We study flux and spectral variability of the high energy peaked TeV blazar PG 1553 + 113 on diverse timescales using the data collected from 2005 to 2019 which also includes the intensive intra-night monitoring of the target. Additionally, we recorded the brightest flare of the blazar PG 1553 + 113 during April 2019 when the source attained an R-band magnitude of 13.2. Analyzing the spectral evolution of the source during the flare gave a clockwise spectral hysteresis loop and a time lag with V-band variations leading to the R-band ones. Various statistical tests, fitting procedures and cross-correlation techniques are applied to search for periodicity and examine the color-magnitude relationship. We find a median period of (2.21 ± 0.04) y...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) gamma-ray emitter classified as a BL Lac object...
PG 1553+113 is a very-high-energy (VHE, E>100 GeV) gamma-ray emitter classified as a BL Lac object. ...
PG1553+113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray ban...
We study flux and spectral variability of the high energy peaked TeV blazar PG 1553 + 113 on diverse...
Context. The TeV BL Lac object PG 1553+113 is one of the primary candidates for a binary supermassiv...
We report the flux and spectral variability of PG 1553+113 on intra-night (IDV) to short-term timesc...
We report the results from our study of the blazar S5 1803+784 carried out using the quasi-simultane...
Context. Observations of very high-energy γ-rays from blazars provide information about acceleration...
Context. The TeV BL Lac object PG1553+113 is one of the primary candidates for a binary supermassive...
PKS 2155-304 is a blazar located in the Southern Hemisphere, monitored with the High Energy Stereosc...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) \u3b3-ray emitter classified as a BL Lac object...
Blazars are known to emit exceptionally variable non-thermal emission over the wide range (from radi...
PG 1553+113 is a very-high-energy (VHE, $E>100\,\mathrm{GeV}$) $\gamma$-ray emitter classified as a ...
We present our optical photometric observations of three TeV blazars, PKS 1510-089, PG 1553+113, and...
Abstract: PG 1553+113 is a well-known TeV blazar, whose redshift is still uncertain (z>0.4, [1])....
PG 1553+113 is a very high energy (VHE, E > 100 GeV) gamma-ray emitter classified as a BL Lac object...
PG 1553+113 is a very-high-energy (VHE, E>100 GeV) gamma-ray emitter classified as a BL Lac object. ...
PG1553+113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray ban...
We study flux and spectral variability of the high energy peaked TeV blazar PG 1553 + 113 on diverse...
Context. The TeV BL Lac object PG 1553+113 is one of the primary candidates for a binary supermassiv...
We report the flux and spectral variability of PG 1553+113 on intra-night (IDV) to short-term timesc...
We report the results from our study of the blazar S5 1803+784 carried out using the quasi-simultane...
Context. Observations of very high-energy γ-rays from blazars provide information about acceleration...
Context. The TeV BL Lac object PG1553+113 is one of the primary candidates for a binary supermassive...
PKS 2155-304 is a blazar located in the Southern Hemisphere, monitored with the High Energy Stereosc...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) \u3b3-ray emitter classified as a BL Lac object...
Blazars are known to emit exceptionally variable non-thermal emission over the wide range (from radi...
PG 1553+113 is a very-high-energy (VHE, $E>100\,\mathrm{GeV}$) $\gamma$-ray emitter classified as a ...
We present our optical photometric observations of three TeV blazars, PKS 1510-089, PG 1553+113, and...
Abstract: PG 1553+113 is a well-known TeV blazar, whose redshift is still uncertain (z>0.4, [1])....
PG 1553+113 is a very high energy (VHE, E > 100 GeV) gamma-ray emitter classified as a BL Lac object...
PG 1553+113 is a very-high-energy (VHE, E>100 GeV) gamma-ray emitter classified as a BL Lac object. ...
PG1553+113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray ban...