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J/A+A/265/77     VBLUW Observations of TT Ari   (Hollander+ 1992)

Quasi-periodic oscillations in TT Ari Hollander A., van Paradijs J. <Astron. Astrophys. 265, 77 (1992)> =1992A&A...265...77H
ADC_Keywords: Stars, variable; Photometry, VBLUW; Binaries, cataclysmic Keywords: accretion disk - stars: TT Ari - stars: cataclysmic variables - X-rays: binaries - photometry Description: TT Ari was observed in the 5 passbands VBLUW (544, 430, 384, 362 and 324nm) during 3 nights on the 90cm telescope at ESO (La Silla), between July and November 1988, with an integration time of 16s. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 02 06 53.1 +15 17 43 TT Ari = 2E 0204.1+1503 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tt-ari.dat 84 731 VBLUW fluxes of TT Ari
See also: J/A+A/242/401 : Walraven photometry of WX Hyi (Kuulkers+ 1991) J/A+AS/101/87 : Walraven photometry of 8 Cataclysmic variables: BV Cen, HL Aqr, V426 Oph, V603 Aql, V2051 Oph, V3885 Sgr, VY Scl, WW Cet (Hollander+ 1993) Byte-by-byte Description of file: tt-ari.dat
Bytes Format Units Label Explanations
1- 14 F14.6 d BJED [2447389/2447401]+ Barycentric corrected Julian Ephemeris Date 16- 28 E13.6 mJy V ?=-99. Flux in V-band (1) 30- 42 E13.6 mJy B ?=-99. Flux in B-band (1) 44- 56 E13.6 mJy L ?=-99. Flux in L-band (1) 58- 70 E13.6 mJy U ?=-99. Flux in U-band (1) 72- 84 E13.6 mJy W ?=-99. Flux in W-band (1)
Note (1): Bad integrations have a value of -99.
Historical Notes: * 11-Feb-1993: first archived * 05-Jul-1995: converted the documentation; replaced the original BJED which was starting at 2447000.00 by the full date * 20-Dec-2002: added the description and object position.
(End) Francois Ochsenbein [CDS] 05-Jul-1995
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

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