

Working on the fundamental properties of cataclysmic variables using HST astrometry, and infrared spectroscopy: such as U Gem, SS Cyg and SS Aur ( SS Cyg light curve), at NMSU, in Las Cruces, New Mexico (a nice view of NM & AZ).
Observatory Astronomer, Astronomy Department, New Mexico State University
Resume
Classes:
Here are some new SPEX spectra of CVs:
Here are some infrared argon arc lamp spectra (with the vacuum wavelengths of the strongest lines identified) obtained using SPEX:
OH lines in the K-band using OSIRIS (2.10 to 2.26 microns)
DIS arcs:
(Remember that blue is on the right in raw DIS red spectra)
Campus Observatory webcam images:
First Quarter Moon (3/28/04) shots (in mediocre seeing):
My YouTube playlist:
Or just the highlight singles:
Some random images:
My wife (her homepage), Buzz Aldrin,
Eta Car, An X-Ray Binary
, The Coma Cluster,
Shoemaker- Levy, The Cygnus Loop , Nova Cygni 1992,
Distant Cluster , Jupiter, Saturn, Titan, M87, M100, Inside a red dwarf, NGC1850,
NGC253, ,the VLA,
NM Chile.
M83 from CTIO with the 0.9 meter (in B&W).
Cen A from CTIO with the 0.9 meter (in B&W).
Images from our campus observatory Meade 16" telescope with ST8 CCD:
1) 180s R-band exposure of M42 (unguided, 2X2
binning).
The initial tracking quality on our 16" was rather poor, after much fiddling,
we have reduced this to about 1" r.m.s. Proof is shown in the R-band image of
M67, which has an exposure time of 4 minutes (one complete worm revolution).
2) 240s R-band Exposure of M67 (unguided, raw
image).
3) 240s R-band Exposure of M51 (unguided).