Hello from James in USA
Posted: Fri Feb 19, 2016 10:07 pm
Hello to all ARAS members
My name is James Foster and I am doing astronomy from Los Angeles and Mt Pinos (2500mters), California, USA.
I have mostly contributed to astrometry and photometry data to MPC and AASVO since 2004 and started film astrophotography in 1988.
I use CCD Autopilot V5 to shoot 20 or more photometric targets nightly. Southern California nights are frequently clear and I'm
far enough from the ocean to be rarely affected by the Pacific ocean's marine layer (fog).
My interest in spectroscopy was from a AASVO meeting we had in Ontario, California in 2014 and I realized that amateurs are able to expand their field of activity in this direction providing Be spectra for archiving in the BeSS datatbase.
I do most of my photometry and specta from my house 8 miles east of downtown LA (close to work!)
I also take 7-10 day vacations to Mt. Pinos (100 miles north) where the light pollution is minimal and altitude is over 2500 above sea level!
I use the following instruments at home and in the field:
Telescopes: Planwave CDK17(43cm aperture), Clasical Cassegrain 33cm F/7.5, C-11, Newtonian 10" F4.5, and Genesis 4" F/5 Refractor
Mount(s): Two AP1200GTO mounts, iOptron CEM60, and Losmandy EQ100
Camera: SBIG STL-11K, ST-10XME (main photometry/spectra camera), & ST-8XE
Spectrographs: (1) JTW Engineering L-200 (Littrow style) Spectrometer with 150, 300, 600, 1200, & 1800 Ln/mm gratings
(2) SA200 1.25" grating used in carousel of ST-10XME camera
One of my spectroscopic highlight was the observation of nova Sag 2015 that had very prominent emission lines.
Best regards
James Foster
Los Angeles, CA
http://www.astroimage.info
My name is James Foster and I am doing astronomy from Los Angeles and Mt Pinos (2500mters), California, USA.
I have mostly contributed to astrometry and photometry data to MPC and AASVO since 2004 and started film astrophotography in 1988.
I use CCD Autopilot V5 to shoot 20 or more photometric targets nightly. Southern California nights are frequently clear and I'm
far enough from the ocean to be rarely affected by the Pacific ocean's marine layer (fog).
My interest in spectroscopy was from a AASVO meeting we had in Ontario, California in 2014 and I realized that amateurs are able to expand their field of activity in this direction providing Be spectra for archiving in the BeSS datatbase.
I do most of my photometry and specta from my house 8 miles east of downtown LA (close to work!)
I also take 7-10 day vacations to Mt. Pinos (100 miles north) where the light pollution is minimal and altitude is over 2500 above sea level!
I use the following instruments at home and in the field:
Telescopes: Planwave CDK17(43cm aperture), Clasical Cassegrain 33cm F/7.5, C-11, Newtonian 10" F4.5, and Genesis 4" F/5 Refractor
Mount(s): Two AP1200GTO mounts, iOptron CEM60, and Losmandy EQ100
Camera: SBIG STL-11K, ST-10XME (main photometry/spectra camera), & ST-8XE
Spectrographs: (1) JTW Engineering L-200 (Littrow style) Spectrometer with 150, 300, 600, 1200, & 1800 Ln/mm gratings
(2) SA200 1.25" grating used in carousel of ST-10XME camera
One of my spectroscopic highlight was the observation of nova Sag 2015 that had very prominent emission lines.
Best regards
James Foster
Los Angeles, CA
http://www.astroimage.info