Melissa L. Graham (she/her)

Research Scientist
A headshot of me smiling in my home office, in black and white, wearing a hoodie sweatshirt with my plants visible behind me.

Contact Information

PAB B356C

Biography

Research Scientist, U. of Washington, 2016-present
Postdoc, UC Berkeley, 2013-2016
Postdoc, Las Cumbres Observatory & UC Santa Barbara, 2010-2013
Ph.D., Astrophysics, University of Victoria, Canada, 2004-2010
B.Sc.H., Astrophysics, Queen's University, Canada, 2000-2004

I am currently a research staff scientist in the Department of Astronomy at the University of Washington in Seattle WA USA, where I work with the Rubin Observatory and its Legacy Survey of Space and Time (LSST) as the Lead Community Scientist. My main research focus is supernovae, especially those of Type Ia.

Rubin Lead Community Scientist. I lead the Community Science team in the Data Management department, which oversees our user-facing resources and provides support for scientists and students using the LSST data products. The volume and complexity of the LSST data products requires a proportionally innovative and progressive model for engaging and supporting the large and diverse community of scientists that it was designed to serve. Together we are building high-quality documentation and tutorials, and the support infrastructure necessary to foster a vibrant, inclusive, and self-sustaining research community. To get involved in preparations for Rubin Observatory and the LSST, visit the Rubin Observatory's For Scientists website.

Research on Type Ia Supernovae. I am an observational astrophysicist who studies supernovae, stellar explosions so energetic they produce the light of a billion suns. Supernovae exhibit a variety of characteristics, and most of them are in galaxies so far away that the original star cannot be resolved. It is important to understand how stars explode because supernovae release the heavy elements fused in the star’s interior which form metal-enriched objects like planets, and because they are used as “standard candles” for cosmological studies of dark energy. I focus on understanding the thermonuclear explosions of carbon-oxygen white dwarf stars as Type Ia supernovae (SN Ia). I have used a variety of observatories such as Hubble, Keck, Gemini, MMT, Blanco, CFHT, Lick, SOAR, Las Cumbres, and the DAO.

From Queen’s to the cosmos: Alumna helps lead groundbreaking new observatory in Chile

Professional Affiliations
American Astronomical Society (AAS), Canadian Astronomical Society (CASCA), LSST Transients and Variable Stars Science Collaboration, LSST Dark Energy Science Collaboration
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