Spectral Chracterization of Microvariability in Quasars

Details Spectral Chracterization of Microvariability in Quasars Spectral Chracterization of Microvariability in Quasars

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..106r&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

1

Galaxies, Agn, Environment

Scientific paper

These are the preliminary results of our BVR photometric study. The quasar 1628.5+3808 is shown here only for the sake of illustration of our research. This object showed variations in the three bands. It was observed with a 1.5-meter telecope from the Observatorio Astronómico Nacional at San Pedro Mártir, México. Only non-variable field stars were taken into account to carry out the differential photometry. Problems with standard stars did not allow the calibration process.

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