Ellen Howell (National Astronomy and Ionospheric Centre, NAIC, Arecibo Observatory) and Mikko Kaasalainen (Helsinki University) were provided
with photometric data to support radar observations and asteroid shape modeling respectively.
Not exact matches
Abstract: We present: 1) a kinematic and morphological study of the giant Lya nebula associated
with the radio galaxy MRC2104 - 242 (z = 2.49) based on integral field spectroscopic VIMOS
data from VLT; 2) a
photometric study of the host (proto?)
We distill these candidates into sets of 104 validated planets (57 in multi-planet systems), 30 false positives, and 63 remaining candidat... ▽ More We present 197 planet candidates discovered using
data from the first year of the NASA K2 mission (Campaigns 0 - 4), along
with the results of an intensive program of
photometric analyses, stellar spectroscopy, high - resolution imaging, and statistical validation.
Recent progress has been made to address this: (1) the discovery that gamma Cas is an eccentric binary system (P = 203.59 d)
with unknown secondary type, (2) the accumulation of RXTE
data at 9 epochs in 1996 - 2000, and (3) the collation of robotic telescope B, V - band
photometric observations over 4 seasons.
Abstract: We studied solar - like oscillations in 115 red giants in the three open clusters NGC 6791, NGC 6811, and NGC 6819, based on
photometric data covering more than 19 months
with NASA's Kepler space telescope.
Mid-infrared
photometric data with -LCB- \ it -LCB- AKARI -RCB--RCB- / IRC MIR - S / S7, S9W, and S11 bands have shown excess emission over the thermal emission by hot amorphous carbon of 800K.
We confirm that the radial velocimetry and
photometric survey
data sets are compatible within the statistical errors, assuming that planets
with periods between 1 and 2 days are approximately 5 times less frequent than planets
with periods between 2 and 5 days.