28 research outputs found
The relative wavelength independence of IR lags in active galactic nuclei: implications for the distribution of the hot dust
We show that, contrary to simple predictions, most AGNs show at best only a
small increase of lags in the J, H, K, and L bands with increasing wavelength.
We suggest that a possible cause of this near simultaneity of the variability
from the near-IR to the mid-IR is that the hot dust is in a hollow bi-conical
outflow of which we only see the near side. Although most AGNs show near
simultaneity of IR variability, there was at least one epoch when NGC 4151
showed the sharply increasing IR lag with the increase of the wavelength. This
behaviour might also be present in GQ Comae. We discuss these results briefly.
The relative wavelength independence of IR lags simplifies the use of IR lags
for estimating cosmological parameters.Comment: 6 pages, 5 figures, for the Odessa Astronomical Publicatio
Image reconstruction technique and optical monitoring of the QSO2237+0305 from Maidanak Observatory in 2002 -- 2003
We have observed the gravitational lens system Q2237+0305 from the Maidanak
Observatory over the period from August 2002 to November 2003. Here we report
the results of our observations. We implemented a two-stage technique that has
been developed specifically for the purpose of gravitational lens image
reconstruction. The technique is based on the Tikhonov regularization approach
and allows one to obtain astrometric and photometric characteristics of the
gravitational lens system. Light curves with 78 data points for the four quasar
components are obtained. Slow brightness variations over the observational
period are found in all components. Images A, C, D have a tendency to decrease
in brightness. Image B does not vary more than 0.05mag. The observations did
not reveal evidence for large variations in brightness of the components due to
microlensing effects. To provide an overall picture of the photometry
behaviour, our data are combined with the Maidanak observations published for
1995 -- 2000.Comment: 9 pages, 4 figures, accepted by MNRA
Determining time delay in the gravitationally lensed system QSO2237+0305
Aims.We considered the possibility of measuring time delays
between components of the multiplied quasar QSO2237+0305 and between
V and R band variations.
Methods.The analysis is based on the flux
variations of four components observed by the OGLE collaboration and
Maidanak group during the last quarter of 2003. The observed
gradients of the brightness variations in this period for OGLE data
in V band are 3.4 mmag/day, 2.2 mmag/day, 2.4 mmag/day, and 1.1 mmag/day for the components A, B, C, and D, respectively. The
variations are probably intrinsic source variations. The basic
method used for time-delay measurements is the cross-correlation
technique. To estimate the uncertainty of the time-delay
measurements, Monte Carlo simulations were carried out.
Results.The
calculations showed the impossibility of unambiguously measuring the
differential time delays between the components. The observations at
shorter wavelengths seem to be the only way to achieve robust time
delay measurements in the system. The wavelength-dependent time
delays can be used to provide the evidence of an accretion-disk
structure of the central optical variable source. The observed V and
R band variations of component C show good correlation with the
correlation coefficient of 0.83. However, the obtained time delay,
about 16.2 days, and its accuracy are far from reliable