Josh Lothringer

453 posts

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Josh Lothringer

Josh Lothringer

@JDLothringer

Assistant Astronomer @STScI researching exoplanet and brown dwarf atmospheres. (he/him)

Katılım Eylül 2009
521 Takip Edilen630 Takipçiler
Josh Lothringer
Josh Lothringer@JDLothringer·
We hope this is just the start at looking at these population-level trends, now with more robust and reliable measurements. We'll continue to collect measurements as they become available and update the table. We plan to extend this to include free retrieval results.
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Josh Lothringer
Josh Lothringer@JDLothringer·
We've collected 65 individual exoplanet atmosphere composition measurements to look for population-level trends 🔭#exoplanets To do this, we had to create a toolkit to standardize between definitions of . We call it ExoComp. (Yes, that's a Star Trek reference 😀).
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Josh Lothringer
Josh Lothringer@JDLothringer·
Abstracts are due by tomorrow for the 12th installment of the Chesapeake Bay Area Exoplanet Meeting! Link below. The meeting will be December 5th, 2025 at JHU Applied Physics Lab. Hope to see you there.
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Josh Lothringer retweetledi
JWST Observer
JWST Observer@JWSTObserver·
Read the latest about JWST's Rocky Worlds Director's Discretionary Time program, including final targets and an upcoming information session: ow.ly/KfoB50WReQu
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Josh Lothringer
Josh Lothringer@JDLothringer·
And a big shout-out to lead-author Yayaati for seeing this project through from proposal to paper and showing that HST still has lots to say about exoplanet atmospheres in the JWST-era! Check out the paper here: arxiv.org/abs/2508.10092. Accepted for publication in AJ!
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Josh Lothringer
Josh Lothringer@JDLothringer·
We find tentative evidence for a limb asymmetry in the huge NUV feature. 3D GCM models (with mag fields!) to show that the data is (tentatively) more consistent with a model *with* a magnetic field than without! More obs of, e.g., the hot spot offset, could help.
Josh Lothringer tweet mediaJosh Lothringer tweet media
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Josh Lothringer
Josh Lothringer@JDLothringer·
I'm very excited to be able to share Yayaati Chachan's Hubble/WFC3 transit spectrum of ultra-hot Jupiter KELT-20b. Using *all* of WFC3's grisms, we get a 0.2-1.7 micron spectrum showing absorption by metals at in the UV and only weak absorption by water in the IR.
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Josh Lothringer
Josh Lothringer@JDLothringer·
Abstracts close this Friday for the Fall 2025 STScI Science Workshop on Atmospheric Escape and Replenishment. We'd love to see you in Baltimore in November! Check it out and let me know if you've any questions. stsci.edu/contents/event…
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Josh Lothringer
Josh Lothringer@JDLothringer·
Personally, these funds were vital in enabling me to do research with how busy I was teaching during the academic year at UVU. These data took years to fully analyze, and without the funding it would still be languishing.
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Josh Lothringer
Josh Lothringer@JDLothringer·
🔭 Because it is more relevant now more than ever, this research was supported by funding from both NASA and NSF which allowed me, four undergraduate students, and two co-authors to spend time analyzing these data.
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Josh Lothringer
Josh Lothringer@JDLothringer·
Popping in to say: 🔭 New paper day on the arXiv! arxiv.org/abs/2503.15472 We observed ultra-hot Jupiter WASP-178b with HST and JWST to try to figure out where the planet comes from!
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