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Early phases of the Galaxy from the chemical imprint on the iron-poor stars J0815+4729 and J0023+0307. (arXiv:2303.14142v1 [astro-ph.GA])
- Volume 18, Issue 13 - article #2
- Jonay I. González Hernández, David S. Aguado, Carlos Allende-Prieto, Adam Burgasser, Rafael Rebolo
- http://arxiv.org/abs/2303.14142
The chemical characterisation of halo substructure in the Milky Way based on APOGEE. (arXiv:2204.04233v1 [astro-ph.GA])
- Volume 17, Issue 15 - article #2
- Danny Horta, Ricardo P. Schiavon, J. Ted Mackereth, David H. Weinberg, Sten Hasselquist, Diane Feuillet, Robert W. O'Connell, Borja Anguiano, Carlos Allende-Prieto, Rachael L. Beaton, Dmitry Bizyaev, Katia Cunha, Doug Geisler, D. A. García-Hernández, Jon Holtzman, Henrik Jönsson, Richard R. Lane, Steve R. Majewski, Szabolcs Mészáros, Dante Minniti, Christian Nitschelm, Matthew Shetrone, Verne V. Smith, Gail Zasowski
- http://arxiv.org/abs/2204.04233
J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline. (arXiv:2109.11600v1 [astro-ph.SR])
- Volume 16, Issue 40 - article #2
- Carlos Andrés Galarza (1), Simone Daflon (1), Vinicius M. Placco (2), Carlos Allende-Prieto (3, 4), Marcelo Borges Fernandes (1), Haibo Yuan (5), Carlos López-Sanjuan (6), Young Sun Lee (7), Enrique Solano (8), F. Jiménez-Esteban (8), David Sobral (9), Alvaro Alvarez Candal (1, 17), Claudio B. Pereira (1), Stavros Akras (10), Eduardo Martín (3, 8), Yolanda Jiménez Teja (16), Javier Cenarro (6), David Cristóbal-Hornillos (6), Carlos Hernández-Monteagudo (6), Antonio Marín-Franch (6), Mariano Moles (6), Jesús Varela (6), Héctor Vázquez Ramió, (6), Jailson Alcaniz (1), Renato Dupke (1, 13, 14, 15), Alessandro Ederoclite (11), Laerte Sodré, Jr. (11), Raul E. Angulo (12) ((1) Observatório Nacional - MCTI ON, Rio de Janeiro, Brazil, (2) NSF's NOIRLab, Tucson, AZ 85719, USA, (3) Instituto de Astrofísica de Canarias, Tenerife, Spain, (4) Universidad de La Laguna, Departamento de Astrofísica, Tenerife, Spain, (5) Department of Astronomy, Beijing Normal University, Beijing, People's Republic of China, (6) Centro de Estudios de Física del Cosmos de Aragón CEFCA, Unidad Asociada al CSIC, Teruel, Spain, (7) Department of Astronomy, Space Science, Chungnam National University, South Korea, (8) Departamento de Astrofísica, Centro de Astrobiología CSIC-INTA, ESAC Campus, Villanueva de la Cañada, Madrid, Spain, (9) Department of Physics, Lancaster University, Lancaster, UK, (10) Institute for Astronomy, Astrophysics, Space Applications, Remote Sensing, National Observatory of Athens, GR Penteli, Greece, (11) Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, São Paulo, Brazil, (12) Ikerbasque, Basque Foundation for Science, Bilbao, Spain, (13) Department of Astronomy, University of Michigan, Ann Arbor, MI USA, (14) Eureka Scientific Inc., Oakland, CA, USA, (15) Department of Physics, Astronomy, University of Alabama, Tuscaloosa, AL, USA, (16) Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía, Granada, Spain, (17) Universidad de Alicante, San Vicente del Raspeig, Alicante, Spain)
- http://arxiv.org/abs/2109.11600
NLTE for APOGEE: Simultaneous Multi-Element NLTE Radiative Transfer. (arXiv:2003.13353v1 [astro-ph.SR])
- Volume 15, Issue 14 - article #2
- Yeisson Osorio, Carlos Allende-Prieto, Ivan Hubeny, Szabolcs Meszaros, Matthew Shetrone
- http://arxiv.org/abs/2003.13353

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