J/A+A/621/A110   Two new giant planets around metal-poor stars  (Barbato+, 2019)

The GAPS Programme with HARPS-N at TNG. XVIII. Two new giant planets around the metal-poor stars HD 220197 and HD 233832. Barbato D., Sozzetti A., Biazzo K., Malavolta L., Santos N.C., Damasso M., Lanza A.F., Pinamonti M., Affer L., Benatti S., Bignamini A., Bonomo A.S., Borsa F., Carleo I., Claudi R., Cosentino R., Covino E., Desidera S., Esposito M., Giacobbe P., Gonzalez-Alvarez E., Gratton R., Harutyunyan A., Leto G., Maggio A., Maldonado J., Mancini L., Masiero S., Micela G., Molinari E., Nascimbeni V., Pagano I., Piotto G., Poretti E., Rainer M., Scandariato G., Smareglia R., Colombo L.S., Di Fabrizio L., Faria J.P., Martinez Fiorenzano A., Molinaro M., Pedani M. <Astron. Astrophys. 621, A110 (2019)> =2019A&A...621A.110B 2019A&A...621A.110B (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Stars, giant ; Radial velocities Keywords: techniques: radial velocities - methods: data analysis - planetary systems - stars: abundances - stars: individual: HD 220197 - stars: individual: HD 233832 Abstract: Statistical studies of exoplanets have shown that giant planets are more commonly hosted by metal-rich dwarf stars than low-metallicity stars, while no such correlation is evident for lower mass planets. The search for giant planets around metal-poor stars and the estimate of their occurrence fp is an important element in providing support to models of planet formation. We present results from the HARPS-N search for giant planets orbiting metal-poor (-1.0≤[Fe/H]≤-0.5dex) stars in the northern hemisphere, complementing a previous HARPS survey on southern stars in order to update the estimate of fp. High-precision HARPS-N observations of 42 metal-poor stars were used to search for planetary signals to be fitted using differential evolution Markov chain Monte Carlo single-Keplerian models. We then joined our detections to the results of the previous HARPS survey on 88 metal-poor stars to provide a preliminary estimate of the two-hemisphere fp. We report the detection of two new giant planets around HD 220197 and HD 233832. The first companion has Msini=0.20-0.04+0.07MJup and an orbital period of 1728-80+162days, and for the second companion, we find two solutions of equal statistical weight with periods of 2058-40+47 and 4047-117+91days and minimum masses of 1.78-0.06+0.08 and 2.72-0.23+0.23MJup, respectively. Joining our two detections with the three from the southern survey, we obtain a preliminary and conservative estimate of the global frequency of fp=3.84-1.06+2.45% for giant planets around metal-poor stars. The two new giant planets orbit dwarf stars at the metal-rich end of the HARPS-N metal-poor sample. This corroborates previous results that suggested that giant planet frequency is still a rising function of the host star [Fe/H]. We also note that all detections in the overall sample are giant long-period planets. Description: We carried out high-precision HARPS-N observations of two metal-poor stars and report the discovery of two long-period giant planets. For each of the target stars and each datapoint epoch of observation, exposure time, radial velocity measurement, RV error, bisector, full-width at half-maximum, logRHK and air mass are given. Objects: ---------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------- 23 21 58.29 +16 37 57.1 HD 220197 = HIP 115359 11 26 05.48 +50 22 32.8 HD 233832 = HIP 55806 ---------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 93 168 HARPS-N radial velocity measurements and exposure times, activity indexes and airmass -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 ---- Star Host star name (HD 220197 or HD 233832) 13- 26 F14.6 d BJD Epochs of radial velocities 30- 33 I4 s Texp Exposure time 36- 43 F8.4 km/s RV Radial velocity 47- 52 F6.4 km/s e_RV Radial velocity uncertainty 56- 61 F6.3 km/s BIS Bisector inverse span 65- 69 F5.3 km/s FWHM CCF full-width at half-maximum 73- 77 F5.3 km/s FWHMcorr ? CCF full-width at half-maximum (corrected) 81- 86 F6.3 ---- logRHK Activity index logRHK 90- 93 F4.2 ---- AirMass Air mass at exposure start -------------------------------------------------------------------------------- Acknowledgements: Domenico Barbato, domenico.barbato(at)inaf.it
(End) Patricia Vannier [CDS] 20-Nov-2018
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