activity
20172025
most citedTarget Selection for the SDSS-IV APOGEE-2 Survey

293 citations · 296 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.GA20251 cited

The large-scale kinematics of young stars in the Milky Way disc: first results from SDSS-V

Eleonora Zari, Jaime Villaseñor, Marina Kounkel +17

We present a first large-scale kinematic map of 50,000 young OB stars ( K), based on BOSS spectroscopy from the Milky Way Mapper OB program in the on…

astro-ph.SR2025

Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability

Rakesh Pandey, Aina Palau, Javier Serna +8

Using optical time series with Telescopi Joan Oró (TJO), Gaia, TESS, and NEOWISE archival data, we performed a variability study on the candidate bloated massive young stellar obje…

astro-ph.IM20242 cited

tonalli: an asexual genetic code to characterise APOGEE-2 stellar spectra. I. Validation with synthetic and solar spectra

Lucía Adame, Carlos Román-Zúñiga, Jesús Hernández +2

We present tonalli, a spectroscopic analysis python code that efficiently predicts effective temperature, stellar surface gravity, metallicity, -element abundance, and rotationa…

astro-ph.GA2024

Gravity or turbulence? VI. The physics behind the Kennicutt-Schmidt relations

Javier Ballesteros-Paredes, Manuel Zamora-Avilés, Carlos Román-Zúñiga +6

We explain the large variety of star formation laws in terms of one single, simple law that can be inferred from the definition of the star formation rate and basic algebra. The re…

astro-ph.SR2024

Atmospheric parameters and chemical abundances within 100 pc. A sample of G, K, and M main-sequence stars

Ricardo López-Valdivia, Lucía Adame, Eduardo Zagala Lagunas +9

To date, we have access to enormous inventories of stellar spectra that allow the extraction of atmospheric parameters and chemical abundances essential in stellar studies. However…

astro-ph.GA2024

SDSS-V Local Volume Mapper (LVM): A Glimpse into Orion

K. Kreckel, O. V. Egorov, E. Egorova +37

The Orion Molecular Cloud complex, one of the nearest (D = 406 pc) and most extensively studied massive star-forming regions, is ideal for constraining the physics of stellar feedb…