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PINES (the Perkins INfrared Exosatellite Survey) began observations this week! 3 nights down, 357 to go.pic.twitter.com/Ys1eVjmgc8
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Shoutout sklearn.cluster for saving me probably a week of work.pic.twitter.com/TJqhO77kEP
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Patrick Tamburo proslijedio/la je Tweet
If you don’t have a team in the playoffs I’m pretty sure you should be rooting for Lamar Jackson and the Ravens.
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Patrick Tamburo proslijedio/la je Tweet
Very excited for a new year and a new research project: PINES: The Perkins INfrared Exosatellite Survey. (image credit:
@PatrickTamburo)pic.twitter.com/QsYAYw81LS
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Patrick Tamburo proslijedio/la je TweetHvala. Twitter će to iskoristiti za poboljšanje vaše vremenske crte. PoništiPoništi
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Patrick Tamburo proslijedio/la je Tweet
A highlight of 2019 for me? I saw one of those big American sandwiches (longer than a desk) in person. Man, what a day that was.
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When you're a white dwarf approaching a mass of 1.4 M⊙︎pic.twitter.com/gNREoJ7z75
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If you're at
#AGU2019, swing by the poster hall this afternoon to hear about my side hustle on Saturn's ionosphere. Poster 3509, WAY in the back.pic.twitter.com/t9Zq2KrE4i
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Patrick Tamburo proslijedio/la je Tweet
Night 4 of 7. Love this job.
@AstronomyatBU@LowellObspic.twitter.com/allo6yW8z1Hvala. Twitter će to iskoristiti za poboljšanje vaše vremenske crte. PoništiPoništi -
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Apparently my last name roughly translates to "drum of complaints" and frankly that explains a lotpic.twitter.com/PndEyHBEg4
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Forever and always the post-observing moodhttps://www.youtube.com/watch?v=PVtUlEcIoG4 …
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Our recent paper was featured on
@astrobites!https://astrobites.org/2019/08/19/finding-planets-l-t-dwarfs/ …Hvala. Twitter će to iskoristiti za poboljšanje vaše vremenske crte. PoništiPoništi -
Patrick Tamburo proslijedio/la je Tweet
Think the transit method is only for short-period planets? Head toward the water in the
#ExSS4 poster room to check out poster 307.02 on Kepler-167e: a cold (130 K) Jupiter analog. Our new Spitzer observations of a transit of this P=1071-day exoplanet will surprise you!pic.twitter.com/KuLxc3JGA5
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From that analysis, we find that an efficient survey design uses a 2-m telescope and a duration of 3-4 years. Here are some distributions showing the parameters of detected planets over thousands of simulations of such a survey (note the radius and insolation distributions!).pic.twitter.com/qBZIRSl5ij
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We varied the survey duration, telescope size, number of targets observed per night, and time spent observing an individual target in order to optimize the planet yield. We simulated each combination thousands of times, recording the number of planets detected with each.pic.twitter.com/58WFqFPPmf
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We then used this detector in simulated transit surveys. We simulated planetary systems around a sample of LTs, observed the sample, and recorded the number of "detections" we observed at > 7.1 sigma. Here's an example of a detection lightcurve, showing 2 planets.pic.twitter.com/UzqcNRqy5z
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We first determined the optimal detector setup for performing a transit search, by simulating photometry for a sample of LTs. We show that the highest precision lightcurves can be achieved in H-band.pic.twitter.com/mHoeId2LLA
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Large transit depths also facilitate transmission spectroscopy; exo-Earths around the brightest LTs may be the first terrestrial planets whose atmospheres we successfully characterize in the JWST era. Of course, we have to find some first, and that is the point of our paper.
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