2016MNRAS.456..417J

Query : 2016MNRAS.456..417J

2016MNRAS.456..417J - Mon. Not. R. Astron. Soc., 456, 417-430 (2016/February-2)

Bright stars observed by FIMS/SPEAR.

JO Y.-S., SEON K.-I., MIN K.-W., CHOI Y.-J., LIM T.-H., LIM Y.-M., EDELSTEIN J. and HAN W.

Abstract (from CDS):

In this paper, we present a catalogue of the spectra of bright stars observed during the sky survey using the Far-Ultraviolet Imaging Spectrograph (FIMS), which was designed primarily to observe diffuse emissions. By carefully eliminating the contamination from the diffuse background, we obtain the spectra of 70 bright stars observed for the first time with a spectral resolution of 2-3Å over the wavelength of 1370-1710Å. The far-ultraviolet spectra of an additional 139 stars are also extracted with a better spectral resolution and/or higher reliability than those of the previous observations. The stellar spectral type of the stars presented in the catalogue spans from O9 to A3. The method of spectral extraction of the bright stars is validated by comparing the spectra of 323 stars with those of the International Ultraviolet Explorer (IUE) observations.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): instrumentation: spectrographs - methods: data analysis - techniques: spectroscopic - catalogues - stars: general - ultraviolet: stars

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 46

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Number of rows : 46
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 * v Eri * 03 30 37.0583178770 -05 04 30.532729396   4.631 4.725     B9III 89 0
2 * 35 Eri * 04 01 32.0471006496 -01 32 58.771121676 4.58 5.13 5.28     B5III/IV 115 0
3 HD 31726 * 04 57 44.6845893336 -14 13 54.901969680   5.939 6.139     B2V 136 0
4 * psi Eri ** 05 01 26.3457823592 -07 10 26.273231188 3.87 4.61 4.78     B3IV 114 0
5 BD+52 913 WD* 05 05 30.6180977592 +52 49 51.919301604 10.25 11.44 11.69 11.93 12.108 DA.8 1153 0
6 * eps Dor V* 05 49 53.5294723780 -66 54 04.313513558 4.48 4.97 5.11     B6V 75 0
7 HD 46487 Pu* 06 33 37.9213970040 -01 13 12.553237092   4.934 5.079     B5IV/V 86 0
8 HD 49643 ** 06 49 16.4057835624 -02 16 19.370394984 5.18 5.644 5.750     B8V 70 0
9 * P Pup ** 07 49 14.2975995620 -46 22 23.518739728 2.92 3.93 4.11 4.19 4.36 B0III 162 0
10 HD 64740 * 07 53 03.6344819483 -49 36 46.956285817 3.48 4.40 4.63 4.76 4.97 B2V 223 0
11 HD 64802 Pu* 07 54 11.0098192344 -35 52 38.228288340 4.57 5.288 5.463     B2V 95 0
12 * N Pup * 07 57 18.4210020610 -44 06 35.495378009   4.899 5.064     B2III/IV 54 0
13 HD 65176 Em* 07 57 25.1634345168 -01 36 46.298963916 7.41 8.01 8.05     B1Ib/II 41 0
14 * 16 Pup * 08 09 01.6363885089 -19 14 42.122308587 3.65 4.239 4.393     B5V 103 0
15 HD 68217 Pu* 08 09 35.9137276680 -44 07 21.962716896   5.010 5.183     B2IV 77 0
16 HD 68895 ** 08 12 30.7927258144 -46 15 51.445044238       7.26   B5V 56 0
17 HD 69302 ** 08 14 23.8746718618 -45 50 04.250534667 4.84 5.661 5.836     B2IV 82 0
18 HD 70839 bC? 08 21 12.0991599408 -57 58 23.592023796 5.06 5.849 5.954     B2III 64 0
19 HD 70556 Y*O 08 21 21.0444005256 -36 29 03.036690528 4.17 4.989 5.176     B2IV/V 65 0
20 * f Vel SB* 08 50 33.4606230120 -46 31 45.075306720 3.92 4.90 5.11 5.20 5.36 B1Ib 165 0
21 HD 76004 * 08 51 50.0352140688 -44 09 03.353593392   6.216 6.350     B3V 40 0
22 * c Car PM* 08 55 02.8480985300 -60 38 40.594250640 3.28 3.74 3.80     B8II-III 83 0
23 HD 76566 * 08 55 19.2021546912 -45 02 30.024113964 5.47 6.10 6.26     B3IV 78 0
24 * H Vel SB* 08 56 19.2630167160 -52 43 24.506826528   4.591 4.723     B5/6IV 76 0
25 * i Car * 09 11 16.7220151749 -62 19 01.119842846 3.13 3.774 3.943     B3V 118 0
26 * L Vel * 09 34 08.7934716637 -51 15 18.958114695 4.04 5.01 5.03     B2IV 67 0
27 * m Car V* 09 39 21.0112812689 -61 19 40.979181659   4.432 4.498     B9IV/V 87 0
28 HD 84567 Be* 09 45 22.0073045904 -30 12 09.896445036 5.38 6.32 6.45     B0IV 73 0
29 * pi. Cen ** 11 21 00.4170807171 -54 29 27.964002014           B5Vn 127 0
30 * tet Crt PM* 11 36 40.9092052035 -09 48 08.001725582   4.604 4.673     B9.5V 226 0
31 * rho Cen Pu* 12 11 39.1197479712 -52 22 06.384420264 3.20 3.81 3.96 4.05 4.21 B3V 136 0
32 * G Cen Pu* 12 26 31.7600444794 -51 27 02.288916487 4.02 4.654 4.808     B3V(n) 93 0
33 * del Sco SB* 16 00 20.00528 -22 37 18.1431 1.30 2.20 2.32 2.36 2.49 B0.3IV 776 0
34 * iot Oph PM* 16 54 00.4715319173 +10 09 55.300984028 3.98 4.30 4.38     B8V 118 0
35 * del Ara PM* 17 31 05.9135939049 -60 41 01.841838888 3.21 3.52 3.62     B8Vn 98 0
36 * tet Ara s*b 18 06 37.8681946272 -50 05 29.327579099 2.73 3.58 3.66     B0.5Iab 201 0
37 * 102 Her * 18 08 45.4919267342 +20 48 52.404584093 3.38 4.177 4.347     B2IV 194 0
38 HD 172910 Y*O 18 44 19.3604882816 -35 38 31.158238101 3.97 4.69 4.87 5.02 5.18 B2V 102 0
39 * 23 Cyg ** 19 53 17.3781586824 +57 31 24.506900436   5.001 5.132     B5V 98 0
40 HD 199661 Pu* 20 56 17.0115667320 +56 53 15.063536868 5.37 6.049 6.218     B2.5IV 75 0
41 HD 199739 ** 20 56 40.7977182408 +56 55 35.989544496 8.18 8.35 7.96     B8 23 0
42 * pi.02 Cyg SB* 21 46 47.6097792927 +49 18 34.454260528 3.4 4.11 4.18     B2.5III 180 0
43 * gam Gru PM* 21 53 55.7163006264 -37 21 53.539981264 2.52 2.89 3.01 3.06 3.12 B8IV-Vs 144 0
44 * 8 Lac B * 22 35 52.0990532376 +39 37 41.339738568 4.61 5.52 5.67 5.88 6.06 B1.Vs 120 0
45 * 8 Lac A Be* 22 35 52.2827504304 +39 38 03.586773768 4.68 5.52 5.69     B1Vne 179 0
46 * 10 Lac ** 22 39 15.6786372 +39 03 00.971152 3.650 4.670 4.880 4.98 5.19 O9V 790 0

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