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Simone Migliari
Simone Migliari
Aurora Technology BV
Verified email at aurora.nl
Title
Cited by
Cited by
Year
Jets in neutron star X-ray binaries: a comparison with black holes
S Migliari, RP Fender
Monthly Notices of the Royal Astronomical Society 366 (1), 79-91, 2006
3952006
Modulated high-energy gamma-ray emission from the microquasar Cygnus X-3
Fermi LAT Collaboration, AA Abdo, M Ackermann, M Ajello, M Axelsson, ...
Science 326 (5959), 1512-1516, 2009
3392009
The large observatory for X-ray timing (LOFT)
M Feroci, L Stella, M Van der Klis, TJL Courvoisier, M Hernanz, R Hudec, ...
Experimental Astronomy 34, 415-444, 2012
287*2012
Hard X-ray states and radio emission in GRS 1915+ 105
M Klein-Wolt, RP Fender, GG Pooley, T Belloni, S Migliari, EH Morgan, ...
Monthly Notices of the Royal Astronomical Society 331 (3), 745-764, 2002
2532002
Jet-dominated advective systems: radio and X-ray luminosity dependence on the accretion rate
EG Körding, RP Fender, S Migliari
Monthly Notices of the Royal Astronomical Society 369 (3), 1451-1458, 2006
1882006
Iron emission lines from extended X-ray jets in SS 433: Reheating of atomic nuclei
S Migliari, R Fender, M Méndez
Science 297 (5587), 1673-1676, 2002
1712002
Stingray: a modern Python library for spectral timing
D Huppenkothen, M Bachetti, AL Stevens, S Migliari, P Balm, O Hammad, ...
The Astrophysical Journal 881 (1), 39, 2019
1692019
Disc–jet coupling in the 2009 outburst of the black hole candidate H1743− 322
JCA Miller-Jones, GR Sivakoff, D Altamirano, M Coriat, S Corbel, ...
Monthly Notices of the Royal Astronomical Society 421 (1), 468-485, 2012
1582012
Truncation of the inner accretion disk around a black hole at low luminosity
JA Tomsick, K Yamaoka, S Corbel, P Kaaret, E Kalemci, S Migliari
The Astrophysical Journal 707 (1), L87, 2009
1362009
Tracing the power-law component in the energy spectrum of black hole candidates as a function of the QPO frequency
F Vignarca, S Migliari, T Belloni, D Psaltis, M Van Der Klis
Astronomy & Astrophysics 397 (2), 729-738, 2003
1362003
A systematic analysis of the broad iron Kα line in neutron-star LMXBs with XMM-Newton
C Ng, MD Trigo, MC Bel, S Migliari
Astronomy & Astrophysics 522, A96, 2010
1132010
A systematic analysis of the broad iron Kα line in neutron-star LMXBs with XMM-Newton
C Ng, MD Trigo, MC Bel, S Migliari
Astronomy & Astrophysics 522, A96, 2010
1132010
The variability plane of accreting compact objects
EG Körding, S Migliari, R Fender, T Belloni, C Knigge, I McHardy
Monthly Notices of the Royal Astronomical Society 380 (1), 301-310, 2007
1052007
The spectral energy distribution of quiescent black hole X-ray binaries: new constraints from Spitzer
E Gallo, S Migliari, S Markoff, JA Tomsick, CD Bailyn, S Berta, R Fender, ...
The Astrophysical Journal 670 (1), 600, 2007
1042007
Disc-jet coupling in an atoll-type neutron star X-ray binary: 4U 1728–34 (GX 354–0)
S Migliari, RP Fender, M Rupen, PG Jonker, M Klein-Wolt, RM Hjellming, ...
Monthly Notices of the Royal Astronomical Society 342 (4), L67-L71, 2003
1042003
A radio parallax to the black hole X-ray binary MAXI J1820+ 070
P Atri, JCA Miller-Jones, A Bahramian, RM Plotkin, AT Deller, PG Jonker, ...
Monthly Notices of the Royal Astronomical Society: Letters 493 (1), L81-L86, 2020
1022020
Broadband X-Ray Spectra of GX 339–4 and the Geometry of Accreting Black Holes in the Hard State
JA Tomsick, E Kalemci, P Kaaret, S Markoff, S Corbel, S Migliari, ...
The Astrophysical Journal 680 (1), 593, 2008
1022008
The complete spectrum of the neutron star X-ray binary 4U 0614+ 091
S Migliari, JA Tomsick, JCA Miller-Jones, S Heinz, RI Hynes, RP Fender, ...
The Astrophysical Journal 710 (1), 117, 2010
992010
A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni
JCA Miller-Jones, AJ Tetarenko, GR Sivakoff, MJ Middleton, D Altamirano, ...
Nature 569 (7756), 374-377, 2019
962019
Baryons in the relativistic jets of the stellar-mass black-hole candidate 4U 1630-47
MD Trigo, JCA Miller-Jones, S Migliari, JW Broderick, T Tzioumis
Nature 504 (7479), 260-262, 2013
962013
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