CURious Variables Experiment (CURVE): CCD photometry of active dwarf nova DI Ursae Majoris
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Findings: The diagnostic performance of salivary Lf in the cohort 1 had an area under the curve [AUC] of 095 (0911 0992) for the differentiation of the prodromal AD/AD group
Figure 10 shows the relative transit depths of the WASP-79b LDSS-3C data for eight wavelength bins for the light curve extraction using the Divide –White normalization method..
We estimated the radius of the transiting object using multicolour transit modelling, and we set upper limits for its mass, effective temperature, and Bond albedo using a phase
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The orbital period of 514 days is much longer than the estimated rotation period of 198 ± 92 days (P rot / sin i = 128 − 332 days within uncertainties), which, together with absence
Middle: detrended light curve after removing the GP model (see Sect. 2.1) and including the median transit model obtained with PASTIS for the 3 planets in the system (grey solid