Around the Clock Observations of the Q0957+561 A,B Gravitationally Lensed Quasar II: Results for the second observing season
arXiv:astro-ph/0210400 · doi:10.1086/368076
Abstract
We report on an observing campaign in March 2001 to monitor the brightness of the later arriving Q0957+561 B image in order to compare with the previously published brightness observations of the (first arriving) A image. The 12 participating observatories provided 3543 image frames which we have analyzed for brightness fluctuations. From our classical methods for time delay determination, we find a 417.09 +/- 0.07 day time delay which should be free of effects due to incomplete sampling. During the campaign period, the quasar brightness was relatively constant and only small fluctuations were found; we compare the structure function for the new data with structure function estimates for the 1995--6 epoch, and show that the structure function is statistically non-stationary. We also examine the data for any evidence of correlated fluctuations at zero lag. We discuss the limits to our ability to measure the cosmological time delay if the quasar's emitting surface is time resolved, as seems likely.
AAS LaTeX, 5 PostScript figures
References in corpus (9)
- A Structure for Quasars
- A Robust Determination of the Time Delay in 0957+561A,B and a Measurement of the Global Value of Hubble's Constant
- A Sharp Event in the Image a Light Curve of the Double Quasar 0957+561 and Prediction of the 1996 Image B Light Curve
- Improved Parameters and New Lensed Features for Q0957+561 from WFPC2 Imaging
- Time delay in QSO 0957+561 from 1984-99 optical data
- Measuring the Size of Quasar Broad-Line Clouds Through Time Delay Light-Curve Anomalies of Gravitational Lenses
- Hourly Variability in Q0957+561
- Precision Photometry for Q0957+561 Images A and B
- 'Round the Clock Observations of the Q0957+561 A,B Gravitationally Lensed Quasar
Cited by in corpus (26)
- A New Channel for Detecting Dark Matter Substructure in Galaxies: Gravitational Lens Time Delays
- The Importance of Lens Galaxy Environments
- COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses I. How to sample the light curves of gravitationally lensed quasars to measure accurate time delays
- Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
- A Rapid Microlensing Event in the Q0957+561 A,B Gravitational Lens System
- Cosmological distance indicators
- Observations Supporting the Existence of an Intrinsic Magnetic Moment Inside the Central Compact Object Within the Quasar Q0957+561
- Observational determination of the time delays in gravitational lens system Q2237+030
- New aperture photometry of QSO 0957+561; application to time delay and microlensing
- A Comparison of Cosmological Models Using Time Delay Lenses
- New database for a sample of optically bright lensed quasars in the northern hemisphere
- Improved Constraints on the Gravitational Lens Q0957+561. I. Weak Lensing
- Anomalous Fluctuations in Observations of Q0957+561 A,B: Smoking Gun of a Cosmic String?
- Microlensing of a Ring Model for Quasar Structure
- Revealing the structure of the lensed quasar Q 0957+561: I. Accretion disk size
- Accretion Disc Structure and Orientation in the Lensed and Microlensed Q0957+561 Quasar
- MiNDSTEp differential photometry of the gravitationally lensed quasars WFI2033-4723 and HE0047-1756: Microlensing and a new time delay
- Cosmological test using strong gravitational lensing systems
- Five nights of intensive R- and V-band photometry of QSO 0957+561A,B
- Bayesian approach to gravitational lens model selection: constraining H_0 with a selected sample of strong lenses
- Revealing the nonlinear behaviour of the lensed quasar Q0957+561
- Spectroscopy and polarimetry of the gravitationally lensed quasar Q0957+561
- The Mass Function of Primordial Rogue Planet MACHOs in quasar nanolensing
- Primordial Planet Formation
- Model selection using time-delay lenses
- A partially occulting MACHO-microlensing event in the Twin Quasar Q0957+561