activity
20172021
most citedThe effect of stellar activity on the spectroscopic stellar parameters of the young solar twin HIP 36515

54 citations · 189 across the 9 of their papers we have counts for

collaborators

15 papers

astro-ph.SR20213 cited

M dwarf spectral indices at moderate resolution: accurate and [Fe/H] for 178 southern stars

E. Costa-Almeida, G. F. Porto de Mello, R. E. Giribaldi +2

We present a spectroscopic and photometric calibration to derive effective temperatures and metallicities [Fe/H] for M dwarfs, based on a Principal Component Ana…

astro-ph.SR2021

Rocky planet engulfment in the binary system HIP 71726-37

J. Yana Galarza, R. López-Valdivia, J. Meléndez +1

Binary stars are supposed to be chemically homogeneous, as they are born from the same molecular cloud. However, high precision chemical abundances show that some binary systems di…

astro-ph.SR20213 cited

Radial velocity precision of ESPRESSO through the analysis of the solar twin HIP 11915

Yuri Netto, Diego Lorenzo-Oliveira, Jorge Meléndez +4

Different stellar phenomena affect radial velocities (RVs), causing variations large enough to make it difficult to identify planet signals from the stellar variability. RV variati…

astro-ph.SR202120 cited

Searching for new solar twins: The Inti survey for the Northern Sky

J. Y. Galarza, R. López-Valdivia, D. Lorenzo-Oliveira +9

Solar twins are key in different areas of astrophysics, however only just over a hundred were identified and well-studied in the last two decades. In this work, we take advantage o…

astro-ph.SR202111 cited

Explosive nucleosynthesis of a metal-deficient star as the source of a distinct odd-even effect in the solar twin HIP 11915

Jhon Yana Galarza, Jorge Meléndez, Amanda I. Karakas +2

The abundance patterns observed in the Sun and in metal-poor stars show a clear odd-even effect. An important question is whether the odd-even effect in solar-metallicity stars is…

astro-ph.SR202015 cited

Rotation of solar analogs cross-matching Kepler and Gaia DR2

Jose-Dias do Nascimento, Leandro de Almeida, Eduardo Nunes Velloso +10

A major obstacle to interpreting the rotation period distribution for main-sequence stars from Kepler mission data has been the lack of precise evolutionary status for these object…