Identification and Follow-Up Observations of Low-Mass Eclipsing Binaries from Kepler
An outstanding problem in Astronomy for the past 15+ years has been that the radii of low-mass, (M 1.0 M&sun;), main-sequence stars in eclipsing binary systems...
Identification and monitoring program of OH/IR stars
We present the results of a long-term near infrared monitoring program (observations in the J, H and K bands) which was carried out on a selected sample of 25...
Identification of Optical Counterparts of ULX sources
We present the results of an on-going program for the identification and characterization of optical counterparts of Ultra-Luminous X-ray (ULX) sources. The...
Identification of pulsation modes from spectroscopy
Time-series of high-resolution spectra of massive main-sequence pulsators contain information on the degree l and azimuthal number m of a pulsation mode. I...
Identification of Superclusters and their Properties in the Sloan Digital Sky Survey
Superclusters are the largest massive structures in the cosmic web on tens to hundreds of megaparsecs (Mpc) scales. They are the largest assembly of galaxy...
Identifying the fingerprints of r-process heavy metals in a short GRB
The afterglow of some short GRBs displays a late-time rebrightening, visible in the near-infrared a few days after the burst. This late-time bump could be...