activity
20062025
most citedReconstructing the Subsurface Three-Dimensional Magnetic Structure of A Solar Active Region Using SDO/HMI Observations

269 citations · 616 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2025

Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Resolved Stellar Populations Studies in M31 and its Satellites

C. Gallart, E. Fernández-Alvar, A. B. A. Queiroz +48

A 30 m class optical/near-IR telescope in the Northern Hemisphere, equipped for diffraction-limited imaging and high-resolution, multi-object spectroscopy of faint stars, would ena…

astro-ph.HE2024

Evidence for inflows and outflows in the nearby black hole transient Swift J1727.8-162

D. Mata Sánchez, T. Muñoz-Darias, M. Armas Padilla +2

We present 20 epochs of optical spectroscopy obtained with the GTC-10.4m telescope across the bright discovery outburst of the black hole candidate Swift J1727.8-162. The spectra c…

astro-ph.IM2018★ 20 cited

MOLPOP-CEP: An Exact, Fast Code for Multi-Level Systems

A. Asensio Ramos, M. Elitzur

We present MOLPOP-CEP, a universal line transfer code that allows the exact calculation of multi-level line emission from a slab with variable physical conditions for any arbitrary…

astro-ph.GA2018★ 31 cited

Local anti-correlation between star-formation rate and gas-phase metallicity in disk galaxies

J. Sanchez Almeida, N. Caon, C. Munoz-Tunon +2

Using a representative sample of 14 star-forming dwarf galaxies in the local Universe, we show the existence of a spaxel-to-spaxel anti-correlation between the index N2 (log([NII]6…

astro-ph.EP2015★ 1 cited

CanariCam/GTC observations of (99942) Apophis

J. Licandro, T. Müller, C. Alvarez +2

The potentially hazardous asteroid (PHA) (99942) Apophis is one of the most remarkable near-Earth asteroids (NEA) in terms of impact hazard. A good determination of its surface the…

astro-ph.GA2015

The trace of a substantial assembly of massive E-S0 galaxies at 0.8<z<1.5 in galaxy number counts

Mercedes Prieto, M. Carmen Eliche-Moral

K-band galaxy number counts (GNCs) exhibit a slope change at K~17.5 mag not present in optical bands. To unveil the nature of this feature, we have derived the contribution of diff…