2020A&A...640A.130C


C.D.S. - SIMBAD4 rel 1.7 - 2020.10.26CET14:43:46

2020A&A...640A.130C - Astronomy and Astrophysics, volume 640A, 130-130 (2020/8-1)

Fast and Automated Peak Bagging with DIAMONDS (FAMED).

CORSARO E., McKEEVER J.M. and KUSZLEWICZ J.S.

Abstract (from CDS):

Stars of low and intermediate mass that exhibit oscillations may show tens of detectable oscillation modes each. Oscillation modes are a powerful tool to constrain the internal structure and rotational dynamics of the star, hence allowing one to obtain an accurate stellar age. The tens of thousands of solar-like oscillators that have been discovered thus far are representative of the large diversity of fundamental stellar properties and evolutionary stages available. Because of the wide range of oscillation features that can be recognized in such stars, it is particularly challenging to properly characterize the oscillation modes in detail, especially in light of large stellar samples. Overcoming this issue requires an automated approach, which has to be fast, reliable, and flexible at the same time. In addition, this approach should not only be capable of extracting the oscillation mode properties of frequency, linewidth, and amplitude from stars in different evolutionary stages, but also able to assign a correct mode identification for each of the modes extracted. Here we present the new freely available pipeline FAMED (Fast and AutoMated pEak bagging with DIAMONDS), which is capable of performing an automated and detailed asteroseismic analysis in stars ranging from the main sequence up to the core-helium-burning phase of stellar evolution. This, therefore, includes subgiant stars, stars evolving along the red giant branch (RGB), and stars likely evolving toward the early asymptotic giant branch. In this paper, we additionally show how FAMED can detect rotation from dipolar oscillation modes in main sequence, subgiant, low-luminosity RGB, and core-helium-burning stars.

Abstract Copyright: © ESO 2020

Journal keyword(s): asteroseismology - methods: numerical - methods: statistical - methods: data analysis - stars: solar-type - stars: late-type

Simbad objects: 8

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Number of rows : 8

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 KIC 4448777 RG* 19 05 51.0326035588 +39 30 41.141228997           K2 24 0
2 2MASS J19093566+3929507 RG* 19 09 35.6702135726 +39 29 50.698237174   11.25 10.19 9.835   ~ 25 0
3 KIC 12008916 RG* 19 16 23.1885554023 +50 25 37.851149303   13.53 11.94     K1III 20 0
4 2MASS J19193459+4128508 RG* 19 19 34.5940948128 +41 28 51.058611564   11.93 10.78     K2III 25 0
5 2MASS J19231435+3852566 RG* 19 23 14.3564748705 +38 52 56.483832818   11.77 10.62     ~ 15 0
6 BD+44 3149 RG* 19 29 08.4408390104 +44 38 28.450809705   10.84 10.08 9.843   G9.5IV 30 0
7 KIC 2309524 Ro* 19 31 32.1590038057 +37 38 36.141540431           ~ 5 0
8 * 16 Cyg A ** 19 41 48.9539315338 +50 31 30.218780803 6.79 6.59 5.95 5.50 5.17 G1.5Vb 679 1

    Equat.    Gal    SGal    Ecl

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2020.10.26-14:43:46

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