output
20052026
most citedCarbon Enhanced Metal-Poor Stars. I. Chemical Compositions of 26 Stars

508 citations

Showing 2023Show all

12 papers · 1 filter

astro-ph.CO2023

Building an Efficient Cluster Cosmology Software Package for Modeling Cluster Counts and Lensing

M. Aguena, O. Alves, J. Annis +60

We introduce a software suite developed for galaxy cluster cosmological analysis with the Dark Energy Survey Data. Cosmological analyses based on galaxy cluster number counts and w…

astro-ph.GA202317 cited

Probing magnetic fields in the circumgalactic medium using polarization data from MIGHTEE

K. Böckmann, M. Brüggen, V. Heesen +10

The detection and study of magnetic fields surrounding galaxies is important to understand galaxy evolution since magnetic fields are tracers for dynamical processes in the circumg…

astro-ph.CO20236 cited

Central radio galaxies in galaxy clusters: Joint surveys by eROSITA and ASKAP

K. Böckmann, M. Brüggen, B. Koribalski +18

The extended ROentgen Survey with an Imaging Telescope Array (eROSITA) telescope onboard the Spectrum-Roentgen-Gamma (SRG) mission has finished the first eROSITA All-Sky Survey (eR…

astro-ph.SR202310 cited

The CARMENES search for exoplanets around M dwarfs. Behaviour of the Paschen lines during flares and quiescence

B. Fuhrmeister, S. Czesla, J. H. M. M. Schmitt +17

The hydrogen Paschen lines are known activity indicators, but studies of them in M~dwarfs during quiescence are as rare as their reports in flare studies. This situation is mostly…

astro-ph.EP202323 cited

Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD235088 b (TOI-1430 b) with CARMENES

J. Orell-Miquel, M. Lampón, M. López-Puertas +31

HD235088 (TOI-1430) is a young star known to host a sub-Neptune-sized planet candidate. We validated the planetary nature of HD235088 b with multiband photometry, refined its plane…

astro-ph.SR20239 cited

The CARMENES search for exoplanets around M dwarfs -- A deep transfer learning method to determine Teff and [M/H] of target stars

A. Bello-García, V. M. Passegger, J. Ordieres-Meré +17

The large amounts of astrophysical data being provided by existing and future instrumentation require efficient and fast analysis tools. Transfer learning is a new technique promis…