activity
20162020
most citedMulti-band behaviour of the TeV blazar PG 1553+113 in optical range on diverse timescales

23 citations · 60 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.HE202023 cited

Multi-band behaviour of the TeV blazar PG 1553+113 in optical range on diverse timescales

A. Agarwal, B. Mihov, I. Andruchow +11

Context. The TeV BL Lac object PG 1553+113 is one of the primary candidates for a binary supermassive black hole system. Aims. We study the flux and spectral variability of PG 1553…

astro-ph.GA202011 cited

Microvariability in AGNs: study of different statistical methods II. Light curves from simulated images

L. Zibecchi, I. Andruchow, S. A. Cellone +1

In a previous paper, we studied two statistical methods used to analyse the variability of active galactic nuclei (AGNs): the C and F statistics. Applying them to observed differen…

astro-ph.EP2019

Indications for transit timing variations in the exo-Neptune HAT-P-26b

C. von Essen, S. Wedemeyer, M. S. Sosa +8

From its discovery, the low density transiting Neptune HAT-P-26b showed a 2.1-sigma detection drift in its spectroscopic data, while photometric data showed a weak curvature in the…

astro-ph.HE2017

Multiwavelength monitoring of a very active dwarf nova AX J1549.85416 with an unusually high duty cycle

Guobao Zhang, Joseph D. Gelfand, David M. Russell +5

We present the results of our analysis of new optical, ultraviolet (UV) and X-ray observations of a highly variable source AX J1549.85416. Both the detection of several fast…

astro-ph.GA201715 cited

Microvariability in AGNs: study of different statistical methods - I. Observational analysis

L. Zibecchi, I. Andruchow, S. A. Cellone +3

We present the results of a study of different statistical methods currently used in the literature to analyse the (micro)variability of active galactic nuclei (AGNs) from ground-b…

astro-ph.GA2016

Optical flux behaviour of a sample of Fermi blazars

E. J. Marchesini, I. Andruchow, S. A. Cellone +7

Aims: We aim at investigating the time-behaviour of a sample of gamma-ray blazars. We present the results from a 13 month-long optical photometry monitoring campaign of the blazars…