J/A+A/310/173 TY Pyx IUE FES observations (Neff+, 1996)
Rotational modulation and flares on RS Canum Venaticorum and BY Draconis stars.
XIX. Simultaneous IUE, ROSAT, VLA, and visual observations of TY Pyxidis
Neff J.E., Pagano I., Rodono M., Brown A., Dempsey R.C., Fox D.C.,
Linsky J.L.
<Astron. Astrophys. 310, 173 (1996)>
=1996A&A...310..173N 1996A&A...310..173N (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable
Mission_Name: IUE
Keywords: stars: activity - stars: chromospheres - stars: coronae -
stars: individual: HD 77137 - stars: starspots
Description:
This is a 3-part table presenting a log of the IUE Fine-Error Sensor
Observations of TY Pyxidis in November 1990. In order to determine
accurate magnitudes from FES measurements, a focus and a
reference-point offset corrections must be applied. The data presented
in the paper (Figure 1) have these corrections applied and are
averages of two or more measures taken close in time.
Objects:
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RA (2000) DE Name
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08 59 42.7 -27 48 55 HD 77137 = TY Pyx
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 41 147 Log of IUE Fine-Error Sensor (FES) Observations
table1.tex 85 405 LaTeX version of table1
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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- 8 A8 "DD/MM/YY" OBSdate Observation date
10- 11 I2 h OBSh Observation time (UT), hours
13- 14 I2 min OBSm Observation time (UT), minutes
16- 17 I2 s OBSs Observation time (UT), seconds
19- 22 I4 --- Count Counts (f/o), Fast-Track Overlap mode.
24- 25 I2 --- dX Reference-point offset correction in X
27- 28 I2 --- dY Reference-point offset corrections in Y
30- 35 F6.4 --- Phase Phase. Phases are computed using the
ephemeris HJD2443548.6695 + 3.198584E.
37- 41 F5.2 --- Step ? Focus step
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(End) Patricia Bauer [CDS] 01-Mar-1996