216 research outputs found
Multi-Band Intra-Night Optical Variability of BL Lacertae
We monitored BL Lacertae frequently during 2014 - 2016 when it was generally
in a high state. We searched for intra-day variability for 43 nights using
quasi-simultaneous measurements in the B, V, R, and I bands (totaling 143 light
curves); the typical sampling interval was about eight minutes. On hour-like
timescales, BL Lac exhibited significant variations during 13 nights in various
optical bands. Significant spectral variations are seen during most of these
nights such that the optical spectrum becomes bluer when brighter. The
amplitude of variability is usually greater for longer observations but is
lower when BL Lac is brighter. No evidence for periodicities or characteristic
variability time-scales in the light curves was found. The color variations are
mildly chromatic on long timescales.Comment: 15 pages, 5 Figures, 3 Tables; Accepted for publication in Galaxies;
a special issue on Microvariability of Blazar
Radio Properties of Low Redshift Broad Line Active Galactic Nuclei Including Extended Radio Sources
We present a study of the extended radio emission in a sample of 8434 low
redshift (z < 0.35) broad line active galactic nuclei (AGN) from the Sloan
Digital Sky Survey (SDSS). To calculate the jet and lobe contributions to the
total radio luminosity, we have taken the 846 radio core sources detected in
our previous study of this sample and performed a systematic search in the
Faint Images of the Radio Sky at Twenty-centimeters (FIRST) database for
extended radio emission that is likely associated with the optical
counterparts. We found 51 out of 846 radio core sources have extended emission
(> 4" from the optical AGN) that is positively associated with the AGN, and we
have identified an additional 12 AGN with extended radio emission but no
detectable radio core emission. Among these 63 AGN, we found 6 giant radio
galaxies (GRGs), with projected emission exceeding 750 kpc in length, and
several other AGN with unusual radio morphologies also seen in higher redshift
surveys. The optical spectra of many of the extended sources are similar to
that of typical broad line radio galaxy spectra, having broad H
emission lines with boxy profiles and large M_BH. With extended emission taken
into account, we find strong evidence for a bimodal distribution in the
radio-loudness parameter R, where the lower radio luminosity core-only sources
appear as a population separate from the extended sources, with a dividing line
at log(R) . This dividing line ensures that these are indeed the
most radio-loud AGN, which may have different or extreme physical conditions in
their central engines when compared to the more numerous radio quiet AGN.Comment: 25 pages, 6 figures, accepted to A
Multi-band optical variability of three TeV Blazars on Diverse Timescales
We present our optical photometric observations of three TeV blazars, PKS
1510-089, PG 1553+113 and Mrk 501 taken using two telescopes in India, one in
Bulgaria, one in Greece and one in Serbia during 2012 - 2014. These
observations covered a total of 95 nights with a total of 202 B filter frames,
247 images in V band, 817 in R band while 229 images were taken in the I
filter. This work is focused on multi-band flux and colour variability studies
of these blazars on diverse timescales which are useful in understanding the
emission mechanisms. We studied the variability characteristics of above three
blazars and found all to be active over our entire observational campaigns. We
also searched for any correlation between the brightness of the sources and
their colour indices. During the times of variability, no significant evidence
for the sources to display spectral changes correlated with magnitude was found
on timescales of a few months. We briefly discuss the possible physical
mechanisms most likely responsible for the observed flux variability.Comment: 11 pages, 7 figures, 9 tables. Accepted for publication in MNRA
- …