Aims: We investigate a high frequency turn-over effect in radio spectra for pulsars with positive or flat spectral index. Methods. Using GMRT and Effelsberg observatory, we estimated the flux density to reconstruct pulsar spectra. Results. We find objects that have a maximum flux in their spectrum above 1 GHz, whose emitted energy decreases below 1 GHz and whose spectral indices are positive at lower frequencies. Some pulsars with a turn-over in their spectrum at high frequencies are found to exist in very interesting environments. We call these objects gigahertz-peaked spectra pulsars
Measurements of pulsar flux densities are of great importance for understanding the pulsar emission ...
© 2017. The American Astronomical Society. All rights reserved. We present a sample of 1483 sources ...
We present the results of the first low frequency measurements of the flux densities of a large samp...
Aims.The main aim is to investigate the possibility of a high frequency turn-over in the radio spec...
Aims.The main aim is to investigate the possibility of a high frequency turn-over in the radio spect...
Abstract. We have collected pulsar flux density observa-tions and compiled spectra of 281 objects. T...
We present the results of our radio interferometric observations of pulsars at 325 and 610 MHz using...
In this paper, we present results from flux-density measurements for 21 pulsars over a wide frequenc...
The flux density spectra of radio pulsars are known to be steep and, to first order, de-scribed by a...
Pulsars are known to emit non-thermal radio emission that is generally a power-law function of frequ...
We conducted radio interferometric observations of six pulsars at 610 MHz using the Giant Metrewave ...
We present pulse shapes of 87 pulsars at 4.85 GHz. Pulse widths and flux densities are measured. The...
Aims.The behaviour of the pulsar spectrum at high radio frequencies can provide decisive information...
New radio spectra of High Frequency Peakers (HFP) obtained from the Jansky Very Large Array (JVLA) s...
The results of a comprehensive analysis of continuous radio spectra of a sample of Gigahertz-Peaked ...
Measurements of pulsar flux densities are of great importance for understanding the pulsar emission ...
© 2017. The American Astronomical Society. All rights reserved. We present a sample of 1483 sources ...
We present the results of the first low frequency measurements of the flux densities of a large samp...
Aims.The main aim is to investigate the possibility of a high frequency turn-over in the radio spec...
Aims.The main aim is to investigate the possibility of a high frequency turn-over in the radio spect...
Abstract. We have collected pulsar flux density observa-tions and compiled spectra of 281 objects. T...
We present the results of our radio interferometric observations of pulsars at 325 and 610 MHz using...
In this paper, we present results from flux-density measurements for 21 pulsars over a wide frequenc...
The flux density spectra of radio pulsars are known to be steep and, to first order, de-scribed by a...
Pulsars are known to emit non-thermal radio emission that is generally a power-law function of frequ...
We conducted radio interferometric observations of six pulsars at 610 MHz using the Giant Metrewave ...
We present pulse shapes of 87 pulsars at 4.85 GHz. Pulse widths and flux densities are measured. The...
Aims.The behaviour of the pulsar spectrum at high radio frequencies can provide decisive information...
New radio spectra of High Frequency Peakers (HFP) obtained from the Jansky Very Large Array (JVLA) s...
The results of a comprehensive analysis of continuous radio spectra of a sample of Gigahertz-Peaked ...
Measurements of pulsar flux densities are of great importance for understanding the pulsar emission ...
© 2017. The American Astronomical Society. All rights reserved. We present a sample of 1483 sources ...
We present the results of the first low frequency measurements of the flux densities of a large samp...