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Planet-finding near infrared spectrograph deployed on the 10 m Hobby Eberly Telescope in 2017-18.

Penn State University
Joined November 2014
Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)Photo by HPF (@HPFspectrograph)
Joint gathering of the NEID and @HPFspectrograph teams at #EPRV5. Exciting to have such a talented and growing team!
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Congratulations to Shubham Kanodia and Caleb Cañas on their successful Ph.D defenses this week! @HPFspectrograph @NEID_at_WIYN @AstroPSU @shubhamkanodia
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Congratulations to @gummiks on winning the 2020 Robert J. Trumpler Award for his PhD dissertation, "Extreme Precision Photometry and Radial Velocimetry from the Ground"! astrosociety.org/who-we-are/…
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To Separate Starspots from Planets When it comes to M dwarfs, how do you distinguish between starspots and planets? aasnova.org/2020/10/02/to-se… @UCIPhysAstro
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The discovery of a Jupiter-sized planet transiting an M dwarf star — made by a team including Eberly's Caleb Cañas, @gummiks, @shubhamkanodia, @SuvrathM, and @Astro_Wright — could help astronomers better understand how these planets form. buff.ly/33r7XoK @HPFspectrograph
⚠️New paper⚠️ led by Caleb Cañas @PSUScience: using precision radial velocities from @HPFspectrograph, we confirm the planetary nature of TOI-1899b, the first Warm Jupiter (Period~29days) orbiting an early M-dwarf star as observed by @NASA_TESS !
The discovery of a Jupiter-sized planet transiting an M dwarf star — made by a team including Eberly's Caleb Cañas, @gummiks, @shubhamkanodia, @SuvrathM, and @Astro_Wright — could help astronomers better understand how these planets form. buff.ly/33r7XoK @HPFspectrograph
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This paper was a fantastic collaboration of a number of people, some of which are on Twitter: @HPFSpectrograph, @PSUScience,@PU_Astro,@SuvrathM,@Astro_Wright, @shubhamkanodia,@wistwitski,@rcterrien, @planet_hunter,@lesliehebb,@ChadFBender - let me know if I missed anyone!
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Congratulations @shubhamkanodia for leading this new HPF result confirming a warm super Neptune exoplanet transiting an M dwarf star. @PSUScience @HPFspectrograph @mcdonaldobs
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Exciting new @HPFspectrograph planet paper led by @shubhamkanodia on TOI-1728b, a super-Neptune orbiting a nearby bright M0 star, and a promising @JWSTObserver target! Paper discusses mass measurement, ground-based transits (#diffusers), He 10830 absorption constraints, and more!
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Guess what the image in the lower right corner is in this tweet from NIST. Its our Habitable-zone Planet Finder (HPF) spectrometer on the 10m Hobby Eberly Telescope! (its primary calibration source is a frequency stabilized laser comb). @HPFspectrograph @NIST @mcdonaldobs
Our researchers work hard to get their innovations in measurement science out to the marketplace. Learn about NIST’s impact on quality of life: nist.gov/featured-stories/ni… #NationalInventorsMonth
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🚨New paper ! 🚨Our paper on the validation on the nearby M-dwarf planet G 9-40b is now accepted for publication and available on the arXiv: arxiv.org/abs/1912.00291 Highlights from the paper below.
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IT'S HAPPENING! NEID is on the truck and headed to WIYN. neid.psu.edu/2019/10/25/neid…
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Registration for Extreme Solar Systems IV is now open ! Looking forward to seeing you all there ! #ExSS4
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(2/2) And how HPF with the LFC is pushing near-infrared Doppler precision: sites.psu.edu/hzpf/2019/02/1…
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The future is here! NIR RV precision breaks 3 m/s! Metcalf et al. arxiv.org/abs/1902.00500 @HPFspectrograph I knew it would work! So happy.
This is the 3D profile of the polka dot pattern!
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One of the most important piece of info from her talk: @HPFspectrograph is doing 1.3 m/s over several weeks on a real target!!! State of the art of NIR PRV is upon us! xitter.gq/johannateske/status/10…
Replying to @johannateske
Arpita Roy is now digging into the nitty gritty details of RV data reduction and analysis. She emphasizes that at <1 m/s level, need to gather the right info when observing to make good analysis possible. Beautiful example of data from @HPFspectrograph! #sagan2018