Skip navigation
  • INAF logo
  • Home
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects
  • Explore by
    • Research outputs
    • Researchers
    • Organization units
    • Projects
  • Login:
    • My DSpace
    • Receive email
      updates
    • Edit Account details
  • Italian
  • English

  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/32380
Title: Overview of the LAMOST-Keplerproject
Authors: Fu, Jian Ning
de Cat, Peter
Zong, Weikai
FRASCA, Antonio 
Gray, Richard O.
Ren, An Bin
Molenda-Zakowicz, Joanna
Corbally, Christopher J.
CATANZARO, Giovanni 
Shi, Jian Rong
Luo, A. Li
Zhang, Hao Tong
Issue Date: 2020
Journal: RESEARCH IN ASTRONOMY AND ASTROPHYSICS 
Number: 20
Issue: 10
First Page: 167
Abstract: The NASA Keplermission obtained long-term high-quality photometric observations for a large number of stars in its original field of view from 2009 to 2013. To provide reliable stellar parameters in a homogeneous way, the LAMOST telescope began to carry out low-resolution spectroscopic observations for as many stars as possible in the Kepler field in 2012. By June 2018, 238 386 low-resolution spectra with SNRg 6 had been collected for 155 623 stars in the Kepler field, enabling the determination of atmospheric parameters and radial velocities, as well as spectral classification of the target stars. This information has been used by astronomers to carry out research in various fields, including stellar pulsations and asteroseismology, exoplanets, stellar magnetic activity and flares, peculiar stars and the Milky Way, binary stars, etc. We summarize the research progress in these fields where the usage of data from the LAMOST-Kepler (LK) project has played a role. In addition, time-domain medium-resolution spectroscopic observations have been carried out for about 12000 stars in four central plates of the Kepler field since 2018. The currently available results show that the LAMOST-Keplermedium resolution (LK-MRS) observations provide qualified data suitable for research in additional science projects including binaries, high-amplitude pulsating stars, etc. As LAMOST is continuing to collect both low- and medium-resolution spectra of stars in the Kepler field, we expect more data to be released continuously and new scientific results to appear based on the LK project data.
URI: http://hdl.handle.net/20.500.12386/32380
URL: https://iopscience.iop.org/article/10.1088/1674-4527/20/10/167
https://api.elsevier.com/content/abstract/scopus_id/85096085889
ISSN: 1674-4527
DOI: 10.1088/1674-4527/20/10/167
Fulltext: open
Appears in Collections:1.01 Articoli in rivista

Files in This Item:
File Description SizeFormat
2008.10776.pdfpreprint2.2 MBAdobe PDFView/Open
Fu_2020_Res._Astron._Astrophys._20_167.pdf[Administrators only]2.23 MBAdobe PDF
Show full item record

Page view(s)

16
checked on Jan 30, 2023

Download(s)

4
checked on Jan 30, 2023

Google ScholarTM

Check

Altmetric

Altmetric


Items in DSpace are published in Open Access, unless otherwise indicated.


Explore by
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects

Informazioni e guide per autori

https://openaccess-info.inaf.it: tutte le informazioni sull'accesso aperto in INAF

Come si inserisce un prodotto: le guide a OA@INAF

La Policy INAF sull'accesso aperto

Documenti e modelli scaricabili

Feedback
Built with DSpace-CRIS - Extension maintained and optimized by Logo 4SCIENCE