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The possible orbital period of the nova V1493 Aquilae
Astrophysics · Submitted 11 Nov 2005
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Following the sinusoidal shape of the phased light curve, we interpret this periodicity as possibly orbital in nature which is consistent with a cataclysmic variable above the period gap.
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The abstract, sentence by sentence
Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 no. 1) performed during 12 nights through I and R filters a few weeks after maximum is presented. The PDM method for period analysis (Stellingwerf 1978) is used. The photometric data is modulated with a period of 0.156 +- 0.001 d. Following the sinusoidal shape of the phased light curve, we interpret this periodicity as possibly orbital in nature which is consistent with a cataclysmic variable above the period gap.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 no. 1) performed during 12 nights through I and R filters a few weeks after maximum is presented. | contribution 0.68 | 0.94 | 0.04 | asserted 0.88 |
| s1 | The PDM method for period analysis (Stellingwerf 1978) is used. | method 1.00 | 0.28 | 0.02 | asserted 0.99 |
| s2 | The photometric data is modulated with a period of 0.156 +- 0.001 d. | result 1.00 | 0.94 | 0.35 | asserted 1.00 |
| s3 | Following the sinusoidal shape of the phased light curve, we interpret this periodicity as possibly orbital in nature which is consistent with a cataclysmic variable above the period gap. | interpretation 1.00 | 0.79 | 0.86 | hedged possibility 0.99 |
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The paper
Original abstract
Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 no. 1) performed during 12 nights through I and R filters a few weeks after maximum is presented. The PDM method for period analysis (Stellingwerf 1978) is used. The photometric data is modulated with a period of 0.156 +- 0.001 d. Following the sinusoidal shape of the phased light curve, we interpret this periodicity as possibly orbital in nature which is consistent with a cataclysmic variable above the period gap.
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