J/ApJS/123/283 Library of FOE spectra of late-type stars (Montes, 1999)
Library of Medium-Resolution Fiber Optic Echelle Spectra of F, G, K,
and M Field Dwarfs to Giant Stars
Montes D., Ramsey L.W., Welty A.D.
<Astrophys. J. Suppl. Ser. 123, 283 (1999)>
=1999ApJS..123..283M 1999ApJS..123..283M
ADC_Keywords: Spectroscopy ; Stars, late-type
Keywords: atlases - stars: activity - stars: chromospheres - stars: late-type
Abstract:
We present a library of Penn State Fiber Optic Echelle (FOE)
observations of a sample of field stars with spectral types F to M and
luminosity classes V to I. The spectral coverage is from 3800 to
10000Å with a nominal resolving power of 12,000. These spectra
include many of the spectral lines most widely used as optical and
near-infrared indicators of chromospheric activity such as the Balmer
lines (Hα to Hδ), Ca II H & K, the Mg I b triplet, Na I
D1, D2, He I D3, and Ca II IRT lines. There are also a large
number of photospheric lines, which can also be affected by
chromospheric activity, and temperature-sensitive photospheric
features such as TiO bands. The spectra have been compiled with the
goal of providing a set of standards observed at medium resolution. We
have extensively used such data for the study of active chromosphere
stars by applying a spectral subtraction technique. However, the data
set presented here can also be utilized in a wide variety of ways
ranging from radial velocity templates to study of variable stars and
stellar population synthesis. This library can also be used for
spectral classification purposes and determination of atmospheric
parameters (Teff, logg, [Fe/H]). A digital version of all the fully
reduced spectra is available via ftp and the World Wide Web (WWW) in
FITS format.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table3.dat 118 130 Stars
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See also: Digital version with all the fully reduced spectra:
http://www.ucm.es/info/Astrof/fgkmsl/FOEfgkmsl.html : Digital version
with all the fully reduced spectra
J/A+AS/123/473 : Late-type star spectra (Montes+ 1997)
J/A+AS/128/485 : Library of UES spectra late-type stars (Montes+ 1998)
Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1 A1 --- Type [FGKM] Type of star
3- 8 I6 --- HD ? HD (Cat. III/135) number
9 A1 --- m_HD Multiplicity index on HD
11- 14 I4 --- HR ? HR (Cat. V/50) number
15 A1 --- m_HR Multiplicity index on HR
17- 21 F5.1 --- GJ ? Gliese (Cat. V/70) number
22- 23 A2 --- m_GJ Multiplicity index on GJ
25- 36 A12 --- Name Other name
38- 54 A17 --- SpType Spectral type and luminosity class (1)
56- 58 A3 --- MK [MK* ] Note about the spectral class (2)
60- 65 F6.3 [Sun] [Fe/H] ? Metallicity
67- 71 F5.2 d Prot ? Rotational period
73- 74 A2 --- l_vsini [≤ ] Limit flag on vsini
75- 78 F4.1 km/s vsini ? Rotational velocity
80- 84 F5.3 --- S ? Ca II H & K spectrophotometric index (3)
86-112 A27 --- Run Observing runs (4)
114-118 A5 --- Ref Star present in other papers:
I: star in Paper I, Cat. J/A+AS/123/473
II: star in Paper II, Cat. J/A+AS/128/485
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Note (1): from the BSC (Cat. V/50), the CNS3 (Cat. V/70A),
and the Perkins Catalog of Revised MK Types for the Cooler Stars (Cat.
III/150). The exception is some of the M dwarfs for which are listed
more recent spectral types determination given by
Henry et al. 1994AJ....108.1437H 1994AJ....108.1437H.
SB = spectroscopic binary (Duquennoy & Mayor 1991A&A...248..485D 1991A&A...248..485D)
Note (2): the symbols are:
MK: the star is a Morgan and Keenan Standard Star from Garcia (1989,
Cat. III/149) and Keenan & McNeil (1989, Cat. III/150)
MK*: star included in the list of Anchor Points for the MK System
compiled by Garrison (1994, ASP Conf. Ser. 60, 3)
Note (3): Index from Baliunas et al. (1995ApJ...438..269B 1995ApJ...438..269B) and
Duncan et al. (1991ApJS...76..383D 1991ApJS...76..383D)
Note (4): observing run or runs in which each star has been observed,
using code given in first column of Table 1 below;
the number in parentheses gives the number of spectra available
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Table 1: Summary of Observations
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Number of
Code Date CCD Detector Echelle Wavelength Dispersion Range
No. (yyy/mm) orders Range (Å/pix)
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1 1994/12 T1KA (1024x1024) 34 3875-9400 0.123-0.296
2 1994/05 T1KA (1024x1024) 33 3875-9000 0.124-0.284
3 1993/12 T1KA (1024x1024) 34 3875-9400 0.121-0.288
4 1992/11 T2KB (2048x2048) 36 3700-9050 0.113-0.276
5 1991/09 TI3 (800x800) 34 3810-8950 0.077-0.180
6 1991/05 TEK2 (512x512) 32 3950-8975 0.152-0.310
7 1990/10 RCA1 (512x512) 40 3690-10700 0.130-0.378
8 1989/12 TI2 (800x800) 15 7250-9000 0.130-0.158
9 1989/04 RCA3 (512x512) 34 3890-9350 0.151-0.359
10 1988/09 RCA3 (512x512) 33 3880-8950 0.150-0.344
11 1987/03 RCA1 (512x512) 33 3880-8950 0.151-0.346
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Table 2: Lines included in FOE Spectral Orders in each Observing Run
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Order
No. 1,2,3,10,11 4,7 5 6 9 8
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1 Ca II K Ca II H
2 Ca II H
3 Ca II H H delta Ca II IRT
4 H delta Ca II K
5 Ca II H H delta
6 H gamma
7 H gamma H delta
8 H gamma
9
10 H gamma Li I
11 H beta H alpha
12 H beta Ca II IRT
13 H beta Ca II IRT
14 Mg I b
15 Mg I b H beta Na I D
16 Mg I b
17
18 Mg I b
19 Na I D
20 Na I D Mg I b
21 Na I D
22
23 Na I D H alpha H beta
24 H alpha Li I
25 Li I H alpha
26 Li I
27 H alpha
28 Li I H gamma
29
30
31 Ca II IRT H delta
32 Ca II IRT
33 Ca II IRT Ca II H
34 Ca II K
35 Ca II IRT
36
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History:
From electronic ApJS edition.
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(End) Gail L. Schneider [NASA/ADC] 06-Jun-2000