activity
20172026
most citedA Quasar microlensing event towards J1249+3449?

17 citations · 69 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE20264 cited

Timing analysis of a sample of five cataclysmic variable candidates observed by the XMM-Newton satellite

A. A. Nucita, S. M. Lezzi, F. De Paolis +4

Intermediate polars are a class of cataclysmic variables in which a white dwarf accretes material from a companion star. The intermediate polar nature confirmation usually derives…

astro-ph.HE2021

Optical Variability Correlated with X-ray Spectral Transition in the Black-Hole Transient ASASSN-18ey = MAXI J1820+070

Keito Niijima, Mariko Kimura, Yasuyuki Wakamatsu +49

How a black hole accretes matter and how this process is regulated are fundamental but unsolved questions in astrophysics. In transient black-hole binaries, a lot of mass stored in…

astro-ph.HE20203 cited

VZ Sex: X-ray confirmation of its intermediate polar nature

A. A. Nucita, F. De Paolis, D. Licchelli +3

Intermediate polars are members of the cataclysmic variable binary stars. They are characterized by a moderately magnetized white dwarf accreting matter from a cool main-sequence c…

astro-ph.HE20204 cited

HP Cet and Swift J0820.6-2805: two candidate intermediate polars observed by XMM-Newton

A. A. Nucita, F. De Paolis, F. Strafella +1

We report on the XMM-Newton observation of HP Cet and Swift J0820.6-2805, two X-ray photon sources that are candidates to be members of the intermediate polar class of cataclysmic…

astro-ph.HE201915 cited

DW Cancri in x-rays

A. A. Nucita, L. Conversi, D. Licchelli

We report on the -Newton observation of DW Cnc, a candidate intermediate polar candidate whose historical optical light curve shows the existence of periods at , $\…

astro-ph.HE20173 cited

Optical, near-IR and -ray observations of SN 2015J and its host galaxy

A. A. Nucita, F. De Paolis, R. Saxton +7

SN 2015J was discovered on April 27th 2015 and is classified as a type IIn supernova. At first, it appeared to be an orphan SN candidate, i.e. without any clear identification of i…