Jason T. Wright, Onsi Fakhouri, Geoffrey W. Marcy, Eunkyu Han, Y. Katherina Feng, John Asher Johnson, Andrew W. Howard, Debra A. Fischer, Jeff A. Valenti, Jay Anderson, Nikolai Piskunov,
... searchable, filterable, and sortable form online through the Exoplanets Data Explorer table, and the data can be plotted and explored through the Exoplanet Data Explorer plotter. We use the Data Explorer to generate publication-ready plots, giving three examples of the signatures of exoplanet migration and dynamical evolution: We illustrate the character ...
Tópico(s): Astronomy and Astrophysical Research
2011 - Institute of Physics | Publications of the Astronomical Society of the Pacific
Eunkyu Han, Sharon X. Wang, Jason T. Wright, Y. Katherina Feng, M. Zhao, Onsi Fakhouri, Jacob I. Brown, Colin Hancock,
... literature. The EOD can be navigated through the Exoplanet Data Explorer (EDE) plotter and table, available on the World Wide Web at exoplanets.org. The EOD contains data for 1492 confirmed exoplanets as of 2014 July. ...
Tópico(s): Astronomy and Astrophysical Research
2014 - Institute of Physics | Publications of the Astronomical Society of the Pacific
... data of 211 well-known exoplanets from the Exoplanet Data Explorer data base with ours.
Tópico(s): Astronomy and Astrophysical Research
2019 - Oxford University Press | Monthly Notices of the Royal Astronomical Society
Kevin K. Hardegree-Ullman, Jessie L. Christiansen, David R. Ciardi, Ian J. M. Crossfield, Courtney D. Dressing, John H. Livingston, Kathryn Volk, Eric Agol, Thomas Barclay, Geert Barentsen, Björn Benneke, Varoujan Gorjian, Martti H. Kristiansen,
... orbital periods below 40 days. While analyzing K2 data through the Exoplanet Explorers project, citizen scientists helped discover one super-Earth ...
Tópico(s): Astrophysics and Star Formation Studies
2021 - Institute of Physics | The Astronomical Journal
... systems given in the Exoplanet Orbit Database and Exoplanet Data Explorer (exoplanet.org). The orbital element distribution of the exoplanets ...
Tópico(s): Astrophysics and Star Formation Studies
2018 - American Institute of Physics | AIP conference proceedings
Brittany Miles, Evgenya L. Shkolnik,
... compared to Sun-like stars, time-resolved UV data are needed for more accurate input conditions for exoplanet atmospheric modeling. The Galaxy Evolution Explorer ( GALEX ) provides multi-epoch photometric observations in two ...
Tópico(s): Astrophysics and Star Formation Studies
2017 - Institute of Physics | The Astronomical Journal
D. Woods, J. Ruprecht, Michael C. Kotson, Erin Main, Elizabeth W. Evans, J. Varey, John E. Vaillancourt, H. Viggh, Joshua Brown, András Pál,
... Transiting Exoplanet Survey Satellite (TESS) is a NASA Explorer-class mission designed for finding exoplanets around nearby stars. TESS image data can also serve as a valuable resource for ...
Tópico(s): Gamma-ray bursts and supernovae
2021 - Institute of Physics | Publications of the Astronomical Society of the Pacific
Ajla Suljevic-Pasic, Sadina Gagula-Palalic,
... and reliable algorithm. The data is taken from exoplanet data explorer which was cross checked and filtered with NASA’ ...
Tópico(s): Stellar, planetary, and galactic studies
2016 - International University of Sarajevo | Southeast Europe Journal of Soft Computing
... of 263 well-known planets given in The Exoplanet Data Explorer, while Hansen & Barman (2007) used data on 18 ...
Tópico(s): Astrophysics and Star Formation Studies
2018 - American Institute of Physics | AIP conference proceedings
... known hot Jupiters (HJs) were selected from the Exoplanet Data Explorer database and the classification of these HJs together ...
Tópico(s): Gamma-ray bursts and supernovae
2020 - Elsevier BV | New Astronomy
Kevin H. Knuth, Ben Placek, Daniel Angerhausen, Jennifer L. Carter, Bryan Daniel D'Angelo, Anthony D. Gai, Bertrand Carado,
... improve the characterization of exoplanets. The EXONEST Exoplanetary Explorer is a Bayesian exoplanet inference engine based on nested sampling and originally designed to analyze archived Kepler Space Telescope and CoRoT (Convection Rotation et Transits planétaires) exoplanet mission data. We discuss the EXONEST software package and describe ...
Tópico(s): Astro and Planetary Science
2017 - Multidisciplinary Digital Publishing Institute | Entropy
Farisa Y. Morales, Deborah Padgett, G. Bryden, M. W. Werner, Elise Furlan,
We use data from the Wide-field Infrared Survey Explorer (WISE) all-sky release to explore the incidence of warm dust in the habitable zones around exoplanet-host stars. Dust emission at 12 and/or 22 μm (Tdust ∼ 300 and/or ∼150 K) traces events ...
Tópico(s): Astro and Planetary Science
2012 - IOP Publishing | The Astrophysical Journal
Rishi R. Paudel, Thomas Barclay, Joshua E. Schlieder, Elisa V. Quintana, Emily A. Gilbert, Laura D. Vega, Allison Youngblood, Michele L. Silverstein, Rachel A. Osten, M. A. Tucker, Daniel Huber, A. Do, Kenji Hamaguchi, D. J. Mullan, John E. Gizis, Teresa Monsue, Knicole D. Colón, Patricia T. Boyd, James R. A. Davenport, Lucianne M. Walkowicz,
... flares on nearby active M dwarfs. We acquired data of the nearby dM3.5e star EV Lac using five different observatories: NASA’s Transiting Exoplanet Survey Satellite (TESS), NASA’s Neil Gehrels Swift Observatory (Swift), NASA’s Neutron Interior Composition Explorer (NICER), the University of Hawaii 2.2-meter ...
Tópico(s): Stellar, planetary, and galactic studies
2021 - IOP Publishing | The Astrophysical Journal
Luca Amendola, A. C. O. Leite, C. J. A. P. Martins, N. J. Nunes, P. O. J. Pedrosa, A. Seganti,
... performance of this method when future better-quality data sets are available, focusing on two forthcoming European southern observatory (ESO) spectrographs---Echelle spectrograph for rocky exoplanet and stable spectroscopic observations (ESPRESSO) for the very large telescope (VLT) and Cosmic dynamics explorer (CODEX) for the European extremely large telescope (E- ...
Tópico(s): Gamma-ray bursts and supernovae
2012 - American Physical Society | Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology
Param Rekhi, Sagi Ben-Ami, V. Perdelwitz, Yossi Shvartzvald,
... dwarfs are common stellar hosts of habitable-zone exoplanets. Near-UV (NUV) radiation can severely impact the atmospheric and surface conditions of such planets, making the characterization of NUV flaring activity a key aspect in determining habitability. We use archival data from the Galaxy Evolution Explorer (GALEX) and XMM-Newton telescopes to study the ...
Tópico(s): Gamma-ray bursts and supernovae
2023 - IOP Publishing | The Astrophysical Journal
Kevin France, Keri Hoadley, Brian Fleming, Robert Kane, Nicholas Nell, Matthew Beasley, James C. Green,
... Imaging Spectrograph for Transition region Irradiance from Nearby Exoplanet host stars (SISTINE) form a progression of instrument designs and component-level technology maturation. SLICE is a pathfinder instrument for the development of new data handling, storage, and telemetry techniques. CHESS and SISTINE are testbeds for technology and instrument design enabling high-resolution ([Formula: see text]) point source spectroscopy and high throughput imaging spectroscopy, respectively, in support of future Explorer, Probe, and Flagship-class missions. The CHESS and ...
Tópico(s): Astro and Planetary Science
2016 - World Scientific | Journal of Astronomical Instrumentation
Adina D. Feinstein, Joshua E. Schlieder, John H. Livingston, David R. Ciardi, Andrew W. Howard, Lauren Arnold, Geert Barentsen, Makennah Bristow, Jessie L. Christiansen, Ian J. M. Crossfield, Courtney D. Dressing, Erica J. Gonzales, Molly Kosiarek, Chris Lintott, Grant Miller, Farisa Y. Morales, Erik A. Petigura, Beverly Thackeray, Joanne Ault, Elisabeth Baeten, Alexander F. Jonkeren, James K. Langley, Houssen Moshinaly, Kirk Pearson, Christopher Tanner, Joanna Treasure,
... provided the astronomical community with unprecedented amounts of data to search for transiting exoplanets and other astrophysical phenomena. Here, we present K2-288, a low-mass binary system (M2.0 +/- 1.0; M3.0 +/- 1.0) hosting a small (Rp = 1.9 REarth), temperate (Teq = 226 K) planet observed in K2 Campaign 4. The candidate was first identified by citizen scientists using Exoplanet Explorers hosted on the Zooniverse platform. Follow-up observations ...
Tópico(s): Astronomy and Astrophysical Research
2019 - Institute of Physics | The Astronomical Journal
Avi M. Mandell, Jacob Lustig‐Yaeger, Kevin B. Stevenson, Johannes Staguhn,
... the stellar and planetary spectral signatures. This new data-analysis technique, called planetary infrared excess (PIE), holds the potential to open up the opportunity for measuring mid-infrared (MIR) phase curves of nontransiting rocky planets around the nearest stars with a relatively modest telescope aperture. We present simulations of the performance and science yield for a mission and instrument concept that we call the MIR Exoplanet CLimate Explorer, a concept for a moderately sized cryogenic telescope ...
Tópico(s): Spectroscopy and Laser Applications
2022 - Institute of Physics | The Astronomical Journal
... atmospheres presses forward with missions such as NASA Explorer Program's Transiting Exoplanet Survey Satellite (TESS) slated for launch in 2017 and ESA's PLATO mission scheduled for launch in 2024. These future missions pose daunting data processing challenges in terms of the number of ...
Tópico(s): Gamma-ray bursts and supernovae
2015 - Cambridge University Press | Proceedings of the International Astronomical Union
W. K. Peterson, D. A. Brain, N. R. Schnepf, Y. Dong, Phillip C. Chamberlin, A. W. Yau,
... surface habitability. Current models of atmospheric escape from exoplanets are not well constrained by observations. Atmospheric escape observations from the terrestrial planets are available in public data archives. We recast oxygen escape rates from Earth derived from an instrument on Dynamics Explorer‐1 as function of solar wind and compare ...
Tópico(s): Ionosphere and magnetosphere dynamics
2024 - American Geophysical Union | Geophysical Research Letters
Τ. S. Metcalfe, Jennifer L. van Saders, Daniel Huber, Derek L. Buzasi, R. A. García, Keivan G. Stassun, Sarbani Basu, Sylvain Breton, Zachary R. Claytor, E. Corsaro, M. B. Nielsen, J. M. Joel Ong, Nicholas Saunders, Amalie Stokholm, T. R. Bedding,
... term stellar activity surveys, but archival International Ultraviolet Explorer data revealed a 12 yr activity cycle. Previous ground-based asteroseismology suggested that the star is slightly more massive and substantially larger and older than the Sun, so the similarity of both the rotation rate and the activity cycle period to solar values is perplexing. We use two months of precise time-series photometry from the Transiting Exoplanet Survey Satellite to detect solar-like oscillations in ...
Tópico(s): Astrophysics and Star Formation Studies
2024 - IOP Publishing | The Astrophysical Journal
Pieter Deroo, Mark G. Swain, Robert O. Green,
FINESSE (Fast INfrared Exoplanet Spectroscopic Survey Explorer) will provide uniquely detailed information on the growing number of newly discovered planets by characterizing their atmospheric composition and temperature structure. This NASA Explorer mission, selected for a competitive Phase A study, is unique in its breath and scope thanks to broad instantaneous spectroscopy from the optical to the mid-IR (0.7 – 5 micron), with a survey of exoplanets measured in a consistent, uniform way. For 200 ...
Tópico(s): Astronomy and Astrophysical Research
2012 - SPIE | Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE
Xue Li, Song Wang, Henggeng Han, Jifeng Liu,
Abstract The ongoing discovery of exoplanets has sparked significant interest in finding suitable worlds that could potentially support life. Stellar ultraviolet (UV; 100–3000 Å) radiation may play a crucial role in determining the habitability of their planets. In this paper, we conducted a detailed analysis of the UV photometry of over 2700 host stars with confirmed planets, using observational data from the Galaxy Evolution Explorer and Swift Ultraviolet/Optical Telescope missions. We performed aperture photometry on single-exposure images and provided photometric catalogs that can be ...
Tópico(s): Photoreceptor and optogenetics research
2025 - Institute of Physics | The Astrophysical Journal Supplement Series
Mikkel N. Lund, R. Handberg, H. Kjeldsen, W. J. Chaplin, J. Christensen‐Dalsgaard,
The Transiting Exoplanet Survey Satellite (TESS) is a NASA Astrophysics Explorer mission. Following its scheduled launch in 2017, TESS will focus on detecting exoplanets around the nearest and brightest stars in the ...
Tópico(s): Astro and Planetary Science
2017 - EDP Sciences | EPJ Web of Conferences
Peter Sullivan, Joshua N. Winn, Zachory K. Berta-Thompson, David Charbonneau, Drake Deming, Courtney D. Dressing, David W. Latham, Alan M. Levine, P. R. McCullough, Timothy D. Morton, G. Ricker, R. Vanderspek, D. Woods,
The Transiting Exoplanet Survey Satellite (TESS) is a NASA-sponsored Explorer mission that will perform a wide-field survey for planets that transit bright host stars. Here, we predict ...
Tópico(s): Astrophysics and Star Formation Studies
2015 - IOP Publishing | The Astrophysical Journal
Produção Nacional
Revisado por pares
P. G. Beck, S. Mathur, K. Hambleton, R. A. García, L. Steinwender, Nora L. Eisner, J.-D. do Nascimento, P. Gaulme, S. Mathis,
... the NASA missions Kepler , K2, and TESS (Transiting Exoplanet Survey Satellite) as well as the BRITE (BRIght Target Explorer) constellation mission, we find 99 systems, which were ...
Tópico(s): Astro and Planetary Science
2022 - EDP Sciences | Astronomy and Astrophysics
Tam T. Nguyen, E. Morgan, R. Vanderspek, Alan M. Levine, Miranda Kephart, James Francis, Joseph Zapetis, Kerri Cahoy, G. Ricker,
The Transiting Exoplanet Survey Satellite (TESS) is an MIT-led, NASA-funded Explorer-class planet finder launched in April 2018. TESS will carry out a 2-year all-sky survey with the primary goal of detecting small transiting exoplanets around bright and nearby stars. The TESS instrument ...
Tópico(s): Inertial Sensor and Navigation
2018 - SPIE | Journal of Astronomical Telescopes Instruments and Systems
Pieter Deroo, Mark G. Swain, Robert O. Green,
FINESSE (Fast INfrared Exoplanet Spectroscopic Survey Explorer) will provide uniquely detailed information on the growing number of newly discovered planets by characterizing their atmospheric composition and temperature structure. This NASA Explorer mission, selected for a competitive Phase A study, is unique in its breath and scope thanks to broad instantaneous spectroscopy from the optical to the mid-IR (0.7 - 5 micron), with a survey of exoplanets measured in a consistent, uniform way. For 200 ...
Tópico(s): Astronomy and Astrophysical Research
2012 - SPIE | Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE
G. Ricker, Joshua N. Winn, R. Vanderspek, David W. Latham, G. Á. Bakos, Jacob L. Bean, Zachory K. Berta-Thompson, Timothy M. Brown, Lars A. Buchhave, N. Butler, R. Paul Butler, W. J. Chaplin, David Charbonneau, J. Christensen‐Dalsgaard, Mark Clampin, Drake Deming, J. Doty, Nathan De Lee, Courtney D. Dressing, Edward W. Dunham, Michael Endl, François Fressin, Jian Ge, Thomas Henning, Matthew J. Holman, Andrew W. Howard, Shigeru Ida, Jon Jenkins, G. Jernigan, John Asher Johnson, Lisa Kaltenegger, N. Kawai, H. Kjeldsen, Gregory Laughlin, Alan M. Levine, D. N. C. Lin, Jack J. Lissauer, Phillip J. MacQueen, Geoffrey W. Marcy, P. R. McCullough, Timothy D. Morton, Norio Narita, Martin Paegert, Ε. Πάλλη, F. Pepe, Joshua Pepper, A. Quirrenbach, Stephen A. Rinehart, Dimitar Sasselov, Bun’ei Sato, Sara Seager, A. Sozzetti, Keivan G. Stassun, Peter Sullivan, Andrew Szentgyorgyi, Guillermo Torres, S. Udry, J. Villaseñor,
The Transiting Exoplanet Survey Satellite (TESS ) will search for planets transiting bright and nearby stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer mission. The spacecraft will be placed into a highly elliptical 13.7-day orbit around the Earth. During ...
Tópico(s): Astrophysics and Star Formation Studies
2014 - SPIE | Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE
G. Ricker, Joshua N. Winn, R. Vanderspek, David W. Latham, G. Á. Bakos, Jacob L. Bean, Zachory K. Berta-Thompson, Timothy M. Brown, Lars A. Buchhave, N. Butler, R. Paul Butler, W. J. Chaplin, David Charbonneau, J. Christensen‐Dalsgaard, Mark Clampin, Drake Deming, J. Doty, Nathan De Lee, Courtney D. Dressing, Edward W. Dunham, Michael Endl, François Fressin, Jian Ge, Thomas Henning, Matthew J. Holman, Andrew W. Howard, Shigeru Ida, Jon M. Jenkins, G. Jernigan, John Asher Johnson, Lisa Kaltenegger, N. Kawai, H. Kjeldsen, Gregory Laughlin, Alan M. Levine, D. N. C. Lin, Jack J. Lissauer, Phillip J. MacQueen, Geoffrey W. Marcy, P. R. McCullough, Timothy D. Morton, Norio Narita, Martin Paegert, Ε. Πάλλη, F. Pepe, Joshua Pepper, A. Quirrenbach, Stephen A. Rinehart, Dimitar Sasselov, Bun’ei Sato, Sara Seager, A. Sozzetti, Keivan G. Stassun, Peter Sullivan, Andrew Szentgyorgyi, Guillermo Torres, S. Udry, J. Villaseñor,
The Transiting Exoplanet Survey Satellite (TESS) will search for planets transiting bright and nearby stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer mission. The spacecraft will be placed into a highly elliptical 13.7-day orbit around the Earth. During ...
Tópico(s): Astrophysics and Star Formation Studies
2014 - SPIE | Journal of Astronomical Telescopes Instruments and Systems