JINA - Segue Virtual Journal,
27 November 2020
Volume 15, Issue 48 (14 Articles)
- # 1 - A Blueprint for the Milky Way's Stellar Populations. II. Improved Isochrone Calibration in the SDSS and Pan-STARRS Photometric Systems. (arXiv:2011.10740v1 [astro-ph.GA])
- # 2 - Estimating of ages and metallicities of M31 star clusters from LAMOST DR6. (arXiv:2011.11853v1 [astro-ph.GA])
- # 3 - HIRES, the high-resolution spectrograph for the ELT. (arXiv:2011.12317v1 [astro-ph.IM])
- Alessandro Marconi, Manuel Abreu, Vardan Adibekyan, Matteo Aliverti, Carlos Allende Prieto, Pedro J. Amado, Manuel Amate, Etienne Artigau, Sergio R. Augusto, Susana Barros, Santiago Becerril, Bjorn Benneke, Edwin Bergin, Philippe Berio, Naidu Bezawada, Isabelle Boisse, Xavier Bonfils, Francois Bouchy, Christopher Broeg, Alexandre Cabral, Rocio Calvo-Ortega, Bruno Leonardo Canto Martins, Bruno Chazelas, Andrea Chiavassa, Lise B. Christensen, Roberto Cirami, Igor Coretti, Stefano Cristiani, Vanderlei Cunha Parro, Guido Cupani, Izan de Castro Leao, Jose Renan de Medeiros, Marco Antonio Furlan de Souza, Paolo Di Marcantonio, Igor Di Varano, Valentina D'Odorico, Rene Doyon, Holger Drass, Pedro Figueira, Ana Belen Fragoso, Johan Peter Uldall Fynbo, Elena Gallo, Matteo Genoni, Jonay I. Gonzalez Hernandez, et al. (58 additional authors not shown)
- http://arxiv.org/abs/2011.12317
- # 4 - Nearly 30,000 late-type main-sequence stars with stellar age from LAMOST DR5. (arXiv:2011.12477v1 [astro-ph.GA])
- # 5 - Purveyors of fine halos III. Chemical abundance analysis of a potential omega Cen associate. (arXiv:2011.12303v1 [astro-ph.GA])
- # 6 - The Gaia spectrophotometric standard stars survey -- IV. Results of the absolute photometry campaign. (arXiv:2011.08625v2 [astro-ph.SR] UPDATED)
- G. Altavilla (1, 2), S. Marinoni (1, 2), E. Pancino (3, 2), S. Galleti (4), M. Bellazzini (4), N. Sanna (3), M. Rainer (3), G. Tessicini (4), J.M. Carrasco (5), A. Bragaglia (4), W.J. Schuster (6), G. Cocozza (4), M. Gebran (7), H. Voss (5), L. Federici (4), E. Masana (5), C. Jordi (5), M. Monguió, (5), A. Castro (8, 9), M.A. Peña-Guerrero (10), A. Pérez-Villegas (11, 6) ((1) INAF -- Osservatorio Astronomico di Roma, Italy, (2) Space Science Data Center -- ASI, Italy, (3) INAF -- Osservatorio Astrofisico di Arcetri, Italy, (4) INAF -- Osservatorio di Astrofisica e Scienza dello Spazio, Italy, (5) Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Spain, (6) Instituto de Astronomía, Universidad Nacional Autónoma de México, México, (7) Department of Physics, Astronomy, Notre Dame University-Louaize, Lebanon, (8) Observatorio Astronómico Nacional, Universidad Nacional Autónoma de México, México, (9) Consorcio de Investigación del Golfo de México, CICESE, México, (10) Space Telescope Science Institute, USA, (11) Universidade de São Paulo, IAG, Brazil)
- http://arxiv.org/abs/2011.08625
- # 7 - The Gaia-ESO Survey: Oxygen abundance in the Galactic thin and thick disks. (arXiv:2011.11473v1 [astro-ph.GA])
- Mariagrazia Franchini, Carlo Morossi, Paolo Di Marcantonio, Miguel Chavez, Vardan Adibekyan, Thomas Bensby, Angela Bragaglia, Anais Gonneau, Ulrike Heiter, Georges Kordopatis, Laura Magrini, Donatella Romano, Luca Sbordone, Rodolfo Smiljanic, Gra{ž}ina Tautvaišien{. e}, Gerry Gilmore, Sofia Randich, Amelia Bayo, Giovanni Carraro, Lorenzo Morbidelli, Simone Zaggia
- http://arxiv.org/abs/2011.11473
- # 8 - The search for extratidal star candidates around Galactic globular clusters NGC 2808, NGC 6266, and NGC 6397 with {textit{Gaia}} DR2 astrometry. (arXiv:2011.10525v2 [astro-ph.GA] UPDATED)
- # 9 - Untangling the Galaxy. II. Structure within 3 kpc
- # 10 - Production of Heavy Elements during the Explosion of a Low-Mass Neutron Star in a Close Binary
- # 11 - University rankings need a rethink
- # 12 - Arecibo radio telescope to be decommissioned
- # 13 - A Stream of Hypervelocity Stars from the Galactic Center
- # 14 - The Ultimately Large Telescope: What Kind of Facility Do We Need to Detect Population III Stars?
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
