The Guide Star Photometric Catalog-II (GSPC-II)
is being created by the STScI Catalogs and Survey Branch and the
Osservatorio Astronomico di Torino (OATo) to provide photometric
calibrators for the Guide Star Catalog-II (GSC-II).
Most of the GSPC-II star sequences extend the GSPC-I
sequences to a limiting magnitude of V = 19 or fainter based on
CCD data in the V and R bandpasses of the Johnson-Kron-Cousins system.
Where resources were available, which is for a large part of the
southern hemisphere and for a few northern fields, a B band was
also included, and the limiting magnitude brought to ~20. While
the southern second-epoch plates used for GSC-II lie on the same
5 deg grid pattern used for for GSC-I and require no additional
sequences, the northern POSS-II plates supporting GSC-II lie on
a similar 5 deg grid which differs from the 6 deg grid used for
GSC-I. This results in a number of POSS II plates being considerably
shifted with respect to the original grid, and therefore poorly
covered by the GSPC-I sequences. New northern sequences are being
added in GSPC-II to support calibration of such POSS-II plates.
The observations were obtained with mostly
one-meter class telescopes at ten observatories. Most of the northern
GSPC-II sequences were imaged at the Kitt
Peak and Wise Observatories,
whereas southern declinations were covered by Cerro
Tololo and ESO-La
Silla observations. Data also were acquired at Mt.
Hopkins, Mt. Laguna,
Lowell, Mt.
Megantic, McDonald
and JKT La Palma observatories. The observation strategy was to
take CCD frames centered on the faintest star of the corresponding
GSPC-I sequence where one was available. When necessary, both long
(~8-15 min) and short (<3 min) exposures were acquired in each
field. Short exposures times were chosen to be appropriate for the
typical 14.5 mag target star. For new POSS-II fields lacking GSPC-I
sequences, the telescope was pointed to the nominal center of the
corresponding survey plate, and the pointing adjusted to avoid bright
stars.
For more information see: the journal article:
"An
All Sky Set of (B)- V-R Photometric Calibrators for Schmidt Surveys:
GSPC2.1: First Release", Bucciarelli, et al. A&A 368, pp
335-346, 2001
|