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This is a long page - please scroll down to see light curves and spectra!
Nova V459 Vulpeculae: Discovered independently by H. Kaneda (25 Dec 07) and A. Tago (26 Dec 07). GVO observations made from 27 Dec 07 into early Jan 08. The star appears light orange in the telescope; the measured color indices show a spectral shift in the energy output: B-V decreased by 2X while V-R and V-I increased by ~10%. V459 Vul faded by more than 1 magnitude in 10 days, suggesting a Type NA nova. The proximity to the horizon and attendant time constraints preclude our obtaining spectra, but we have been able to make single-channel multi-band photometric measurements in BVRI and Wing ABC bands.
The table lists the BVRI results, transformed to the standard system and corrected for atmospheric extinction.
V459 Vul: RA(2000) 19:48:09 DEC(2000) +21:15:26
Comet 17P/Holmes: 28-29 October 2007: Observed by eye, binoculars, and 14 inch telescope with CCD spectrograph. html pages: Comet 17P/Holmes Spectroscopy pdf file: Comet 17P/Holmes Spectroscopy Comet 17P/Holmes in Perseus: 27 Oct 07 Front Royal, VA Hand-held Olympus SP-310 Digital Camera, 3 sec 28 Oct 07 29 Oct 07 Spectra taken with Celestron CGE 1400 and SBIG SGS/ST7-XME, corrected for system quantum efficiency only
Red variable stars (2007-2008): Nine-color photometric data of red semi-regular variable stars in visible and near-IR bands. In some cases, 10 orders of magnitude difference are measured from B to H bands!
BVRI and Wing band data with SSP3 (3 x 10 sec integrations), JH band data with SSP4 (4 x 10 sec integrations)
Visual band light curves of selected GVO Program Stars for 2006-2007.
Near IR spectral data (680 nm to 760 nm) for selected GVO Program Stars for 2006-2007.
Spectra of the eclipsing binary system Epsilon Aurigae in late 2005 and late 2006:
Selected spectral data for selected GVO Program Stars. In the near future, data will be available by object name.
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