"My fellow citizens of the world: ask not what America will do for you, but what together we can do for the freedom of man."

Thanks for visiting my website. It is a mix of personal interests and professional experience.

My professional background is focused on software quality assurance, but not just pointing and clicking! My approach to quality assurance is engineering based with an emphasis on "pushing left" and building teams from the "ground up". This means understanding the importance of being involved early in the software development lifecycle, being able to create detailed documentation, reliable processes, automating error-prone, mission critical and mundane tests, as well as harnessing human strengths (like exploratory testing).

I also have speaking experience on a variety of topics software quality assurance-related. My contact information is in the footer if you are interested in having me speak at an event.

When I'm not being a software quality assurance guru I enjoy a variety of activities, some of which are represented on my website. I like making craft cocktails , building things , and listening to podcasts.

- Krypton -

NASA Astronomy Picture of the Day [APOD] NASA APOD

Messier 104

A gorgeous spiral galaxy, Messier 104 is famous for its nearly edge-on profile featuring a broad ring of obscuring dust lanes. Seen in silhouette against an extensive central bulge of stars, the swath of cosmic dust lends a broad brimmed hat-like appearance to the galaxy suggesting a more popular moniker, the Sombrero Galaxy. Also known as NGC 4594, the Sombrero galaxy can be seen across the spectrum and is host to a central supermassive black hole. About 50,000 light-years across and 28 million light-years away, M104 is one of the largest galaxies at the southern edge of the Virgo Galaxy Cluster. Still, the spiky foreground stars in this field of view lie well within our own Milky Way. This broad view of the well-known galaxy was processed to reveal M104's extended halo, as well as a faint tidal stellar stream. It was captured by the Dark Energy Camera (DECam) on the Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory.