Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
K2 rotation periods for low-mass Hyads and a quantitative comparison of the distribution of slow rotators in the Hyades and Praesepe
ST Douglas, JL Curtis, MA Agüeros… - The Astrophysical …, 2019 - iopscience.iop.org
K2 Rotation Periods for Low-mass Hyads and a Quantitative Comparison of the Distribution of
Slow Rotators in the Hyades and Praesepe - IOPscience Skip to content IOP Science home …
Slow Rotators in the Hyades and Praesepe - IOPscience Skip to content IOP Science home …
The solar neighborhood. xxxvii. the mass–luminosity relation for main-sequence m dwarfs
GF Benedict, TJ Henry, OG Franz… - The Astronomical …, 2016 - iopscience.iop.org
THE SOLAR NEIGHBORHOOD. XXXVII. THE MASS–LUMINOSITY RELATION FOR MAIN-SEQUENCE
M DWARFS - IOPscience Skip to content IOP Science home Accessibility Help Search …
M DWARFS - IOPscience Skip to content IOP Science home Accessibility Help Search …
A temporary epoch of stalled spin-down for low-mass stars: insights from NGC 6811 with Gaia and Kepler
JL Curtis, MA Agüeros, ST Douglas… - The Astrophysical …, 2019 - iopscience.iop.org
A Temporary Epoch of Stalled Spin-down for Low-mass Stars: Insights from NGC 6811 with
Gaia and Kepler - IOPscience Skip to content IOP Science home Accessibility Help Search all …
Gaia and Kepler - IOPscience Skip to content IOP Science home Accessibility Help Search all …
Zodiacal exoplanets in time (ZEIT). IV. Seven transiting planets in the praesepe cluster
Open clusters and young stellar associations are attractive sites to search for planets and to
test theories of planet formation, migration, and evolution. We present our search for, and …
test theories of planet formation, migration, and evolution. We present our search for, and …
Variability properties of four million sources in the TESS input catalog observed with the Kilodegree Extremely Little Telescope survey
Abstract The Kilodegree Extremely Little Telescope (KELT) has been surveying more than
70% of the celestial sphere for nearly a decade. While the primary science goal of the survey …
70% of the celestial sphere for nearly a decade. While the primary science goal of the survey …
When do stalled stars resume spinning down? Advancing gyrochronology with Ruprecht 147
JL Curtis, MA Agüeros, SP Matt, KR Covey… - The Astrophysical …, 2020 - iopscience.iop.org
Recent measurements of rotation periods (Prot) in the benchmark open clusters Praesepe
(670 Myr), NGC 6811 (1 Gyr), and NGC 752 (1.4 Gyr) demonstrate that, after converging …
(670 Myr), NGC 6811 (1 Gyr), and NGC 752 (1.4 Gyr) demonstrate that, after converging …
Lithium depletion boundary, stellar associations, and Gaia
Context. Stellar ages are key to improving our understanding of different astrophysical
phenomena. However, many techniques to estimate stellar ages are highly model …
phenomena. However, many techniques to estimate stellar ages are highly model …
The factory and the beehive. II. Activity and rotation in Praesepe and the Hyades
ST Douglas, MA Agüeros, KR Covey… - The Astrophysical …, 2014 - iopscience.iop.org
Open clusters are collections of stars with a single, well-determined age, and can be used to
investigate the connections between angular-momentum evolution and magnetic activity …
investigate the connections between angular-momentum evolution and magnetic activity …
Diagnosing the Stellar Population and Tidal Structure of the Blanco 1 Star Cluster
We present the stellar population, using Gaia DR2 parallax, kinematics, and photometry, of
the young (∼ 100 Myr), nearby (∼ 230 pc) open cluster, Blanco 1. A total of 644 member …
the young (∼ 100 Myr), nearby (∼ 230 pc) open cluster, Blanco 1. A total of 644 member …
KELT: The Kilodegree Extremely Little Telescope, a Survey for Exoplanets Transiting Bright, Hot Stars
The KELT project was originally designed as a small-aperture, wide-field photometric survey
that would be optimally sensitive to planets transiting bright (V~ 8-10) stars. This magnitude …
that would be optimally sensitive to planets transiting bright (V~ 8-10) stars. This magnitude …