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We report the detection of high polarization in the first detailed optical linear polarization measurements on the BL Lac object CGRaBS J0211+1051, which flared in $\gamma$-rays on 2011 January 23 as reported by Fermi. The observations were…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Sunil Chandra , Kiran S Baliyan , Shashikiran Ganesh , Umesh Joshi

Long-term (up to 10000d) monitoring has been undertaken for 41 Seyferts in the near-IR (JHKL). All but 2 showed variability, with K ampl in the range <0.1 to > 1.1 mags. The timescale for detectable change is from about one week to a few…

Astrophysics · Physics 2009-11-10 I. S. Glass

We present the results of a multi-frequency analysis of the structural variability in the parsec-scale jet of the blazar S5 1803+784. More than 90 epochs of observations at 6 frequencies from 1.6 GHz up to 22 GHz have been combined and…

The distribution of ultra-narrow linewidth laser radiation is an integral part of many challenging metrological applications. Changes in the optical pathlength induced by environmental disturbances compromise the stability and accuracy of…

Instrumentation and Detectors · Physics 2018-07-31 Benjamin Rauf , Maria Carmen Velez Lopez , Pierre Thoumany , Marco Pizzocaro , Davide Calonico

The radio, optical, and $\gamma$-ray light curves of the blazar S5 1803+784, from the beginning of the {\it Fermi} Large Area Telescope (LAT) mission in August 2008 until December 2018, are presented. The aim of this work is to look for…

High Energy Astrophysical Phenomena · Physics 2021-03-03 R. Nesci , S. Cutini , C. Stanghellini , F. Martinelli , A. Maselli , V. M. Lipunov , V. Kornilov , R. R. Lopez , A. Siviero , M. Giroletti , M. Orienti

The goal of our work is to study the mode changes of the radio-quiet gamma-ray pulsar PSR J2021+4026 with improved detail. By accurately characterizing variations in the gamma-ray spectrum and pulse profile, we aim to relate the Fermi-LAT…

High Energy Astrophysical Phenomena · Physics 2024-03-13 A. Fiori , M. Razzano , A. K. Harding , M. Kerr , R. P. Mignani , P. M. Saz Parkinson

Variability is a typical observation feature of Fermi blazars, sometimes it shows quasi-periodic oscillation (QPO). In this work, we obtained 5-day binned light curves (with a time coverage of $\sim$ 12.9 yr) for S5 1044+71 based on Fermi…

High Energy Astrophysical Phenomena · Physics 2022-04-27 G. G. Wang , J. T. Cai , J. H. Fan

A polarization switching pulse interleaver is shown to be effective in reducing timing noise due to polarization mode dispersion in time and frequency transfer based on mode-locked lasers and standard single-mode fibres. In closed-loop time…

We present a detailed statistical analysis of the alignment of polarizations of radio sources at high redshift. We use the JVAS/CLASS 8.4-GHz surveys for our study. This study is motivated by the puzzling signal of alignment of…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-20 Prabhakar Tiwari , Pankaj Jain

IRAS 22568+6141 has been classified as a low-ionisation planetary nebula (PN) and presents non-thermal radio continuum emission, which could be a signature of nascent PNe. We present intermediate-resolution long-slit spectra obtained in…

We report optical and X-ray observations of the high-field polar RXJ1007.5-2017 performed between 1990 and 2012. It has an orbital period of 208.60 min determined from the ellipsoidal modulation of the secondary star in an extended low…

High Energy Astrophysical Phenomena · Physics 2015-06-11 H. -C. Thomas , K. Beuermann , K. Reinsch , A. D. Schwope , V. Burwitz

In this paper, the post-1977 photometric observations of PKS 2155-304 are compiled and used to discuss the variation periodicity. Largest amplitude variations ($\Delta U = 1^{m}.5$; $\Delta B = 1^{m}.65$; $\Delta V = 1^{m}.85 $; $\Delta R =…

Astrophysics · Physics 2007-05-23 J. H. Fan , R. G. Lin

We present the results of optical (R band) photometric and polarimetric monitoring and Very Long Baseline Array (VLBA) imaging of the blazar S5 0716+714 along with Fermi gamma-ray data during a multi-waveband outburst in 2011 October. We…

We present photometric and spectroscopic observations of the cataclysmic variable MASTER OT J132104.04+560957.8 which strongly indicate that it is a polar with an orbital period of 91 minutes. The optical light curve shows two maxima and…

Solar and Stellar Astrophysics · Physics 2014-12-30 Colin Littlefield , Peter Garnavich , Katrina Magno , Marc Murison , Shanel Deal , Colin McClelland , Benjamin Rose

We report the detection of phase-locked polarization in the bright ($m_V$=2.98-3.24) semidetached eclipsing binary $\mu^1$ Sco (HD 151890). The phenomenon was observed in multiple photometric bands using two different HIPPI-class (HIgh…

Solar and Stellar Astrophysics · Physics 2020-07-22 Daniel V. Cotton , Jeremy Bailey , Lucyna Kedziora-Chudczer , Ain De Horta

The ~15.1 years period found in the long-term UBV photoelectric and photographic photometry of the symbiotic nova V1016 Cyg is detected also in the (J-K) colour index and in the UV continuum and emission line fluxes from IUE and HUT…

Astrophysics · Physics 2009-11-07 S. Parimucha , D. Chochol , T. Pribulla , L. M. Buson , A. A. Vittone

The correlation between optical and $\gamma$-ray flux variations in blazars reveals a complex behaviour. In this study, we present our analysis of the connection between changes in optical and $\gamma$-ray emissions in the blazar Ton 599…

High Energy Astrophysical Phenomena · Physics 2023-12-25 Bhoomika Rajput , Amit Kumar Mandal , Ashwani Pandey , C. S. Stalin , Walter Max-Moerbeck , Blesson Mathew

We present a detailed analysis of 30 very long baseline interferometric observations of the BL Lac object S5 1803+784 (z=0.679), obtained between mean observational time 1994.67 and 2012.91 at observational frequency 15 GHz. The long-term…

High Energy Astrophysical Phenomena · Physics 2018-09-12 E. Kun , M. Karouzos , K. É. Gabányi , S. Britzen , O. M. Kurtanidze , L. Á. Gergely

In this work, we present the first results of a study of a new sample of 7 polar candidates from polarimetric data obtained at the Pico dos Dias / LNA observatory. From the four polars analysed so far, we confirm the presence of high and…

Solar and Stellar Astrophysics · Physics 2014-01-31 K. M. G. Silva , C. V. Rodrigues , J. E. R. Costa , D. Cieslinski , L. A. Almeida , V. S. Magalhães

We present a multi-wavelength spectral and temporal investigation of OJ 287 emission during its strong optical-to-X-ray activity between July 2016 - July 2017. The daily $\gamma$-ray fluxes from \emph{Fermi}-LAT are consistent with no…