1.9k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.1k papers
- European Organization for Nuclear ResearchCH1.1k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT1k papers
- University of CagliariIT1k papers
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di FrascatiIT1k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR1k papers
- Heidelberg UniversityDE998 papers
- National Institute for Subatomic PhysicsNL997 papers
- University of BirminghamGB974 papers
- Institute of Nuclear Physics, Polish Academy of SciencesPL967 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BariIT956 papers
- University of LiverpoolGB935 papers
8 papers · 2 filters
Evidence of non-luminous matter in the center of M62
Federico Abbate, Andrea Possenti, Monica Colpi +1
Theoretical models suggest that intermediate mass black holes (IMBHs) may form and reside in the centers of globular clusters. IMBHs are still elusive to observations, but the acce…
New insights on the puzzling LMXB 1RXS J180408.9-342058: the intermediate state, the clocked type-I X-ray bursts and much more
A. Marino, M. Del Santo, M. Cocchi +7
1RXS J180408.9--342058 is a low mass X-ray binary hosting a neutron star, which shows X-ray activity at very different mass-accretion regimes, from very faint to almost the Eddingt…
X-ray dips and a complex UV/X-ray cross-correlation function in the black hole candidate MAXI J1820+070
J. J. E. Kajava, S. E. Motta, A. Sanna +3
MAXI J1820+070, a black hole candidate first detected in early March 2018, was observed by XMM-Newton during the outburst rise. In this letter we report on the spectral and timing…
Indications of non-conservative mass-transfer in AMXPs
A. Marino, T. Di Salvo, L. Burderi +7
Context. Since the discovery of the first Accreting Millisecond X-ray Pulsar SAX J1808.4-3658 in 1998, the family of these sources kept growing on. Currently, it counts 22 members.…
Updated orbital ephemeris of the ADC source X 1822-371: a stable orbital expansion over 40 years
S. M. Mazzola, R. Iaria, T. Di Salvo +6
The source X 1822-371 is an eclipsing compact binary system with a period close to 5.57 hr and an orbital period derivative of 1.51(7) s s$^{-1…
Spectral analysis of the dipping LMXB system XB 1916-053
A. F. Gambino, R. Iaria, T. Di Salvo +6
Context: XB 1916-053 is a low mass X-ray binary system (LMXB) hosting a neutron star (NS) and showing periodic dips. The spectrum of the persistent emission was modeled with a blac…
IGR J17503-2636: a candidate supergiant fast X-ray transient
C. Ferrigno, E. Bozzo, A. Sanna +4
IGR J17503-2636 is a hard X-ray transient discovered by INTEGRAL on 2018 August 11. This was the first ever reported X-ray emission from this source. Following the discovery, follo…
Study of the X-ray properties of the neutron-star binary 4U 172834 from the soft to hard state
Yanan Wang, Mariano Méndez, Diego Altamirano +7
We studied five XMM-Newton observations of the neutron-star binary 4U 172834 covering the hard, intermediate and soft spectral states. By jointly fitting the spectra with severa…