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. =2006PAZh...32..672R =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/m^2^/m) at all wavelengths of the spectral range at 2.5 nm intervals. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- 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) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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) -------------------------------------------------------------------------------- Note (1): Observing site as follows: Ch = Chile A = Armenia B = Bolivia -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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 320-370{AA} 25- 28 F4.2 W/m2/m Snk4 ? Standard error of observation averaged over spectral interval of 410-507.5{AA} 31- 34 F4.2 W/m2/m Snk5 ? Standard error of observation averaged over spectral interval of 510-737.5{AA} 37- 40 F4.2 W/m2/m Snk7 ? Standard error of observation averaged over spectral interval of 740-900{AA} 43- 46 F4.2 W/m2/m Snk9 ? Standard error of observation averaged over spectral interval of 902.5-1080{AA} -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5a.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5c.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- ================================================================================ (End) Veta Avedisova [INASAN] 13-Aug-2007