About

I am an Astrophysicist and Software Engineer at the Space Telescope Science Institute (STScI). Originally from Syracuse, NY, I earned my B.S. in Physics from St. Lawrence University and my Ph.D. in Astrophysics from Keele University in England. After four-years as a postdoctoral fellow at STScI within the Interstellar Medium group, I worked as an Instrument and Observatory Scientist for the Stratospheric Observatory for Infrared Astronomy (SOFIA). I now work as a Software Engineer at STScI while continuing my research.

As a researcher, I study the late evolutionary stages of Asymptotic Giant Branch (AGB) stars—sun-like stars nearing the ends of their lives. These stars shed vast amounts of gas and dust, returning up to 85% of their mass to the interstellar medium. By observing them across radio, infrared, and optical wavelengths, I investigate how they enrich galaxies with the raw materials that ultimately form new stars, planets, and even life itself.

As a science software engineer, I maintain calibration software for both the Hubble and James Webb Space Telescopes. I also serve as the Hubble Calibration Pipeline Lead, ensuring that the hundreds of terabytes of Hubble data are constantly updated, calibrated, and ready for discovery.

CV

The Dusty Evolved Star Kit (DESK)

Dusty Evolved Star Kit graphic The Dusty Evolved Star Kit is a simple tool for fitting the Spectral Energy Distribution of evolved stars with pre-computed grids of radiative transfer models. Let us know if you have a grid that you would like included in the DESK!

Contact me

  • Address

    3700 San Martin Drive
    Baltimore, MD 21218
    United States
  • Email

    sgoldman@stsci.edu