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Durnal latitudes obtained in Pulkovo with zenith-telescope ZTF-135 during
1904-1941 and1948-2005 by seven Talkott - programs are represented. In 1941-
1948 observations could not carried out because of destroying of Pulkovo
observatory during the second world war. After reconstruction of
observatory ZTF-135 was installed to the south from the previous place so
latitudes of second period were decreased by 1".599.
The programs were made in such a way as to be observed during 20 years
and to guarantee the maximum inclusion of the same stars of list. Several
stars were observed during all period. Besides in 1915-1928 and 1955-1962
the observations were made «from sunset to sunrise» to investigate diurnal
latitude variations.
All files are given in HIPPARCOS system and reduced in ICRS system
with the model IAU2000A (Convention 2000).

The format is as follows:

DAT MJD N SFI D DS
FORMAT ( I8, F11.3, I4, 3F7.3 )

DAT - the data of observation
MJD - modifyed Julian data (jd-2400000.5)
N - the number of instantenious latitudes obtained in the
data
SFI - diurnal latitude on the data (in arcsec)
( plus 59њ 46'12" for the period 1904-1941, 59њ 46'10" for the period
1948-2006)
D - mean square error of instantenious latitude (in arcsec).
DS - mean square error of diurnal latitude (in arcsec)

All questions could be adressed on: natmiller@list.ru