J/A+A/278/449          Long-term photometry of FK Com    (Jetsu+ 1993)

Spot and flare activity of FK Comae Berenices: long-term photometry JETSU L., PELT J., TUOMINEN I. <Astron. Astrophys. 278, 449 (1993)> =1993A&A...278..449J 1993A&A...278..449J
Keywords: stars: individual: FK Comae - stars: activity - stars: variable - stars: flares File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 119 41 Normalized photometry table2 59 23 Photometric phases of FK Comae flares table3 127 41 Mean brightness in UBVRI table4 134 41 Amplitude of the rotational modulation of brightness in UBVRI -------------------------------------------------------------------------------- Byte-per-byte Description of file: table1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 9 F7.2 yr Year Average observing time 17- 23 F7.5 d Pphot Photometric rotation period 32- 38 F7.5 d e_Pphot rms uncertainty on Pphot 44- 48 F5.3 --- Phi(min) Phase of the light minimum 54- 58 F5.3 --- e_Phi(min) rms uncertainty on Phi(min) 64- 73 F10.4 d t_min Heliocentric julian date of the light minimum 79- 83 F5.3 --- Phi(tmin) Photometric phase 88- 93 F6.3 --- Phi(coh) Coherence length 99-104 F6.4 --- e_Phi(coh) rms uncertainty on Phi(coh) 109-110 I2 --- SET Division into subset of the observing time -------------------------------------------------------------------------------- Notes to table1: The photometric rotation period Pphot and the phase of the light minimum Phi(min) were derived for the subsets with at least 8 and 7 nights of non-flare observations, respectively. The heliocentric julian date of the light minimum t_min was derived for the photometric rotation period and its photometric phase Phi(t_min) from Eq. 1. The coherence length Phi(coh) was solved from Eq. 4 Byte-per-byte Description of file: table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 12 F10.4 d HJD_flare Average time 18- 23 F6.3 --- Phi(flare) Photometric phase 28- 33 F6.3 --- Delta Phase difference (Phi(flare) - Phi(min)) between the flare and the photometric minimum of the subset 39- 40 I2 --- SET Division into subsets of the observing time 48- 53 A6 --- F Category of the flare detection -------------------------------------------------------------------------------- Byte-per-byte Description of file: table3 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 8 F7.2 yr YEAR Average observing time 14- 18 F5.3 mag M(U) Mean brightness in U filter 24- 28 F5.3 mag e_M(U) rms uncertainty on M(U) 34- 38 F5.3 mag M(B) Mean brightness in B filter 44- 48 F5.3 mag e_M(B) rms uncertainty on M(B) 61- 65 F5.3 mag M(V) Mean brightness in V filter 71- 75 F5.3 mag e_M(V) rms uncertainty on M(V) 81- 85 F5.3 mag M(R) Mean brightness in R filter 91- 95 F5.3 mag e_M(R) rms uncertainty on M(R) 101-105 F5.3 mag M(I) Mean brightness in I filter 111-115 F5.3 mag e_M(I) rms uncertainty on M(I) 122-123 I2 --- SET Division into subsets of the observing time -------------------------------------------------------------------------------- Byte-per-byte Description of file: table4 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 9 F7.2 yr YEAR Average observing time 18- 22 F5.3 --- A(U) Amplitude of the rotational modulation of brightness in U filter 28- 32 F5.3 --- e_A(U) rms uncertainty on A(U) 38- 42 F5.3 --- A(B) Amplitude of the rotational modulation of brightness in B filter 48- 52 F5.3 --- e_A(B) rms uncertainty on A(B) 58- 62 F5.3 --- A(V) Amplitude of the rotational modulation of brightness in V filter 68- 72 F5.3 --- e_A(V) rms uncertainty on A(V) 86- 90 F5.3 --- A(R) Amplitude of the rotational modulation of brightness in R filter 96-100 F5.3 --- e_A(R) rms uncertainty on A(R) 106-110 F5.3 --- A(I) Amplitude of the rotational modulation of brightness in I filter 116-120 F5.3 --- e_A(I) rms uncertainty on A(I) 128-129 I2 --- SET Division into subset of observing time --------------------------------------------------------------------------------
(End) Patricia Bauer [CDS] 28-Oct-1993
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