Table 1.
QPO frequencies for TT Ari.
Observation | Observation details | Passband/ | f peaks | f range | References |
---|---|---|---|---|---|
Year | filters | (d−1) | (d−1) | ||
1961–1962 | 1 observing run (3 hours) of observations. | UV | 34.1, 81.8 and 103.6 | ... | 1 |
1961, 1962 and 1966 | 15 observing runs, each of 2–5 hours. | V and U | ... | 36–140 | 2 |
1961–1985 | 30 observing runs. | Varied (U, B, UB, UVB) | 53.3 in 1961, up to 84.7 in 1985 | ... | 3 |
1987–1988 | 12 nights of observation. | Filter V | 72 | 65.4–80 | 4 |
1988 | 3 nights. Around 250 observations per night. | 3250–5500 Å | 94.1 | ... | 5 |
1988 | 16 nights. | 5 bands, but mostly B | 27.9, 52.4, 60.7 and 101.4 | ... | 6 |
1987–1998 | 45 observing runs. Over 600 measurements. | Standard UBV system | ... | 41.1–120 | 7 |
1994 | 16 nights (258 hours) of observation, 51 299 data points. | Close to B | 48 and 68.5 | 24–139 | 8 |
2005 | 51 observational runs, covering 226 hours. | Filter R | 66.7 (mean) | ... | 9 |
2012 | 15 days (361 hours) of continuous observation and 21 166 data points. | 3500–7500 Å | 42.5 & 77.5 | 27–98 | 10 |
Notes. Most of the presented studies involve a periodogram analysis and some sort of pre-whitening of unwanted periods. Details about the methods are found in the articles themselves. Columns 4 and 5 show information about frequencies (f) related to QPOs: f peaks refers to specific frequencies found as peaks in the periodogram, while f range presents frequency ranges in which QPOs are more common.
(1) Williams (1966); (2) Smak (2014); (3) Semeniuk et al. (1987); (4) Udalski (1988); (5) Hollander & van Paradijs (1992); (6) Tremko et al. (1996); (7) Kraicheva et al. (1999); (8) Andronov et al. (1999); (9) Kim et al. (2009); (10) dominant frequencies from this work.
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