J/AJ/169/293    Angular diameters of 145 stars from the NPOI     (Baines+, 2025)

Vintage NPOI: New and updated angular diameters for 145 stars. Baines E.K., Clark J.H.I., Kingsley B.I., Schmitt H.R., Stone J.M. <Astron. J., 169, 293 (2025)> =2025AJ....169..293B 2025AJ....169..293B
ADC_Keywords: Stars, diameters; Interferometry; Optical; Photometry; Effective temperatures; MK spectral classification; Reddening; Stars, masses Keywords: Stellar astronomy ; Fundamental parameters of stars ; High angular resolution ; Optical interferometry Abstract: We present new or updated angular diameters, physical radii, and effective temperatures for 145 stars from the Navy Precision Optical Interferometer (NPOI) data archive. We used data from 1996 to late 2021, and we describe the differences between early and late data, which hinge upon an update of the beam combiner in 2002. We came across several subcategories of stars of interest: 13 of our stars are promising targets for the Habitable World Observatory and therefore require as much study as possible, and 14 more are asteroseismic targets and have stellar masses after we combined our radii and effective temperatures with frequencies of maximum oscillation power values from the literature. In addition to this, many of the stars here show measurements to the first null in the visibility curve and beyond, which is the gateway to determining second-order effects such as direct measurements of limb darkening. Finally, we consider the stars in the larger context of previous NPOI measurements and find the majority (75%) of the angular diameters in the overall NPOI sample have uncertainties of 2% or less. Description: The NPOI is an optical interferometer on Anderson Mesa, near Flagstaff, Arizona, and has been in operation since 1996. For the handful of years from 1996 to mid 2002, the original version of the "Classic" beam combiner was used. It recorded data on one baseline1 per spectrograph, of which there were three, and it observed over 32 spectral channels from 430 to 860nm. Each 2ms data frame was split into eight temporal bins, and each scan was 90s long. Starting in mid 2002 the NPOI system changed to recording data from 16 channels (550-860nm) and two spectrographs, using 30s scans. The new procedure allowed for the simultaneous recording of all 15 baselines but required the use of 64 temporal bins for each 2ms data frame. The baseline, which is the distance between two siderostats or telescopes, goes from a mere 7.2 to 79.4m in this study. Other optical/infrared interferometers use telescopes but the NPOI uses siderostats, which are flat mirrors. Over the last almost 30yr, the NPOI has observed hundreds of stars, and here we present measurements for 145 of them. The data set presented here is by far the largest ever published in one place from the NPOI, totaling very nearly 360,000 data points. The dates of observations range from 1996 May to when the NPOI temporarily shut down after 2021 October. All of the scientific targets were observed alternately with calibrator stars, chosen so that the scientific target's angular diameter measurement would be only weakly dependent on the calibrator star's angular diameter determination (Baines+2018, J/AJ/155/30). When observing, we made two basic assumptions about the scientific targets: that they are effectively single, and that they do not rotate rapidly enough to be oblate and experience gravity darkening (van Belle+2012, J/other/A+ARV/20.51). A good number of the targets discussed here do indeed have stellar companions, but in the majority of cases, those companions are well outside the NPOI's detection sensitivity. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 86 145 Sample star properties table4.dat 111 1691 Observing log table5.dat 96 107 Calibrator stars' SED inputs and resulting angular diameters table6.dat 102 145 Interferometric results table7.dat 80 145 Derived stellar parameters table8.dat 27 35 Stars in the WDS table9.dat 27 13 Promising HWO targets table10.dat 60 14 Stellar oscillators table11.dat 8 120 Zero-crossing stars fig3/* . 145 Visibility curves in JPG format (Data behind Figure 3) -------------------------------------------------------------------------------- See also: B/pastel : The PASTEL catalogue (Soubiran+, 2016-) B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020) I/149A : Fifth Fundamental Catalogue (FK5) Part I (Fricke+, 1988) I/175 : Fifth Fundamental Catalogue (FK5) - Extension (Fricke+ 1991) I/284 : The USNO-B1.0 Catalog (Monet+ 2003) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) I/345 : Gaia DR2 (Gaia Collaboration, 2018) I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) II/62 : Catalogue of Extinction Data (Neckel+, 1980) II/114 : UV Interstellar Extinction (Savage+ 1985) II/168 : Homogeneous Means in the UBV System (Mermilliod 1991) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) II/346 : JMMC Stellar Diameters Catalogue - JSDC. Version 2 (Bourges+, 2017) II/354 : HIP and TGAS stars reddening and extinction (Gontcharov+ 2018) III/39A : UV Bright Star Spectrophotometric Catalog (Jamar+, 1976) III/135A : Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989) III/164 : Catalog of Eq.Widths of Interstellar 217nm Band (Friedemann 1992) III/232 : STELIB: A library of stellar spectra at R∼2000 (Le Borgne+, 2003) IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019) IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021) V/50 : Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991) V/137D : Extended Hipparcos Compilation (XHIP) (Anderson+, 2012) J/A+AS/118/481 : ROSAT all-sky survey catalogue of OB stars (Berghoefer+ 1996) J/A+AS/117/227 : Dwarf effective temperatures (Alonso+ 1996) J/A+A/352/555 : Fundamental parameters of stars (Allende Prieto+, 1999) J/A+A/393/183 : Catalogue of calibrator stars for LBSI (Borde+, 2002) J/AJ/126/2048 : NStars project: the Northern Sample. I. (Gray+, 2003) J/AJ/127/1227 : Synthetic Stroemgren photometry (Clem+, 2004) J/ApJS/152/251 : Indo-US library of coude feed stellar spectra (Valdes+, 2004) J/A+A/440/305 : Fundamental parameters of fast-rotating B stars (Fremat+, 2005) J/ApJ/626/446 : Effective temperature scale of FGK stars (Ramirez+, 2005) J/ApJ/647/312 : FUSE survey of OVI in the Milky Way (Otte+, 2006) J/MNRAS/367/1478 : Interstellar NaI, TiII & CaIIK obs. (Hunter+, 2006) J/MNRAS/371/1793 : Metallicity calibrations for UBV photometry (Karatas+, 2006) J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006) J/A+A/475/1003 : Stellar parameters of G and K giant stars (Hekker+, 2007) J/ApJS/176/276 : PTI calibrator catalog (van Belle+, 2008) J/ApJ/700/1299 : Gas-phase element depletions in the ISM (Jenkins, 2009) J/A+A/501/297 : Effective temperatures of B Supergiants (Zorec+, 2009) J/ApJ/722/605 : A stellar rotation census of B stars (Huang+, 2010) J/A+A/522/A79 : Faint, high-Gal-latitude red clump stars (Valentini+, 2010) J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 2011) J/A+A/525/A90 : Thick disc vertical properties (Katz+, 2011) J/MNRAS/414/1227 : Mg/Fe ratio of MILES stars (Milone+, 2011) J/A+A/531/A165 : MILES atmospheric parameters (Prugniel+, 2011) J/A+A/525/A71 : Atmospheric parameters for 1273 stars (Wu+, 2011) J/other/A+ARV/20.51 : Rapidly rotating stars (Van Belle, 2012) J/ApJS/199/8 : A compilation of interstellar column dens. (Gudennavar+, 2012) J/ApJ/768/128 : K-band calibrated visibilities of 24 Be stars (Touhami+, 2013) J/A+A/549/A129 : Equivalent widths of cool stars (Cesetti+, 2013) J/AJ/150/151 : DSSI obs. of binaries. VI. Measures in 2014 (Horch+, 2015) J/AJ/150/123 : Catalog of 316 K giant candidates (Rebull+, 2015) J/MNRAS/459/1170 : Coulour-Period relation for Cepheids (Scowcroft+, 2016) J/A+A/595/A132 : Be star rotational velocities distribution (Zorec+, 2016) J/A+A/589/A83 : PCA-based inversion of stellar parameters (Gebran+, 2016) J/ApJ/826/171 : IR data of debris disk vs metallicity of stars (Gaspar+, 2016) J/MNRAS/471/770 : Parameters & IR excesses of Gaia DR1 stars (McDonald+, 2017) J/AJ/155/30 : Fundamental parameters of 87 stars from the NPOI (Baines+, 2018) J/AJ/156/102 : The TESS Input Catalog & Candidate Target List (Stassun+, 2018) J/A+A/619/A134 : ATHOS. Flux ratio based stellar parameteriz. (Hanke+, 2018) J/A+A/623/A72 : Binar. of Hipparcos stars from Gaia pm anom. (Kervella+, 2019) J/AJ/158/167 : Speckle obs. & orbits of multiple stars (Tokovinin+, 2019) J/A+A/633/A34 : Lithium in red giant stars (Charbonnel+, 2020) J/ApJ/889/157 : Ages of FGK stars considering C and O abundances (Chen+, 2020) J/MNRAS/504/3730 : Synthetic RGB photometry of bright stars (Cardiel+, 2021) J/AJ/162/198 : Fundamental parameters of 44 stars with NPOI (Baines+, 2021) J/ApJ/919/131 : Oscillating red giants from the TESS QLP (Hon+, 2021) J/ApJ/915/13 : 1997-2019 automated B,V phot. of gam Cas (Smith+, 2021) J/MNRAS/517/2925 : ORB6 binaries in Gaia EDR3 (Chulkov+, 2022) J/A+A/657/A7 : Stellar & substellar companions from Gaia EDR3 (Kervella+, 2022) J/A+A/658/A48 : 7 giants/subgiants limb-darkening coeff. (Karovicova, 2022) J/A+A/657/A7 : Stellar & substellar companions from Gaia EDR3 (Kervella+, 2022) J/ApJS/266/6 : In the Trenches of the solar-stellar connect. VII. (Ayres, 2023) J/A+A/683/A161 : Solar-like stars global oscillation propert. (Corsaro+, 2024) J/ApJS/272/30 : Habitable Worlds Observatory (HWO): 164 targets (Harada+, 2024) J/A+A/689/A270 : An all-sky cat. of stellar reddening values (Paunzen+, 2024) J/A+A/682/A145 : Gaia FGK benchmark stars v3 (Soubiran+, 2024) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD [432/223047] Henry Draper catalog (III/135A) identifier 8- 11 I4 --- HR [21/9003] Yale Bright star catalog (V/50) identifier 13- 16 I4 --- FK5 [2/3799]? Fifth Fundamental catalogue (I/149A, I/175) identifier 18- 27 A10 --- WDS Washington Double Star (B/wds) identifier 29- 41 A13 --- Name Other name for target 43- 56 A14 --- SpType Spectral Type, from SIMBAD 58- 61 F4.2 mag Vmag [0.03/5.58] V-band magnitude, from Mermilliod, 1991 (II/168) 63- 68 F6.2 mas plx [1.42/284.56] Parallax 70- 73 F4.2 mas e_plx [0.02/2.23] Uncertainty in plx 75- 80 A6 --- r_plx Reference for plx (1) 82- 84 I3 km/s vsini [0/329]? Projected rotational velocity, from Hoffleit+1964 (V/50) 86 A1 --- Pub [YN] Previously Published? (2) -------------------------------------------------------------------------------- Note (1): References for parallax are as follows: CM22 = J/MNRAS/517/2925 (Chulkov+, 2022); 1 occurrence Gaia18 = I/345 (Gaia DR2, 2018); 3 occurrences Gaia22 = I/355 (Gaia DR3, 2022); 109 occurrences vL07 = I/311 (van Leeuwen, 2007); 32 occurrences Note (2): Flag as follows: Y = Previously published (83 occurrences) N = Not previously published (62 occurrences) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD [432/223047] Henry Draper catalog (III/135A) identifier 8 A1 --- f_HD [*] Flag on HD (column added by CDS) (2) 10- 15 I6 --- Calib [886/222173] Henry Draper catalog (III/135A) calibrator star identifier 17- 27 A11 "Y:M:D" Date UT date (YYYY-MM-DD) 29- 103 A75 --- Baselines Baselines used (1) 105- 106 I2 --- Nscans [1/39] Number of scans per baseline 108- 111 I4 --- Npoints [6/2010] Number of calibrated V2 (visibility) measurements points -------------------------------------------------------------------------------- Note (1): Baseline length between telescope pairs as follows: AC-AE = 18.9m AC-AN = 22.8m AC-AW = 22.2m AC-E2 = 7.2m AC-E6 = 34.4m AC-W4 = 8.8m AC-W7 = 51.3m AE-AN = 34.9m AE-AW = 37.5m AE-E2 = 15.9m AE-E6 = 15.9m AE-E7 = 37.1m AE-W4 = 26.7m AE-W7 = 64.2m AN-AW = 38.2m AN-E2 = 20.0m AN-E6 = 45.6m AN-W7 = 66.4m AW-E2 = 29.1m AW-E3 = 31.9m AW-E4 = 34.5m AW-E6 = 53.3m AW-E7 = 73.5m AW-W4 = 14.0m AW-W7 = 29.5m E2-E4 = 7.8m E2-W7 = 58.7m E3-W4 = 18.6m E6-W4 = 42.5m E6-W7 = 79.4m E7-W7 = 97.5m Note (2): The flagged observation had a typo in its HD identifier. The original data has "HD 113208" but it has been corrected to "HD 133208" in this table. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- Calib [886/222173] Henry Draper catalog (III/135A) calibrator star identifier 8- 18 A11 --- SpType Spectral Type, from SIMBAD 20- 23 F4.2 mag Umag [0.48/6.71] U-band mag, from Mermilliod, 1991 (II/168) 25- 28 F4.2 mag Bmag [1.41/6.07] B-band mag, from Mermilliod, 1991 (II/168) 30- 33 F4.2 mag Vmag [1.64/5.46] V-band mag, from Mermilliod, 1991 (II/168) 35- 38 F4.2 mag Rmag [1.71/5.36] R-band mag, from USNO-B1.0 catalog (Monet+2003, I/284) 40- 43 F4.2 mag Imag [1.84/5.26] I-band mag, from USNO-B1.0 catalog (Monet+2003, I/284) 45- 48 F4.2 mag Jmag [2.15/5.22] J-band mag, from 2MASS (Cutri+2003, II/246) 50- 53 F4.2 mag Hmag [2.13/5.02] H-band mag, from 2MASS (Cutri+2003, II/246) 55- 58 F4.2 mag Ksmag [2.07/4.93] Ks-band mag, from 2MASS (Cutri+2003, II/246) 60- 64 I5 K Teff [4750/29242] Surface effective temperature 66- 69 F4.2 [cm/s2] logg [1.8/5.11] Log, surface gravity, cgs 71- 75 A5 --- Ref Reference for Teff, logg (1) 77- 80 F4.2 mag E(B-V) [0/0.33] Reddening 82- 86 A5 --- r_E(B-V) Reference for E (B-V) (1) 88- 91 F4.2 mas theta-est [0.23/1.5] Estimated angular diameter (2) 93- 96 F4.2 mas e_theta-est [0.01/0.07] Uncertainty in theta-est -------------------------------------------------------------------------------- Note (1): References for Teff, logg, and E(B-V) values are as follows: sA23 = J/ApJS/266/6 (Ayres, 2023) A96 = J/A+AS/117/227 (Alonso+ 1996) APL99 = J/A+A/352/555 (Allende Prieto+, 1999) B96 = J/A+AS/118/481 (Berghoefer+ 1996) C04 = J/AJ/127/1227 (Clem+, 2004) C21 = J/MNRAS/504/3730 (Cardiel+, 2021) F05 = J/A+A/440/305 (Fremat+, 2005) F92 = III/164 (Friedemann 1992) G03 = J/AJ/126/2048 (Gray+, 2003) G12 = J/ApJS/199/8 (Gudennavar+, 2012) G16 = J/A+A/589/A83 (Gebran+, 2016) GM18 = II/354 (Gontcharov+ 2018) H06 = J/MNRAS/367/1478 (Hunter+, 2006) HGM10 = J/ApJ/722/605 (Huang+, 2010) J09 = J/ApJ/700/1299 (Jenkins, 2009) J95 = III/39A (Jamar+, 1976) K19 = J/A+A/623/A72 (Kervella+, 2019) KAT22 = J/A+A/657/A7 (Kervella+, 2022) KS06 = J/MNRAS/371/1793 (Karatas+, 2006) LB03 = III/232 (Le Borgne+, 2003) MZW17 = J/MNRAS/471/770 (McDonald+, 2017) N80 = II/62 (Neckel+, 1980) OD06 = J/ApJ/647/312 (Otte+, 2006) P07 = 2007astro.ph..3658P 2007astro.ph..3658P (Prugniel+, 2007) P24 = J/A+A/689/A270 (Paunzen+, 2024) RM05 = J/ApJ/626/446 (Ramirez+, 2005) S85 = II/114 (Savage+ 1985) SB06 = J/MNRAS/371/703 (Sanchez-Blazquez+, 2006) Sou16 = B/pastel (Soubiran+, 2016-) T13 = J/ApJ/768/128 (Touhami+, 2013) V04 = J/ApJS/152/251 (Valdes+, 2004) VM10 = J/A+A/522/A79 (Valentini+, 2010) W11 = J/A+A/525/A71 (Wu+, 2011) Z09 = J/A+A/501/297 (Zorec+, 2009) vB08 = J/ApJS/176/276 (van Belle+, 2008) Note (2): The estimated angular diameter is calculated using the method described in Section 3. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD [432/223047] Henry Draper catalog (III/135A) identifier 8 A1 --- Flag Flag on diameter fit (1) 10- 14 F5.3 mas theta-ud [0.77/8.83] Apparent uniform disk (UD) angular diameter 16- 20 F5.3 mas e_theta-ud [0.002/0.4] Uncertainty in theta-ud 22- 26 I5 K Teff [3431/35210] Surface effective temperature 28- 31 F4.2 [cm/s2] logg [0.05/4.6] Log, surface gravity 33- 39 A7 --- Ref Reference for stellar parameters (2) 41- 45 F5.2 [-] [Fe/H] [-0.56/0.3] Metallicity, [Fe/H] 47- 51 A5 --- r_[Fe/H] Reference for FeH (2) 53- 56 F4.2 --- mu-i [0.24/0.86] Initial limb-darkening coefficient (3) 58- 62 F5.3 mas theta-ld-i [0.8/9.63] Initial limb-darkening angular diameter 64- 68 F5.3 mas e_theta-ld-i [0.002/0.41] Uncertainty in theta-ld-i 70- 73 F4.2 --- mu-f [0.32/0.86] Final limb-darkening coefficient (3) 75- 79 F5.3 mas theta-ld-f [0.8/9.7] Final limb-darkening angular diameter 81- 85 F5.3 mas e_theta-ld-f [0.001/0.42] Uncertainty in theta-ld-f 87- 90 F4.1 % sigtheta [0.1/45.6] Percent uncertainty in theta-ld-f 92- 96 F5.1 10+6/s MaxSF [28.5/150.7] Maximum spatial frequency for the diameter measurement, 10+6cycles/second 98- 102 I5 --- Nfit [60/17514] Number of data points in angular diameter fit -------------------------------------------------------------------------------- Note (1): Flag as follows: * = See Section 5 for discussion about potential sources of bias for this star. Note (2): References for Teff, logg are as follows: AF12 = V/137D (Anderson+, 2012) APL99 = J/A+A/352/555 (Allende Prieto+, 1999) B02 = J/A+A/393/183 (Borde+, 2002) C13 = J/A+A/549/A129 (Cesetti+, 2013) C21 = J/MNRAS/504/3730 (Cardiel+, 2021) Cha20 = J/A+A/633/A34 (Charbonnel+, 2020) Che20 = J/ApJ/889/157 (Chen+, 2020) GRB16 = J/ApJ/826/171 (Gaspar+, 2016) Gaia22 = I/355 (Gaia DR3, 2022) H07 = J/A+A/475/1003 (Hekker+, 2007) H18 = J/A+A/619/A134 (Hanke+, 2018) K11 = J/A+A/525/A90 (Katz+, 2011) LB03 = III/232 (Le Borgne+, 2003) M11 = J/MNRAS/414/1227 (Milone+, 2011) MZW17 = J/MNRAS/471/770 (McDonald+, 2017) P07 = 2007astro.ph..3658P 2007astro.ph..3658P (Prugniel+, 2007) P11 = J/A+A/531/A165 (Prugniel+, 2011) S18 = J/AJ/156/102 (Stassun+, 2018) S19 = IV/38 (Stassun+, 2019) Sco16 = J/MNRAS/459/1170 (Scowcroft+, 2016) Sou16 = B/pastel (Soubiran+, 2016-) V04 = J/ApJS/152/251 (Valdes+, 2004) Z16 = J/A+A/595/A132 (Zorec+, 2016) Note (3): The initial linear, limb-darkening coefficient, mu-i, is based on the Teff and logg listed in the table; the final mu-f is based on the new Teff determination; see Section 4. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD [432/223047] Henry Draper catalog (III/135A) identifier 8- 13 F6.2 Rsun Rad [0.8/426.8] Derived stellar radius 15- 19 F5.2 Rsun E_Rad [0.1/69.5]?=" Upper uncertainty in Rad 21- 26 F6.2 Rsun e_Rad [0.01/107.4] Symmetric or lower uncertainty in Rad 28- 31 F4.1 % sigRad [0.3/45.6] Percent uncertainty in Rad 33- 39 F7.1 Lsun L [0.6/41422.3] Stellar luminosity 41- 45 F5.1 Lsun e_L [0/298] Uncertainty in L 47- 52 A6 --- r_L Reference for L (1) 54- 59 F6.1 10-9W/m2 Fbol [19.2/2882] Bolometric flux, 10-6erg/s/cm2, SED fit 61- 64 F4.1 10-9W/m2 e_Fbol [0.2/98] Uncertainty in Fbol 66- 70 I5 K Teff [2285/14159] Final derived stellar effective temperature 72- 75 I4 K e_Teff [7/1268] Uncertainty in Teff 77- 80 F4.1 % sigTeff [0.1/23] Percent uncertainty in Teff -------------------------------------------------------------------------------- Note (1): References for L as follows: AF12 = V/137A (Anderson+, 2012) Gaia22 = I/355 (Gaia DR3, 2022) MZW17 = J/MNRAS/471/770 (McDonald+, 2017) S24 = J/A+A/682/A145 (Soubiran+, 2024) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD [5394/223047] Henry Draper catalog (III/135A) identifier 8- 12 A5 --- Comp Components of multi-star system 14- 18 F5.2 mag dVmag [1.9/10.5]? V-band magnitude difference in Comp 20- 25 F6.2 arcsec Sep [0/999.9] Separation, in Comp 27 A1 --- Disc Needs Discussion? (1) -------------------------------------------------------------------------------- Note (1): Some of these systems are large and complex, so we only consider the innermost binary star pair because the other stars are well outside our range of detection of 0.86" and dVmag of 3.0. The exceptions to this are HD 165908 and HD 223047, so they have multiple lines in this table. See Section 5 for more discussion of the stars that require it. Flag as follows: Y = Needs discussion (9 occurrences) N = Does not need discussion (26 occurrences) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD [9826/165341] Henry Draper catalog (III/135A) identifier 8- 12 F5.3 Rsun RadNPOI [0.71/2.09] Derived NPOI stellar radius 14- 18 F5.3 Rsun e_RadNPOI [0.01/0.21] Uncertainty in RadNPOI 20- 24 F5.3 Rsun RadHWO [0.77/2.3] Predicted NASA ExEP radius (1) 26- 27 I2 % Diff [0/27] Percentage difference -------------------------------------------------------------------------------- Note (1): RadHWO is the radius predicted by the "NASA ExEP Mission Star List for HWO" document, which can be found at: https://exoplanetarchive.ipac.caltech.edu/docs/2645_NASA_ExEP_Target_List_HWO_Documentation_2023.pdf -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD [9408/218452] Henry Draper catalog (III/135A) identifier 8- 12 F5.2 Rsun Rad [2.03/23.36] Derived stellar radius 14- 17 F4.2 Rsun e_Rad [0.04/0.82] Uncertainty in Rad 19- 22 I4 K Teff [4217/6676] Final derived stellar effective temperature 24- 26 I3 K e_Teff [8/358] Uncertainty in Teff 28- 32 F5.1 uHz nuMax [8.5/676.0] Frequency of maximum oscillation power (1) 34- 37 F4.1 uHz e_nuMax [1.1/12.2] Uncertainty in nuMax 39- 42 F4.2 Msun Mass [0.91/2.35] Stellar mass (2) 44- 47 F4.2 Msun e_Mass [0.05/0.37] Uncertainty in Mass 49- 50 I2 % sigMass [5/26] Percent uncertainty in Mass 52- 60 A9 --- Ref Reference (column added by CDS) (3) -------------------------------------------------------------------------------- Note (1): From Hon+2021 (J/ApJ/919/131) for all the stars except HD 23249, which is from Corsaro+2024 (J/A+A/683/A161). Note (2): From the following equation: (Mass/M) = (nuMax/nuMax)(Rad/R)2(Teff/Teff)1/2 Note (3): Two stars are from previous work's samples. References as follows: B18 = J/AJ/155/30 (Baines+, 2018) B21 = J/AJ/162/198 (Baines+, 2021) This work = See Table 2 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table11.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Set [1/2] Zero-Crossing star set (1) 3- 8 I6 --- HD [1013/222404] Henry Draper catalog (III/135A) identifier -------------------------------------------------------------------------------- Note (1): Set as follows: 1 = Zero-crossing stars from this work (69 occurrences) 2 = Zero-crossing stars from previous works (51 occurrences) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Robin Leichtnam [CDS] 23-Feb-2026
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