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We present the results of polarimetric ($R$ band) and multicolor photometric ($BVRIJHK$) observations of the blazar AO 0235+16 during an outburst in 2006 December. The data reveal a short timescale of variability (several hours), which…

We report on dual-frequency radio polarimetry observations of two young, energetic pulsars, PSRs J0940-5428 and J1301-6305. These were among the first Vela-like pulsars discovered in the Parkes Multibeam survey. We conducted observations of…

Astrophysics · Physics 2008-11-26 F. Crawford , C. L. Tiffany

We aim to detect low-frequency radio emission from exoplanetary systems, which can provide insights into planetary magnetic fields, star-planet interactions, stellar activity, and exo-space weather. The HD 189733 system, hosting a…

We analyze and model rapid rotations of polarization orientations in PSR B1919+21's single pulses based on Five-hundred-meter Aperture Spherical radio Telescope observation data. In more than one-third of B1919+21's single pulses, the…

High Energy Astrophysical Phenomena · Physics 2025-04-04 Shunshun Cao , Jinchen Jiang , Jaroslaw Dyks , Kejia Lee , Jiguang Lu , Lucy S. Oswald , Weiyang Wang , Renxin Xu

With the ever-increasing sensitivity and timing baselines of modern radio telescopes, a growing number of pulsars are being shown to exhibit transitions in their rotational and radio emission properties. In many of these cases, the two are…

High Energy Astrophysical Phenomena · Physics 2022-05-11 B. Shaw , B. W. Stappers , P. Weltevrede , P. R. Brook , A. Karastergiou , C. A. Jordan , M. J. Keith , M. Kramer , A. G. Lyne

We aim to study the nature of the faint, polarised radio source population whose source composition and redshift dependence contain information about the strength, morphology, and evolution of magnetic fields over cosmic timescales. We use…

Cosmology and Nongalactic Astrophysics · Physics 2021-09-29 A. Berger , B. Adebahr , N. Herrera Ruiz , A. H. Wright , I. Prandoni , R. -J. Dettmar

We study the correlations between the jet ejection event and changes in the continuum emission of the radio-loud galaxy 3C 390.3, using the archived monitoring data in radio, optical and X-ray. We present evidence for the link between the…

Astrophysics · Physics 2008-11-26 Tigran G. Arshakian , Tomaso Belloni

In May 2007 the compact radio source Sgr A* was observed in a global multi-frequency monitoring campaign, from radio to X-ray bands. Here we present and discuss first and preliminary results from polarization sensitive VLBA observations,…

Astrophysics · Physics 2014-11-18 R. -S. Lu , T. P. Krichbaum , A. Eckart , S. König , D. Kunneriath , G. Witzel , A. Witzel , J. A. Zensus

New VLA detections of the variable radio continuum source VLA J181335.1$-$174957, associated with the energetic X-ray pulsar PSR~J1813$-$1749 and the TeV source HESS J1813-178, are presented. The radio source has a right circular…

High Energy Astrophysical Phenomena · Physics 2018-10-24 Sergio A. Dzib , Luis F. Rodríguez , Ramesh Karupussamy , Laurent Loinard , Sac-Nicté X. Medina

Narrow line Seyfert 1 galaxies (NLSy1s) constitute the AGN subclass associated with systematically smaller black hole masses. A few radio loud ones have been detected in MeV -- GeV energy bands by Fermi and evidence for the presence of…

Astrophysics of Galaxies · Physics 2018-10-23 E. Angelakis , S. Kiehlmann , I. Myserlis , D. Blinov , J. Eggen , R. Itoh , N. Marchili , J. A. Zensus

The polarisation properties of the intrinsically small (< 20 kpc) radio sources are briefly discussed. At centimetric and decimetric wavelengths, substantial polarised emission is often detected in quasars and, at a lower level, in radio…

Astrophysics · Physics 2007-05-23 D. Dallacasa

The radiation by relativistic plasma particles is beamed in the direction of field line tangents in the corotating frame, but in an inertial frame it is aberrated toward the direction of rotation. We have revised the relation of aberration…

Astrophysics · Physics 2007-05-23 R. T. Gangadhara

We present multiepoch VLBA observations of the compact jet of GRS 1915+105 conducted at 15.0 and 8.4 GHz during a {\it plateau} state of the source in 2003 March-April. These observations show that the compact jet is clearly asymmetric.…

Astrophysics · Physics 2007-05-23 M. Ribo , V. Dhawan , I. F. Mirabel

We report the first detection of polarization angle (PA) orthogonal jumps, a phenomenon previously only observed from radio pulsars, from a fast radio burst (FRB) source FRB 20201124A. We find three cases of orthogonal jumps in over two…

Microstructure emission, involving short time scale, often quasi-periodic, intensity fluctuations in subpulse emission, is well known in normal period pulsars. In this letter, we present the first detections of quasi-periodic microstructure…

High Energy Astrophysical Phenomena · Physics 2016-12-06 Kishalay De , Yashwant Gupta , Prateek Sharma

Recent observations of the periodic Fast Radio Burst source 180916.J0158+65 (FRB 180916) find small linear polarization position angle swings during and between bursts, with a burst activity window that becomes both narrower and earlier at…

High Energy Astrophysical Phenomena · Physics 2021-03-24 Dongzi Li , J. J. Zanazzi

Time-resolved optical and infrared polarimetric observations of black hole and neutron star low-mass X-ray binaries are presented. Data were acquired with the VLT, UKIRT and HIPPO on the SAAO 1.9-m. We find that for some sources in…

High Energy Astrophysical Phenomena · Physics 2015-03-19 David M. Russell , Piergiorgio Casella , Rob Fender , Paolo Soleri , Magaretha L. Pretorius , Fraser Lewis , Michiel van der Klis

We report on results of a multi-band monitoring campaign from radio to gamma rays of the high-redshift flat spectrum radio quasar S5 0836+710 during a high activity period detected by the Large Area Telescope on board the Fermi Gamma-ray…

High Energy Astrophysical Phenomena · Physics 2019-11-06 M. Orienti , F. D'Ammando , M. Giroletti , D. Dallacasa , G. Giovannini , S. Ciprini

QS Vir is a low-accretion rate cataclysmic variable (CV), or pre-CV, as the M dwarf companion is just filling its Roche lobe. We recently identified radio emission from QS Vir in the Very Large Array Sky Survey, at a flux of ~1 mJy. The…

High Energy Astrophysical Phenomena · Physics 2025-03-12 M. E. Ridder , A. K. Hughes , C. O. Heinke , G. R. Sivakoff , R. D. Sydora

In this study, we report multi-year polarization measurements of four repeating FRBs initially discovered by CHIME: FRBs~20190117A, 20190208A, 20190303A, and 20190417A. We observed the four repeating FRBs with FAST, detecting a total of 66…