Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
Gaia's binary star renaissance
K El-Badry - New Astronomy Reviews, 2024 - Elsevier
Stellar multiplicity is among the oldest and richest problems in astrophysics. Binary stars are
a cornerstone of stellar mass and radius measurements that underpin modern stellar …
a cornerstone of stellar mass and radius measurements that underpin modern stellar …
Gaia data release 3-summary of the content and survey properties
A Vallenari, AGA Brown, T Prusti… - Astronomy & …, 2023 - aanda.org
Context. We present the third data release of the European Space Agency's Gaia mission,
Gaia DR3. This release includes a large variety of new data products, notably a much …
Gaia DR3. This release includes a large variety of new data products, notably a much …
Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry
Context. Gravitational waves from black-hole (BH) merging events have revealed a
population of extra-galactic BHs residing in short-period binaries with masses that are …
population of extra-galactic BHs residing in short-period binaries with masses that are …
Gaia Data Release 3-Astrophysical parameters inference system (Apsis). I. Methods and content overview
OL Creevey, R Sordo, F Pailler, Y Frémat… - Astronomy & …, 2023 - aanda.org
Gaia Data Release 3 contains a wealth of new data products for the community.
Astrophysical parameters are a major component of this release, and were produced by the …
Astrophysical parameters are a major component of this release, and were produced by the …
Gaia data release 3-catalogue validation
C Babusiaux, C Fabricius, S Khanna… - Astronomy & …, 2023 - aanda.org
Context. The third Gaia data release (DR3) provides a wealth of new data products. The
early part of the release, Gaia EDR3, already provided the astrometric and photometric data …
early part of the release, Gaia EDR3, already provided the astrometric and photometric data …
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 …
Nitrogen enrichment and clustered star formation at the dawn of the Galaxy
V Belokurov, A Kravtsov - Monthly Notices of the Royal …, 2023 - academic.oup.com
Anomalously high nitrogen-to-oxygen abundance ratios [N/O] are observed in globular
clusters (GCs), among the field stars of the Milky Way (MW), and even in the gas in az≈ 11 …
clusters (GCs), among the field stars of the Milky Way (MW), and even in the gas in az≈ 11 …
Gaia Data Release 3-Summary of the variability processing and analysis
L Eyer, M Audard, B Holl, L Rimoldini… - Astronomy & …, 2023 - aanda.org
Context. Gaia has been in operations since 2014, and two full data releases (DR) have been
delivered so far: DR1 in 2016 and DR2 in 2018. The third Gaia data release expands from …
delivered so far: DR1 in 2016 and DR2 in 2018. The third Gaia data release expands from …
Gaia Data Release 3-Astrometric binary star processing
JL Halbwachs, D Pourbaix, F Arenou… - Astronomy & …, 2023 - aanda.org
Context. The Gaia Early Data Release 3 contained the positions, parallaxes, and proper
motions of 1.5 billion sources, some of which did not show a good fit to the 'single star'model …
motions of 1.5 billion sources, some of which did not show a good fit to the 'single star'model …
The initial mass function based on the full-sky 20 pc census of∼ 3600 stars and brown Dwarfs
JD Kirkpatrick, F Marocco, CR Gelino… - The Astrophysical …, 2024 - iopscience.iop.org
A complete accounting of nearby objects—from the highest-mass white dwarf progenitors
down to low-mass brown dwarfs—is now possible, thanks to an almost complete set of …
down to low-mass brown dwarfs—is now possible, thanks to an almost complete set of …