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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 …
220 million sources in the wavelength range 330 nm≤ λ≤ 1050 nm (XP spectra). Synthetic …
The state of the dark energy equation of state circa 2023
We critically examine the state of current constraints on the dark energy (DE) equation of
state (EoS) w. Our study is motivated by the observation that, while broadly consistent with …
state (EoS) w. Our study is motivated by the observation that, while broadly consistent with …
The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
S **, 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 …
for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2 …
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 …
dwarfs (WDs) that, together with the excellent photometry and astrometry, represent an …
The BINGO project-I. Baryon acoustic oscillations from integrated neutral gas observations
Context. Observations of the redshifted 21-cm line of neutral hydrogen (HI) are a new and
powerful window of observation that offers us the possibility to map the spatial distribution of …
powerful window of observation that offers us the possibility to map the spatial distribution of …
HETDEX Public Source Catalog 1: 220 K Sources Including Over 50 K Lyα Emitters from an Untargeted Wide-area Spectroscopic Survey
EM Cooper, K Gebhardt, D Davis… - The Astrophysical …, 2023 - iopscience.iop.org
We present the first publicly released catalog of sources obtained from the Hobby-Eberly
Telescope Dark Energy Experiment (HETDEX). HETDEX is an integral field spectroscopic …
Telescope Dark Energy Experiment (HETDEX). HETDEX is an integral field spectroscopic …
Euclid preparation-XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis
S Ilić, N Aghanim, C Baccigalupi… - Astronomy & …, 2022 - aanda.org
The combination and cross-correlation of the upcoming Euclid data with cosmic microwave
background (CMB) measurements is a source of great expectation since it will provide the …
background (CMB) measurements is a source of great expectation since it will provide the …
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 …
survey of∼ 9300 deg2 in the southern sky in a 12-band photometric system. This paper …
Low-redshift estimates of the absolute scale of baryon acoustic oscillations
Measurements of the characteristic length scale rs of the baryon acoustic oscillations (BAO)
provide a robust determination of the distance-redshift relation. Currently, the best (sub-per …
provide a robust determination of the distance-redshift relation. Currently, the best (sub-per …
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 …
resolution of R∼ 60) in order to demonstrate the scientific potential of the Javalambre …