EMIR: the GTC NIR multi-object imager-spectrograph
We present the final global design and performances of EMIR, the NIR multiobject spectrograph of the GTC, as well as the plan for its early scientific...
Emission lines in EX Lup optical spectrum (Sipos+, 2009)
A high-resolution optical spectrum of EX Lupi was obtained on 2007 July 30 with FEROS at the 2.2m MPG/ESO telescope in ESO La Silla, Chile. The spectrum shows...
Empirical calibration of the near-IR Ca triplet (Cenarro+ 2001)
File table contains details of the new near-IR stellar library observed to calibrate the Ca II triplet. It includes the indices CaT*, CaT and PaT measured over...
Empirical calibration of the near-IR Ca triplet (Cenarro+ 2001)
File table contains details of the new near-IR stellar library observed to calibrate the Ca II triplet. It includes the indices CaT*, CaT and PaT measured over...
Evaluation of a Magnetic Field Inversion Method Using Only Stokes I
We compare a method for inferring the photospheric vector magnetic field using only spectroscopy to a conventional method based on polarimetry. The magnetic...
Evidence for Evolved Stellar Binary Mergers in Observed B-type Blue Supergiants
Blue supergiants are the brightest stars in their host galaxies, and yet their evolutionary status has been a long-standing problem in stellar astrophysics. In...
Evidence for the Accretion of Gas in Star-forming Galaxies: High N/O Abundances in Regions of Anomalously Low Metallicity
While all models for the evolution of galaxies require the accretion of gas to sustain their growth via on-going star formation, it has proven difficult to...