Evidence for planet engulfment by the star HD82943
Current models of the evolution of the known extrasolar planetary systems need to incorporate orbital migration and/or gravitational interactions among giant...
Evidence for Population-dependent Vertical Motions and the Long-lived Nonsteady Lopsided Milky Way Warp
We present a Galactic disk vertical velocity analysis using OB type stars (OB stars), red clump (RC) stars, and main-sequence turnoff (MSTO) stars with...
Evidence for Quasi-Isotropic Magnetic Fields from Hinode Quiet-Sun Observations
Some recent investigations of spectropolarimetric observations of the Zeeman effect in the Fe I lines at 630 nm carried out with the Hinode solar space...
Evidence for quiescent synchrotron emission in the black hole X-ray transient Swift J1357.2-0933
We present high time resolution ULTRACAM optical and NOTCam infrared observations of the edge-on black hole X-ray transient Swift J1357.2-0933. Our data taken...
Evidence for Rotational Motions in the Feet of a Quiescent Solar Prominence
We present observational evidence of apparent plasma rotational motions in the feet of a solar prominence. Our study is based on spectroscopic observations...
Evidence for Spin─Orbit Alignment in the TRAPPIST-1 System
In an effort to measure the Rossiter─McLaughlin effect for the TRAPPIST-1 system, we performed high-resolution spectroscopy during transits of planets e, f, and...
Evidence for stellar contamination and water absorption in NGTS-5b's transmission spectra with GTC/OSIRIS
Context. Transmission spectroscopy serves as a valuable tool for probing atmospheric absorption features in the terminator regions of exoplanets. Stellar...
Evidence for stellar contamination in the transmission spectra of HAT-P-12b
Context. Transmission spectroscopy characterizes the wavelength dependence of transit depth, revealing atmospheric absorption features in planetary terminator...
Evidence for Substructure on the Inner Broad Line Region of the Lensed Quasar SDSS J1004+4112 from the Recurrence of Microlensing in the C IV Emission Line
We use microlensing to probe the inner broad line region (BLR) of the lensed quasar SDSS J1004+4112, finding evidence of substructure. We study the recurrent...