2012A&A...543A..54A


Query : 2012A&A...543A..54A

2012A&A...543A..54A - Astronomy and Astrophysics, volume 543A, 54-54 (2012/7-1)

Oscillation mode frequencies of 61 main-sequence and subgiant stars observed by Kepler.

APPOURCHAUX T., CHAPLIN W.J., GARCIA R.A., GRUBERBAUER M., VERNER G.A., ANTIA H.M., BENOMAR O., CAMPANTE T.L., DAVIES G.R., DEHEUVELS S., HANDBERG R., HEKKER S., HOWE R., REGULO C., SALABERT D., BEDDING T.R., WHITE T.R., BALLOT J., MATHUR S., SILVA AGUIRRE V., ELSWORTH Y.P., BASU S., GILLILAND R.L., CHRISTENSEN-DALSGAARD J., KJELDSEN H., UDDIN K., STUMPE M.C. and BARCLAY T.

Abstract (from CDS):

Solar-like oscillations have been observed by Kepler and CoRoT in several solar-type stars, thereby providing a way to probe the stars using asteroseismology We provide the mode frequencies of the oscillations of various stars required to perform a comparison with those obtained from stellar modelling. We used a time series of nine months of data for each star. The 61 stars observed were categorised in three groups: simple, F-like, and mixed-mode. The simple group includes stars for which the identification of the mode degree is obvious. The F-like group includes stars for which the identification of the degree is ambiguous. The mixed-mode group includes evolved stars for which the modes do not follow the asymptotic relation of low-degree frequencies. Following this categorisation, the power spectra of the 61 main-sequence and subgiant stars were analysed using both maximum likelihood estimators and Bayesian estimators, providing individual mode characteristics such as frequencies, linewidths, and mode heights. We developed and describe a methodology for extracting a single set of mode frequencies from multiple sets derived by different methods and individual scientists. We report on how one can assess the quality of the fitted parameters using the likelihood ratio test and the posterior probabilities. We provide the mode frequencies of 61 stars (with their 1-σ error bars), as well as their associated echelle diagrams.

Abstract Copyright:

Journal keyword(s): asteroseismology - stars: solar-type - stars: oscillations

VizieR on-line data: <Available at CDS (J/A+A/543/A54): list.dat tablea.dat>

Simbad objects: 63

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Number of rows : 63
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 HD 49933 PM* 06 50 49.8309774552 -00 32 27.167495244   6.147 5.771 7.04   F3V 361 2
2 BD+47 2683 * 18 43 42.4230433392 +47 56 16.009897416   9.85 9.26     G0V 63 0
3 2MASS J18441281+4332024 RG* 18 44 12.8095920264 +43 32 02.367065760   10.756 9.676 9.465   K1IV 32 0
4 HD 172910 Pu* 18 44 19.3590068 -35 38 31.154592 3.97 4.69 4.87 5.02 5.18 B2V 88 1
5 HD 173701 PM* 18 44 35.1191008536 +43 49 59.790008892   8.37 7.52     G8V 150 0
6 BD+46 2555 Ro* 18 47 39.2486448504 +46 41 09.979229364   9.98 9.52     F6IV 45 0
7 BD+43 3102 Ro* 18 51 39.5934542496 +43 38 09.727323360   10.10 9.44     G5V 53 0
8 BD+42 3187 RG* 18 54 16.9544655840 +42 59 00.384912816       9.6   G2 80 0
9 BD+45 2796 PM* 18 56 21.2642726544 +45 30 53.234154468   9.80 9.29     G0.5IV 79 0
10 HD 176071 Er* 18 56 22.1268370056 +45 30 25.361404632   8.81 8.33     F8IV 77 0
11 HD 176153 Ro* 18 56 36.6514583496 +47 39 23.133492756   9.20 8.68     F9IV-V 71 0
12 HD 176693 Ro* 18 59 08.6844743448 +48 25 23.600359776   9.34 8.83     F8V 108 0
13 TYC 3541-1117-1 RG* 18 59 09.8407415520 +46 17 05.703253368   11.99 10.99     ~ 21 0
14 TYC 3120-180-1 * 19 00 42.9751446288 +38 34 24.884003820   10.33 9.84     G0IV 21 0
15 HD 177723 * 19 03 45.1355799960 +45 36 30.189464856   9.54 9.10     F8IV 52 0
16 TYC 3545-1033-1 * 19 04 45.6026995824 +48 21 33.390090000   11.349 10.909 10.871   F6IV 23 0
17 BD+38 3428 PM* 19 05 45.2617733112 +38 31 22.560830328   9.77 9.22     F9IV-V 53 0
18 HD 178509 Ro* 19 06 55.9481056080 +42 40 19.342963020   9.39 8.86     F8IV 46 0
19 BD+42 3247 PM* 19 06 58.3280630808 +42 26 08.260897020   10.32 9.75     G0.5IV 59 0
20 HD 178688 * 19 07 43.5917202168 +41 56 15.730146420   9.48 9.02     F6IV 38 0
21 HD 178971 Ro* 19 09 01.9438328856 +38 53 59.485809012   8.79 8.36     F5IV-V 60 0
22 HD 179070 Ro* 19 09 26.8349590368 +38 42 50.455534860   8.767 8.25 8.00   F6IV 152 1
23 TYC 3550-300-1 * 19 09 55.5029520480 +49 15 04.351525056   11.69 10.95     G4-5IV-V 32 0
24 HD 179260 * 19 10 11.6372611944 +38 04 55.831675296   8.94 8.49     F5IV-V 55 0
25 TYC 3125-915-1 * 19 10 35.1292987128 +40 50 35.025862956   11.61 10.72     G3.5III 21 0
26 HD 179732 * 19 11 53.4817713600 +42 06 27.748644156   9.19 8.74     F5IV-V 38 0
27 TYC 3129-1587-1 PM* 19 12 02.2414844760 +42 40 18.811066440   11.49 10.84     ~ 25 0
28 TYC 3121-559-1 * 19 12 16.6298175336 +38 49 03.612586404   10.35 9.75     ~ 29 0
29 HD 234856 Ro* 19 17 45.8018919144 +50 28 48.274775580   9.87 9.32     F9IV-V 71 0
30 HD 181207 PM* 19 17 46.3565007888 +41 24 36.838219932   9.06 8.47     F9IV-V 77 0
31 BD+41 3315 PM* 19 20 29.3442099120 +41 17 28.510142676   9.92 9.38     F9IV-V 38 0
32 BD+43 3221 * 19 20 47.9392965792 +44 09 18.751522032   10.03 9.50     F9IV-V 67 0
33 TYC 3555-1403-1 * 19 20 52.7286151344 +51 28 18.186868416   10.68 9.78     K0III-IV 33 0
34 BD+48 2882 ** 19 21 24.640392 +48 30 53.31924   10.27 9.45 9.36   G1V 52 0
35 BD+48 2887 * 19 22 20.2267974168 +48 41 43.496977812   9.43 9.01     F5IV 39 0
36 HD 182633 * 19 23 36.9148636608 +43 53 28.653685440   8.97 8.47     F5IV-V 28 0
37 BD+41 3338 * 19 24 11.1933479232 +42 03 09.726975180   9.97 9.19     G8IV-V 63 0
38 HD 183298 PM* 19 26 22.0906256352 +50 59 14.334181836   8.71 8.16     G0.5IV 89 0
39 TYC 3551-149-1 PM* 19 27 20.4900952416 +48 57 12.010523580   10.59 9.85     G5IV 48 0
40 BD+36 3570 Ro* 19 28 19.8441075024 +37 03 35.403120000   9.40 8.97     F8IV 53 0
41 HD 184401 PM* 19 32 14.5949892072 +45 18 38.308886100   9.63 8.95     G4V 45 0
42 TYC 3564-2640-1 Ro* 19 34 00.2762796624 +48 50 08.883866472   11.60 10.88     G8IV-V 24 0
43 BD+46 2726 Ro* 19 34 43.0022454096 +46 51 09.938179044   10.36 9.64     K0V 106 0
44 TYC 3143-53-1 Ro* 19 35 03.7372740120 +42 44 16.724850540   10.31 9.85     F8IV 55 0
45 BD+44 3183 PM* 19 35 50.5739000112 +44 52 50.022974316   9.38 8.92     G0IV 52 0
46 BD+49 3061 * 19 36 18.8482043712 +49 49 26.946226164   10.32 9.49     G8IV 30 0
47 BD+44 3197 PM* 19 37 54.5252033200 +44 59 04.630621506       9.3   G0IV 66 0
48 TYC 3556-909-1 PM* 19 37 56.6968217208 +45 57 52.273038852   11.31 10.78     F5 38 0
49 HD 185834 * 19 39 00.6724153968 +46 54 06.984718740   9.26 8.78     F6IV 38 0
50 TYC 3556-3445-1 PM* 19 40 21.2108930904 +45 29 20.963746392   10.48 9.91     G3V 62 0
51 * 16 Cyg A ** 19 41 48.9534996168 +50 31 30.219536784 6.79 6.59 5.95 5.50 5.17 G1.5Vb 714 1
52 HD 186700 PM* 19 43 39.6223173216 +48 55 43.808906244   8.86 8.47     F5IV-V 62 0
53 TYC 3565-1303-1 * 19 43 57.7105385736 +49 55 21.497410956   12.02 11.89     G0 28 0
54 TYC 3565-1235-1 PM* 19 45 45.9639229488 +49 59 18.851817444   10.68 9.84     K1V 34 0
55 BD+44 3244 * 19 46 17.8465825824 +44 49 39.614328156   10.24 9.51     G5IV-V 38 0
56 HD 234998 PM* 19 46 37.7417153592 +51 01 13.527778440   9.16 8.75     F5 42 0
57 HD 187160 SB* 19 46 41.3411982432 +44 20 54.601189476   7.650 7.083     F9IV-V 88 0
58 BD+43 3368 * 19 48 14.2913289840 +43 44 48.961091040   9.63 9.17     F8V 41 0
59 HD 187582 PM* 19 48 22.4074859616 +49 14 11.852056752   9.40 8.71     G3V 38 0
60 BD+47 2934 Ro* 19 50 14.2728443568 +47 28 25.166654760   9.68 9.24     F5IV-V 39 0
61 HD 188819 Ro* 19 54 54.1810396872 +47 08 42.949406328   9.12 8.66     F8IV 57 0
62 HD 190166 PM* 20 01 51.4248305136 +44 21 14.147515008   10.13 9.58     F8V 47 0
63 HD 190319 PM* 20 02 33.3210896856 +44 31 58.994152536   10.63 9.91     G2.5V 36 0

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2022.07.03-19:28:40

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