output
19922026
most citedThe SIESTA method for ab initio order-N materials simulation

12k citations

Showing 2020 · astro-ph.EPShow all

46 papers · 2 filters

astro-ph.EP2020★ 8 cited

A physico-chemical model to study the ion densitydistribution in the inner coma of comet C/2016 R2(Pan-STARRS)

Susarla Raghuram, Anil Bhardwaj, Damien Hutsemékers +3

The recent observations show that comet C/2016 R2 (Pan-Starrs) has a unique and peculiar composition when compared with several other comets observed at 2.8 au heliocentric distanc…

astro-ph.EP2020★ 44 cited

Mercury's crustal thickness correlates with lateral variations in mantle melt production

Mikael Beuthe, Bernard Charlier, Olivier Namur +2

Mercury's crust has a complex structure resulting from a billion years of volcanism. The surface variations in chemical composition have been identified from orbit by the spacecraf…

astro-ph.EP2020★ 19 cited

Luminous efficiency based on FRIPON meteors

Esther Drolshagen, Theresa Ott, Detlef Koschny +36

In meteor physics the luminous efficiency is used to convert the meteor's magnitude to the corresponding meteoroid's mass. However, lack of sufficiently accurate verification m…

astro-ph.EP2020★ 106 cited

SPECULOOS -- Ultracool Dwarf Transit Survey: Target List and Strategy

D. Sebastian, M. Gillon, E. Ducrot +20

One of the most promising avenues for the detailed study of temperate Earth-sized exoplanets is the detection of such planets in transit in front of stars small and nearby enough t…

astro-ph.EP2020★ 47 cited

The CARMENES search for exoplanets around M dwarfs -- LP 714-47b (TOI 442.01): Populating the Neptune desert

S. Dreizler, I., J. +134

We report the discovery of a Neptune-like planet (LP 714-47 b, P = 4.05204 d, m_b = 30.8 +/- 1.5 M_earth , R_b = 4.7 +/- 0.3 R_earth ) located in the 'hot Neptune desert'. Confirma…

astro-ph.EP2020★ 17 cited

TOI 122b and TOI 237b, two small warm planets orbiting inactive M dwarfs, found by \textit{TESS}

William C. Waalkes, Zachory K. Berta-Thompson, Karen A. Collins +39

We report the discovery and validation of TOI 122b and TOI 237b, two warm planets transiting inactive M dwarfs observed by \textit{TESS}. Our analysis shows TOI 122b has a radius o…