J/ApJ/723/1469      Flux calibrations and WZ Oph photometry      (Wilson+, 2010)

Flux calibrations from nearby eclipsing binaries and single stars. Wilson R.E., Van Hamme W., Terrell D. <Astrophys. J., 723, 1469-1492 (2010)> =2010ApJ...723.1469W 2010ApJ...723.1469W
ADC_Keywords: Binaries, eclipsing ; Photometry, UBVRI ; Photometry, uvby ; Stars, nearby Keywords: binaries: close - binaries: eclipsing - binaries: spectroscopic - stars: distances Abstract: Among several EB distance algorithms, direct comparison of observed and theoretical fluxes is particularly straightforward, although it requires absolute flux calibrations for which only a modest number of publications exist. Here, we measure UBV RI and uvby flux calibrations and calibration ratios from astronomical objects in ways not previously tried, specifically for EBs, single stars within 80pc, and the Sun. All of the single stars are below about 6500K temperature. Interstellar extinction is avoided by a restriction to nearby targets. Some photometric band calibrations in the literature are accurate enough for very good EB distance determinations if star temperatures are accurately known, especially considering that estimated distance has only a square-root dependence on calibration constant, but accurate band-to-band calibration ratios are keys to the combined temperature-distance problem. Band-independent canceling factors (star radii and distances) allow calibration ratio measurement with enhanced accuracy, compared to individual band calibrations. A physical EB model with embedded stellar atmosphere emission optimally matches theory to observations for the binaries. Single star candidates are identified as reliably single if their radial velocity variations are below 100m/s. For the most part, we find good agreement with some of the previous calibrations and the ratios are improved. Description: WZ Oph was observed on 28 nights in 2008 May and June with the 0.4m Schmidt-Cassegrain telescope at Sonoita Research Observatory (SRO) in Sonoita, AZ. Objects: ------------------------------------------------------------- RA (2000) DE Designation(s) (Orbit Period) ------------------------------------------------------------- 17 06 39.04 +07 46 57.8 WZ Oph = SBC9 944 (P=4.18) ------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 141 829 *Cband's and Cband ratios for individual stars table14.dat 40 751 New WZ Oph photometric observations -------------------------------------------------------------------------------- Notes on table2.dat: Rows 1-462 (set 1): Stromgren uvby (1=u, 2=v, 3=b, 4=y); Rows 463-772 (set 2): Johnson UBV (1=U, 2=B, 3=V); Rows 773-829 (set 3): Johnson UBVRI (1=U, 2=B, 3=V, 4=RC, 5=IC). -------------------------------------------------------------------------------- See also: V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) V/121 : Catalog of DMS-type eclipsing binaries (Svechnikov+, 1999) II/215 : uvby-beta Catalogue (Hauck+ 1997) II/183 : UBVRI Photometric Standards (Landolt 1992) II/116 : Photoelectric Photometry in Johnson UBVRI System (Lanz 1986) J/A+A/498/527 : Calibration of Stromgren phot. for late-type stars (Onehag+, 2009) J/AJ/137/4186 : UBVRI standards around celestial equator (Landolt, 2009) J/A+A/487/1081 : uvby photometry of 6 eclipsing binaries (Clausen+, 2008) J/A+A/487/1095 : Radial velocities of AD Boo, VZ Hya, WZ Oph (Clausen+, 2008) J/PASP/120/1128 : Calibrated griz magnitudes of Tycho star (Ofek, 2008) J/MNRAS/389/585 : Fundamental parameters of M dwarfs (Casagrande+, 2008) J/AJ/133/2502 : UBVRI Standard Stars (Landolt, 2007) J/MNRAS/373/13 : Lower MS stars fundamental param. (Casagrande+, 2006) J/A+A/446/785 : Catalogue of eclipsing variables (Malkov+, 2006) J/ApJ/652/313 : BV phot. of a detached EB in M 33 (Bonanos+, 2006) J/AJ/129/1642 : Calibration of synthetic photometry (Fitzpatrick+, 2005) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD Star HD Number 7- 15 F9.5 dW/m3 C1 ?=99.99999 Band 1 Calibration; in erg/s/cm3 16- 24 F9.5 dW/m3 C2 ?=99.99999 Band 2 Calibration; in erg/s/cm3 25- 33 F9.5 dW/m3 C3 ?=99.99999 Band 3 Calibration; in erg/s/cm3 34- 42 F9.5 dW/m3 C4 ?=99.99999 Band 4 Calibration; in erg/s/cm3 43- 51 F9.5 dW/m3 C5 ?=99.99999 Band 5 Calibration; in erg/s/cm3 52- 60 F9.5 --- C1/C2 ?=99.99999 Band Calibration Ratio 61- 69 F9.5 --- C1/C3 ?=99.99999 Band Calibration Ratio 70- 78 F9.5 --- C1/C4 ?=99.99999 Band Calibration Ratio 79- 87 F9.5 --- C1/C5 ?=99.99999 Band Calibration Ratio 88- 96 F9.5 --- C2/C3 ?=99.99999 Band Calibration Ratio 97-105 F9.5 --- C2/C4 ?=99.99999 Band Calibration Ratio 106-114 F9.5 --- C2/C5 ?=99.99999 Band Calibration Ratio 115-123 F9.5 --- C3/C4 ?=99.99999 Band Calibration Ratio 124-132 F9.5 --- C3/C5 ?=99.99999 Band Calibration Ratio 133-141 F9.5 --- C4/C5 ?=99.99999 Band Calibration Ratio -------------------------------------------------------------------------------- Byte-by-byte Description of file: table14.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 F12.4 --- HJD Heliocentric Julian Date of observation 13- 19 F7.3 mag Bmag B band magnitude 20- 26 F7.3 mag Vmag V band magnitude 27- 33 F7.3 mag Rcmag Rc band magnitude 34- 40 F7.3 mag Icmag Ic band magnitude -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 26-Jul-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line