Search Results - "Kozlowski, Szymon"

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    A degeneracy in DRW modelling of AGN light curves by Kozlowski, Szymon

    “…Individual light curves of active galactic nuclei (AGNs) are nowadays successfully modelled with the damped random walk (DRW) stochastic process, characterized…”
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    Journal Article
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    REVISITING STOCHASTIC VARIABILITY OF AGNs WITH STRUCTURE FUNCTIONS by Koz owski, Szymon

    Published in The Astrophysical journal (01-08-2016)
    “…ABSTRACT Discrepancies between reported structure function (SF) slopes and their overall flatness as compared to the expectations from the damped random walk…”
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    Journal Article
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    A Method to Measure the Unbiased Decorrelation Timescale of the AGN Variable Signal from Structure Functions by Koz owski, Szymon

    Published in The Astrophysical journal (01-02-2017)
    “…A simple, model-independent method to quantify the stochastic variability of active galactic nuclei (AGNs) is the structure function (SF) analysis. If the SF…”
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    Mid-infrared Period–Luminosity Relations for Miras in the Large Magellanic Cloud by Iwanek, Patryk, Soszyński, Igor, Kozłowski, Szymon

    Published in The Astrophysical journal (01-10-2021)
    “…Abstract We present the mid-infrared (mid-IR) period–luminosity relations (PLRs) using over 1000 Mira variables in the Large Magellanic Cloud, for the four…”
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    No large population of unbound or wide-orbit Jupiter-mass planets by Mróz, Przemek, Udalski, Andrzej, Skowron, Jan, Poleski, Radosław, Kozłowski, Szymon, Szymański, Michał K., Soszyński, Igor, Wyrzykowski, Łukasz, Pietrukowicz, Paweł, Ulaczyk, Krzysztof, Skowron, Dorota, Pawlak, Michał

    Published in Nature (London) (10-08-2017)
    “…In an analysis of a large sample of microlensing events, a few suggest the existence of Earth-mass free-floating planets, but only the expected number of…”
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    The Proper Motion Field of the Small Magellanic Cloud: Kinematic Evidence for Its Tidal Disruption by Zivick, Paul, Kallivayalil, Nitya, van der Marel, Roeland P., Besla, Gurtina, Linden, Sean T., Koz owski, Szymon, Fritz, Tobias K., Kochanek, C. S., Anderson, J., Sohn, Sangmo Tony, Geha, Marla C., Alcock, Charles R.

    Published in The Astrophysical journal (01-09-2018)
    “…We present a new measurement of the systemic proper motion of the Small Magellanic Cloud (SMC), based on an expanded set of 30 fields containing background…”
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    From Brush to Dendritic Structure: Tool for Tunable Interfacial Compatibility between the Iron-Based Particles and Silicone Oil in Magnetorheological Fluids by Kozłowski, Szymon, Osička, Josef, Ilcikova, Marketa, Galeziewska, Monika, Mrlik, Miroslav, Pietrasik, Joanna

    Published in Langmuir (12-03-2024)
    “…Comprehensive magnetic particle stability together with compatibility between them and liquid medium (silicone oil) is still a crucial issue in the case of…”
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    Quasar Main Sequence in the UV Plane by niegowska, Marzena, Koz owski, Szymon, Czerny, Bo ena, Panda, Swayamtrupta, Hryniewicz, Krzysztof

    Published in The Astrophysical journal (01-09-2020)
    “…Active galaxies form a clear pattern in the optical plane showing the correlation between the FWHM of the Hβ line and the ratio of the equivalent width (EW) of…”
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    No massive black holes in the Milky Way halo by Mróz, Przemek, Udalski, Andrzej, Szymański, Michał K., Soszyński, Igor, Wyrzykowski, Łukasz, Pietrukowicz, Paweł, Kozłowski, Szymon, Poleski, Radosław, Skowron, Jan, Skowron, Dorota, Ulaczyk, Krzysztof, Gromadzki, Mariusz, Rybicki, Krzysztof, Iwanek, Patryk, Wrona, Marcin, Ratajczak, Milena

    Published in Nature (London) (22-08-2024)
    “…The gravitational wave detectors have shown a population of massive black holes that do not resemble those observed in the Milky Way 1 – 3 and whose origin is…”
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    QUASAR VARIABILITY IN THE MID-INFRARED by Koz owski, Szymon, Kochanek, Christopher S., Ashby, Matthew L. N., Assef, Roberto J., Brodwin, Mark, Eisenhardt, Peter R., Jannuzi, Buell T., Stern, Daniel

    Published in The Astrophysical journal (01-02-2016)
    “…ABSTRACT The Decadal IRAC Boötes Survey is a mid-IR variability survey of the ∼9 sq. deg. of the NDWFS Boötes Field and extends the time baseline of its…”
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