Sarah Tuttle

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Sarah Tuttle is an astrophysicist and assistant professor of astrophysics at the University of Washington.[1] Tuttle builds spectrographs to detect nearby galaxies, including work on VIRUS[2] (the Visible Integral-field Replicable Unit Spectrograph) installed on McDonald Observatory's Hobby–Eberly Telescope to study dark energy, and FIREBall (Faint Intergalactic medium Redshifted Emission Balloon), the world's first fiber fed ultraviolet spectrograph.[3][4][5]

Tuttle was born and raised in Santa Cruz,[6] studied physics at the University of California, Santa Cruz and graduated with a B.Sc in 2001.[7] From 2001 to 2002, she worked for Add-Vision in Scotts Valley as a research scientist,[7] and was part of the team that built the first screen-printed polymer light emitting diodes.[8]

Tuttle received a M.Sc and M.Phil in astronomy from Columbia University in 2006 and 2007,[9] and obtained her Ph.D in 2010,[7] working with David Schiminovich on the Faint Intergalactic medium Redshifted Emission Balloon (FIREBall).[3][4][5] Tuttle built the world's first fiber fed ultraviolet spectrograph, which launched on FIREBall in 2009.[5][10]

Research and career

FIREBall (Faint Intergalactic Redshifted Emission Balloon), an experiment aimed at measuring emission from the intergalactic and circumgalactic medium in the ultraviolet, during launch

Tuttle's research applies novel hardware approaches to spectrograph instrumentation design, particularly aimed to isolate star formation regulation in galaxies through emission and infall from the interstellar medium.[11]

During her Ph.D. at Columbia, Tuttle built the spectrograph for FIREBall, a balloon-borne telescope that is coupled to an ultraviolet spectrograph and designed to discover the intergalactic medium (IGM) in emission.[12][10] The FIREBall spectrograph built by Tuttle was the world's first fiber fed ultraviolet spectrograph and placed upper constraints on IGM emission.[5][10]

Nine of Tuttle's VIRUS spectrograph units awaiting testing for later installation on the Hobby Eberly Telescope.

Tuttle served as the lead for the Hobby–Eberly Telescope's VIRUS detector from 2010 until 2012, where she prototyped, finalized and characterized the VIRUS spectrograph.[13][14][15][16][17] The instrument consists of 156 spectroscopic channels fed by 34944 fiberoptic channels, covering a 22 arcminute field of view.[18] Tuttle and her colleagues' current astrophysics work still utilizes VIRUS data.[19]

In 2016 she joined the University of Washington as an assistant professor.[11] As of May 2019, Tuttle was leading the recommissioning of the KOSMOS spectrograph for the Apache Point Observatory, an instrument originally stationed at Kitt Peak Observatory.[11][20]

Her science-outreach work includes appearances on the podcast 365 Days of Astronomy in 2009 and writing for The Toast in 2014.[9][4][21] She regularly appears as an astronomy expert in articles in The Seattle Times, The Mercury News and Gizmodo.[22][23][24][25] In 2014, the National Academy of Sciences honored her as a Kavli Fellow.[26][27] Tuttle has also contributed to American Astronomical Society workshops and supported new guidelines to build a more diverse and inclusive environment.[28]

Activism

See also

References

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