add kepler/tess text to introduction

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2025-06-01 23:04:44 +02:00
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@@ -654,6 +654,114 @@ archivePrefix = {arXiv},
doi = {10.26093/cds/vizier}, doi = {10.26093/cds/vizier},
} }
@article{kepler_mission_stellar_and_instrument_noise,
doi = {10.1088/0067-0049/197/1/6},
url = {https://dx.doi.org/10.1088/0067-0049/197/1/6},
year = {2011},
month = {oct},
publisher = {The American Astronomical Society},
volume = {197},
number = {1},
pages = {6},
author = {Gilliland, Ronald L. and Chaplin, William J. and Dunham, Edward W. and Argabright, Vic S. and Borucki, William J. and Basri, Gibor and Bryson, Stephen T. and Buzasi, Derek L. and Caldwell, Douglas A. and Elsworth, Yvonne P. and Jenkins, Jon M. and Koch, David G. and Kolodziejczak, Jeffrey and Miglio, Andrea and van Cleve, Jeffrey and Walkowicz, Lucianne M. and Welsh, William F.},
title = {KEPLER MISSION STELLAR AND INSTRUMENT NOISE PROPERTIES},
journal = {The Astrophysical Journal Supplement Series}
}
@ARTICLE{Kepler_first_results,
author = {{Borucki}, William J. and {Koch}, David and {Basri}, Gibor and {Batalha}, Natalie and {Brown}, Timothy and {Caldwell}, Douglas and {Caldwell}, John and {Christensen-Dalsgaard}, J{\o}rgen and {Cochran}, William D. and {DeVore}, Edna and {Dunham}, Edward W. and {Dupree}, Andrea K. and {Gautier}, Thomas N. and {Geary}, John C. and {Gilliland}, Ronald and {Gould}, Alan and {Howell}, Steve B. and {Jenkins}, Jon M. and {Kondo}, Yoji and {Latham}, David W. and {Marcy}, Geoffrey W. and {Meibom}, S{\o}ren and {Kjeldsen}, Hans and {Lissauer}, Jack J. and {Monet}, David G. and {Morrison}, David and {Sasselov}, Dimitar and {Tarter}, Jill and {Boss}, Alan and {Brownlee}, Don and {Owen}, Toby and {Buzasi}, Derek and {Charbonneau}, David and {Doyle}, Laurance and {Fortney}, Jonathan and {Ford}, Eric B. and {Holman}, Matthew J. and {Seager}, Sara and {Steffen}, Jason H. and {Welsh}, William F. and {Rowe}, Jason and {Anderson}, Howard and {Buchhave}, Lars and {Ciardi}, David and {Walkowicz}, Lucianne and {Sherry}, William and {Horch}, Elliott and {Isaacson}, Howard and {Everett}, Mark E. and {Fischer}, Debra and {Torres}, Guillermo and {Johnson}, John Asher and {Endl}, Michael and {MacQueen}, Phillip and {Bryson}, Stephen T. and {Dotson}, Jessie and {Haas}, Michael and {Kolodziejczak}, Jeffrey and {Van Cleve}, Jeffrey and {Chandrasekaran}, Hema and {Twicken}, Joseph D. and {Quintana}, Elisa V. and {Clarke}, Bruce D. and {Allen}, Christopher and {Li}, Jie and {Wu}, Haley and {Tenenbaum}, Peter and {Verner}, Ekaterina and {Bruhweiler}, Frederick and {Barnes}, Jason and {Prsa}, Andrej},
title = "{Kepler Planet-Detection Mission: Introduction and First Results}",
journal = {Science},
keywords = {ASTRONOMY},
year = 2010,
month = feb,
volume = {327},
number = {5968},
pages = {977},
doi = {10.1126/science.1185402},
adsurl = {https://ui.adsabs.harvard.edu/abs/2010Sci...327..977B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@misc{tess_tess,
title={{TESS begins its second extended mission}},
url={https://tess.mit.edu/science/},
auther={TESS},
urldate={2025-06-01}
}
@misc{tess_extended_mission_2,
title={{TESS begins its second extended mission}},
url={https://tess.mit.edu/news/tess-begins-its-second-extended-mission/},
auther={TESS},
urldate={2025-06-01}
}
@misc{tess_extended_mission_1,
title={{TESS Extended Mission}},
url={https://archive.stsci.edu/contents/newsletters/august-2020/tess-extended-mission},
auther={{Mikulski Archive for Space Telescopes}},
urldate={2025-06-01}
}
@misc{tess_nasa,
title={TESS},
url={https://exoplanets.nasa.gov/tess/},
auther={NASA},
urldate={2025-06-01}
}
@misc{tess_missions_and_data_mast,
title={{Transiting Exoplanet Survey Satellite (TESS)}},
url={https://archive.stsci.edu/missions-and-data/tess},
auther={{Mikulski Archive for Space Telescopes}},
urldate={2025-06-01}
}
@misc{kepler_end_nasa_press,
title={{NASA Retires Kepler Space Telescope}},
url={https://www.jpl.nasa.gov/news/nasa-retires-kepler-space-telescope/},
auther={NASA},
urldate={2025-06-01}
}
@misc{kepler_end_nytimes,
title={{Kepler, the Little NASA Spacecraft That Could, No Longer Can}},
url={https://web.archive.org/web/20181030211627/https://www.nytimes.com/2018/10/30/science/nasa-kepler-exoplanet.html},
auther={Dennis Overbye},
urldate={2025-06-01}
}
@misc{kepler_missions_caltech,
title={Kepler Mission Information},
url={https://exoplanetarchive.ipac.caltech.edu/docs/KeplerMission.html},
auther={{NASA Exoplanet Archive}},
urldate={2025-06-01}
}
@misc{k2_missions_and_data_mast,
title={K2},
url={https://archive.stsci.edu/missions-and-data/k2},
auther={{Mikulski Archive for Space Telescopes}},
urldate={2025-06-01}
}
@misc{kepler_missions_and_data_mast,
title={Kepler},
url={https://archive.stsci.edu/missions-and-data/kepler},
auther={{Mikulski Archive for Space Telescopes}},
urldate={2025-06-01}
}
@misc{nasa_kepler_in_depth,
title={{Kepler - In Depth}},
url={https://science.nasa.gov/mission/kepler/in-depth/},
auther={NASA},
urldate={2025-06-01}
}
@misc{astrophysics_group_uk_spectral_types, @misc{astrophysics_group_uk_spectral_types,
title={The Classification of Stellar Spectra}, title={The Classification of Stellar Spectra},
url={http://www.star.ucl.ac.uk/~pac/spectral_classification.html}, url={http://www.star.ucl.ac.uk/~pac/spectral_classification.html},
@@ -1174,7 +1282,7 @@ doi = {10.1371/journal.pone.0210236}
Publisher = {{Apple Inc.}}, Publisher = {{Apple Inc.}},
Title = {Pages '09 User Guide}, Title = {Pages '09 User Guide},
Year = {2010}} Year = {2010}}
@article{KeplerCadenceNyquist, @article{KeplerCadenceNyquist,
author = {Murphy, Simon J.}, author = {Murphy, Simon J.},
title = {An examination of some characteristics of Kepler short- and long-cadence data}, title = {An examination of some characteristics of Kepler short- and long-cadence data},
@@ -42,20 +42,32 @@ The spectral types are a way to classify the vast amount of stars into various t
\section{Flares and Spots \label{sec:intro:flares_and_spots}} \section{Flares and Spots \label{sec:intro:flares_and_spots}}
\subsection{Spots}
\subsection{Flares}
% Stellar Activity, % Stellar Activity,
\section{Space missions \label{sec:intro:space_missions}} \section{Space missions \label{sec:intro:space_missions}}
% TESS, Kepler/K2 % TESS, Kepler/K2
This section gives a short overview on the space mission from which the data was used for this study.
\subsection{Kepler} \subsection{Kepler and K2}
\subsection{K2}
The Kepler space telesope was named after Johannes Kepler and was launched in 2009 (\cite{nasa_kepler_in_depth}) and its primary mission lasted till May 2013 (\cite{kepler_missions_and_data_mast}). Its main scientific goal was the discovery of exoplanets, especially Earth-sized ones, in the habitable zone around their host star (\cite{kepler_missions_caltech}, \cite{Kepler_first_results}). This was done by observing transits of planets around their host star (\cite{kepler_missions_caltech}, \cite{kepler_missions_and_data_mast}, \cite{Kepler_first_results}). \\
It provides two different types of data: short cadence (1 minute exposure) and long cadence (30 minute exposure) data (\cite{Kepler_first_results}, \cite{kepler_missions_and_data_mast}). While short cadence data provides a higher temporal resolution, it was used for fewer targets (\cite{Kepler_first_results}). It had a fixed exposure time of 6.02 seconds for its photometer with a field of view of 115 $deg^{2}$ near the cygnus constellation (\cite{Kepler_first_results}, \cite{kepler_missions_and_data_mast}). The data was then for selected targets accumulated to either short or long cadence, and then downloaded (\cite{Kepler_first_results}). The space telescope could accomondate data of around 170,000 targets with long cadence and 512 targets with short cadence (\cite{Kepler_first_results}). The resolution of each of the 42 CCDs was 4 arcseconds per pixel (\cite{doyle_2019}, \cite{kepler_mission_stellar_and_instrument_noise}).\\
The K2 mission is the continuation mission of Kepler after the second of four of its reaction wheels broke in 2013 (\cite{nasa_kepler_in_depth}, \cite{k2_missions_and_data_mast}). Due to this, a new mission was proposed, keeping the now limited capabilities in mind (\cite{nasa_kepler_in_depth}). The mission was active from February 2014 till September 2018 when its fuel ran out (\cite{k2_missions_and_data_mast}, \cite{kepler_end_nytimes}, \cite{kepler_end_nasa_press}). It discovered a total of over 2600 planets as of 2018 (\cite{kepler_end_nytimes}, \cite{kepler_end_nasa_press}).
\subsection{TESS} \subsection{TESS}
The Transiting Exoplanet Survey Satellite (TESS) was launched in 2018, with its primary mission lasting two years (\cite{tess_nasa}). Since 2020 TESS is in its extended missions, the first being from 2020 to 2022 (\cite{tess_extended_mission_1}), the second from 2022 to 2024 (\cite{tess_extended_mission_2}). TESS has four identical cameras, with each providing a 24 times 24 degree field of view (\cite{tess_tess}, \cite{TESS2014}). TESS's CCDs have a pixel scale of 21 arcseconds (\cite{TESS2014}, \cite{doyle_2019}). The data is provided in 2 minute cadence for individual stars and 30 minute cadence for full frame images (\cite{tess_tess}).\\
TESS observes its targets in so called sectors. Each sector is observed for 27 days (\cite{tess_tess}).
%\section{Current knowledge \label{sec:intro:current_knowledge}} %\section{Current knowledge \label{sec:intro:current_knowledge}}
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@@ -1264,6 +1264,391 @@
\verb https://lweb.cfa.harvard.edu/~pberlind/atlas/htmls/note.html \verb https://lweb.cfa.harvard.edu/~pberlind/atlas/htmls/note.html
\endverb \endverb
\endentry \endentry
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{{hash=b8783ae7a1a805fd17d0937dd94b65fe}{%
family={{Bruhweiler}},
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{{hash=09ee0596e9901673b99fe6d3dc1a8205}{%
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{{hash=4a4f870a74484f36fbbc7bb96eb69540}{%
family={{Prsa}},
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\field{journaltitle}{Science}
\field{month}{2}
\field{number}{5968}
\field{title}{{Kepler Planet-Detection Mission: Introduction and First Results}}
\field{volume}{327}
\field{year}{2010}
\field{pages}{977}
\range{pages}{1}
\verb{doi}
\verb 10.1126/science.1185402
\endverb
\keyw{ASTRONOMY}
\endentry
\entry{orig_harvard_system_sptype_definition}{article}{}{} \entry{orig_harvard_system_sptype_definition}{article}{}{}
\name{author}{2}{}{% \name{author}{2}{}{%
{{hash=37d9c5cd0aaf837f70c6930aeef2d871}{% {{hash=37d9c5cd0aaf837f70c6930aeef2d871}{%
@@ -1635,6 +2020,132 @@
\endverb \endverb
\keyw{astrobiology,techniques: spectroscopic,planets and satellites: detection,stars: fundamental parameters,stars: late-type,stars: low-mass,Astrophysics - Solar and Stellar Astrophysics} \keyw{astrobiology,techniques: spectroscopic,planets and satellites: detection,stars: fundamental parameters,stars: late-type,stars: low-mass,Astrophysics - Solar and Stellar Astrophysics}
\endentry \endentry
\entry{kepler_mission_stellar_and_instrument_noise}{article}{}{}
\name{author}{17}{}{%
{{hash=6bd6b75ba5e030b70eeae1169a494183}{%
family={Gilliland},
familyi={G\bibinitperiod},
given={Ronald\bibnamedelima L.},
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{{hash=32ad9690d3379d7726f93a560eed416f}{%
family={Chaplin},
familyi={C\bibinitperiod},
given={William\bibnamedelima J.},
giveni={W\bibinitperiod\bibinitdelim J\bibinitperiod}}}%
{{hash=1374862852dc88e3610cc1e0fececb20}{%
family={Dunham},
familyi={D\bibinitperiod},
given={Edward\bibnamedelima W.},
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{{hash=795adf4207f188b75272a1e58e1bbd83}{%
family={Argabright},
familyi={A\bibinitperiod},
given={Vic\bibnamedelima S.},
giveni={V\bibinitperiod\bibinitdelim S\bibinitperiod}}}%
{{hash=8c0eff532b591fcda33946ba1b6c4984}{%
family={Borucki},
familyi={B\bibinitperiod},
given={William\bibnamedelima J.},
giveni={W\bibinitperiod\bibinitdelim J\bibinitperiod}}}%
{{hash=9f2ac918346114450f1833a0e16da45c}{%
family={Basri},
familyi={B\bibinitperiod},
given={Gibor},
giveni={G\bibinitperiod}}}%
{{hash=4ed01ec6cd7e83b9eea5be248558a6ab}{%
family={Bryson},
familyi={B\bibinitperiod},
given={Stephen\bibnamedelima T.},
giveni={S\bibinitperiod\bibinitdelim T\bibinitperiod}}}%
{{hash=2ec97bc65453e6791e5d485c91e0d649}{%
family={Buzasi},
familyi={B\bibinitperiod},
given={Derek\bibnamedelima L.},
giveni={D\bibinitperiod\bibinitdelim L\bibinitperiod}}}%
{{hash=141303e7aef9a18504e1db58c89643e4}{%
family={Caldwell},
familyi={C\bibinitperiod},
given={Douglas\bibnamedelima A.},
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{{hash=fac7dc989574725686436c9ba14ab120}{%
family={Elsworth},
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given={Yvonne\bibnamedelima P.},
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{{hash=6ec5ab96601498ff4ac4d2404d1bf0c3}{%
family={Jenkins},
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given={Jon\bibnamedelima M.},
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{{hash=c2c0f8688cd9e92d125b3366d194a5a0}{%
family={Koch},
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given={David\bibnamedelima G.},
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{{hash=1817db02e4f1e8bf21d78c34861251cd}{%
family={Kolodziejczak},
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{{hash=35b151fb026f71c99d0c267814a8dbb5}{%
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{{hash=b3f9de358f894c608081e78cc05c8d73}{%
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{{hash=da82af9f91a0f156725a8953a1d8394b}{%
family={Walkowicz},
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{{hash=51d8a4c8c7e9560952a32628ff733f10}{%
family={Welsh},
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given={William\bibnamedelima F.},
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}
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{The American Astronomical Society}%
}
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\field{abstract}{Kepler mission results are rapidly contributing to fundamentally new discoveries in both the exoplanet and asteroseismology fields. The data returned from Kepler are unique in terms of the number of stars observed, precision of photometry for time series observations, and the temporal extent of high duty cycle observations. As the first mission to provide extensive time series measurements on thousands of stars over months to years at a level hitherto possible only for the Sun, the results from Kepler will vastly increase our knowledge of stellar variability for quiet solar-type stars. Here, we report on the stellar noise inferred on the timescale of a few hours of most interest for detection of exoplanets via transits. By design the data from moderately bright Kepler stars are expected to have roughly comparable levels of noise intrinsic to the stars and arising from a combination of fundamental limitations such as Poisson statistics and any instrument noise. The noise levels attained by Kepler on-orbit exceed by some 50% the target levels for solar-type, quiet stars. We provide a decomposition of observed noise for an ensemble of 12th magnitude stars arising from fundamental terms (Poisson and readout noise), added noise due to the instrument and that intrinsic to the stars. The largest factor in the modestly higher than anticipated noise follows from intrinsic stellar noise. We show that using stellar parameters from galactic stellar synthesis models, and projections to stellar rotation, activity, and hence noise levels reproduce the primary intrinsic stellar noise features.}
\field{journaltitle}{The Astrophysical Journal Supplement Series}
\field{month}{10}
\field{number}{1}
\field{title}{KEPLER MISSION STELLAR AND INSTRUMENT NOISE PROPERTIES}
\field{volume}{197}
\field{year}{2011}
\field{pages}{6}
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\verb{doi}
\verb 10.1088/0067-0049/197/1/6
\endverb
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\verb https://dx.doi.org/10.1088/0067-0049/197/1/6
\endverb
\verb{url}
\verb https://dx.doi.org/10.1088/0067-0049/197/1/6
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{{hash=9f597dfaaa61fb28e8dbda878a4dab55}{% {{hash=9f597dfaaa61fb28e8dbda878a4dab55}{%
@@ -2368,6 +2879,60 @@
\verb 10.1086/126150 \verb 10.1086/126150
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\field{urlmonth}{6}
\field{urlyear}{2025}
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\verb{urlraw}
\verb https://archive.stsci.edu/missions-and-data/kepler
\endverb
\verb{url}
\verb https://archive.stsci.edu/missions-and-data/kepler
\endverb
\endentry
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\field{title}{{Kepler - In Depth}}
\field{urlday}{1}
\field{urlmonth}{6}
\field{urlyear}{2025}
\field{urldateera}{ce}
\verb{urlraw}
\verb https://science.nasa.gov/mission/kepler/in-depth/
\endverb
\verb{url}
\verb https://science.nasa.gov/mission/kepler/in-depth/
\endverb
\endentry
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\field{title}{Kepler Mission Information}
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\field{urlmonth}{6}
\field{urlyear}{2025}
\field{urldateera}{ce}
\verb{urlraw}
\verb https://exoplanetarchive.ipac.caltech.edu/docs/KeplerMission.html
\endverb
\verb{url}
\verb https://exoplanetarchive.ipac.caltech.edu/docs/KeplerMission.html
\endverb
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\entry{V471tau_magnetic_activity}{article}{}{} \entry{V471tau_magnetic_activity}{article}{}{}
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{{hash=7741bee37e2b3b818cfd6daff1bcc632}{% {{hash=7741bee37e2b3b818cfd6daff1bcc632}{%
@@ -2738,6 +3303,81 @@
\endverb \endverb
\keyw{starspots,stars: flare,stars: late-type,Zenodo community cs20} \keyw{starspots,stars: flare,stars: late-type,Zenodo community cs20}
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{{hash=03d4831cc720f5ed189bdfebe9f78a99}{%
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{{hash=68e70c86c91dec9289cd263d8f1087a8}{%
family={{Notsu}},
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{{hash=e21242c02073dce96845c446abd3ec2b}{%
family={{Notsu}},
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{{hash=ce5c945a58e32e3fe998c8dd0774a246}{%
family={{Nagao}},
familyi={N\bibinitperiod},
given={Takashi},
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{{hash=dfb4db096d8c83f9983ab035ab0c84ce}{%
family={{Kusaba}},
familyi={K\bibinitperiod},
given={Satoshi},
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{{hash=4774e2f7f9f58fdbb25f8619f89af9d9}{%
family={{Honda}},
familyi={H\bibinitperiod},
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{{hash=20abe3812625b1f32105a33f66474a37}{%
family={{Nogami}},
familyi={N\bibinitperiod},
given={Daisaku},
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{{hash=f1b717a188c0398fdf0b2eb36a34f93b}{%
family={{Shibata}},
familyi={S\bibinitperiod},
given={Kazunari},
giveni={K\bibinitperiod}}}%
}
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\field{number}{7399}
\field{title}{{Superflares on solar-type stars}}
\field{volume}{485}
\field{year}{2012}
\field{pages}{478\bibrangedash 481}
\range{pages}{4}
\verb{doi}
\verb 10.1038/nature11063
\endverb
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\name{author}{7}{}{% \name{author}{7}{}{%
{{hash=5d1d3d270a3612684876f6dbf5344ae7}{% {{hash=5d1d3d270a3612684876f6dbf5344ae7}{%
@@ -2784,7 +3424,7 @@
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\field{extradatescope}{labelyear} \field{extradatescope}{labelyear}
@@ -3456,6 +4096,59 @@
\verb https://www.stsci.edu/~inr/intrins.html \verb https://www.stsci.edu/~inr/intrins.html
\endverb \endverb
\endentry \endentry
\entry{TESS2014}{article}{}{}
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{{hash=3138bcbc51be7bd63f9154e68b56fad1}{%
family={Ricker},
familyi={R\bibinitperiod},
given={George\bibnamedelima R.},
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{{hash=987e5cdf8fdc979662d7296c44dfcc49}{%
family={Winn},
familyi={W\bibinitperiod},
given={Joshua\bibnamedelima N.},
giveni={J\bibinitperiod\bibinitdelim N\bibinitperiod}}}%
{{hash=7006e388d8ff953fe0c3700abe2d4117}{%
family={Vanderspek},
familyi={V\bibinitperiod},
given={Roland},
giveni={R\bibinitperiod}}}%
{{hash=4a9ed99fe5d2d07a818204600c06001c}{%
family={Latham},
familyi={L\bibinitperiod},
given={David\bibnamedelima W.},
giveni={D\bibinitperiod\bibinitdelim W\bibinitperiod}}}%
}
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\field{journaltitle}{Journal of Astronomical Telescopes, Instruments, and Systems}
\field{title}{Transiting Exoplanet Survey Satellite}
\field{volume}{1}
\field{year}{2014}
\field{pages}{1\bibrangedash 10}
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\verb{doi}
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\verb http://dx.doi.org/10.1117/1.JATIS.1.1.014003
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{{hash=4bd52b64a9681a323e2ac999d1a23602}{% {{hash=4bd52b64a9681a323e2ac999d1a23602}{%
@@ -4010,6 +4703,80 @@
\verb https://doi.org/10.5281/zenodo.3509134 \verb https://doi.org/10.5281/zenodo.3509134
\endverb \endverb
\endentry \endentry
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\field{title}{TESS}
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\field{urlmonth}{6}
\field{urlyear}{2025}
\field{urldateera}{ce}
\verb{urlraw}
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\verb{url}
\verb https://exoplanets.nasa.gov/tess/
\endverb
\endentry
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\field{title}{{TESS begins its second extended mission}}
\field{urlday}{1}
\field{urlmonth}{6}
\field{urlyear}{2025}
\field{urldateera}{ce}
\verb{urlraw}
\verb https://tess.mit.edu/news/tess-begins-its-second-extended-mission/
\endverb
\verb{url}
\verb https://tess.mit.edu/news/tess-begins-its-second-extended-mission/
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\field{title}{{TESS begins its second extended mission}}
\field{urlday}{1}
\field{urlmonth}{6}
\field{urlyear}{2025}
\field{urldateera}{ce}
\verb{urlraw}
\verb https://tess.mit.edu/science/
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\verb{url}
\verb https://tess.mit.edu/science/
\endverb
\endentry
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\field{urlyear}{2025}
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\verb{urlraw}
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\verb{url}
\verb https://archive.stsci.edu/contents/newsletters/august-2020/tess-extended-mission
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{{hash=049c4329ad9329da7fdb92ba5065cce0}{% {{hash=049c4329ad9329da7fdb92ba5065cce0}{%
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