2 papers
astro-ph.EP2020
A new method for deriving composition of S-type asteroids from noisy and incomplete near-infrared spectra
Juan A. Sanchez, Cristina Thomas, Vishnu Reddy +3
The surface composition of S-type asteroids can be determined using band parameters extracted from their near-infrared (NIR) spectra (0.7-2.50 m) along with spectral calibration…
astro-ph.GA2018
Searching for Inflow Towards Massive Starless Clump Candidates Identified in the Bolocam Galactic Plane Survey
Jenny Calahan, Yancy Shirley, Brian Svoboda +22
Recent Galactic plane surveys of dust continuum emission at long wavelengths have identified a population of dense, massive clumps with no evidence for on-going star formation. The…