We investigate the clustering properties of radio sources in the Alternative Data Release 1 of the TIFR GMRT Sky Survey (TGSS), focusing on large angular scales...
CO<SUB>2</SUB> as the main parent source of atomic oxygen in comet C/2017 K2 (Pan-STARRS)
C/2017 K2 (Pan-STARRS) is an Oort cloud comet discovered in May 2017. Ground observations have revealed that this long-period comet was active at heliocentric...
Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems
The exoplanet population characterized by relatively short orbital periods (P < 100 d) around solar-type stars is dominated by super-Earths and sub-Neptunes...
Color study of asteroid families within the MOVIS catalog
The aim of this work is to study the compositional diversity of asteroid families based on their near-infrared colors, using the data within the MOVIS catalog...
Comparing approximate methods for mock catalogues and covariance matrices II: power spectrum multipoles
We study the accuracy of several approximate methods for gravitational dynamics in terms of halo power spectrum multipoles and their estimated covariance matrix...
Comparing the emission spectra of U and Th hollow cathode lamps and a new U line list
Context. Thorium hollow cathode lamps (HCLs) are used as frequency calibrators for many high resolution astronomical spectrographs, some of which aim for...
Comparison of Damping Mechanisms for Transverse Waves in Solar Coronal Loops
We present a method to assess the plausibility of alternative mechanisms to explain the damping of magnetohydrodynamic transverse waves in solar coronal loops...
Comparison of theoretical and observed Ca II 8542 Stokes profiles in quiet regions at the centre of the solar disc
Context. Interpreting the Stokes profiles observed in quiet regions of the solar chromosphere is a challenging task. The Stokes Q and U profiles are dominated...
Comparison of Two Fitting Methods for Ring Diagram Analysis of Very High L Solar Oscillations
A new method of fitting tridimensional power spectra of solar oscillations is described and compared with a previous one whose use has been more common. The new...