Zobrazeno 1 - 10
of 26
pro vyhledávání: '"M Serim"'
We present a timing and noise analysis of the Be/X-ray binary system Swift J0243.6+6124 during its 2017-2018 super-Eddington outburst using NICER/XTI observations. We apply a synthetic pulse timing analysis to enrich the Fermi/GBM spin frequency hist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04a73cf90c79d21dd8beb46d3d999ac1
http://arxiv.org/abs/2304.11937
http://arxiv.org/abs/2304.11937
We investigate timing and spectral characteristics of the transient X-ray pulsar 2S 1417$-$624 during its 2018 outburst with \emph{NICER} follow up observations. We describe the spectra with high-energy cut-off and partial covering fraction absorptio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4dce8ab48397cd8b7718ada39dabe8cb
https://aperta.ulakbim.gov.tr/record/233272
https://aperta.ulakbim.gov.tr/record/233272
We probe the properties of the transient X-ray pulsar MAXI J1409$-$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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54c4536d24d16ce4b4ad15dbc6fd2eb8
http://arxiv.org/abs/1911.02871
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::552d330f25e1aa732cc137316a49e55b
https://aperta.ulakbim.gov.tr/record/71803
https://aperta.ulakbim.gov.tr/record/71803
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f576cd9300be622d75e8c58f5b518763
http://arxiv.org/abs/1706.00727
http://arxiv.org/abs/1706.00727
Publikováno v:
Scopus-Elsevier
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7583da07333852333c52d8f3852291ec
http://arxiv.org/abs/1701.04332
http://arxiv.org/abs/1701.04332
Publikováno v:
Scopus-Elsevier
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c4751ee54d8db579d1b1fe7a0ab97dfd
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad19883a23a656952f6f4bd14264e172
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 434:2772-2778
We analyze \emph{RXTE} and \emph{Swift} observations of SWIFT J1729.9$-$3437 after its outburst from 2010 July 20 to 2010 August 12. We calculate a spin frequency and spin frequency derivative of $1.8734(8) \times 10^{-3}$ Hz and $6.42(6) \times 10^{
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d40d66b879c49e7751eb045afec265a6
https://doi.org/10.1093/mnras/stt1127
https://doi.org/10.1093/mnras/stt1127
