Search Publications

VLT/FLAMES high-resolution chemical abundances in Sculptor: a textbook dwarf spheroidal galaxy
DOI: 10.1051/0004-6361/201833950 Bibcode: 2019A&A...626A..15H

Spite, M.; Skúladóttir, Á.; Jablonka, P. +12 more

We present detailed chemical abundances for 99 red-giant branch stars in the centre of the Sculptor dwarf spheroidal galaxy, which have been obtained from high-resolution VLT/FLAMES spectroscopy. The abundances of Li, Na, α-elements (O, Mg, Si, Ca Ti), iron-peak elements (Sc, Cr, Fe, Co, Ni, Zn), and r- and s-process elements (Ba, La, Nd, Eu) were…

2019 Astronomy and Astrophysics
Gaia 103
First Gaia Dynamics of the Andromeda System: DR2 Proper Motions, Orbits, and Rotation of M31 and M33
DOI: 10.3847/1538-4357/ab001b Bibcode: 2019ApJ...872...24V

van der Marel, Roeland P.; Watkins, Laura L.; Fardal, Mark A. +5 more

The 3D velocities of M31 and M33 are important for understanding the evolution and cosmological context of the Local Group. Their most massive stars are detected by Gaia, and we use Data Release 2 (DR2) to determine the galaxy proper motions (PMs). We select galaxy members based on, e.g., parallax, PM, color-magnitude diagram location, and local s…

2019 The Astrophysical Journal
Gaia eHST 103
SDSS-IV MaStar: A Large and Comprehensive Empirical Stellar Spectral Library—First Release
DOI: 10.3847/1538-4357/ab3ebc Bibcode: 2019ApJ...883..175Y

Zhao, Gang; Bizyaev, Dmitry; Kinemuchi, Karen +45 more

We present the first release of the MaNGA Stellar Library (MaStar), which is a large, well-calibrated, high-quality empirical library covering the wavelength range 3622-10354 Å at a resolving power of R ∼ 1800. The spectra were obtained using the same instrument as used by the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) project, by…

2019 The Astrophysical Journal
Gaia 103
Cosmological Constraints from Multiple Probes in the Dark Energy Survey
DOI: 10.1103/PhysRevLett.122.171301 Bibcode: 2019PhRvL.122q1301A

Bacon, D.; Bechtol, K.; Challis, P. +161 more

The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically confirmed type Ia supernova light curves, the baryon acoustic oscillation feature, weak gravitational lensing, and galaxy cluster…

2019 Physical Review Letters
eHST 103
SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ∼ 6-7: Strong Associations of Dusty Star-forming Galaxies
DOI: 10.3847/1538-4357/ab2cd5 Bibcode: 2019ApJ...883..142H

Ono, Yoshiaki; Ouchi, Masami; Goto, Tomotsugu +32 more

We have obtained three-dimensional maps of the universe in ∼200 × 200 × 80 comoving Mpc3 (cMpc3) volumes each at z = 5.7 and 6.6 based on a spectroscopic sample of 179 galaxies that achieves ≳80% completeness down to the Lyα luminosity of {log}({L}Lyα }/[{erg} {{{s}}}-1])=43.0, based on our Keck and Gemi…

2019 The Astrophysical Journal
Herschel 102
Resolved Young Binary Systems and Their Disks
DOI: 10.3847/1538-4357/aaff6a Bibcode: 2019ApJ...872..158A

Jensen, Eric L. N.; Carpenter, John; Ricci, Luca +4 more

We have conducted a survey of young single and multiple systems in the Taurus-Auriga star-forming region with the Atacama Large Millimeter Array (ALMA), substantially improving both the spatial resolution and sensitivity with which individual protoplanetary disks in these systems have been observed. These ALMA observations can resolve binary separ…

2019 The Astrophysical Journal
Gaia 102
No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations
DOI: 10.1038/s41586-019-1096-4 Bibcode: 2019Natur.568..517K

Montmessin, Franck; Belyaev, Denis A.; Fedorova, Anna A. +123 more

The detection of methane on Mars has been interpreted as indicating that geochemical or biotic activities could persist on Mars today1. A number of different measurements of methane show evidence of transient, locally elevated methane concentrations and seasonal variations in background methane concentrations2-5. These measur…

2019 Nature
ExoMars-16 102
On the ridges, undulations, and streams in Gaia DR2: linking the topography of phase space to the orbital structure of an N-body bar
DOI: 10.1093/mnras/stz1875 Bibcode: 2019MNRAS.488.3324F

White, S. D. M.; Katz, D.; Fragkoudi, F. +7 more

We explore the origin of phase-space substructures revealed by the second Gaia data release in the disc of the Milky Way, such as the ridges in the Vϕ-r plane, the undulations in the Vϕ-r-Vr space and the streams in the Vϕ-Vr plane. We use a collisionless N-body simulation with cospatial thin …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 101
A New Class of Changing-look LINERs
DOI: 10.3847/1538-4357/ab3a38 Bibcode: 2019ApJ...883...31F

Cenko, S. Bradley; Duev, Dmitry A.; Rusholme, Ben +28 more

We report the discovery of six active galactic nuclei (AGNs) caught “turning on” during the first nine months of the Zwicky Transient Facility (ZTF) survey. The host galaxies were classified as low-ionization nuclear emission-line region galaxies (LINERs) by weak narrow forbidden line emission in their archival SDSS spectra, and detected by ZTF as…

2019 The Astrophysical Journal
XMM-Newton eHST 101
Tracing the formation of the Milky Way through ultra metal-poor stars
DOI: 10.1093/mnras/stz043 Bibcode: 2019MNRAS.484.2166S

Fouesneau, Morgan; Sestito, Federico; Navarro, Julio F. +11 more

We use Gaia DR2 astrometric and photometric data, published radial velocities and MESA models to infer distances, orbits, surface gravities, and effective temperatures for all ultra metal-poor stars ([Fe/H] < -4.0 dex) available in the literature. Assuming that these stars are old (> 11 Gyr) and that they are expected to belong to the Milky …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 100