English
Related papers

Related papers: Building a Large Solar Analog Sample Using K2

200 papers

Solar analogs, broadly defined as stars similar to the Sun in mass or spectral type, provide a useful laboratory for exploring the range of Sun-like behaviors and exploring the physical mechanisms underlying some of the Sun's most elusive…

A major obstacle to interpreting the rotation period distribution for main-sequence stars from Kepler mission data has been the lack of precise evolutionary status for these objects. We address this by investigating the evolutionary status…

Stars similar to the Sun, known as solar analogues, provide an excellent opportunity to study the preceding and following evolutionary phases of our host star. The unprecedented quality of photometric data collected by the \Kepler NASA…

High-precision time series photometry with the Kepler satellite has been crucial to our understanding both of exoplanets, and via asteroseismology, of stellar physics. After the failure of two reaction wheels, the Kepler satellite has been…

Instrumentation and Methods for Astrophysics · Physics 2015-10-28 Benjamin Pope , Timothy White , Daniel Huber , Simon Murphy , Tim Bedding , Douglas Caldwell , Aleksa Sarai , Suzanne Aigrain , Thomas Barclay

The space missions MOST, COROT and Kepler are going to provide us with high-precision optical photometry of solar-like stars with time series extending from tens of days to several years. They can be modelled to obtain information on…

Astrophysics · Physics 2008-11-26 A. F. Lanza , A. S. Bonomo , M. Rodono'

Several observatories around the globe started regular full-disc imaging of the solar atmosphere in the Ca II K line in the early decades of the 20th century. These observations are continued today at a few sites with either old…

Solar and Stellar Astrophysics · Physics 2019-01-30 Ilaria Ermolli , Theodosios Chatzistergos , Natalie A. Krivova , Sami K. Solanki

The solar analogues are fundamental targets for a better understanding of our Sun and Solar System. Notwithstanding the efforts, this research is usually limited to field stars. The open cluster M67 offers a unique opportunity to search for…

Astrophysics · Physics 2008-07-08 K. Biazzo , L. Pasquini , P. Bonifacio , S. Randich , L. R. Bedin

We use various method to extract surface rotation periods of Kepler targets exhibiting solar-like oscillations and compare their results.

Solar and Stellar Astrophysics · Physics 2015-10-21 T. Ceillier , R. A. Garcia , D. Salabert , S. Mathur

We provide the first full K2 transiting exoplanet sample, using photometry from Campaigns 1-8 and 10-18, derived through an entirely automated procedure. This homogeneous planet candidate catalog is a crucial to perform a robust demographic…

We address the importance of historical full disc Ca II K spectroheliograms for solar activity and irradiance reconstruction studies. We review our work on processing such data to enable them to be used in irradiance reconstructions. We…

Solar and Stellar Astrophysics · Physics 2019-01-30 Theodosios Chatzistergos , Ilaria Ermolli , Natalie A. Krivova , Sami K. Solanki

Accurate surface rotation measurements are crucial to estimate stellar ages and improve our understanding of stellar rotational evolution. Comparisons of datasets obtained from different space missions on common targets represent in this…

Solar and Stellar Astrophysics · Physics 2025-09-24 Sylvain N. Breton , Elisa Distefano , Alessandro C. Lanzafame , Dinil B. Palakkatharappil

The Kepler mission provides an exciting opportunity to study the lightcurves of stars with unprecedented precision and continuity of coverage. This is the first look at a large sample of stars with photometric data of a quality that has…

We are carrying out a search for planets around a sample of solar twin stars using the HARPS spectrograph. The goal of this project is to exploit the advantage offered by solar twins to obtain chemical abundances of unmatched precision.…

Solar and Stellar Astrophysics · Physics 2014-12-03 I. Ramirez , J. Melendez , J. Bean , M. Asplund , M. Bedell , T. Monroe , L. Casagrande , L. Schirbel , S. Dreizler , J. Teske , M. Tucci Maia , A. Alves-Brito , P. Baumann

The recently approved NASA K2 mission has the potential to multiply by an order of magnitude the number of short-period transiting planets found by Kepler around bright and low-mass stars, and to revolutionise our understanding of stellar…

Instrumentation and Methods for Astrophysics · Physics 2015-06-23 Suzanne Aigrain , Simon T. Hodgkin , Michael J. Irwin , Jim R. Lewis , Stephen J. Roberts

The coming years will see routine use of solar data of unprecedented spatial and spectral resolution, time cadence, and completeness in the wavelength domain. To capitalize on the soon to be available radio facilities such as the expanded…

Solar and Stellar Astrophysics · Physics 2015-05-20 Gregory D. Fleishman , Gelu M. Nita , Dale E. Gary

Stellar activity remains a limiting factor in measuring precise planet parameters from radial velocity spectroscopy, not least in the search for Earth mass planets orbiting in the habitable zones of Sun-like stars. One approach to mitigate…

Earth and Planetary Astrophysics · Physics 2020-05-27 Molly R. Kosiarek , Ian J. M. Crossfield

Solar analogs, stars that closely match the fundamental properties of the Sun, provide key benchmarks for testing stellar structure and evolution across different ages and activity levels. Their detailed characterization helps place the Sun…

Precise photometry from the Kepler space telescope allows not only the measurement of rotation in solar-type field stars, but also the determination of reliable masses and ages from asteroseismology. These critical data have recently…

Solar and Stellar Astrophysics · Physics 2016-08-29 Travis S. Metcalfe , Ricky Egeland , Jennifer van Saders

K2 is the mission concept for a repurposed Kepler mission that uses two reaction wheels to maintain the satellite attitude and provide ~85 days of coverage for ten 105-deg^2 fields along the ecliptic in the first 2.5 years of operation. We…

Solar and Stellar Astrophysics · Physics 2015-06-19 A. Prsa , A. Robin , T. Barclay
‹ Prev 1 2 3 10 Next ›