[PDF] Top 20 Photometric variability in the cstar field: results from the 2008 data set

... the 2008 observing season, the installation provided long-baseline and high-cadence photometric observations in the i- band for 18,145 targets within 20 deg 2 CSTAR field around the South Celestial ... See full document

... telescopes. CSTAR is located at Dome A, Antarctica and covers 20 deg 2 of sky around the South Celestial ...exoplanets. CSTAR has been operational since 2008, and has taken a rich and high-precision ... See full document

... any set of 21 parameters can be obtained from the Ia and non-Ia ...nonlinear data (Hastie et al. 2009). The idea was to combine decisions from a group of weak classifiers to make a more ... See full document

... large set of separate facet values (see KT); the former is an efficient tool when de- termining the rotation ...end results may differ some- what (especially when the number of lightcurves or observing ... See full document

... the field may be in- complete as we accepted only those red objects showing slow ir- regular variability that are either matched with a known variable star or their variability can be confirmed ... See full document

... the results obtained with the TDS-1 where, beside the scattering, no spurious signal in the time series of the Euler angle correction estimations is visible (see ...vector data lead to any significant local ... See full document

... recovery from shading information has recently regained importance due to the improvement towards making the Photometric Stereo technique more reliable in terms of appearance of reflective ...exhaustive ... See full document

... flux from a source when centered on the source centroid; we set the fraction of collected light to be the 90% of the total flux (but this is an arbitrary choice, as long as the fraction is the same for ... See full document

... are from 24 programs that are listed on the MAST ...a set of extraordinary data that will have legacy value for the community into the JWST era and ... See full document

... (V6) data released by Remote Sensing Systems in 2006 (as used by Wentz et ...V6 data (including total precipitable water, brightness temperature, and wind speed retrieval), covering the period July 1987 to ... See full document

... Students from 2014 onwards generally had better EPQ grade outcomes than similar students (in terms of values on the set of variables used for comparison) from 2013 and ...grade from 2013 to ... See full document

... ranging from v24 to v40, in keeping with the nomenclature of Park & Nemec (2000, hereafter ...the results from our search for hot Jupiters in the NITES survey ...of variability is found to be ... See full document

... ) from the photo- z ...zero-point from a model fit to the NB. In practice we find better results from fitting to both NB and BB data, applying zero-points to both ... See full document

... M DATA I N T H E C O S M O S F I E L D As the start of the survey suffered from adverse weather conditions, the data for the COSMOS field were collected over a longer period in the semesters ... See full document

... 3.2. Rejecting False Positives False positives come from four sources. The first source is diurnal variation. Though very weak after detrending, it still should be taken into consideration. Second, stars at the ... See full document

... of variability that we want to search and according to the number of σ that could be observed in literature in the different ...each data point is substituted with a median of n nearest points in temporal ... See full document

... organizational arrangements of these businesses; and the characteristics of their founders. The KFS will undercount the number of new firms because the D&B frame is not the universe of all U.S. firms, nor does it capture ... See full document

... continued photometric follow-up observations after discovery may already be sufficient for a preliminary ...a set of minor planet models, we can already start to perform statistical ...deviation from ... See full document

... 3.1. Flux Density Normalization and Phase Alignment In order to compare pulse pro fi le shapes, we need to align them in phase and normalize them in fl ux density as effectively as possible. In many cases, the TOAs deviate ... See full document

... ray data, a slightly larger target geometry should be ...measurement data, a so-called volume mode is available as an alternative for calculating the starting points onto the surface of the target ... See full document