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The southern stellar stream spectroscopic survey (S5): Overview, target selection, data reduction, validation, and early science
We introduce the southern stellar stream spectroscopy survey (S 5), an on-going program to
map the kinematics and chemistry of stellar streams in the southern hemisphere. The initial …
map the kinematics and chemistry of stellar streams in the southern hemisphere. The initial …
The GALAH+ survey: Third data release
The ensemble of chemical element abundance measurements for stars, along with precision
distances and orbit properties, provides high-dimensional data to study the evolution of the …
distances and orbit properties, provides high-dimensional data to study the evolution of the …
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 …
GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with∼ 4,000,000 Galaxies at z∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and …
We present new measurements of rest-UV luminosity functions and angular correlation
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
The target-selection pipeline for the dark energy spectroscopic instrument
AD Myers, J Moustakas, S Bailey… - The Astronomical …, 2023 - iopscience.iop.org
Abstract In 2021 May, the Dark Energy Spectroscopic Instrument (DESI) began a 5 yr survey
of approximately 50 million total extragalactic and Galactic targets. The primary DESI dark …
of approximately 50 million total extragalactic and Galactic targets. The primary DESI dark …
S 5: Probing the Milky Way and Magellanic Clouds potentials with the 6D map of the Orphan–Chenab stream
We present a 6D map of the Orphan–Chenab (OC) stream by combining the data from
Southern Stellar Stream Spectroscopic Survey (S 5) and Gaia. We reconstruct the proper …
Southern Stellar Stream Spectroscopic Survey (S 5) and Gaia. We reconstruct the proper …
The GALAH Survey: second data release
ABSTRACT The Galactic Archaeology with HERMES (GALAH) survey is a large-scale stellar
spectroscopic survey of the Milky Way, designed to deliver complementary chemical …
spectroscopic survey of the Milky Way, designed to deliver complementary chemical …
The GALAH survey: scientific motivation
GM De Silva, KC Freeman… - Monthly Notices of …, 2015 - academic.oup.com
Abstract The Galactic Archaeology with HERMES (GALAH) survey is a large high-resolution
spectroscopic survey using the newly commissioned High Efficiency and Resolution Multi …
spectroscopic survey using the newly commissioned High Efficiency and Resolution Multi …
Measuring the mass of the Large Magellanic Cloud with stellar streams observed by S 5
Stellar streams are excellent probes of the underlying gravitational potential in which they
evolve. In this work, we fit dynamical models to five streams in the Southern Galactic …
evolve. In this work, we fit dynamical models to five streams in the Southern Galactic …
The Pristine Inner Galaxy Survey–VIII. Characterizing the orbital properties of the ancient, very metal-poor inner Milky Way
A Ardern-Arentsen, G Monari… - Monthly Notices of …, 2024 - academic.oup.com
The oldest stars in the Milky Way (born in the first few billion years) are expected to have a
high density in the inner few kpc, spatially overlap** with the Galactic bulge. We use …
high density in the inner few kpc, spatially overlap** with the Galactic bulge. We use …