---
res:
  bibo_abstract:
  - During the survey phase of the Kepler mission, several thousand stars were observed
    in short cadence, allowing for the detection of solar-like oscillations in more
    than 500 main-sequence and subgiant stars. These detections showed the power of
    asteroseismology in determining fundamental stellar parameters. However, the Kepler
    Science Office discovered an issue in the calibration that affected half of the
    store of short-cadence data, leading to a new data release (DR25) with corrections
    on the light curves. In this work, we re-analyzed the one-month time series of
    the Kepler survey phase to search for solar-like oscillations that might have
    been missed when using the previous data release. We studied the seismic parameters
    of 99 stars, among which there are 46 targets with new reported solar-like oscillations,
    increasing, by around 8%, the known sample of solar-like stars with an asteroseismic
    analysis of the short-cadence data from this mission. The majority of these stars
    have mid- to high-resolution spectroscopy publicly available with the LAMOST and
    APOGEE surveys, respectively, as well as precise Gaia parallaxes. We computed
    the masses and radii using seismic scaling relations and we find that this new
    sample features massive stars (above 1.2 M⊙ and up to 2 M⊙) and subgiants. We
    determined the granulation parameters and amplitude of the modes, which agree
    with the scaling relations derived for dwarfs and subgiants. The stars studied
    here are slightly fainter than the previously known sample of main-sequence and
    subgiants with asteroseismic detections. We also studied the surface rotation
    and magnetic activity levels of those stars. Our sample of 99 stars has similar
    levels of activity compared to the previously known sample and is in the same
    range as the Sun between the minimum and maximum of its activity cycle. We find
    that for seven stars, a possible blend could be the reason for the non-detection
    with the early data release. Finally, we compared the radii obtained from the
    scaling relations with the Gaia ones and we find that the Gaia radii are overestimated
    by 4.4%, on average, compared to the seismic radii, with a scatter of 12.3% and
    a decreasing trend according to the evolutionary stage. In addition, for homogeneity
    purposes, we re-analyzed the DR25 of the main-sequence and subgiant stars with
    solar-like oscillations that were previously detected and, as a result, we provide
    the global seismic parameters for a total of 525 stars.@eng
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: S.
      foaf_name: Mathur, S.
      foaf_surname: Mathur
  - foaf_Person:
      foaf_givenName: R. A.
      foaf_name: García, R. A.
      foaf_surname: García
  - foaf_Person:
      foaf_givenName: S.
      foaf_name: Breton, S.
      foaf_surname: Breton
  - foaf_Person:
      foaf_givenName: A. R. G.
      foaf_name: Santos, A. R. G.
      foaf_surname: Santos
  - foaf_Person:
      foaf_givenName: B.
      foaf_name: Mosser, B.
      foaf_surname: Mosser
  - foaf_Person:
      foaf_givenName: D.
      foaf_name: Huber, D.
      foaf_surname: Huber
  - foaf_Person:
      foaf_givenName: M.
      foaf_name: Sayeed, M.
      foaf_surname: Sayeed
  - foaf_Person:
      foaf_givenName: Lisa Annabelle
      foaf_name: Bugnet, Lisa Annabelle
      foaf_surname: Bugnet
      foaf_workInfoHomepage: http://www.librecat.org/personId=d9edb345-f866-11ec-9b37-d119b5234501
    orcid: 0000-0003-0142-4000
  - foaf_Person:
      foaf_givenName: A.
      foaf_name: Chontos, A.
      foaf_surname: Chontos
  bibo_doi: 10.1051/0004-6361/202141168
  bibo_volume: 657
  dct_date: 2022^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/0004-6361
  - http://id.crossref.org/issn/1432-0746
  dct_language: eng
  dct_publisher: EDP Sciences@
  dct_subject:
  - Space and Planetary Science
  - Astronomy and Astrophysics
  dct_title: Detections of solar-like oscillations in dwarfs and subgiants with Kepler
    DR25 short-cadence data@
...