We present the determination of stellar parameters and individual elemental abundances for
6 million stars from∼ 8 million low-resolution (R∼ 1800) spectra from LAMOST DR5. This is …

Abstract The EXtreme-PREcision Spectrograph (EXPRES) is an environmentally stabilized,
fiber-fed, R= 137,500, optical spectrograph. It was recently commissioned at the 4.3 m …

The Wide-Field Infrared Transient Explorer (WINTER) is a new infrared time-domain survey
instrument which will be deployed on a dedicated 1 meter robotic telescope at the Palomar …

We report the APOGEE-2S+ discovery of a unique collection of nitrogen-enhanced mildly
metal-poor giant stars, peaking at [Fe/H]∼− 0.89 with no carbon enrichment, toward the …

We present early results from the Epoch of Giant Planet Migration program, a precise radial
velocity (RV) survey of more than 100 intermediate-age (∼ 20–200 Myr) G and K dwarfs …

If the mysterious Fermi-LAT GeV γ-ray excess is due to an unresolved population of
millisecond pulsars (MSP) in the Galactic bulge, one expects this very same population to …

KELT-24b: A 5MJ Planet on a 5.6 day Well-aligned Orbit around the Young V = 8.3 F-star HD
93148 - IOPscience This site uses cookies. By continuing to use this site you agree to our use …

Transiting exoplanets orbiting young nearby stars are ideal laboratories for testing theories
of planet formation and evolution. However, to date only a handful of stars with age< 1 Gyr …

Located on the campus of the Thacher School in Southern California, the Thacher
Observatory has a legacy of astronomy research and education that dates back to the late …

Super Jupiters are giant planets with several Jupiter masses. It remains an open question
whether these planets originate with such high masses or grow through collisions. Previous …