J/A+A/651/A70 SHINE sample definition (Desidera+, 2021)
The SPHERE infrared survey for exoplanets (SHINE).
I. Sample definition and target characterization
Desidera S., Chauvin G., Bonavita M., Messina S., LeCoroller H., Schmidt T.,
Gratton R., Lazzoni C., Meyer M., Schlieder J., Cheetham A., Hagelberg J.,
Bonnefoy M., Feldt M., Lagrange A-M., Langlois M., Vigan A., Tan T.G.,
Hambsch F.-J., Millward M., Alcala J., Benatti S., Brandner W., Carson J.,
Covino E., Delorme P., D'Orazi V., Janson M., Rigliaco E., Beuzit J.-L.,
Biller B., Boccaletti A., Dominik F.Cantalloube C., Fontanive C.,
Galicher R., Henning T., Lagadec E., Ligi R., Maire A-L., Menard F.,
Mesa D., Mueller A., Samland M., Schmid H.M., Sissa E., Turatto M., Udry S.,
Zurlo A., Asensio-Torres R., Kopytova T., Rickman E., Abe L., Antichi J.,
Baruolo A., Baudoz P., Baudrand J., Blanchard P., Bazzon A., Buey T.,
Carbillet M., Carle M., Charton J., Cascone E., Claudi R., Costille A.,
Deboulbe A., De Caprio V., Dohlen K., Fantinel D., Feautrier P., Fusco T.,
Gigan P., Giro E., Gisler D., Gluck L., Hubin N., Hugot E., Jaquet M.,
Kasper M., Madec F., Magnard Y., Martinez P., Maurel D., Le Mignant D.,
Moeller-Nilsson O., Llored M., Moulin T., Origne A., Pavlov A., Perret D.,
Petit C., Pragt J., Puget P., Rabou P., Ramos J., Rigal F., Rochat S.,
Roelfsema R., Rousset G., Roux A., Salasnich B., Sauvage J.-F., Sevin A.,
Soenke C., Stadler E., Suarez M., Weber L., Wildi F.
<Astron. Astrophys. 651, A70 (2021)>
=2021A&A...651A..70D 2021A&A...651A..70D (SIMBAD/NED BibCode)
ADC_Keywords: Stars, pre-main sequence ; Photometry ; Space velocities ;
Effective temperatures ; Stars, masses ; Stars, ages
Keywords: stars: fundamental parameters - stars: rotation - stars: activity -
stars: pre-main sequence - stars: kinematics and dynamics -
planets and satellites: general
Abstract:
Large surveys with new-generation high-contrast imaging instruments
are needed to derive the frequency and properties of exoplanet
populations with separations from 5 to 300au. A careful assessment of
the stellar properties is crucial for a proper understanding of when,
where, and how frequently planets form, and how they evolve. The
sensitivity of detection limits to stellar age makes this a key
parameter for direct imaging surveys.
We describe the SpHere INfrared survey for Exoplanets (SHINE), the
largest direct imaging planet-search campaign initiated at the VLT in
2015 in the context of the SPHERE Guaranteed Time Observations of the
SPHERE consortium. In this rst paper we present the selection and the
properties of the complete sample of stars surveyed with SHINE,
focusing on the targets observed during the rst phase of the survey
(from February 2015 to February 2017). This early sample composed of
150 stars is used to perform a preliminary statistical analysis of the
SHINE data, deferred to two companion papers presenting the survey
performance, main discoveries, and the preliminary statistical
constraints set by SHINE.
We describe the SpHere INfrared survey for Exoplanets (SHINE), the
largest direct imaging planet-search campaign initiated at the VLT in
2015 in the context of the SPHERE Guaranteed Time Observations of the
SPHERE consortium. In this rst paper we present the selection and the
properties of the complete sample of stars surveyed with SHINE,
focusing on the targets observed during the first phase of the survey
(from February 2015 to February 2017). This early sample composed of
150 stars is used to perform a preliminary statistical analysis of the
SHINE data, deferred to two companion papers presenting the survey
performance, main discoveries, and the preliminary statistical
constraints set by SHINE.
Based on a large database collecting the stellar properties of all
young nearby stars in the solar vicinity (including kinematics,
membership to moving groups, isochrones, lithium abundance, rotation,
and activity), we selected the original sample of 800 stars that were
ranked in order of priority according to their sensitivity for planet
detection in direct imaging with SPHERE. The properties of the stars
that are part of the early statistical sample were revisited,
including for instance measurements from the GAIA Data Release 2.
Rotation periods were derived for the vast majority of the late-type
objects exploiting TESS light curves and dedicated photometric
observations.
The properties of individual targets and of the sample as a whole are
presented.
Description:
We described SHINE, the largest direct imaging survey for exoplanets
at VLT performed as part of SPHERE GTO.
A subsample of 150 stars with first epoch observations done before
February, 2017 was defined for a preliminary statistical assessment of
the frequency of planets and brown dwarfs in wide orbits (5-300au).
This paper presents the characterization of the individual targets and
of this subsample as a whole.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table5.dat 123 149 Summary of target parameters: names, coordinates,
and photometry (V, J, H and K magnitude,
B-V and V-I colors)
table6.dat 127 150 Summary of target parameters: name, trigonometric
parallax , proper motion, radial velocity, U, V,
W space velocities, moving group membership
table7.dat 127 150 Summary of target parameters: name, X-ray
luminosity, RX=logLX/Lbol, logRHK, rotation
period, vsini, Lithium 6708 EW,
effective temperature, and stellar mass
table8.dat 81 150 Summary of target parameters: name, spectral
type, effective temperature, stellar mass, and
flag on the presence of disks
table9.dat 76 150 Summary of target parameters: stellar ages
table10.dat 107 46 Wide companions to targets in the sample
table11.dat 90 149 Parameters adopted in the original selection
--------------------------------------------------------------------------------
See also:
J/A+A/651/A71 : SHINE II (Langlois+, 2021)
Byte-by-byte Description of file: table5.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/150] Sequential number
5- 19 A15 --- Name Name
21- 35 A15 --- OName Other name
37- 47 A11 --- OName2 Other name
49- 50 I2 h RAh Right ascension (J2000)
52- 53 I2 min RAm Right ascension (J2000)
55- 59 F5.2 s RAs Right ascension (J2000)
61 A1 --- DE- Declination sign (J2000)
62- 63 I2 deg DEd Declination (J2000)
65- 66 I2 arcmin DEm Declination (J2000)
68- 72 F5.2 arcsec DEs Declination (J2000)
74- 79 F6.3 mag Gmag ?=- Gaia DR2 magnitude
81- 86 F6.3 mag BP-RP ?=- Gaia DR2 BP-RP colour index
88- 92 F5.2 mag Vmag V magnitude
94- 99 F6.3 mag B-V ?=- B-V colour index
101-105 F5.2 mag V-I ?=- V-I colour index
107-111 F5.3 mag Jmag 2MASS J magnitude
113-117 F5.3 mag Hmag 2MASS H magnitude
119-123 F5.3 mag Kmag 2MASS K magnitude
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table6.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/150] Sequential number
5- 20 A16 --- Name Name
22- 36 A15 --- OName Other name
38- 43 F6.2 mas plx Parallax
45- 48 F4.2 mas e_plx Parallax error
50- 54 A5 --- r_plx Reference for plx (1)
56- 62 F7.2 mas/yr pmRA Proper motion along RA
64- 67 F4.2 mas/yr e_pmRA Proper motion along RA error
69- 75 F7.2 mas/yr pmDE Proper motion along DE
77- 80 F4.2 mas/yr e_pmDE Proper motion along DE error
82- 86 A5 --- r_pmRA Reference for proper motions (1)
88- 92 F5.1 km/s RV ? Radial velocity
94- 97 F4.1 km/s e_RV ? Radial velocity error
99-103 A5 --- r_RV Reference for RV (1)
105-109 F5.1 km/s Uvel ? Galactic U velocity
111-115 F5.1 km/s Vvel ? Galactic V velocity
117-121 F5.1 km/s Wvel ? Galactic W velocity
123-127 A5 --- Memb Moving group membership
--------------------------------------------------------------------------------
Note (1): References as follows:
Gaia2 = Gaia DR2 Gaia Collaboration et al. (2018A&A...616A...1G 2018A&A...616A...1G. Cat I/345)
VL07 = van Leeuwen (2007A&A...474..653V 2007A&A...474..653V, Cat. I/311)
Des20 = this paper
Car18 = Carleo et al. (2018A&A...613A..50C 2018A&A...613A..50C)
Cha17 = Chauvin et al. (2017A&A...605L...8L 2017A&A...605L...8L, Cat. J/A+A/605/L8)
Che18 = Cheetham et al. (2018A&A...615A.160C 2018A&A...615A.160C)
Che11 = Chen et al. (2011ApJ...738..122C 2011ApJ...738..122C, Cat. J/ApJ/738/122)
Des15 = Desidera et al. (2015A&A...573A.126D 2015A&A...573A.126D. Cat. J/A+A/573/A126)
Duf95 = Dufflot et al. (1995A&AS..110..177D 1995A&AS..110..177D, Cat. J/A+AS/110/177)
Ell14 = Elliott et al. (2014A&A...568A..26E 2014A&A...568A..26E, Cat. J/A+A/568/A26)
Eva67 = Evans (1967, IAU Symposium, 30, 57))
Fer08 = Fernandez et al. (2008A&A...480..735F 2008A&A...480..735F, Cat. J/A+A/480/735)
Gon06 = Gontcharov (2006AstL...32..759G 2006AstL...32..759G, Cat. III/252)
Kis11 = Kiss et al. (2011MNRAS.411..117K 2011MNRAS.411..117K)
Kra14 = Kraus et al. (2014AJ....147..146K 2014AJ....147..146K, Cat. J/AJ/147/146)
Mal14 = Malo et al. (2014ApJ...788...81M 2014ApJ...788...81M, Cat. J/ApJ/788/81)
Mam13 = Mamajek et al. (2013AJ....146..154M 2013AJ....146..154M)
Mon01 = Montes et al. (2001MNRAS.328...45M 2001MNRAS.328...45M, Cat. J/MNRAS/328/45)
Nid02 = Nidever et al. (2002ApJS..141..503N 2002ApJS..141..503N, Cat. J/ApJS/141/503)
Nor04 = Nordstroem et al. (2004A&A...418..989N 2004A&A...418..989N, Cat. V/117)
SACY = Torres et al. (2006A&A...460..695T 2006A&A...460..695T, Cat., J/A+A/460/695)
XHIP = Anderson & Francis (2012AstL...38..331A 2012AstL...38..331A, Cat. V/137)
Whi07 = White et al. (2007AJ....133.2524W 2007AJ....133.2524W, Cat. J/AJ/133/2524)
Zuk01 = Zuckerman et al. (2001ApJ...562L..87Z 2001ApJ...562L..87Z)
Zuk11 = Zuckerman et al. (2011ApJ...732...61Z 2011ApJ...732...61Z)
Source of data for previously unpublished RV determinations.
ESO Program ID is provided for HARPS spectra:
HIP 490: 074.C-0037, 075.C-0202, 076.C-0010, 192.C-0224, 099.C-0205
HIP 1113: 084.C-1039, 192.C-0224
HIP 1481: 074.C-0037, 192.C-0224
HIP 1993: 074.C-0037, 075.C-0202, 077.C-0012
HIP 6276: 192.C-0224, 098.C-0739
HIP 6856: 078.D-0245
HIP 13402: 192.C-0224, 098.C-0739
TYC 5882-1169-1: 074.C-0037, 076.C-0010
TYC 5899-0026-1: 097.C-0864
HIP 23200: 192.C-0224, 097.C-0864, 098.C-0739
HIP 23309: 074.C-0037, 076.C-0010, 192.C-0224
HIP 25283: 072.C-0488, 192.C-0224, 098.C-0739
HIP 30034: 074.C-0037, 076.C-0010, 078.D-0245, 192.C-0224, 098.C-0739
HIP 30314: 083.C-0794, 084.C-1039, 192.C-0224, 098.C-0739
GSC 8894-0426: 097.C-0864
HIP 31878: 192.C-0224, 098.C-0739
HIP 32235: 074.C-0037, 076.C-0010
HIP 36948: 184.C-0815, 192.C-0224, 0102.C-0584
HIP 44526: 192.C-0224
HIP 47135: 074.C-0037, 076.C-001
HIP 51228: 074.C-0364
HIP 51317: 072.C-0488, 082.C-0718, 183.C-0437, 191.C-0873, 192.C-0224,
099.C-020
TWA 7: 074.C-0037, 075.C-0202, 076.C-0010, 077.C-0012, 079.C-0046
HIP 54155: 074.C-0037, 075.C-0202, 082.C-0427, 082.C-0390
HIP 66252: 075.C-0202, 192.C-0224
HIP 69989: Borgniet et al. (2019A&A...621A..87B 2019A&A...621A..87B), reduced spectra
available on OHP archive
HIP 81084: 097.C-0864
HIP 95270: 083.C-0794, 084.C-1039, 192.C-0224
HIP 102409: 075.C-0202, 192.C-0224, 098.C-0739, 099.C-0205
HIP 107350: 192.C-0224, 099.C-0205
HIP 107412: 098.C-0739, 192.C-0224, 099.C-0205, 1101.C-0557
HIP 113283: 60.A-9036
HIP 114530: 192.C-0224
HIP 114948: 075.C-0689, 077.C-0295, 080.C-0712, 184.C-0815
HIP 118008: 084.C-1039, 192.C-0224, 099.C-0205
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table7.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/150] Sequential number
5- 27 A23 --- Name Name
29- 43 A15 --- OName Other name
45- 49 F5.2 [10-7W] logLX ?=- X-ray luminosity
51- 55 F5.2 --- RX ?=- X-ray-to-bolometric luminosity ratio
57- 60 F4.2 --- S ?=- S value (1)
62- 66 F5.2 [-] logRHK ?=- Mount Wilson logRHK index
68- 72 A5 --- r_logLX Reference for logLX (2)
74- 80 F7.4 d Prot ?=- Rotational period
82- 87 F6.4 d e_Prot ?=- Rotational period error
90- 96 F7.5 mag Amp ?=- Amplitude of variation
98-104 A7 --- r_Prot Rotational period references (2)
105-109 F5.1 km/s vsini ?=- Rotational velocity
111-115 A5 --- r_vsini Rotational velocity reference (2)
117-121 F5.1 0.1pm EWLi ? Lithium equivalent width
123-127 A5 --- r_EWLi Lithium equivalent width reference (2)
--------------------------------------------------------------------------------
Note (1): The S-values were constructed as S=α(H+K)/(R+V), where H, K, R,
and V refer to the flux in the corresponding bandpasses and α was
calculated to be 2.4 to make the mean S correspond to the mean F determined
from the HKP-1 observations.
Note (2): References for rotation period as follows:
1a = this study (TESS data)
1b = this study (ASAS data)
1c = this study (ROAD data)
1d = this study (K2 data)
1e = this study (PEST data)
1f = this study (Hipparcos data)
1g = this study (YCO data)
2 = Messina et al. (2010A&A...520A..15M 2010A&A...520A..15M, Cat. J/A+A/520/A15)
3 = Messina et al. (2017A&A...600A..83M 2017A&A...600A..83M, Cat. J/A+A/600/A83)
4 = Messina et al. (2001A&A...366..215M 2001A&A...366..215M)
5 = Koen & Eyer (2002MNRAS.331...45K 2002MNRAS.331...45K, Cat. J/MNRAS/331/45)
6 = Kiraga (2012AcA....62...67K 2012AcA....62...67K, Cat. J/AcA/62/67)
7 = Cutispoto et al. (2003A&A...400..659C 2003A&A...400..659C, Cat. J/A+A/400/659)
8 = Carleo et al. (2018A&A...613A..50C 2018A&A...613A..50C)
9 = Messina et al. (2011A&A...532A..10M 2011A&A...532A..10M, Cat. J/A+A/532/A10)
10 = Desidera et al. (2011A&A...529A..54D 2011A&A...529A..54D)
11 = Lawson & Crause (2005MNRAS.357.1399L 2005MNRAS.357.1399L)
12 = Cutispoto et al. (1999A&AS..138...87C 1999A&AS..138...87C, Cat. J/A+AS/138/87)
13 = Gaidos et al. (2000AJ....120.1006G 2000AJ....120.1006G)
14 = Marsden et al. (2011MNRAS.413.1939M 2011MNRAS.413.1939M)
15 = Maire et al. (2016A&A...587A..56M 2016A&A...587A..56M)
16 = Mosser et al. (2009A&A...506...33M 2009A&A...506...33M)
17 = Folsom et al. (2016MNRAS.457..580F 2016MNRAS.457..580F)
18 = Noyes et al. (1984ApJ...279..763N 1984ApJ...279..763N)
19 = Delorme et al. (2017A&A...608A..79D 2017A&A...608A..79D)
20 = Busko & Torres (1978A&A....64..153B 1978A&A....64..153B)
21 = Donahue et al. (1996ApJ...466..384D 1996ApJ...466..384D)
22 = Oelkers et al. (2018AJ....155...39O 2018AJ....155...39O, Cat. J/AJ/155/39)
23 = Chugainov (1974IzKry..52....3C 1974IzKry..52....3C)
Bal95 = Baliunas et al. (1995ApJ...438..269B 1995ApJ...438..269B)
Bar05 = Barnes (2005MNRAS.364..137B 2005MNRAS.364..137B)
Boe88 = Boesgaard et al. (2018A&A...614A..52B 2018A&A...614A..52B)
Cha17 = Chauvin et al. (2017A&A...605L...9C 2017A&A...605L...9C. Cat. J/A+A/605/L9)
Che18 = Cheetham et al. (2018A&A...615A.160C 2018A&A...615A.160C)
Che11 = Chen et al. (2011ApJ...738..122C 2011ApJ...738..122C, Cat. J/ApJ/738/122)
Cut02 = Cutispoto et al. (2003A&A...400..659C 2003A&A...400..659C, Cat. J/A+A/400/659)
DaS09 = da Silva et al. (2009A&A...508..833D 2009A&A...508..833D, Cat. J/A+A/508/833)
Dav15 = David & Hillenbrand (2015ApJ...804..146D 2015ApJ...804..146D, Cat. J/ApJ/804/146)
Del17 = Delorme et al. (2017A&A...608A..79D 2017A&A...608A..79D)
Des11 = Desidera et al. (2011A&A...529A..54D 2011A&A...529A..54D)
Des15 = Desidera et al. (2015A&A...573A.126D 2015A&A...573A.126D, Cat. J/A+A/573/A126)
Eis13 = Eisenbeiss et al. (2013A&A...556A..53E 2013A&A...556A..53E)
Ers03 = Erspamer & North (2003A&A...398.1121E 2003A&A...398.1121E, Cat. J/A+A/398/1121)
Fav97 = Favata et al. (1997A&A...322..131F 1997A&A...322..131F)
Gai00 = Gaidos et al. (2000AJ....120.1006G 2000AJ....120.1006G)
Gra03 = Gray et al. (2003AJ....126.2048G 2003AJ....126.2048G, Cat. J/AJ/126/2048)
Gra06 = Gray et al. (2006AJ....132..161G 2006AJ....132..161G, Cat. J/AJ/132/161)
Gue07 = Guenther et al. (2007A&A...467.1147G 2007A&A...467.1147G)
Hen96 = Henry et al. (1996AJ....111..439H 1996AJ....111..439H, Cat. J/AJ/111/439)
Hoj19 = Hojjatpanah et al. (2019A&A...629A..80H 2019A&A...629A..80H, Cat. J/A+A/629/A80)
Jef18 = Jeffers et al. (2018A&A...614A..76J 2018A&A...614A..76J, Cat. J/A+A/614/A76)
Jen06 = Jenkins et al. (2006MNRAS.372..163J 2006MNRAS.372..163J, Cat. J/MNRAS/372/163)
Jen11 = Jenkins et al. (2011A&A...531A...8J 2011A&A...531A...8J, Cat. J/A+A/531/A8)
Kin05 = King & Schuler (2005PASP..117..911K 2005PASP..117..911K)
Kis11 = Kiss et al. (2011MNRAS.411..117K 2011MNRAS.411..117K)
Kra14 = Kraus et al. (2014AJ....147..146K 2014AJ....147..146K, Cat. J/AJ/147/146)
Isa10 = Isaacson & Fischer (2010ApJ...725..875I 2010ApJ...725..875I, Cat. J/ApJ/725/875)
MA10 = Martinez-Arnaiz et al. (2010A&A...520A..79M 2010A&A...520A..79M, Cat. J/A+A/520/A79)
Mal13 = Malo et al. (2013ApJ...762...88M 2013ApJ...762...88M, Cat. J/ApJ/762/88)
Mal14 = Malo et al. (2014ApJ...788...81M 2014ApJ...788...81M, Cat. J/ApJ/788/81)
Mar14 = Marsden et al. (2014MNRAS.444.3517M 2014MNRAS.444.3517M, Cat. J/MNRAS/444/3517)
Mes17 = Messina et al. (2017A&A...600A..83M 2017A&A...600A..83M, Cat. J/A+A/600/A83)
Mor01 = Mora et al. (2001A&A...378..116M 2001A&A...378..116M, Cat. J/A+A/378/116)
Nor04 = Nordstroem et al. (2004A&A...418..989N 2004A&A...418..989N, Cat. V/117)
Pal92 = Pallavicini et al. (1992A&A...261..245P 1992A&A...261..245P)
Pri14 = Pribulla et al. (2014MNRAS.443.2815P 2014MNRAS.443.2815P, Cat. J/MNRAS/443/2815)
Rei03 = Reiners & Schmitt (2003A&A...412..813R 2003A&A...412..813R, Cat. J/A+A/412/813)
Rei12 = Reiners et al. (2012AJ....143...93R 2012AJ....143...93R, Cat. J/AJ/143/93)
Roy02 = Royer et al. (2002A&A...393..897R 2002A&A...393..897R, Cat. J/A+A/393/897)
Roy07 = Royer et al. (2007A&A...463..671R 2007A&A...463..671R, Cat. J/A+A/463/671)
SACY = Torres et al. (2006A&A...460..695T 2006A&A...460..695T, Cat. J/A+A/460/695)
Sch07 = Scholz et al. (2007ApJ...662.1254S 2007ApJ...662.1254S)
Sch09 = Schroeder et al. (2009A&A...493.1099S 2009A&A...493.1099S, Cat. J/A+A/493/1099)
Ske08 = Skelly et al. (2008MNRAS.385..708S 2008MNRAS.385..708S)
Tak05 = Takeda & Kawanomoto (2005PASJ...57...45T 2005PASJ...57...45T, Cat. J/PASJ/57/45)
Ues70 = Uesugi & Fukuda (1970CoKwa.189....0U 1970CoKwa.189....0U)
Whi07 = White et al. (2007AJ....133.2524W 2007AJ....133.2524W, Cat. J/AJ/133/2524)
Wic03 = Wichmann et al. (2003A&A...399..983W 2003A&A...399..983W)
Wri04 = Wright et al. (2004ApJS..152..261W 2004ApJS..152..261W, Cat. J/ApJS/152/261)
Zik05 = Zickgraf et al. (2005A&A...433..151Z 2005A&A...433..151Z, Cat. J/A+A/433/151)
Zor12 = Zorec & Royer (2012A&A...537A.120Z 2012A&A...537A.120Z, Cat. J/A+A/537/A120)
Zuk01 = Zuckerman et al. (2001ApJ...562L..87Z 2001ApJ...562L..87Z)
SPH-C = this paper (CORALIE spectra)
SPH-F = this paper (FEROS spectra)
SPH-H = this paper (HARPS spectra)
Source of data for previously unpublished determinations (ESO Program ID
for HARPS and FEROS):
HIP 1113: CORALIE RV survey (Udry et al. 2000)
HIP 6485: 074.C-0037, 075.C-0202, 076.C-0010, 0103.C-0759 (HARPS)
TYC 5882-1169-1: 074.C-0037, 076.C-0010 (HARPS)
HIP 25283: 074.D-0016 (FEROS)
HIP 30030: 60.A-9036, 192.C-0224 (HARPS)
HIP 30034: CORALIE RV survey (Udry et al. 2000)
HIP 31878: 074.D-0016, 083.A-9003 (FEROS)
HIP 32235: 074.C-0037, 076.C-0010 (HARPS)
TYC 1355-214-1: 083.A-9003 (FEROS)
HIP 44526: CORALIE RV survey (Udry et al. 2000)
HIP 66252: 074.D-0016 (FEROS)
HIP 95270: 083.C-0794, 084.C-1039, 192.C-0224 (HARPS)
HIP 114948: 075.C-0689, 077.C-0295, 080.C-0712, 184.C-0815 (HARPS)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table8.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/150] Sequential number
5- 27 A23 --- Name Name
31- 45 A15 --- OName Other name
48- 55 A8 --- SpType Spectral type
56- 60 I5 K Teff Effective temperature
62- 64 I3 K e_Teff Effective temperature error
66- 69 F4.2 Msun Mass Star mass
71- 74 F4.2 Msun e_Mass Star mass error
76- 81 A6 --- Disk Disk flags (1)
--------------------------------------------------------------------------------
Note (1): Disk flags as follows:
RES = spatially resolved disks (not only with SPHERE, only at longer
wavelength in several cases)
IREX = IR excess from SED fitting
IREX2B = IR excess with double components from SED fitting, typically from
Chen et al. (2014ApJS..211...25C 2014ApJS..211...25C, Cat. J/ApJS/211/25)
IREX? = possible IR excess
NO = no detectable IR excess
BCK = IR excess is most likely due to background sources
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table9.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/150] Sequential number
5- 27 A23 --- Name Name
29- 43 A15 --- OName Other name
46- 56 A11 --- OName2 Other name
59- 61 I3 Myr Age Age
63- 65 I3 Myr b_Age Minimum age
67- 70 I4 Myr B_Age Maximum age
72- 76 A5 --- r_Age Age reference (1)
--------------------------------------------------------------------------------
Note (1): References as follows:
MG = age from membership to groups
Des20 = this paper
Boc19 = Boccaletti et al. (2018A&A...614A..52B 2018A&A...614A..52B)
Cha17 = Chauvin et al. (2017, in SF2A-2017: Proceedings of the Annual meeting
of the French Society of Astronomy and Astrophysics, ed. C. Reyle,
P. Di Matteo, F. Herpin, E. Lagadec, A. Lancon, Z. Meliani &
F. Royer, Dia)
Del17 = Delorme et al. (2017A&A...608A..79D 2017A&A...608A..79D)
Laz18 = Lazzoni et al. (2018A&A...611A..43L 2018A&A...611A..43L)
Mam12 = Mamajek (2012ApJ...754L..20M 2012ApJ...754L..20M)
Vig17 = Vigan et al. (2017A&A...603A...3V 2017A&A...603A...3V, Cat. J/A+A/603/A3)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table10.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 15 A15 ---- Name SPH target name
17- 39 A23 --- Comp Companion name
41- 47 F7.1 arcsec rho ?=- Angular separation
49- 54 I6 AU rhol ?=- Linear separation
56- 60 F5.2 mag Dmag ?=- Magnitude difference (1)
62- 64 A3 --- Band Band for magnitude difference
66- 69 F4.2 Msun MassT ?=- Targert mass (2)
71- 75 F5.3 Msun MassC Companion mass (2)
77-103 A27 --- Rem Remarks
105-107 I3 --- Seq Sequential number of target
--------------------------------------------------------------------------------
Note (1): Negative Dmag means that the companion is brighter than the SPHERE
target. When both components are included in the sample, separate entries are
provided.
Note (2): For hierarchical multiple systems the sum of the masses of the
components is listed as the mass of the companion to the SPHERE target.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table11.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/150] Sequential number
5- 19 A15 --- Name Name
21- 35 A15 --- OName Other name
37- 47 A11 --- OName2 Other name
48- 51 F4.2 Msun Mass ? Mass
53- 57 F5.1 pc Dist ? Distance
59- 61 I3 Myr Age ? Age
63- 67 A5 --- Memb Moving group membership
69 I1 --- Prio ? Priority
71- 76 F6.4 --- MF15 ? Merit function for cut-offs of planet
distribution to 15au
78- 83 F6.4 --- MF30 ? Merit function for cut-offs of planet
distribution to 30au
85- 90 F6.4 --- MF50 ? Merit function for cut-offs of planet
distribution to 50au
--------------------------------------------------------------------------------
Acknowledgements:
From pre-print, Silvano Desidera, silvano.desidera(at)oapd.inaf.it
History:
Langlois et al., Paper II 2021A&A...651A..71L 2021A&A...651A..71L, Cat. J/A+A/651/A71
(End) Patricia Vannier [CDS] 18-Jun-2021