Zobrazeno 1 - 10
of 82
pro vyhledávání: '"İnam, S. Ç."'
Autor:
Serim, M. M., Ozudogru, O. C., Donmez, C. K., Sahiner, S., Serim, D., Baykal, A., Inam, S. C.
We investigate timing and spectral characteristics of the transient X-ray pulsar 2S 1417$-$624 during its 2018 outburst with \emph{NICER} follow up observations. We describe the spectra with high-energy cut-off and partial covering fraction absorptio
Externí odkaz:
http://arxiv.org/abs/2107.14492
We probe the properties of the transient X-ray pulsar MAXI J1409$-$619 through \textit{RXTE} and \textit{Swift} follow up observations of the outburst in 2010. We are able to phase connect the pulse arrival times for the 25 days episode during the ou
Externí odkaz:
http://arxiv.org/abs/1911.02871
Using \emph{RXTE}, \emph{Chandra}, \emph{XMM-Newton} and \emph{Swift} observations, we for the first time construct the power spectra and torque noise strengths of magnetars. For some of the sources, we measure strong red noise on timescales months t
Externí odkaz:
http://arxiv.org/abs/1806.00401
We present timing analysis of the accretion powered pulsar SXP 1062, based on the observations of \textit{Swift}, \textit{XMM-Newton} and \textit{Chandra} satellites covering a time span of about 2 years. We obtain a phase coherent timing solution wh
Externí odkaz:
http://arxiv.org/abs/1706.00727
We analyse archival CGRO-BATSE X-ray flux and spin frequency measurements of GX 1+4 over a time span of 3000 days. We systematically search for time dependent variations of torque luminosity correlation. Our preliminary results indicate that the corr
Externí odkaz:
http://arxiv.org/abs/1701.04717
We represent noise strength analysis of Anomalous X-Ray Pulsars (AXPs) 4U 0142+61, 1RXS J170849.9-400910, 1E 1841-045, 1E 2259+586 and Soft Gamma Repeaters (SGRs) SGR J1833-0832, SWIFT J1822.3-1606 and SWIFT J1834.9-0846 together with the X-Ray binar
Externí odkaz:
http://arxiv.org/abs/1701.04332
We present analysis of RXTE--PCA observations of GX 1+4 between March 3, 2001 and January 31, 2003 together with the CGRO--BATSE X-ray flux and frequency derivative time series between 1991 and 1999. From the timing analysis of RXTE-PCA observations,
Externí odkaz:
http://arxiv.org/abs/1701.04328
We present timing and spectral analysis of \emph{Swift}$-$XRT and \emph{RXTE}$-$PCA observations of the transient Be/X-ray pulsar SWIFT J0513.4--6547 during its outburst in 2009 and its rebrightening in 2014. From 2009 observations, short term spin-u
Externí odkaz:
http://arxiv.org/abs/1509.01041
Autor:
Orlandini, M., Doroshenko, V., Zampieri, L., Bozzo, E., Baykal, A., Blay, P., Chernyakova, M., Corbet, R., D'Aì, A., Enoto, T., Ferrigno, C., Finger, M., Klochkov, D., Kreykenbohm, I., Inam, S. C., Jenke, P., Leyder, J. -C., Masetti, N., Manousakis, A., Mihara, T., Paul, B., Postnov, K., Reig, P., Romano, P., Santangelo, A., Shakura, N., Staubert, R., Torrejón, J. M., Walter, R., Wilms, J., Wilson-Hodge, C.
This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of high-mass X-ray binaries and ultra-luminous X-ray sour
Externí odkaz:
http://arxiv.org/abs/1501.02777
We present timing analysis of {\emph{RXTE}}-PCA and {\emph{INTEGRAL}}-ISGRI observations of X Per between 1998 and 2010. All pulse arrival times obtained from the {\emph{RXTE}}-PCA observations are phase connected and a timing solution is obtained us
Externí odkaz:
http://arxiv.org/abs/1405.3803