The data file contains 48,853 RGB stars from Apogee DR16 within the Milky Way disk, for which we determine spectro-photometric parallax estimates (as described in Hogg et al. 2019, AJ, 158, 147), as well as self-calibrated stellar element abundances. The data set is described in detail and analyzed in Eilers et al. 2022 (arXiv: 2112.03295)
© 2017. The American Astronomical Society. All rights reserved.. The orbits, atmospheric parameters,...
Context. The APOGEE survey has obtained high-resolution infrared spectra of more than 100,000 stars....
The spectral analysis and data products in Data Release 16 (DR16; 2019 December) from the high-resol...
Spectrophotometric distances to 44,784 RGB stars predicted with a data-driven model combining spectr...
We combine high-resolution spectroscopic data from APOGEE-2 survey Data Release 16 (DR16) with broad...
Although the use of RGB photometry has exploded in the last decades due to the advent of high-qualit...
International audienceThe Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution...
With contemporary infrared spectroscopic surveys like APO Galactic Evolution Experiment (APOGEE), re...
Context. The APOGEE survey has obtained high-resolution infrared spectra of more than 100 000 stars....
Combining the precise parallaxes and optical photometry delivered by Gaia’s second data release with...
Spectroscopic parameters for 758 red giant branch stars in 51 Milky Way globular clusters. For each ...
Purpose: In order to study the Galactic Chemical Evolution, elemental abundances are needed. The pur...
International audienceContext: The Sagittarius (Sgr) dwarf spheroidal galaxy is currently being disr...
Context. The third Gaia data release (Gaia DR3) contains, beyond the astrometry and photometry, disp...
We combine high-resolution spectroscopic data from APOGEE-2 survey Data Release 16 (DR16) with broad...
© 2017. The American Astronomical Society. All rights reserved.. The orbits, atmospheric parameters,...
Context. The APOGEE survey has obtained high-resolution infrared spectra of more than 100,000 stars....
The spectral analysis and data products in Data Release 16 (DR16; 2019 December) from the high-resol...
Spectrophotometric distances to 44,784 RGB stars predicted with a data-driven model combining spectr...
We combine high-resolution spectroscopic data from APOGEE-2 survey Data Release 16 (DR16) with broad...
Although the use of RGB photometry has exploded in the last decades due to the advent of high-qualit...
International audienceThe Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution...
With contemporary infrared spectroscopic surveys like APO Galactic Evolution Experiment (APOGEE), re...
Context. The APOGEE survey has obtained high-resolution infrared spectra of more than 100 000 stars....
Combining the precise parallaxes and optical photometry delivered by Gaia’s second data release with...
Spectroscopic parameters for 758 red giant branch stars in 51 Milky Way globular clusters. For each ...
Purpose: In order to study the Galactic Chemical Evolution, elemental abundances are needed. The pur...
International audienceContext: The Sagittarius (Sgr) dwarf spheroidal galaxy is currently being disr...
Context. The third Gaia data release (Gaia DR3) contains, beyond the astrometry and photometry, disp...
We combine high-resolution spectroscopic data from APOGEE-2 survey Data Release 16 (DR16) with broad...
© 2017. The American Astronomical Society. All rights reserved.. The orbits, atmospheric parameters,...
Context. The APOGEE survey has obtained high-resolution infrared spectra of more than 100,000 stars....
The spectral analysis and data products in Data Release 16 (DR16; 2019 December) from the high-resol...