…
Spatial identification of the overionized plasma in W49B
Collisionless shock heating of heavy ions in SN 1987A
Aspect angle for interstellar magnetic field in SN 1006
Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B
Unveiling the spatial structure of the overionized plasma in the supernova re…
Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A
Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Sim…
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006
3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission
3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic …
The x-ray emission of the supernova remnant w49b observed with xmm-newton
The x-ray emission of the supernova remnant w49b observed with xmm-new…
Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of Type Ia supernova remnants
Role of ejecta clumping and back-reaction of accelerated cosmic rays in the e…
XMM-Newton observations of the supernova remnant IC 443: II. evidence of stellar ejecta in the inner regions
XMM-Newton observations of the supernova remnant IC 443: II. evidence of s…
Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A
Hydrodynamic simulations unravel the progenitor-supernova-remnant conne…
The fully developed remnant of a neutrino-driven supernova: Evolution of ejecta structure and asymmetries in SNR Cassiopeia A
The fully developed remnant of a neutrino-driven supernova: Evolution of eje…
Supernova 1987A: a Template to Link Supernovae to their Remnants
Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta
Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: …
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
0
500
1000
1500
2000
Created with Highcharts 9.0.1
Fraction [%]
Breakdown of Most Cited Papers (Fraction)
Physical and chemical inhomogeneities inside the Vela SNR shell. Indications of ejecta shrapnels
Physical and chemical inhomogeneities inside the Vela SNR shell. Indications …
XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic acceleration
XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic ac…
Spatially resolved X-ray study of supernova remnants that host magnetars: Implication of their fossil field origin
Spatially resolved X-ray study of supernova remnants that host magnetars: I…
Indication of a Pulsar Wind Nebula in the hard X-ray emission from SN 1987A
Evidence for past interaction with an asymmetric circumstellar shell in the young SNR Cassiopeia A
Evidence for past interaction with an asymmetric circumstellar shell in the y…
Spatial identification of the overionized plasma in W49B
Collisionless shock heating of heavy ions in SN 1987A
Aspect angle for interstellar magnetic field in SN 1006
Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B
Unveiling the spatial structure of the overionized plasma in the supernova re…
Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A
Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Sim…
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006
3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission
3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic …
The x-ray emission of the supernova remnant w49b observed with xmm-newton
The x-ray emission of the supernova remnant w49b observed with xmm-new…
Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of Type Ia supernova remnants
Role of ejecta clumping and back-reaction of accelerated cosmic rays in the e…
XMM-Newton observations of the supernova remnant IC 443: II. evidence of stellar ejecta in the inner regions
XMM-Newton observations of the supernova remnant IC 443: II. evidence of s…
Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A
Hydrodynamic simulations unravel the progenitor-supernova-remnant conne…
The fully developed remnant of a neutrino-driven supernova: Evolution of ejecta structure and asymmetries in SNR Cassiopeia A
The fully developed remnant of a neutrino-driven supernova: Evolution of eje…
Supernova 1987A: a Template to Link Supernovae to their Remnants
Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta
Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: …
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
0
25
50
75
100
Created with Highcharts 9.0.1
Citations/1 Year
Citations/Period
Citations / 1 Year
Moving average
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
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350
1 Month
3 Months
6 Months
12 Months