Gaia Data Release 3-The Galaxy in your preferred colours: Synthetic photometry from Gaia low-resolution spectra

P Montegriffo, M Bellazzini, F De Angeli… - Astronomy & …, 2023 - aanda.org
Gaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for≃
220 million sources in the wavelength range 330 nm≤ λ≤ 1050 nm (XP spectra). Synthetic …

The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies, and redshifts with 12 optical filters

C Mendes de Oliveira, T Ribeiro… - Monthly Notices of …, 2019 - academic.oup.com
ABSTRACT The Southern Photometric Local Universe Survey (S-PLUS) is imaging∼ 9300
deg2 of the celestial sphere in 12 optical bands using a dedicated 0.8 m robotic telescope …

The miniJPAS survey: A preview of the Universe in 56 colors

S Bonoli, A Marín-Franch, J Varela, HV Ramió… - Astronomy & …, 2021 - aanda.org
The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will
scan thousands of square degrees of the northern sky with a unique set of 56 filters using …

Spectral classification of the 100 pc white dwarf population from Gaia-DR3 and the virtual observatory

FM Jiménez-Esteban, S Torres… - Monthly Notices of …, 2023 - academic.oup.com
The third data release of Gaia has provided low-resolution spectra for∼ 100 000 white
dwarfs (WDs) that, together with the excellent photometry and astrometry, represent an …

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

S Jin, SC Trager, GB Dalton, JAL Aguerri… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility
for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2 …

The miniJPAS survey-The role of group environment in quenching star formation

RMG Delgado, JE Rodríguez-Martín… - Astronomy & …, 2022 - aanda.org
The miniJPAS survey has observed∼ 1 deg 2 of the AEGIS field with 60 bands (spectral
resolution of R∼ 60) in order to demonstrate the scientific potential of the Javalambre …

The spectral evolution of white dwarfs: where do we stand?

A Bédard - Astrophysics and Space Science, 2024 - Springer
White dwarfs are the dense, burnt-out remnants of the vast majority of stars, condemned to
cool over billions of years as they steadily radiate away their residual thermal energy. To first …

Chemodynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-s and CEMP-no Stars

J Zepeda, TC Beers, VM Placco, D Shank… - The Astrophysical …, 2023 - iopscience.iop.org
We construct a sample of 644 carbon-enhanced metal-poor (CEMP) stars with abundance
analyses based on moderate-to high-resolution spectroscopic studies. Dynamical …

Data Release 2 of S-PLUS: Accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters

F Almeida-Fernandes, L SamPedro… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT The Southern Photometric Local Universe Survey (S-PLUS) is an ongoing
survey of∼ 9300 deg2 in the southern sky in a 12-band photometric system. This paper …

The miniJPAS survey-Identification and characterization of galaxy populations with the J-PAS photometric system

RMG Delgado, LA Díaz-García, A De Amorim… - Astronomy & …, 2021 - aanda.org
The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will
soon start imaging thousands of square degrees of the northern sky with its unique set of 56 …