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25 April 2024
 
  » arxiv » astro-ph/9403049

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The Hamburg Quasar Monitoring Program (HQM) at Calar Alto. II. Lightcurves of weakly variable objects
K.-J. Schramm ; U. Borgeest ; D. Kühl ; J. v. Linde ; M.D. Linnert ;
Date 23 Mar 1994
Subject astro-ph
AbstractHQM is an optical broad-band photometric monitoring program carried out since Sept.~1988. We use a CCD camera equipped to the MPIA 1.2$,$m telescope. Fully automatic photometric reduction relative to stars in the frames is done within a few minutes after each exposure, thus interesting brightness changes can be followed in detail. The typical photometric error is 1--2,for a 17.5,mag quasar. We here present lightcurves already evaluated but not shown in Paper I. We also discuss existing literature data.
Source arXiv, astro-ph/9403049
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