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Query : 2018A&A...616A.155L |
2018A&A...616A.155L - Astronomy and Astrophysics, volume 616A, 155-155 (2018/8-1)
The GAPS Programme with HARPS-N at TNG. XVII. Line profile indicators and kernel regression as diagnostics of radial-velocity variations due to stellar activity in solar-like stars.
LANZA A.F., MALAVOLTA L., BENATTI S., DESIDERA S., BIGNAMINI A., BONOMO A.S., ESPOSITO M., FIGUEIRA P., GRATTON R., SCANDARIATO G., DAMASSO M., SOZZETTI A., BIAZZO K., CLAUDI R.U., COSENTINO R., COVINO E., MAGGIO A., MASIERO S., MICELA G., MOLINARI E., PAGANO I., PIOTTO G., PORETTI E., SMAREGLIA R., AFFER L., BOCCATO C., BORSA F., BOSCHIN W., GIACOBBE P., KNAPIC C., LETO G., MALDONADO J., MANCINI L., MARTINEZ FIORENZANO A., MESSINA S., NASCIMBENI V., PEDANI M. and RAINER M.
Abstract (from CDS):
Abstract Copyright: © ESO 2018
Journal keyword(s): planetary systems - stars: activity - stars: late-type - starspots - stars: atmospheres - techniques: radial velocities
VizieR on-line data: <Available at CDS (J/A+A/616/A155): asym_ind.pro input/* output.dat mpfit.pro>
Simbad objects: 17
Number of rows : 17 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | HD 11506 | PM* | 01 52 50.5344163920 | -19 30 25.108242192 | 8.11 | 7.51 | G0V | 85 | 1 | |||
2 | HD 13931 | PM* | 02 16 47.3787138792 | +43 46 22.786242816 | 7.2 | G0 | 96 | 1 | ||||
3 | HD 23596 | PM* | 03 48 00.3747144624 | +40 31 50.293996068 | 7.85 | 7.24 | F8 | 126 | 1 | |||
4 | BD+50 1471B | EB* | 07 48 07.4814105508 | +50 13 03.255439301 | 11.927 | 11.086 | 10.631 | 10.216 | G9V | 55 | 0 | |
5 | HD 72659 | PM* | 08 34 03.1898361960 | -01 34 05.582173152 | 8.08 | 7.47 | G2V | 158 | 1 | |||
6 | HD 73534 | PM* | 08 39 15.8031501864 | +12 57 37.346867496 | 9.21 | 8.24 | G5 | 57 | 1 | |||
7 | HD 75898 | PM* | 08 53 50.8052389824 | +33 03 24.520566888 | 8.67 | 8.03 | 10.6 | G0 | 77 | 1 | ||
8 | HD 89307 | PM* | 10 18 21.2877106152 | +12 37 15.990903516 | 7.650 | 7.590 | 6.7 | G0V | 120 | 1 | ||
9 | HD 99109 | PM* | 11 24 17.3585400216 | -01 31 44.666848380 | 9.96 | 9.06 | G8/K0IV | 111 | 1 | |||
10 | HD 106252 | PM* | 12 13 29.5095375792 | +10 02 29.887248516 | 8.00 | 7.0 | G0 | 188 | 1 | |||
11 | HD 108874 | PM* | 12 30 26.8817398344 | +22 52 47.377485192 | 9.49 | 8.3 | G9V | 162 | 1 | |||
12 | HD 155358 | PM* | 17 09 34.6176428924 | +33 21 21.085565784 | 7.0 | G0 | 160 | 1 | ||||
13 | HD 188015 | PM* | 19 52 04.5426976824 | +28 06 01.345077360 | 8.95 | 8.23 | G5IV | 96 | 1 | |||
14 | HD 188105 | * | 19 53 11.0645303352 | +08 03 44.803875744 | 8.79 | 7.61 | K0 | 18 | 0 | |||
15 | HD 189733 | BY* | 20 00 43.7129433648 | +22 42 39.073143456 | 9.241 | 8.578 | 7.648 | 7.126 | 6.68 | K2V | 896 | 1 |
16 | HD 190228 | PM* | 20 03 00.7726656864 | +28 18 24.687065520 | 8.094 | 7.296 | G5IV | 167 | 1 | |||
17 | HD 220773 | PM* | 23 26 27.4448301552 | +08 38 37.841644968 | 6.97 | G0 | 69 | 1 |
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