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A&A 374, 878-894 (2001)
DOI: 10.1051/0004-6361:20010796
A QSO survey via optical variability and zero proper motion in the M 92 field
II. Follow-up spectroscopy and properties of the QSO sample
H. Meusinger and J. BrunzendorfThüringer Landessternwarte Tautenburg, 07778 Tautenburg, Germany
e-mail: meus@tls-tautenburg.de, brunz@tls-tautenburg.de
(Received 10 April 2001 / Accepted 30 May 2001 )
Abstract
The combination of variability and proper motion constraints
(VPM search) is believed to provide an efficient yet unconventional
search strategy for QSOs with selection effects quite different
from conventional optical QSO surveys. We performed a VPM QSO
search in a 10 square degrees field around M 92 on
162 selected digitised Schmidt plates in the Johnson B band
with a time-baseline of more
than three decades. In Paper I, we constructed a sample of VPM QSO
candidates with
. The spectroscopic follow-up
observations revealed 58 QSOs and 7 Seyfert 1 galaxies as well as
27 narrow-emission line galaxies. We present the low-resolution
spectra and the
data for the QSOs and Seyfert galaxies: AGN types,
accurate positions, redshifts, mean B magnitudes, and
colour indices,
along with the selection parameters of the VPM search, i.e.,
indices for variability, proper motion,
and image structure. The redshifts cover the interval
; absolute magnitudes are in the range
. The
statistical properties of the resulting QSO sample
are studied in detail.
No significant differences were found between our VPM QSO sample and
published QSO samples from multicolour or spectroscopic surveys.
The fraction of QSOs with unusual
colours is estimated to be less than 5 per cent within
the magnitude range
.
Key words: galaxies: active -- galaxies: statistics -- quasars: general
Offprint request: H. Meusinger, meus@tls-tautenburg.de
SIMBAD Objects
© ESO 2001
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