giovanni peres
giovanni peres
Professor of Astrophysics, University of Palermo
Verified email at astropa.unipa.it
TitleCited byYear
The X-ray telescope (XRT) for the Hinode mission
L Golub, E Deluca, G Austin, J Bookbinder, D Caldwell, P Cheimets, ...
The Hinode Mission, 27-50, 2008
5802008
Closed coronal structures. II-Generalized hydrostatic model
S Serio, G Peres, GS Vaiana, L Golub, R Rosner
The Astrophysical Journal 243, 288-300, 1981
3391981
Coronal closed structures. IV-Hydrodynamical stability and response to heating perturbations
G Peres, S Serio, GS Vaiana, R Rosner
The Astrophysical Journal 252, 791-799, 1982
2061982
The Sun as an X-ray star. II. Using the Yohkoh/Soft X-ray telescope-derived solar emission measure versus temperature to interpret stellar X-ray observations
G Peres, S Orlando, F Reale, R Rosner, H Hudson
The Astrophysical Journal 528 (1), 537, 2000
2022000
The density of coronal plasma in active stellar coronae
P Testa, JJ Drake, G Peres
The Astrophysical Journal 617 (1), 508, 2004
1132004
XIPE: the X-ray imaging polarimetry explorer
P Soffitta, X Barcons, R Bellazzini, J Braga, E Costa, GW Fraser, S Gburek, ...
Experimental Astronomy 36 (3), 523-567, 2013
992013
The Ultraluminous M81 X-9 Source: 20 Years’ Variability and Spectral States
V La Parola, G Peres, G Fabbiano, DW Kim, F Bocchino
The Astrophysical Journal 556 (1), 47, 2001
982001
TRACE-derived temperature and emission measure profiles along long-lived coronal loops: The role of filamentation
F Reale, G Peres
The Astrophysical Journal Letters 528 (1), L45, 1999
931999
On stellar coronae and solar active regions
JJ Drake, G Peres, S Orlando, JM Laming, A Maggio
The Astrophysical Journal 545 (2), 1074, 2000
922000
Deep ROSAT HRI observations of the NGC 1399/NGC 1404 region: Morphology and structure of the X-ray halo
M Paolillo, G Fabbiano, G Peres, DW Kim
The Astrophysical Journal 565 (2), 883, 2002
902002
Hydrodynamic flare modeling-Comparison of numerical calculations with SMM observations of the 1980 November 12 17: 00 UT flare
G Peres, F Reale, S Serio, R Pallavicini
The Astrophysical Journal 312, 895-908, 1987
891987
Closed coronal structures. V-gasdynamic models of flaring loops and comparison with SMM observations
R Pallavicini, G Peres, S Serio, G Vaiana, L Acton, J Leibacher, R Rosner
The Astrophysical Journal 270, 270-287, 1983
851983
The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds
S Orlando, F Bocchino, F Reale, G Peres, P Pagano
The Astrophysical Journal 678 (1), 274, 2008
842008
Morphology and spectral characteristics of the X-ray emission of M33
G Trinchieri, G Fabbiano, G Peres
The Astrophysical Journal 325, 531-543, 1988
761988
Hydrodynamic modeling of an X-ray flare on Proxima Centauri observed by the Einstein telescope
F Reale, G Peres, S Serio, R Rosner, J Schmitt
The Astrophysical Journal 328, 256-264, 1988
731988
Closed coronal structures. III-Comparison of static models with X-ray, EUV, and radio observations
R Pallavicini, G Peres, S Serio, GS Vaiana, L Golub, R Rosner
The Astrophysical Journal 247, 692-706, 1981
731981
The Sun as an X-ray star. III. Flares
F Reale, G Peres, S Orlando
The Astrophysical Journal 557 (2), 906, 2001
612001
Temperature and density structure of hot and cool loops derived from the analysis of TRACE data
P Testa, G Peres, F Reale, S Orlando
The Astrophysical Journal 580 (2), 1159, 2002
602002
A brightening coronal loop observed by TRACE. II. Loop modeling and constraints on heating
F Reale, G Peres, S Serio, RM Betta, EE DeLuca, L Golub
The Astrophysical Journal 535 (1), 423, 2000
592000
The Sun as an X-ray star. I. Deriving the emission measure distribution versus temperature of the whole solar corona from the Yohkoh/Soft X-ray telescope data
S Orlando, G Peres, F Reale
The Astrophysical Journal 528 (1), 524, 2000
582000
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