HIP 560 = HD 203: Rotational broadening of 150km/s used in simplex solution. HIP 2235 = HD 2454: An F5 dwarf with an overabundance of Strontium. HIP 2235 Ba II 4554 also appears enhanced. HIP 3505 = HD 4247: Simplex fit utilized IUE spectrum SWP17039. HIP 3961 = HD 5028: We were somewhat surprised to find that this metal-weak HIP 3961 F6 star turns out to be in the very chromospherically active HIP 3961 category. However, visual inspection of the spectrum verifies HIP 3961 that the Ca II K & H lines are both shallow. It turns out that HIP 3961 this star is both an X-ray source (Haberl et al., 2000, HIP 3961 Cat. ). Observed 12 Dec, 2002. HIP 4855 = HD 6156: This star is a close visual double with HD 6156B, which is HIP 4855 recorded in Table 1 with a composite spectral type K0V+K5V. This HIP 4855 composite type is probably due to contamination from the much HIP 4855 brighter primary (G9 V), and thus the approximate spectral type HIP 4855 for B is about K5 V. HIP 9711 Supergiant, with a large parallax error: 27.60+/-21.70mas. Also has HIP 9711 quite large proper motions. No clear reason for parallax error. HIP 9711 Evidently not within 40pc. Spectrum is peculiar; the hydrogen lines HIP 9711 suggest a spectral type of A3 Iab, but no metallic lines, except for HIP 9711 the K-line are visible. This is a high-amplitude Hipparcos variable. HIP 10191 = HD 13513: Triple system. The spectral type for HD 13513 is for AB, HIP 10191 HD 13513C is actually CD -36 816C. HD 13513C See HIP 10191 . HIP 11324 = HD 15146: Poor convergence in simplex fit. HIP 11964 = HD 16157: This chromospherically very active star was observed HIP 11964 on 13 Dec, 2002. HD 18622 This is not a Hipparcos star, probably because it is too bright. HD 18622 However, its parallax (from the General Catalog of Trigonometric HD 18622 Parallaxes) is 28+/-11mas. HIP 16247 = HD 21703: This chromospherically very active star was observed HIP 16247 on November 27, 2001. HIP 16846 = HD 22468: This well-known RS CVn variable shows strong emission in HIP 16846 Ca II K & H with infilling in H{beta}. The spectral lines appear HIP 16846 broad. This chromospherically very active star was observed on HIP 16846 December 15, 2002. HIP 18450 = HD 25004: Ba II (4554A) appears slightly enhanced in this K-dwarf. HIP 19248 = HD 26354: This chromospherically very active star was observed HIP 19248 on February 10, 2001. HIP 20338 This chromospherically very active star was observed on 27/11/2001. HIP 20968 F9 dwarf with large parallax error: 120.70+/-56.47mas. Double with HIP 20968 HD 28639, a K2 III (Simbad) with {pi}=2.18. HIP 20968 likely not HIP 20968 within 40pc. HIP 21756 = HD 30003: Spectrum composite A+B. HIP 23309 This chromospherically very active star was observed on 08/02/2001. HIP 25486 = HD 35850: This chromospherically very active star was observed HIP 25486 on March 13, 2001. HIP 25647 = HD 36705: This chromospherically very active star was observed HIP 25647 on December 11, 2002. HIP 26369 This chromospherically very active star was observed on 05/02/2001. HIP 26462 G5 dwarf with large parallax error: 30.99+/-24.17mas. Double with HIP 26462 HD 37761, a G5 III (Simbad) with {pi}=9.58mas. Evidently not HIP 26462 within 40pc. HIP 26380 = HD 38283: This chromospherically very active star was observed HIP 26380 on December 12, 2002. HD 38392 = {gamma} Lep B: This star is not in the Hipparcos catalog, but on HD 38392 the basis of its spectral type, apparent magnitude, and association HD 38392 with {gamma} Lep, it must be closer than 40pc. {gamma} Lep A HD 38392 immediately follows this star in the table (HIP 27072). HIP 27288 = HD 38678: Simplex fit utilized IUE spectrum SWP50070 and HIP 27288 vsini=200km/s. HIP 28103 = HD 40136: Simplex fit utilized IUE spectrum SWP10286. HIP 28796 = HD 41824: This chromospherically very active star was observed HIP 28796 on December 12, 2002. HIP 29804 = HD 43848: This K2 subgiant shows a strong Swan band at 4737 A. HIP 29964 = HD 45081: This chromospherically very active star was observed HIP 29964 on February 9, 2001. HIP 30314 = HD 45270: G-band in stellar spectrum is weak compared to HIP 30314 simplex-fit model. See spectral type for confirmation of weak HIP 30314 G-band. HIP 30362 = HD 256294: This star, classified as B9 III, forms a faint triple HIP 30362 with HIP 30365 (K1 III-IV) and a third star, BD+08 1303B. The two HIP 30362 Hipparcos stars have large parallax errors. Judging from their HIP 30362 spectral types and magnitudes, these stars lie well beyond 40pc. HIP 30476 = HD 45289: A solar twin. HIP 31711 = HD 48189: G-band in stellar spectrum is weak compared to HIP 31711 simplex-fit model. See spectral type for confirmation of weak G-band HIP 37606 = HD 62644: Weak Ca I 4227. HIP 40706 = HD 70060: Simplex fit utilized IUE spectrum SWP56381. HIP 40769 = IDS 08186-6729A: This star has a faint companion about 33" due HIP 40769 south which is not included in the HIP 40769 designation, but which HIP 40769 is designated IDS 08186-6729B, and also LDS 215B. For this HIP 40769 companion, we have left the HIP column blank, but have placed the HIP 40769 designator ``B'' in the "HD/DM" column. LDS 215B = See HIP 40769. HIP 42291 = HD 73524: Ca I strong, but G-band slightly weak for the spectral HIP 42291 type. HIP 43290 = HD 75519: Photometry residuals high in simplex fit. HIP 44713 = HD 78429: Photometry residuals high in simplex fit. HIP 45238 = HD 80007: Simplex fit utilized IUE spectra LWP8843 and SWP43459. HIP 45940 = HD 81639AB: The similarity of the spectral type of the companion HIP 45940 of HD 81639 (G8 V) to the primary (G7 V) coupled with the magnitude HIP 45940 difference (~4 in V) according to Simbad suggests substantial HIP 45940 contamination from the primary in the spectrum of the secondary. HIP 50798 = HD 90034B: K0 giant star with a large parallax error: HIP 50798 98.17+/-79.48mas. The A component (HIP 50804 = HD 90034A) is an HIP 50798 A3 IV-V star (this paper). Its parallax is {pi}=3.29mas. It is not HIP 50798 clear if this is a physical double. HIP 50804 See HIP 50798. HIP 52341 A visual double star; the eastern component is the brightest and is HIP 52341 designated "A" by Simbad. However, Simbad seems to have mixed the HIP 52341 spectral types of the two stars: "A", the eastern companion is HIP 52341 M2.5 in Simbad, B is K7. HIP 54298 F5 dwarf with large parallax error: 155.28+/-78.30mas. Double with HIP 54298 HD 96507, B9 III (Simbad) with {pi}=-0.20mas. Evidently not HIP 54298 within 40pc. HIP 54806 = HD 97578: Carbon star with large parallax error: 31.18+/-14.06mas. HIP 54806 No clear reason for parallax error. HIP 55031 F6 peculiar star with large parallax error: 43.57+/-35.81mas. HIP 55031 Variable star. Has a number of faint companions which probably HIP 55031 account for parallax error. HIP 55705 = HD 99211: Simplex solution utilized IUE spectrum SWP44997. HIP 56280 = HD 100286: Ca I 4226 peculiarly weak. This star is a near-equal HIP 56280 visual double with HD 100287 which does not appear in the Hipparcos HIP 56280 catalog, but which is included in the HIP 56280 designation. HIP 57363 = HD 102249: Simplex fit utilized IUE spectra LWP13333 and SWP33671. HIP 58240 = HD 103742: Is a wide visual double with HIP 58241 = HD 103743. HIP 58240 G-band weak in stellar spectrum compared with simplex-fit model. HIP 58241 See HIP 58240. HIP 59199 = HD 105452: Simplex fit utilized IUE spectrum SWP44996. HIP 59750 = HD 106516: Both the SO and the CTIO spectra agree that this HIP 59750 metal-weak F9 dwarf is a chromospherically active star. The CTIO HIP 59750 spectrum, obtained on December 14, 2002 gives log(R)=-4.158 HIP 59750 (very active) and the SO spectrum, obtained on April 9, 2001 gives HIP 59750 log(R)=-4.410 (active). This star is an X-ray source, and may have HIP 59750 been the source of the January 13, 1993 gamma-ray burst (see HIP 59750 Shibata et al. 1997). HIP 60553 This chromopherically very active star was observed on 08/02/2001. HIP 60853 = HD 108564: This is a very metal-weak K5 star. The radial velocity HIP 60853 of this star (110 km/s) implies it is a member of the halo. HIP 60965 = HD 108767: Simplex fit utilized IUE spectrum SWP18885 and HIP 60965 vsin(i)=200km/s. HIP 61174 = HD 109085: Simplex fit utilized IUE spectrum SWP55354. HIP 62333 = HD 110971: This chromopherically very active star was observed HIP 62333 on February 10, 2001. HIP 62403 = HD 111038: Violet end of spectrum appears veiled, perhaps due to HIP 62403 chromospheric activity. This may have affected simplex solution. HIP 62403 This very chromopherically active star was observed on 10/02/2001. HIP 63033 = HD 112164: Spectrum appears peculiar, and possibly composite. HIP 63033 Metals are about as strong as a G2 V, but enhancement in the HIP 63033 metallic line strengths depends on the wavelength. The Simplex fit HIP 63033 suggests this star is metal-rich ([M/H]=0.22), which gives an HIP 63033 excellent fit to the stellar energy distribution from the UV to HIP 63033 12{mu}m. There is no indication of chromospheric activity - indeed HIP 63033 we classify this star as being in the "Very Inactive" class. HIP 64478 = HD 114630: The entire spectrum appears "veiled". The HIP 64478 low-excitation/resonance lines (such as Ca I, Fe I 4046A, etc.) are HIP 64478 particularly weak, the cores of Ca II K & H are shallow, and H{beta} HIP 64478 appears slightly filled in. The simplex solution is suspect because HIP 64478 of this "veiling". This star is a well-known chromospherically HIP 64478 active binary. HIP 66182 F5 dwarf with large parallax error: 59.10+/-114.46mas. Double with HIP 66182 HD 117809, G8 III (Simbad) with {pi}=1.93mas. HIP 69562 = HD 124498: This chromopherically very active star was observed on HIP 69562 June 5, 2001. HIP 69578 B2 giant with large parallax error: 64.68+/-46.97mas. Double with HIP 69578 HD 124237, B5 V (Simbad) with {pi}=2.21mas. HIP 69578 is clearly a HIP 69578 double-lined spectroscopic binary from our spectrum. HIP 71686 This star is listed as the CD component of the visual multiple star, HIP 71686 ADS 9330. The A component, also in Table 1, is HD 128787. The B HIP 71686 component is a faint close companion to A, whereas CD is located HIP 71686 about 2' to the NE of A. HIP 71908 = HD 128898: broad Ca I K-line. HIP 72399 = HD 130260: visual double with HIP 72400. This chromopherically HIP 72399 very active star was observed on August 8, 2001. HIP 72400 See HIP 72399. HIP 72685 F9 dwarf with large parallax error: 25.68+/-8.87mas. Double with HIP 72685 HD 130922, F5 (Simbad) with {pi}=8.26mas. HIP 74815 This chromopherically very active star was observed on June 5, 2001. HIP 74824 = HD 135379: Simplex fit utilized IUE spectra LWP25218 and SWP47375. HIP 75255 = HD 136466: large photometry residuals in the simplex fit. HIP 76351 = See HIP 76362 HIP 76362 K1 giant with large parallax error: 99.90+/-61.26mas. Double HIP 76362 (probably optical) with HD 137388, K2 IV (this paper) with HIP 76362 {pi}=26.01+/-1.88. HIP 76362 is about 1.8mag fainter than HD 137388, HIP 76362 despite more luminous spectral type. Hence, likely optical double. HIP 76550 Peculiar morphology in the MgH band (violet side weak), seen in both HIP 76550 CTIO and SO spectra. HIP 76629 = HD 139084: This chromopherically very active star was observed HIP 76629 on August 10, 2001. HIP 79958 = HD 146464: This chromopherically very active star was observed HIP 79958 on August 3, 2001. HIP 80062 = HD 147104: This star forms a visual double with HIP 80063, which HIP 80062 has a Hipparcos parallax of -1.46+/-3.43mas. HIP 80062 itself has a HIP 80062 Hipparcos parallax of 26.78+/-7.79mas. Both stars are clearly more HIP 80062 distant than 40pc. HIP 80381 = HD 147555A: Double with HIP 80383, which is a fainter star to the HIP 80381 south and east of HIP 80381. Note, however, the earlier spectral HIP 80381 type of HIP 80383, which is unexpected if the pair is a physical HIP 80381 double. However, the identification is positive. Simbad records a HIP 80381 spectral type of K5 for HIP 80381, similar to our spectral type HIP 80381 of K6 V, but does not record a spectral type for HIP 80383. HIP 80383 See HIP 80381. HIP 81407 = HD 149606: Large photometric residuals in the simplex solution. HIP 81478 = HD 149499: This chromopherically very active star was observed HIP 81478 on August 10, 2001. HIP 82588 = HD 152391: Large photometric residuals in the simplex solution. HIP 82725 Faint K0 subgiant with large parallax error: 203.01+/-29.27mas. HIP 82725 Double with CCDM J16545-6224A, HIP 82724. No spectrum available for HIP 82725 HIP 82724, which has a comparably large parallax and error. HIP 83513 = VdBH 81d: F3 subgiant with large parallax error: 29.70+/-15.98mas. HIP 83513 Is in a compact cluster within VdBH 81i reflection nebula. Close HIP 83513 proximity of cluster members undoubtedly accounts for large HIP 83513 parallax error. Almost certainly outside 40pc. HIP 83541 = HD 154088: Large photometric residuals in the simplex solution. HIP 83990 = HD 154577: Peculiar energy distribution. Region around H{beta} HIP 83990 appears weak-lined. HIP 84084 F5 dwarf with large parallax error: 54.25+/-56.24mas. Double with HIP 84084 HD 155133, K2 (Simbad) with {pi}=1.68mas. HIP 84586 = HD 155555 = V824 Ara: RS CVn type variable. This chromopherically HIP 84586 very active star was observed on June 25, 2002. HIP 85019 = HD 157060: Noisy spectrum; luminosity class uncertain. HIP 86057 Close visual double not referenced as such in Simbad. Components HIP 86057 labeled in the table according to relative brightnesses. "A", the HIP 86057 M1.5 V star is the brighter of the two, and is situated about 4" to HIP 86057 the south and east of the fainter B component. The two components HIP 86057 are not resolved on the second Digital Sky Survey. The faint star HIP 86057 that does appear on the DSS2 about 12 arc seconds to the north and HIP 86057 east of HIP 86057 is not the component we observed. HIP 86486 = HD 160032: Our CTIO spectrum is too noisy for spectral HIP 86486 classification. We have used the spectral type from HIP 86486 Gray (1989AJ.....98.1049G). HIP 86489 K2 giant star with large parallax error: 28.57+/-29.19mas. Double HIP 86489 with HD 160150, F3/5 II (Simbad) with {pi}=1.42mas. HIP 87000 A star with a large parallax error: 27.84+/-40.94. Simbad lists a HIP 87000 spectral type of G5 for this star, which is in conflict with our HIP 87000 type of A1 III-IV. The star HD 161487 is located 22 arc seconds to HIP 87000 the south and west of HIP 87000, but has a spectral type of F3 V, HIP 87784 K2 giant with large parallax error: 31.55+/-18.42mas. Double with HIP 87784 HD 162157, G8 III (simbad) with {pi}=5.85mas. HIP 88908 = HD 165814B: The nomenclature in Simbad for this star appears to be HIP 88908 confused. This star is labeled HD 165530B in Simbad, but HD 165530 HIP 88908 is located about 22' to the east. HIP 88908 is about 15" to the NE HIP 88908 of HD 165814. The telescope coordinates in the FITS header for our HIP 88908 spectrum of HIP 88908 agree with this star being proximate to HIP 88908 HD 165814, and also agree with the coordinates given in Simbad for HIP 88908 HD 165530B. HD 165814 has a parallax of 1.03+/-2.13mas. HIP 88908 HIP 88908 has a parallax of 36.65+/-9.63mas. However, based on its magnitude HIP 88908 and spectral type, this star (like HD 165814, its companion) is HIP 88908 more distant than 40pc. HIP 90706 A close visual double. The "B" component, which is the fainter, is HIP 90706 located a few arc seconds to the north and east of A. HIP 90724 = HD 170368: This is a visual double with a star about 8 arc seconds HIP 90724 to the NNW. This star, labeled HD 170368B in the table also has the HIP 90724 designation CD-36 12714B. This star is a G5 III (this paper). HD 170368B See HIP 90724 HIP 92024 = HD 172555: Simplex fit utilized the IUE spectrum SWP45799. HIP 92742 = HD 174545: Large photometric residuals in the simplex fit. HIP 93174 = HD 175813 = {epsilon} CrA: This is a W UMa type eclipsing binary. HIP 93449 = R CrA: A variable B-type emission-line pre-main-sequence star in a HIP 93449 nebula. Hipparcos parallax has large error: 121.75+/-68.24mas. HIP 96635 = HD 185181: This is a chromospherically active subgiant K2 star and HIP 96635 thus a possible PMS star. Note that Koen & Eyer (2002, HIP 96635 Cat. ) have found that this star is a variable from HIP 96635 Hipparcos photometry, but were unable to determine the type of HIP 96635 variability. This star was observed from CTIO on June 24, 2002, HIP 96635 (log(R)=-4.170) and from SO on June 19, 2002, giving log(R)=-4.201. HIP 96643 = HD 185342B: An F2 dwarf with a large parallax error: 29.48+/-26.57. HIP 96643 This star is a wide visual double with HD 185342A, an A1 V dwarf HIP 96643 (this paper). The "A" component has a parallax of 9.02+/-2.40mas. HIP 96643 Both stars thus probably beyond 40pc. HIP 96646 See HIP 96643. HIP 98470 = HD 189245: This chromospherically very active late F-type star was HIP 98470 observed on June 6, 2001. This star is an extreme ultraviolet HIP 98470 source, a variable star and a rapid rotator (86km/s). HIP 102119 = HD 196998: This chromospherically very active star was observed HIP 102119 on June 6, 2001. HIP 102125 = HD 196067: Primary component in a visual binary with HIP 102128 = HIP 102125 HD 196068. HD 196068 is formally within our sample, as its parallax HIP 102125 is 25.35+/-7.35mas, but HD 196067 is outside, with a parallax of HIP 102125 22.95+/-2.10mas. The photometry residuals in the simplex fit for HIP 102125 HD 196068 are high, perhaps due to contamination from primary? HIP 102128 See HIP 102125. HIP 102333 = HD 197157: Our CTIO spectrum of this star is too noisy for HIP 102333 accurate spectral classification. The listed spectral type (A9 IV) HIP 102333 is from Gray & Garrison (1989ApJS...70..623G). HIP 102333 The simplex solution likewise, is uncertain. HIP 105441 = HD 202746: The violet end of this spectrum appears veiled, and the HIP 105441 photometric residuals for the simplex fit are high. HIP 107427 An F5 dwarf with a large parallax error: 47.82+/-32.04mas. This star HIP 107427 is an astrometric binary, which explains the erroneously large HIP 107427 parallax (Makarov & Kaplan, 2005, Cat. ). HIP 108416 = HD 208573: Photometric residuals for the simplex fit are high. HIP 109427 = HD 210418: Simplex fit utilized IUE spectra LWP15565 and SWP36316. HIP 109670 A metal weak G5 dwarf with a large parallax error: 44.20+/-16.43mas. HIP 109670 This star appears single on the Digitized Sky Survey (The Digitized HIP 109670 Sky Survey was produced at the Space Telescope Science Institute HIP 109670 under U.S. Government grant NAG W-2166) and is not a known HIP 109670 astrometric binary, so the large, and probably erroneous parallax HIP 109670 is not explained. HIP 110468 = HD 212038: Photometric residuals for the simplex fit are high. HIP 110719 = HD 212168B: A close visual double with HD 212168. Sinachopoulos HIP 110719 (1989A&AS...81..103S) concludes this double is optical. The "B" HIP 110719 component has Stromgren uvby colors which are much too red for a G0 HIP 110719 dwarf. Since "A" is also a G0 dwarf and is about 2.7mag brighter, HIP 110719 this is undoubtedly an optical pair. HIP 110922 A close visual double. "A" is the most northerly of the two almost HIP 110922 identical stars. HIP 111870 = HD 214615AB: We have spectra for both components of this nearly HIP 111870 equal close visual binary. The spectra are almost indistinguishable. HIP 111870 The Simplex solution was carried out using the spectrum for HIP 111870 HD 214615A and the composite uvby and Cousins RI photometry, with V HIP 111870 increased by 0.7mag. HIP 113368 = HD 216956: Simplex solution utilized IUE spectra LWP10680 and HIP 113368 SWP30894. HIP 114110 Is a double with HD 218251, which is not in our sample HIP 114110 ({pi}=13.26mas). HIP 114110 has a parallax with a large error HIP 114110 216.52+/-18.28mas. This G1 V star has V=10.2, and thus is HIP 114110 undoubtedly beyond 40pc. Hence the parallax is entirely erroneous. HIP 114986 = HD 219509: Photometic residuals for the simplex fit are high. HIP 115126 = HD 219834A: Double with HIP 115125 = HD 219834B. The spectral type HIP 115126 reported in the table is for the A component only. We have a very HIP 115126 noisy spectrum for the B component. The spectral type is HIP 115126 approximately K2 V, with significant uncertainties. HIP 117410 This chromospherically very active star was observed on 09/11/2001.