VizieR Online Data Catalog: The Perkins INfrared Exosatellite Survey. I. (Tamburo+, 2022)

Perkins INfrared Exosatellite Survey (PINES) is conducted using Boston University's 1.8m Perkins Telescope Observatory (PTO), located on Anderson Mesa, Arizona, at an altitude of 2206m. The telescope is a Cassegrain reflector with a 0.4m diameter secondary mirror.

In the survey, we perform photometric observations of L and T dwarfs using Mimir, a NIR polarimeter, spectrometer, and imager that is permanently housed at the PTO. We use the instrument in its broadband J- and H-band wide-field imaging modes, which provide 10'x10' field-of-view (FOV) images. The J- and H-band filters are from the Mauna Kea Observatories near-infrared (MKO-NIR) set, which was designed in part to avoid contamination from water vapor lines.

(1 data file).