Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Dattilo, Anne"'
Autor:
Dattilo, Anne, Batalha, Natalie M.
The Kepler mission enabled us to look at the intrinsic population of exoplanets within our galaxy. In period-radius space, the distribution of the intrinsic population of planets contains structure that can trace planet formation and evolution histor
Externí odkaz:
http://arxiv.org/abs/2404.15172
Autor:
Soto, Javier Perez, Laguna, Cesar, Gerard, Benjamin L., Dattilo, Anne, Chambouleyron, Vincent, Jensen-Clem, Rebecca
Due to turbulence in the atmosphere images taken from ground-based telescopes become distorted. With adaptive optics (AO) images can be given greater clarity allowing for better observations with existing telescopes and are essential for ground-based
Externí odkaz:
http://arxiv.org/abs/2308.14855
We present Kepler exoplanet occurrence rates for planets between $0.5-16$ R$_\oplus$ and between $1-400$ days. To measure occurrence, we use a non-parametric method via a kernel density estimator and use bootstrap random sampling for uncertainty esti
Externí odkaz:
http://arxiv.org/abs/2308.00103
Autor:
Murphy, Joseph M. Akana, Batalha, Natalie M., Scarsdale, Nicholas, Isaacson, Howard, Ciardi, David R., Gonzales, Erica J., Giacalone, Steven, Twicken, Joseph D., Dattilo, Anne, Fetherolf, Tara, Rubenzahl, Ryan A., Crossfield, Ian J. M., Dressing, Courtney D., Fulton, Benjamin, Howard, Andrew W., Huber, Daniel, Kane, Stephen R., Petigura, Erik A., Robertson, Paul, Roy, Arpita, Weiss, Lauren M., Beard, Corey, Chontos, Ashley, Dai, Fei, Rice, Malena, Van Zandt, Judah, Lubin, Jack, Blunt, Sarah, Polanski, Alex S., Behmard, Aida, Dalba, Paul A., Hill, Michelle L., Rosenthal, Lee J., Brinkman, Casey L., Mayo, Andrew W., Turtelboom, Emma V., Angelo, Isabel, Močnik, Teo, MacDougall, Mason G., Pidhorodetska, Daria, Tyler, Dakotah, Kosiarek, Molly R., Holcomb, Rae, Louden, Emma M., Hirsch, Lea A., Anderson, Jay, Valenti, Jeff A.
With JWST's successful deployment and unexpectedly high fuel reserves, measuring the masses of sub-Neptunes transiting bright, nearby stars will soon become the bottleneck for characterizing the atmospheres of small exoplanets via transmission spectr
Externí odkaz:
http://arxiv.org/abs/2306.16587
Autor:
Tey, Evan, Moldovan, Dan, Kunimoto, Michelle, Huang, Chelsea X., Shporer, Avi, Daylan, Tansu, Muthukrishna, Daniel, Vanderburg, Andrew, Dattilo, Anne, Ricker, George R., Seager, S.
The TESS mission produces a large amount of time series data, only a small fraction of which contain detectable exoplanetary transit signals. Deep learning techniques such as neural networks have proved effective at differentiating promising astrophy
Externí odkaz:
http://arxiv.org/abs/2301.01371
Autor:
Yu, Liang, Vanderburg, Andrew, Huang, Chelsea, Shallue, Christopher J., Crossfield, Ian J. M., Gaudi, B. Scott, Daylan, Tansu, Dattilo, Anne, Armstrong, David J., Ricker, George R., Vanderspek, Roland K., Latham, David W., Seager, Sara, Dittmann, Jason, Doty, John P., Glidden, Ana, Quinn, Samuel N.
NASA's Transiting Exoplanet Survey Satellite (TESS) presents us with an unprecedented volume of space-based photometric observations that must be analyzed in an efficient and unbiased manner. With at least $\sim1,000,000$ new light curves generated e
Externí odkaz:
http://arxiv.org/abs/1904.02726
Autor:
Dattilo, Anne, Vanderburg, Andrew, Shallue, Christopher J., Mayo, Andrew W., Berlind, Perry, Bieryla, Allyson, Calkins, Michael L., Esquerdo, Gilbert A., Everett, Mark E., Howell, Steve B., Latham, David W., Scott, Nicholas J., Yu, Liang
For years, scientists have used data from NASA's Kepler Space Telescope to look for and discover thousands of transiting exoplanets. In its extended K2 mission, Kepler observed stars in various regions of sky all across the ecliptic plane, and theref
Externí odkaz:
http://arxiv.org/abs/1903.10507
Akademický článek
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Autor:
Ruane, Garreth J., Perez Soto, Javier, Laguna, Cesar, Gerard, Benjamin, Dattilo, Anne, Chambouleyron, Vincent, Jensen-Clem, Rebecca
Publikováno v:
Proceedings of SPIE; October 2023, Vol. 12680 Issue: 1 p126801P-126801P-7, 1141217p
We present exoplanet occurrence rates for planets between 0.4-22 Re and between 1-500 days. We apply a non-parametric method via a kernel density estimator to measure occurrence and use Monte Carlo methods for uncertainty estimation. We use a full ch
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::31470b00b33ed321563adc81eaf4e5d2