Hα star formation rates in massive galaxies at z˜ 1
We present a near-infrared spectroscopic study of a stellar mass selected sample of galaxies at z˜ 1 utilizing the Long-slit Intermediate Resolution Infrared...
Hβ spectroscopy of the high-inclination black hole transient Swift J1357.2−0933 during quiescence
Swift J1357.2−0933 is a transient low-mass X-ray binary hosting a stellar-mass black hole. The source exhibits optical dips and very broad emission lines during...
IAC-pop: Finding the Star Formation History of Resolved Galaxies
IAC-pop is a code designed to solve the star formation history (SFH) of a complex stellar population system, like a galaxy, from the analysis of the color...
IAC-STAR: A Code for Synthetic Color-Magnitude Diagram Computation
The code IAC-STAR is presented. It generates synthetic H-R and color-magnitude diagrams (CMDs) and is mainly aimed at star formation history studies in nearby...
IACUB - a New Echelle Spectrograph for Use at the Observatorio del Roque-De
An uncrossed echelle spectrograph has been constructed in a collaboration between the Queen's University of Belfast and the Instituto de Astrofísica de Canarias...
IC 10: More evidence that it is a blue compact dwarf
We present optical spectroscopy of H Ii regions in the Local Group galaxy IC 10 and UBVR photometry of foreground stars in three fields towards this galaxy...
IC 2602: a lithium depletion boundary age and new candidate low-mass stellar members
We report the results from a photometric and spectroscopic survey of ˜1.4 deg2 of the young open cluster IC 2602. Fourteen objects have been identified as...
Identification and Mitigation of a Vibrational Telescope Systematic with Application to Spitzer
We observed Proxima Centauri with the Spitzer Space Telescope Infrared Array Camera five times in 2016 and 2017 to search for transits of Proxima Centauri b...
Identification of a Group III CEMP-no Star in the Dwarf Spheroidal Galaxy Canes Venatici I
CEMP-no stars, a subclass of carbon-enhanced metal-poor (CEMP) stars, are one of the most significant stellar populations in galactic archeology, because they...