International audienceAims. We aim to investigate the flux density modulation from pulsars and the specific behaviour of the modulation index versus frequency. Methods. Several pulsars were observed with the Effelsberg radio telescope at 8.35 GHz. Their flux density time series were corrected for interstellar scintillation effects. Results. We present measurements of modulation indices for eight pulsars. We confirm the presence of a critical frequency at ∼1 GHz for these pulsars (including three new ones from this study). We derived intrinsic modulation indices for the resulting flux density time series. Our data analysis revealed strong single pulses detected from five pulsars
Both the physics of the pulsar emission mechanism and free-free absorption in the intervening inters...
© 2016 ESO. We report the detection of 48 millisecond pulsars (MSPs) out of 75 observed thus far usi...
Context.A large sample of pulsars has been observed to study their subpulse modulation at an observi...
International audienceAims. We aim to investigate the flux density modulation from pulsars and the s...
Aims. We aim to investigate the flux density modulation from pulsars and the specific behaviour of t...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
This Letter explores the possibility of testing pulsar radio emission models by observing pulse-to-p...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
We report on the pulse-to-pulse energy distributions and phase-resolved modulation properties for ca...
The Parkes telescope has been monitoring 286 radio pulsars approximately monthly since 2007 at an ob...
In this paper we report multi-frequency measurements of pulse broadening times Τdfor nine medium dis...
. Monitoring of the flux-densities near 30 GHz are reported for four pulsars. Apparently random vari...
We present low-frequency spectral energy distributions of 60 known radio pulsars observed with the M...
Both the physics of the pulsar emission mechanism and free-free absorption in the intervening inters...
© 2016 ESO. We report the detection of 48 millisecond pulsars (MSPs) out of 75 observed thus far usi...
Context.A large sample of pulsars has been observed to study their subpulse modulation at an observi...
International audienceAims. We aim to investigate the flux density modulation from pulsars and the s...
Aims. We aim to investigate the flux density modulation from pulsars and the specific behaviour of t...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
This Letter explores the possibility of testing pulsar radio emission models by observing pulse-to-p...
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission...
We report on the pulse-to-pulse energy distributions and phase-resolved modulation properties for ca...
The Parkes telescope has been monitoring 286 radio pulsars approximately monthly since 2007 at an ob...
In this paper we report multi-frequency measurements of pulse broadening times Τdfor nine medium dis...
. Monitoring of the flux-densities near 30 GHz are reported for four pulsars. Apparently random vari...
We present low-frequency spectral energy distributions of 60 known radio pulsars observed with the M...
Both the physics of the pulsar emission mechanism and free-free absorption in the intervening inters...
© 2016 ESO. We report the detection of 48 millisecond pulsars (MSPs) out of 75 observed thus far usi...
Context.A large sample of pulsars has been observed to study their subpulse modulation at an observi...