J/PAZh/32/672 Spectrophotometry of 77 variable stars (Ruban+, 2006)
Spectrophotometric observations of variable stars.
Ruban E.V., Alekseeva A.A., Arkharov A.A., Hagen-Thorn E.I., Galkin V.D.,
Nikanorova I.N., Novikov V.V., Pakhomov V.P., Puzakova T.Yu.
<Pis'ma Astron. Zh. 32, 672 (2006)>
=2006PAZh...32..672R 2006PAZh...32..672R
=2006AstL..32...604R 2006AstL..32...604R
ADC_Keywords: Stars, variable ; Spectrophotometry ; Energy distributions
Abstract:
The results of visual and near-infrared spectrophotometric
observations for 77 variable stars obtained during 1971-1991 in Chile,
Armenia and Bolivia. The quasi-monochromatic extra-atmospheric fluxes
from the stars are given in absolute energy units (W/m2/m) at all
wavelengths of the spectral range at 2.5 nm intervals.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 98 77 Coordinates and parameters of stars
table2.dat 32 21 Observing seasons
table3.dat 46 169 Averaged standard errors of single observation
table4.dat 96 19010 Energy distribution for 76 HD stars
table5a.dat 186 245 Individual fluxes for L2 Pup (HD 56096)
table5b.dat 66 245 Individual fluxes for RR Sco (HD 152783)
table5c.dat 146 245 Individual fluxes for V806 Cen (HD 120323)
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Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 6 A6 --- BS/HR ? BS(HR) number
7- 12 I6 --- HD HD number
13- 14 A2 --- m_HD [/5] Multiplicity index on HD
16- 26 A11 --- GCVS4 GCVS4/NSV number
29- 30 I2 h RAh Right Ascension (J2000) (hours)
32- 33 I2 min RAm Right Ascension (J2000) (minutes)
35- 36 I2 s RAs Right Ascension (J2000) (seconds)
39 A1 --- DE- Declination sign (J2000)
40- 41 I2 deg DEd Declination (J2000) (degrees)
43- 44 I2 arcmin DEm Declination (J2000) (minutes)
46- 47 I2 arcsec DEs Declination (J2000) (seconds)
50- 53 F4.2 mag Vmag V magnitude
56- 67 A12 --- SpType MK spectral type
69- 96 A28 --- Var Variability description
98 A1 --- Rem [*] Remarks (see paper)
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 2 I2 --- k Observing season number
4- 7 I4 yr Year1 First year of observation
8 A1 --- n_Year1 [be] b,e : letters mark the first and halves
of the year, respectively
10- 13 I4 yr Year2 ? Second year of observation
16- 20 F5.1 nm SpRange1 Spectral range (nm)
22- 27 F6.1 nm SpRange2 Spectral range (nm)
31- 32 A2 --- Site Observing site (1)
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Note (1): Observing site as follows:
Ch = Chile
A = Armenia
B = Bolivia
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 6 I6 --- HD HD number
7- 8 A2 --- m_HD [/5] Multiplicity index on HD
11- 12 I2 --- k Observing season
15- 16 I2 --- n Observation number
19- 22 F4.2 W/m2/m Snk3 ? Standard error of observation averaged
over spectral interval of 320-370Å
25- 28 F4.2 W/m2/m Snk4 ? Standard error of observation averaged
over spectral interval of 410-507.5Å
31- 34 F4.2 W/m2/m Snk5 ? Standard error of observation averaged
over spectral interval of 510-737.5Å
37- 40 F4.2 W/m2/m Snk7 ? Standard error of observation averaged
over spectral interval of 740-900Å
43- 46 F4.2 W/m2/m Snk9 ? Standard error of observation averaged
over spectral interval of 902.5-1080Å
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Byte-by-byte Description of file: table4.dat
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Bytes Format Units Label Explanations
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1- 2 A2 --- --- [HD]
4- 9 I6 --- HD HD number
10- 11 A2 --- m_HD [/5] Multiplicity index on HD
13- 18 F6.1 0.1nm lambda Spectral line wavelength
20- 21 I2 --- k1 ? Season
23- 31 F9.7 W/m2/m E1 ? Energy distribution for observing season
33- 34 I2 --- k2 ? Season
36- 44 F9.7 W/m2/m E2 ? Energy distribution for observing season
46- 47 I2 --- k3 ? Season
49- 57 F9.7 W/m2/m E3 ? Energy distribution for observing season
59- 60 I2 --- k4 ? Season
62- 70 F9.7 W/m2/m E4 ? Energy distribution for observing season
72- 73 I2 --- k5 ? Season
75- 83 F9.7 W/m2/m E5 ? Energy distribution for observing season
85- 86 I2 --- k6 ? Season
88- 96 F9.7 W/m2/m E6 ? Energy distribution for observing season
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Byte-by-byte Description of file: table5a.dat
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Bytes Format Units Label Explanations
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1- 6 F6.1 0.1nm lambda Spectral line wavelength
8- 16 F9.7 W/m2/m S49 Energy distribution for JD=2447449.85356
18- 26 F9.7 W/m2/m S63 Energy distribution for JD=2447463.84150
28- 36 F9.7 W/m2/m S64 Energy distribution for JD=2447464.81873
38- 46 F9.7 W/m2/m S69 Energy distribution for JD=2447469.83973
48- 56 F9.7 W/m2/m S72 Energy distribution for JD=2447472.85574
58- 66 F9.7 W/m2/m S08 Energy distribution for JD=2447508.82438
68- 76 F9.7 W/m2/m S43 Energy distribution for JD=2447543.81537
78- 86 F9.7 W/m2/m S44 Energy distribution for JD=2447544.72635
88- 96 F9.7 W/m2/m S54 Energy distribution for JD=2447554.75412
98-106 F9.7 W/m2/m S60 Energy distribution for JD=2447560.71395
108-116 F9.7 W/m2/m S75 Energy distribution for JD=2447575.75270
118-126 F9.7 W/m2/m S80 Energy distribution for JD=2447580.61140
128-136 F9.7 W/m2/m S99 Energy distribution for JD=2447599.67247
138-146 F9.7 W/m2/m S01 Energy distribution for JD=2447601.54395
148-156 F9.7 W/m2/m S18 Energy distribution for JD=2447618.62593
158-166 F9.7 W/m2/m S66 Energy distribution for JD=2447666.48426
168-176 F9.7 W/m2/m S68 Energy distribution for JD=2447668.48708
178-186 F9.7 W/m2/m S669 Energy distribution for JD=2447669.50343
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Byte-by-byte Description of file: table5b.dat
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Bytes Format Units Label Explanations
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1- 6 F6.1 0.1nm lambda Spectral line wavelength
8- 16 F9.7 W/m2/m S49 Energy distribution for JD=2447661.73164
and the phase=0.97204
18- 26 F9.7 W/m2/m S63 Energy distribution for JD=2447667.72364
and the phase=0.99333
28- 36 F9.7 W/m2/m S64 Energy distribution for JD=2447668.87559
and the phase=0.99743
38- 46 F9.7 W/m2/m S69 Energy distribution for JD=2447669.72630
and the phase=0.00045
48- 56 F9.7 W/m2/m S72 Energy distribution for JD=2447677.76434
and the phase=0.02901
58- 66 F9.7 W/m2/m S08 Energy distribution for JD=2447681.75111
and the phase= 0.04317
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Byte-by-byte Description of file: table5c.dat
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Bytes Format Units Label Explanations
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1- 6 F6.1 0.1nm lambda Spectral line wavelength
8- 16 F9.7 W/m2/m S49 Energy distribution for JD=2447658.67871
18- 26 F9.7 W/m2/m S63 Energy distribution for JD=2447659.74575
28- 36 F9.7 W/m2/m S64 Energy distribution for JD=2447666.71669
38- 46 F9.7 W/m2/m S69 Energy distribution for JD=2447668.69990
48- 56 F9.7 W/m2/m S72 Energy distribution for JD=2447669.64234
58- 66 F9.7 W/m2/m S08 Energy distribution for JD=2447677.64455
68- 76 F9.7 W/m2/m S43 Energy distribution for JD=2447681.63162
78- 86 F9.7 W/m2/m S44 Energy distribution for JD=2447685.66264
88- 96 F9.7 W/m2/m S54 Energy distribution for JD=2447707.60924
98-106 F9.7 W/m2/m S60 Energy distribution for JD=2447708.62204
108-116 F9.7 W/m2/m S75 Energy distribution for JD=2447713.52611
118-126 F9.7 W/m2/m S80 Energy distribution for JD=2447715.57124
128-136 F9.7 W/m2/m S99 Energy distribution for JD=2447720.55919
138-146 F9.7 W/m2/m S01 Energy distribution for JD=2447721.55048
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(End) Veta Avedisova [INASAN] 13-Aug-2007