activity
20122022
most citedEarly Science with the Large Millimeter Telescope: CO and [C II] Emission in the z=4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1)

58 citations · 222 across the 15 of their papers we have counts for

collaborators
Showing 2014Show all

5 papers · 1 filter

astro-ph.SR2014★ 24 cited

ALMA observations of alpha Centauri: First detection of main-sequence stars at 3mm wavelength

R. Liseau, W. Vlemmings, A. Bayo +19

The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research.…

astro-ph.IM2014

Xitris: A Software to Acquire, Display, Compress, and Publish Data in Real Time using Distributed Mode for the Solar Radio Interferometer RIS

Victor De la Luz, Alejandro Lara

Upgrading the infrastructure of old scientific instruments requires the development of new hardware and software which may be expensive (in general, these projects lack of enough r…

astro-ph.SR2014

The Chromospheric Solar Millimeter-wave Cavity; a Common Property in the Semi-empirical Models

Victor De la Luz, Miguel Chavez, Emanuele Bertone

The semi-empirical models of the solar chromosphere are useful in the study of the solar radio emission at millimeter - infrared wavelengths. However, current models do not reprodu…

astro-ph.SR2014

The Limb Brightening and its Relationship with the Millimeter-wave Cavity

Victor De la Luz, Miguel Chavez, Emanuele Bertone

Through a detailed theoretical analysis of the local emission at millimeter,sub-millimeter and infrared wavelength regimes (from \~ 10 GHz up to \~ 10 THz), we found that, associat…

astro-ph.SR2014★ 12 cited

The Relation between the Radial Temperature Profile in the Chromosphere and the Solar Spectrum at Centimeter, Millimeter, Sub-millimeter, and Infrared Wavelengths

Victor De la Luz, Miguel Chavez, Emanuele Bertone +1

Solar observations from millimeter to ultraviolet wavelengths show that there is a temperature minimum between photosphere and chromosphere. Analysis based on semi-empirical models…