activity
20092021
most citedX-ray bursting neutron star atmosphere models: spectra and color corrections

144 citations · 660 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2021★ 13 cited

Middle aged -ray pulsar J1957+5033 in X-rays: pulsations, thermal emission and nebula

D. A. Zyuzin, A. V. Karpova, Y. A. Shibanov +2

We analyze new XMM-Newton and archival Chandra observations of the middle-aged -ray radio-quiet pulsar J1957+5033. We detect, for the first time, X-ray pulsations with the pulsa…

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.HE2017★ 20 cited

Probing the possibility of hotspots on the central neutron star in HESS J1731-347

V. F. Suleimanov, D. Klochkov, J. Poutanen +1

The X-ray spectra of the neutron stars located in the centers of supernova remnants Cas A and HESS J1731-347 are well fit with carbon atmosphere models. These fits yield plausible…

astro-ph.HE2016★ 38 cited

Detection of burning ashes from thermonuclear X-ray bursts

J. J. E. Kajava, J. Nättilä, J. Poutanen +3

When neutron stars (NS) accrete gas from low-mass binary companions, explosive nuclear burning reactions in the NS envelope fuse hydrogen and helium into heavier elements. The resu…

astro-ph.HE2015★ 37 cited

Measuring the basic parameters of neutron stars using model atmospheres

V. F. Suleimanov, J. Poutanen, D. Klochkov +1

Model spectra of neutron star atmospheres are nowadays widely used to fit the observed thermal X-ray spectra of neutron stars. This fitting is the key element in the method of the…

astro-ph.HE2015★ 135 cited

Equation of state constraints for the cold dense matter inside neutron stars using the cooling tail method

J. Nättilä, A. W. Steiner, J. J. E. Kajava +2

The cooling phase of thermonuclear (type-I) X-ray bursts can be used to constrain the neutron star (NS) compactness by comparing the observed cooling tracks of bursts to accurate t…