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Related papers: On the PSR B1133+16 optical counterpart

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We report detection of PSR B0656$+$14 with the Gran Telescopio Canarias in narrow optical $F657$, $F754$, $F802$, and $F902$ and near-infrared $JHK_s$ bands. The pulsar detection in the $K_s$ band extends its spectrum to 2.2 $\mu$m and…

High Energy Astrophysical Phenomena · Physics 2021-01-27 S. Zharikov , D. Zyuzin , Yu. Shibanov , A. Kirichenko , R. E. Mennickent , S. Geier , A. Cabrera-Lavers

We report the analysis of the first deep optical observations of three isolated $\gamma$-ray pulsars detected by the {\em Fermi Gamma-ray Space Telescope}: the radio-loud PSR\, J0248+6021 and PSR\, J0631+1036, and the radio-quiet PSR\,…

High Energy Astrophysical Phenomena · Physics 2016-09-07 R. P. Mignani , N. Rea , V. Testa , M. Marelli , A. De Luca , M. Pierbattista , A. Shearer , D. F. Torres , E. De Ona Wilhelmi

PSR J0205+6449 is a young ({\approx} 5400 years), Crab-like pulsar detected in radio and at X and {\gamma}-ray energies and has the third largest spin-down flux among known rotation powered pulsars. It also powers a bright synchrotron…

High Energy Astrophysical Phenomena · Physics 2015-06-16 P. Moran , R. P. Mignani , S. Collins , A. de Luca , N. Rea , A. Shearer

We carried out deep optical observations of the middle-aged $\gamma$-ray pulsar PSR J1741-2054 with the Very Large Telescope (VLT). We identified two objects, of magnitudes $m_v=23.10\pm0.05$ and $m_v=25.32\pm0.08$, at positions consistent…

High Energy Astrophysical Phenomena · Physics 2016-07-20 R. P. Mignani , V. Testa , M. Marelli , A. De Luca , D. Salvetti , A. Belfiore , M. Pierbattista , M. Razzano , A. Shearer , P. Moran

The radio and gamma-ray pulsar PSR J2032+4127 was recently found to be in a decades-long orbit with the Be star MT91 213, with the pulsar moving rapidly towards periastron. This binary shares many similar characteristics with the previously…

Solar and Stellar Astrophysics · Physics 2016-10-26 Wynn C. G. Ho , C. -Y. Ng , Andrew G. Lyne , Ben W. Stappers , Malcolm J. Coe , Jules P. Halpern , Tyrel J. Johnson , Iain A. Steele

We detected a nearby (d=360 pc), old (5 Myr) pulsar B1133+16 with Chandra. The observed pulsar's flux is $(0.8\pm 0.2)\times 10^{-14}$ ergs cm$^{-2}$ s$^{-1}$ in the 0.5-8 keV band. Because of the small number of counts detected, the…

Astrophysics · Physics 2014-10-13 O. Kargaltsev , G. G. Pavlov , G. P. Garmire

We report the B band optical observations of an old (17.5 Myr) radiopulsar PSR B0950+08 obtained with the Suprime-Cam at the Subaru telescope. We detected a faint object, B=27.07(16). Within our astrometrical accuracy it coincides with the…

PSR J1357$-$6429 is a young radio pulsar that was detected in X-rays and $\gamma$-rays. We present the high spatial resolution near-infrared imaging of the pulsar field in $J$, $H$ and $K_s$ bands obtained with the VLT/NaCo using the…

Solar and Stellar Astrophysics · Physics 2016-02-19 D. Zyuzin , S. Zharikov , Yu. Shibanov , A. Danilenko , R. E. Mennickent , A. Kirichenko

The young radio pulsar J1124-5916 is associated with a Cas A like supernova remnant G292.0+1.8. It powers a compact torus-like pulsar wind nebula with a jet first detected in X-rays and then identified in the optical and mid-infrared. We…

Solar and Stellar Astrophysics · Physics 2015-06-15 Sergey V. Zharikov , Dmitry A. Zyuzin , Yuri A. Shibanov , Ronald E. Mennickent

The Fermi Large Area Telescope (LAT) discovered the time signature of a radio-silent pulsar coincident with RX J0007.0+7302, a plerion-like X-ray source at the centre of the CTA 1 supernova remnant. The inferred timing parameters of the…

High Energy Astrophysical Phenomena · Physics 2015-06-12 R. P. Mignani , A. de Luca , N. Rea , A. Shearer , S. Collins , D. F. Torres , D. Hadasch , A. Caliandro

An unidentified $\gamma$-ray source 4FGL J1838.2+3223 has been proposed as a pulsar candidate. We present optical time-series multi-band photometry of its likely optical companion obtained with the 2.1-m telescope of Observatorio…

High Energy Astrophysical Phenomena · Physics 2023-11-20 D. A. Zyuzin , A. Yu. Kirichenko , A. V. Karpova , Yu. A. Shibanov , S. V. Zharikov , M. R. Gilfanov , C. Perez Tórtola

We present optical data gathered by the VLT Test Camera in the V-band at the radio (interferometric) position of PSR1706-44. We find no optical counterpart to the pulsar in the VLT image. At a distance of 2.7 arcsec from a nearby bright…

Astrophysics · Physics 2011-02-09 Peter Lundqvist , Jesper Sollerman , Alak Ray , Bruno Leibundgut , Firoza Sutaria

We have searched deep optical images of the globular cluster M4 for a possible optical counterpart for the third body in the PSR B1620-26 system. We identify as a possible optical counterpart a star located within $0.3''$ of the nominal…

Astrophysics · Physics 2009-10-22 C. D. Bailyn , E. P. Rubenstein , T. M. Girard , D. Dinescu , F. A. Rasio , B. Yanny

We analyse archival optical data on the binary companion to the millisecond pulsar \j1045\ obtained with the Very Large Telescope. A possible optical counterpart candidate %source position coincides with the pulsar coordinates is found at…

Solar and Stellar Astrophysics · Physics 2023-07-11 A. V. Bobakov , D. A. Zyuzin , Yu. A. Shibanov

PSRB1055-52 is a middle-aged (~535 kyr) radio, X-ray, and gamma-ray pulsar showing X-ray thermal emission from the neutron star (NS) surface. A candidate optical counterpart to PSRB1055-52 was proposed by Mignani and coworkers based on…

High Energy Astrophysical Phenomena · Physics 2015-05-19 R. P. Mignani , G. G. Pavlov , O. Kargaltsev

We present the results of deep optical imaging of the radio/$\gamma$-ray pulsar PSR J2043+2740, obtained with the Large Binocular Telescope (LBT). With a characteristic age of 1.2 Myr, PSR J2043+2740 is one of the oldest (non recycled)…

High Energy Astrophysical Phenomena · Physics 2017-11-15 V. Testa , R. P. Mignani , N. Rea , M. Marelli , D. Salvetti , A. A. Breeveld , F. Cusano , R. Carini

G292.0+1.8 is a Cas A-like supernova remnant that contains the young pulsar PSR J1124-5916 powering a compact torus-like pulsar wind nebula visible in X-rays. A likely counterpart to the nebula has been detected in the optical VRI bands. To…

High Energy Astrophysical Phenomena · Physics 2010-10-11 D. A. Zyuzin , A. A. Danilenko , S. V. Zharikov , Yu. A. Shibanov

(Abridged) PSR J1357-6429 is a Vela-like radio pulsar that has been recently detected in X-rays and gamma-rays. It powers a compact tail-like X-ray pulsar wind nebula and X-ray-radio plerion associated with an extended TeV source HESS…

Solar and Stellar Astrophysics · Physics 2012-04-26 A. Danilenko , A. Kirichenko , R. E. Mennickent , G. Pavlov , Yu. Shibanov , S. Zharikov , D. Zyuzin

We report on deep BVR-imaging of the field of the nearby millisecond pulsar PSR J0030+0451 obtained with the ESO/VLT/FORS2. We do not detect any optical counterpart down to B>27.3, V>27.0 and R>27.0 in the immediate vicinity of the radio…

Astrophysics · Physics 2009-11-07 A. B. Koptsevich , P. Lundqvist , N. I. Serafimovich , Yu. A. Shibanov , J. Sollerman

We report the results of our search for the near infrared counterpart of the microquasar 1E 1740.7-2942 using the VLT (Based on observations collected at the European Southern Observatory, Chile (ESO No 63.H-0261)). For the first time,…

Astrophysics · Physics 2007-05-23 Josep Marti , I. Felix Mirabel , Sylvain Chaty , Luis F. Rodriguez