J/PASP/123/659 Analysis of flares of V1285 Aql (Dal+, 2011)
The patterns of high-level magnetic activity occurring on the surface of
V1285 Aql: The OPEA model of flares and DFT models of stellar spots.
Dal H.A., Evren S.
<Publ. Astron. Soc. Pac., 123, 659-670 (2011)>
=2011PASP..123..659D 2011PASP..123..659D
ADC_Keywords: Stars, flare ; Photometry, UBVRI
Keywords: methods: data analysis - methods: statistical - stars: spots -
stars: flare - stars: individual (V1285 Aql)
Abstract:
Statistically analysing Johnson UBVR observations of V1285 Aql during
the three observing seasons, both activity level and behaviour of the
star are discussed in respect to obtained results. We also discuss the
variation out-of-flare due to rotational modulation.
Description:
The observations were acquired with a High-Speed Three Channel
Photometer attached to the 48 cm Cassegrain type telescope at Ege
University Observatory.
Objects:
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RA (2000) DE Designation(s)
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18 55 27.41 +08 24 09.0 V1285 Aql = Gliese 735
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2.dat 78 83 The parameters derived from analyses of
the detected flares
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 10 A10 "DD.MM.YYYY" Date Observing date
12- 22 F11.5 d HJD HJD of flare maximum (HJD-2400000)
24- 27 I4 s t.rise Rise time
29- 32 I4 s t.decay Decay time
34- 37 I4 s Dur Total duration
39- 48 F10.5 s EDur Equivalent duration
50- 54 F5.3 mag Amp Flare amplitude
56- 61 F6.3 mag U-B Flare U-B colour index
63- 73 E11.6 10-7W E Flare Energy
75- 78 A4 --- Type [Slow Fast] Flare type ("Slow" or "Fast")
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History:
From electronic version of the journal
(End) Patricia Vannier [CDS] 23-Jan-2013