J/AJ/165/176  Doppler constraints companions to Sun-like stars (Laliotis+, 2023)

Doppler Constraints on Planetary Companions to Nearby Sun-like Stars; An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging Missions. Laliotis K., Burt J.A., Mamajek E.E., Li Z., Perdelwitz V., Zhao J., Butler R.P., Holden B., Rosenthal L., Fulton B.J., Feng F., Kane S.R., Bailey J., Carter B., Crane J.D., Furlan E., Gnilka C.L., Howell S.B., Laughlin G., Shectman S.A., Teske J.K., Tinney C.G., Vogt S.S., Wang S.X., Wittenmyer R.A. <Astron. J., 165, 176 (2023)> =2023AJ....165..176L 2023AJ....165..176L
ADC_Keywords: Exoplanets; Stars, G-type; Spectra, optical; Stars, masses Keywords: Exoplanet astronomy ; Exoplanet systems ; Radial velocity Abstract: Directly imaging temperate rocky planets orbiting nearby, Sun-like stars with a 6m class IR/O/UV space telescope, recently dubbed the Habitable Worlds Observatory, is a high-priority goal of the Astro2020 Decadal Survey. To prepare for future direct imaging (DI) surveys, the list of potential targets should be thoroughly vetted to maximize efficiency and scientific yield. We present an analysis of archival radial velocity data for southern stars from the NASA/NSF Extreme Precision Radial Velocity (EPRV) Working Group's list of high-priority target stars for future DI missions (drawn from the HabEx, LUVOIR, and Starshade Rendezvous studies). For each star, we constrain the region of companion mass and period parameter space we are already sensitive to based on the observational baseline, sampling, and precision of the archival radial velocity (RV) data. Additionally, for some of the targets, we report new estimates of magnetic activity cycle periods, rotation periods, improved orbital parameters for previously known exoplanets, and new candidate planet signals that require further vetting or observations to confirm. Our results show that for many of these stars we are not yet sensitive to even Saturn-mass planets in the habitable zone, let alone smaller planets, highlighting the need for future EPRV vetting efforts before the launch of a DI mission. We present evidence that the candidate temperate super-Earth exoplanet HD85512b is most likely due to the star's rotation, and report an RV acceleration for δPav that supports the existence of a distant giant planet previously inferred from astrometry. Description: In this work, we include data sets consisting of unbinned radial velocity measurements from five different instruments: High Accuracy Radial velocity Planet Searcher (HARPS) on the ESO 3.6m telescope, High Resolution Echelle Spectrometer (HIRES) on the 10m KeckI telescope, the Levy spectrometer on the 2.4m Automated Planet Finder (APF) telescope, Prime Focus Spectrograph (PFS) on the 6.5m Magellan Clay telescope, and University College London Echelle Spectrograph (UCLES) on the 3.9m Anglo-Australian Telescope. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 63 49 Sample and stellar parameters table3.dat 101 59412 Full timeseries data for each target star table4.dat 117 60 Keplerian radial velocity signals identified by RVSearch table6.dat 47 65 S-index signals identified by RVSearch table7.dat 58 28 Ha signals identified by RVSearch table8.dat 52 6 Speckle imaging results table9.dat 143 27 Updated parameters for previously reported exoplanets table12.dat 52 46 Radial velocity sensitivity refs.dat 70 47 References used -------------------------------------------------------------------------------- See also: B/sb9 : 9th Catalogue of Spectroscopic Binary Orbits (Pourbaix+ 2004-2014) B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017) B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020) III/150 : Perkins Revised MK Types for the Cooler Stars (Keenan+ 1989) III/159 : Ca II H and K Measurements Made at MWO (Duncan+ 1991) V/70 : Nearby Stars, Preliminary 3rd Version (Gliese+ 1991) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) I/329 : URAT1 Catalog (Zacharias+ 2015) I/345 : Gaia DR2 (Gaia Collaboration, 2018) I/349 : StarHorse, Gaia DR2 photo-astrometric distances (Anders+, 2019) IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019) V/122 : SB9; 9th Catalogue of Spectroscopic Binary Orbits (Pourbaix+ 2005) J/ApJ/457/L99 : 25yr CaII-HK observations F-K nearby stars (Baliunas+, 1996) J/AJ/121/2148 : Precise spectral types for 372 A, F & G stars (Gray+, 2001) J/A+A/394/927 : Age-metallicity relation for nearby stars (Ibukiyama+, 2002) J/AJ/126/2048 : NStars project; the Northern Sample. I. (Gray+, 2003) J/A+A/418/551 : Galactic disk stars abunds & velocities (Mishenina+, 2004) J/A+A/426/1007 : Abundances of 8 single-lined active binaries (Morel+, 2004) J/A+A/415/1153 : [Fe/H] for 98 extra-solar planet-host stars (Santos+, 2004) J/A+A/438/139 : Abundances in Milky Way's disk (Soubiran+, 2005) J/PASJ/57/27 : Atmospheric parameters of nearby F-K stars (Takeda+, 2005) J/ApJS/159/141 : Spectroscopic properties of cool stars. I. (Valenti+, 2005) J/ApJ/646/505 : Catalog of nearby exoplanets (Butler+, 2006) J/AJ/132/161 : NStars project; The southern sample. I. (Gray+, 2006) J/A+A/469/309 : Chromospheric activity late-type stars (Cincunegui+, 2007) J/A+A/492/277 : Analysis of Collinder 69 stars with VOSA (Bayo+, 2008) J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008) J/A+A/487/373 : Spectroscopic parameters 451 HARPS-GTO stars (Sousa+, 2008) J/MNRAS/403/1368 : Li abundances & vsini star-planet systems (Gonzalez+, 2010) J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010) J/ApJ/708/1366 : Radial velocities for 61 Vir (Vogt+, 2010) J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011) J/A+A/535/A55 : 4 stars with long-period planets (Dumusque+, 2011) J/AJ/141/45 : Speckle observations of HIP stars (Horch+, 2011) J/AJ/142/19 : Speckle observations of KOI (Howell+, 2011) J/A+A/534/A58 : HD20794, HD85512, HD192310 HARPS RVels (Pepe+, 2011) J/ApJ/743/48 : Stars with rotation periods & X-ray lum (Wright+, 2011) J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012) J/A+A/542/A116 : Rotation in A-F stars (Ammler-von Eiff+, 2012) J/ApJ/759/19 : Precise radial velocities of ρ1 Cancri (Endl+, 2012) J/A+A/541/A40 : Metallicity of solar-type stars (Maldonado+, 2012) J/A+A/547/A106 : Li abundances in the FGK dwarfs (Mishenina+, 2012) J/ApJ/756/46 : Lithium abundances in HIP stars (Ramirez+, 2012) J/A+A/555/A11 : DUNES survey observational results (Eiroa+, 2013) J/ApJ/768/25 : Spitzer & Herschel observations debris disks (Gaspar+, 2013) J/AJ/145/41 : Radial velocities 33 spectroscopic binaries (Katoh+, 2013) J/A+A/554/A84 : Abundances of evolved stars (Maldonado+, 2013) J/ApJ/763/L26 : SMARTS observations of eps Eridani (Metcalfe+, 2013) J/ApJ/764/78 : Oxygen abundances in nearby FGK stars (Ramirez+, 2013) J/A+A/560/A4 : Rotation periods of active Kepler stars (Reinhold+, 2013) J/ApJ/764/3 : Hα indices in M low-mass stars (Robertson+, 2013) J/A+A/555/A150 : Physical parameters cool solar-type stars (Tsantaki+, 2013) J/A+A/552/A78 : Solar like stars radial velocities (Zechmeister+, 2013) J/A+A/566/A66 : Correlation logRHK with logIHα (Gomes da Silva+, 2014) J/A+A/564/A133 : Gaia FGK benchmark stars; metallicity (Jofre+, 2014) J/ApJ/785/33 : High quality Spitzer/MIPS obs. F4-K2 stars (Sierchio+, 2014) J/AJ/147/86 : From binaries to multiples I. FG-67 sample (Tokovinin, 2014) J/MNRAS/441/2361 : Stellar magnetism, age and rotation (Vidotto+, 2014) J/A+A/580/A24 : Abundances in dwarfs, subgiants, & giants (da Silva+, 2015) J/ApJ/812/12 : S-index and Stroemgren LC of HD30495 (Egeland+, 2015) J/A+A/582/A81 : Gaia FGK benchmark stars; abundances (Jofre+, 2015) J/ApJ/804/64 : Empirical and model parameters of 183 M dwarfs (Mann+, 2015) J/A+A/591/A34 : Chemical abundances of zeta Reticuly (Adibekyan+, 2016) J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016) J/MNRAS/462/2295 : 25 parsec local white dwarf population (Holberg+, 2016) J/A+A/587/A131 : Solar twins in the ELODIE archive (Mahdi+, 2016) J/A+A/588/A98 : Metallicities & abundances evolved stars (Maldonado+, 2016) J/AJ/153/208 : LCES HIRES/Keck radial velocity Exoplanet (Butler+, 2017) J/ApJ/848/34 : CATalog of Stellar Unified Properties (Hinkel+, 2017) J/AJ/153/21 : Abundances in local region II. F, G, & Kdwarfs (Luck+, 2017) J/A+A/597/A52 : K & Gdwarfs stellar granulation variability (Meunier+, 2017) J/A+A/614/A55 : Li abundance in dwarfs & subgiants (Aguilera-Gomez+, 2018) J/A+A/616/A108 : Cool stars chromospheric activity cat. (Boro Saikia+, 2018) J/A+A/619/A1 : 55 Cnc radial velocities and photometry (Bourrier+, 2018) J/AJ/155/126 : Radial velocities & photometry K dwarf HD26965 (Diaz+, 2018) J/A+A/619/L10 : pi Men radial velocity curves (Gandolfi+, 2018) J/A+A/619/A81 : Multiplicity among solar-type stars. IV. (Halbwachs+, 2018) J/MNRAS/479/1332 : Binaries with F, G or K primaries & M dwarfs (Montes+, 2018) J/AJ/155/39 : KELT Variability properties TIC sources (Oelkers+, 2018) J/ApJ/855/75 : 24 years monitoring of Sun & Sun-like stars (Radick+, 2018) J/A+A/615/A76 : Spectroscopic parameters of stars (SPECIES) I. (Soto+, 2018) J/A+A/616/A7 : Gaia DR2 radial velocity standard stars (Soubiran+, 2018) J/A+A/620/A58 : SWEET-Cat updated (Sousa+, 2018) J/MNRAS/474/2580 : Temporal evolution neutron-capture elements (Spina+, 2018) J/A+A/624/A78 : Masses & ages of 1059 HARPS-GTO stars (Delgado Mena+, 2019) J/MNRAS/482/4570 : Gaia DR2 white dwarf candidates (Gentile Fusillo+, 2019) J/A+A/623/A72 : Binarity of Hipparcos star Gaia pm anomaly (Kervella+, 2019) J/AJ/157/33 : Radial velocity exploration ε Eridani (Mawet+, 2019) J/MNRAS/490/5088 : Stellar companions of exoplanet host stars (Mugrauer, 2019) J/ApJS/241/12 : Asteroseismic Target List (ATL) for TESS (Schofield+, 2019) J/A+A/639/A127 : Age-chemical-clocks-metallicity relations (Casali+, 2020) J/A+A/641/A110 : Chromospheric activity nearby Sun-like stars (Gondoin, 2020) J/A+A/639/A35 : RV jitter & photometric var correlation (Hojjatpanah+, 2020) J/AJ/160/129 : HARPS, HIRES & AAT Radial Velocities HD136352 (Kane+, 2020) J/AJ/159/235 : Radial Velocity jitters ∼600 planet host stars (Luhn+, 2020) J/A+A/640/A81 : Abundances of 72 solar-type stars (Nissen+, 2020) J/ApJS/246/4 : Cat. of ultrawide binary stars from Gaia DR2 (Tian+, 2020) J/A+A/636/A74 : HARPS radial velocity database (Trifonov+, 2020) J/AJ/161/10 : Radial velocities for 4 host stars (Burt+, 2021) J/other/NatAs/5.775 : nu2 Lupi CHEOPS light curves (Delrez+, 2021) J/A+A/645/L6 : zet01 Ret and zet02 activity indexes (Flores+, 2021) J/A+A/646/A77 : Chromospheric activity AMBRE-HARPS (Gomes da Silva+, 2021) J/AJ/161/295 : Differential Speckle Survey Instrument. X. (Horch+, 2021) J/A+A/652/A116 : CARMENES time-resolved CaII H&K catalog (Perdelwitz+, 2021) J/AJ/163/295 : Radial velocity & astrometry for µ Arae (Benedict+, 2022) J/A+A/657/A125 : KI diagnostic capabilities for M dwarfs (Fuhrmeister+, 2022) J/AJ/163/223 : Radial velocity study of π Mensae (Hatzes+, 2022) J/A+A/657/A7 : Stellar & substellar companions Gaia EDR3 (Kervella+, 2022) J/A+A/658/A57 : F-G-K stars activity indicators (Meunier+, 2022) J/A+A/663/A4 : Mean PASTEL atmospheric parameters (Soubiran+, 2022) http://ebps.carnegiescience.edu/ : The earthbound planet search database Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- HD Henry Draper identifier 10- 13 A4 --- GJ Gliese Catalogue of nearby stars identifier 15- 18 I4 K Teff [4400/6169] Surface effective temperature 20- 23 F4.2 [cm/s2] logg [3.64/4.92] log, surface gravity 25- 29 F5.2 [-] [Fe/H] [-0.66/0.46] Metallicity 31- 32 I2 --- r_[Fe/H] Reference for Metallicity 34- 50 A17 --- SpT Spectral Type 52- 53 I2 --- r_SpT [2/20] Reference for SpT? 55- 60 F6.3 [Lsun] [Lum] [-0.81/0.78] log, luminosity, solar units 62- 63 I2 --- r_[Lum] [3/27] Reference for [Lum] (1) -------------------------------------------------------------------------------- Note (1): For [Lum] reference 25 means that the luminosity for this star was calculated using the Virtual Observatory SED Analyzer version 7.0 (VOSA) assuming zero extinction, logg=4.0, and BT-Settl-AGSS2009 model spectra. This produces a best fit log(L/Lsun) value of +0.5407±0.0065 for HD2151. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- HD Henry Draper identifier 10- 22 F13.5 d BJD [2450277/2459361] Barycentric Julian Date at TBD 24- 31 F8.2 m/s RVel [-5628/4997] Radial velocity 33- 37 F5.2 m/s e_RVel [0.1/34] Uncertainty in RVel 39- 48 A10 --- Inst Instrument for RVel 50- 56 F7.4 --- SHK [0.01/12.3]? Mt. Wilson CaII HK activity index 58- 64 A7 --- e_SHK ? Uncertainty in SHK (1) 66- 72 F7.4 0.1pm EWHa [0.49/0.76]? Equivalent width, Hα, 0.1Å 74- 81 F8.5 0.1pm e_EWHa [0.0007/0.02]? Uncertainty in EWHa 83-101 A19 --- File Filename (2) -------------------------------------------------------------------------------- Note (1): Monte Carlo S-index errors for the HARPS data alongside the photon-noise limited errors derived from the HIRES, PFS, and APF data. These errors should not be (and are not here) used in analysis, as they result in an uneven weighting in favor of the iodine-based instruments. Empirical S-index errors (used in this work) are described in Section 3.2. Note (2): The filenames are unique identifiers for the original observation files in the Earth Bound Planet Search database (http://ebps.carnegiescience.edu/). They correspond either to "rq45.152" type identifiers, which are an internal cataloging system or date-time strings that are the first 19 characters of the ESO archive file name for each HARPS observation. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- HD Henry Draper identifier 10- 12 A3 --- Sig Radial Velocity Signal ID 14- 25 F12.6 d Per [0.73/88080]? Orbital period, days 27- 38 F12.6 d e_Per [5e-06/46000]? Uncertainty in Per 40- 47 F8.3 m/s K [0.43/5691]? semi-amplitude 49- 55 F7.3 m/s e_K [0.07/750]? Uncertainty in K 57- 62 F6.4 --- e [0.006/0.89]? Orbital eccentricity 64- 69 F6.4 --- e_e [0.0003/0.3]? Uncertainty in e 71- 79 F9.2 Mgeo Mass [1.86/201859]? Minimum mass 81- 88 F8.2 Mgeo E_Mass [0.3/79294]? Upper uncertainty in Mass 90- 97 F8.2 Mgeo e_Mass [0.2/71307]? Lower uncertainty in Mass 99-107 E9.3 --- FAP [5e-131/1e-3]? False Alarm Probability (1) 109-117 A9 --- Class Classification of each signal (2) -------------------------------------------------------------------------------- Note (1): FAP values were truncated by VizieR team Note (2): Classification as follows: KP = Known Planet; Candidate = promising planet candidate signal; Binary = Binary Star; SRC = Source Requiring Confirmation; ACT-R = Stellar Rotation; ACT-M = Magnetic Activity Cycle; LPS = Long Period Signal that does not return a well sampled posterior and therefore lacks a full orbital solution prompting us to report only the initial ΔBIC periodogram peak; FP = False positive from aliasing or window function of another detection; * = This signal was reported as a planet in other previous works but we believe it to be stellar in nature, see corresponding discussion sections for details. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- HD Henry Draper identifier 10- 13 A4 --- Sig Radial Velocity Signal ID 15- 15 A1 --- f_Sig Flag on ID (1) 17- 23 F7.2 d Per [2.09/6811]? Orbital period 25- 31 F7.2 d e_Per [0/1600]? Uncertainty in Per 33- 39 F7.5 --- SHK [0.003/0.29]? Mt. Wilson CaII HK activity index 41- 47 F7.5 --- e_SHK [0.0008/0.2]? Uncertainty in SHK -------------------------------------------------------------------------------- Note (1): Signals with a * designation failed to return well constrained MCMC results, and so we instead report the MAP fits for their orbital periods. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- HD Henry Draper identifier 10- 12 A3 --- Sig Radial Velocity Signal ID 14- 14 A1 --- f_Sig Flag on ID (1) 16- 24 F9.3 d Per [19/30889]? Orbital period 26- 31 F6.1 d PPer [5293/7653]? period of the original peak 33- 39 F7.2 d e_Per [0.02/2100]? Uncertainty in Per 41- 50 F10.8 0.1pm EWHa [0.001/0.02]? Equivalent width, Hα, 0.1Å 52- 58 F7.5 0.1pm e_EWHa [0.0002/0.005]? Uncertainty in EWHa -------------------------------------------------------------------------------- Note (1): We report the period and EWHα semi-amplitude of each signal. For signal interpretations, see each stars individual discussion section. Systems with a * designation failed to return well constrained MCMC results, generally producing period uncertainties larger than the median period value, and so we instead report their MAP orbital solutions. In three cases, even the MAP period for the long period signal is more than 3x larger than the significant peak in the ΔBIC periodogram and so we note the period of the original peak in "peakPer". -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD Henry Draper identifier 8- 14 A7 --- Inst Instrument 16- 19 I4 yr Obs.Y [2020/2021] Observation year 21- 23 A3 "month" Obs.M Observation month 25- 26 I2 d Obs.D Observation day 28- 31 F4.2 mag dm562-0.1 [4.31/5.02]? instrumental magnitude difference at 562nm and 0.1arcsec 33- 36 F4.2 mag dm562-1.1 [6.02/7.5]? instrumental magnitude difference at 562nm and 1.1arcsec 38- 41 F4.2 mag dm832-0.1 [4.43/5.05] instrumental magnitude difference at 832nm and 0.1arcsec 43- 46 F4.2 mag dm832-1.1 [7.79/9.33] instrumental magnitude difference at 832nm and 1.1arcsec 48- 52 F5.2 --- Coeff [-0.68/-0.06]? Pearson coefficient value, UCLES Radial velocities and Ha EWs -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- HD Henry Draper identifier 10 A1 --- Sig Radial Velocity Signal ID 12 A1 --- f_HD Flag on ID (1) 14- 24 F11.6 d Per-New [0.73/4035]? Orbital period, New 26- 35 F10.6 d e_Per-New [5e-06/120]? Uncertainty in Per-New 37- 44 F8.3 m/s K-New [0.807/5691]? Semi-amplitude, New 46- 50 F5.3 m/s e_K-New [0.08/3]? Uncertainty in K-New 52- 57 F6.4 --- e-New [0.006/0.65]? Orbital eccentricity, New 59- 64 F6.4 --- e_e-New [0.0003/0.2]? Uncertainty in e-New 66- 77 F12.7 d Per-Old [0.73/3947]? Orbital period, Old 79- 88 F10.7 d E_Per-Old [1.3e-06/30]? Upper uncertainty in Per-Old 90- 99 F10.7 d e_Per-Old [1.4e-06/30]? Lower uncertainty in Per-Old 101-107 F7.3 m/s K-Old [0.6/377]? Semi-amplitude, Old 109-113 F5.3 m/s E_K-Old [0/3]? Upper uncertainty in K-Old 115-119 F5.3 m/s e_K-Old [0.1/3]? Lower uncertainty in K-Old 121-126 F6.4 --- e-Old [0/0.9]? Orbital eccentricity, Old 128-133 F6.4 --- E_e-Old [0/0.2]? Upper uncertainty in e-Old 135-140 F6.4 --- e_e-Old [0/0.3]? Lower uncertainty in e-Old 142-143 I2 --- Ref References -------------------------------------------------------------------------------- Note (1): * = Additional signals detected in our best fit solution, see Table 4 for additional information. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table12.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD Henry Draper identifier 8- 11 A4 --- GJ Gliese Catalogue of Nearby Stars identifier 13- 18 F6.4 Msun Mass [0.69/1.3] Star Mass 20- 25 F6.4 Msun e_Mass [0.003/0.07] Uncertainty in Mass 27- 28 I2 --- r_Mass Reference for Mass 30- 35 F6.3 [Lsun] [Lum] [-0.81/0.78] Log, Stellar luminosity 37- 38 A2 --- r_[Lum] Reference for [Lum] 40- 44 F5.3 au EEID [0.39/2.46] Earth Equivalent Insolation Distance 46- 52 F7.1 Mgeo DopSens [3.7/17394] Doppler Sensitivity -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref [1/47] Reference code 4- 23 A20 --- Author Main author 25- 43 A19 --- BIB BIBcode 45- 60 A16 --- Cat. Catalog in VizieR 62- 70 A9 --- Note Additional note -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 11-Sep-2023
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line