2013 AX52
Available from the Minor Planet Center.
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Available from the Minor Planet Center.
Available from the Minor Planet Center.
Available from the Minor Planet Center.
We present our on-going project to unveil the post-nova population by
re-discovering old novae that have been lost after the initial outburst
and in which the binary itself is unobserved. We take UBVR photometry
for candidate selection, long-slit spectroscopy to confirm these
candidates, and time-resolved spectroscopy to measure the orbital period
of the newly confirmed post-novae. Some preliminary results are shown as
examples.
JPCam is a 14-CCD mosaic camera, using the new e2v 9k-by-9k
10microm-pixel 16-channel detectors, to be deployed on a dedicated 2.55m
wide-field telescope at the OAJ (Observatorio Astrofisico de Javalambre)
in Aragon, Spain. The camera is designed to perform a Baryon Acoustic
Oscillations (BAO) survey of the northern sky. The J-PAS survey strategy
will use 54 relatively narrow-band (~13.8nm) filters equi-spaced between
370 and 920nm plus 3 broad-band filters to achieve unprecedented
photometric red-shift accuracies for faint galaxies over ~8000 square
degrees of sky. The cryostat, detector…