Search Publications

Kinematic properties of white dwarfs. Galactic orbital parameters and age-velocity dispersion relation
DOI: 10.1051/0004-6361/202141837 Bibcode: 2022A&A...658A..22R

Rebassa-Mansergas, Alberto; Raddi, Roberto; Torres, Santiago +9 more

Context. Kinematic and chemical tagging of stellar populations have both revealed much information on the past and recent history of the Milky Way, including its formation history, merger events, and mixing of populations across the Galactic disk and halo.
Aims: We present the first detailed 3D kinematic analysis of a sample of 3133 white dwa…

2022 Astronomy and Astrophysics
Gaia 28
AGN Selection Methods Have Profound Impacts on the Distributions of Host-galaxy Properties
DOI: 10.3847/1538-4357/ac3837 Bibcode: 2022ApJ...925...74J

Giavalisco, Mauro; Kirkpatrick, Allison; Ji, Zhiyuan +4 more

We present a comparative study of X-ray and IR active galactic nuclei (AGNs) at z ≈ 2 to highlight the important AGN selection effects on the distributions of host-galaxy properties. Compared with non-AGN star-forming galaxies (SFGs) on the main sequence, X-ray AGNs have similar median star formation (SF) properties, but their incidence (q AG…

2022 The Astrophysical Journal
eHST 28
Dynamical state of galaxy clusters evaluated from X-ray images
DOI: 10.1093/mnras/stac1037 Bibcode: 2022MNRAS.513.3013Y

Yuan, Z. S.; Han, J. L.; Wen, Z. L.

X-ray images of galaxy clusters often show disturbed structures that are indications of cluster mergers. To complement our previous work on the dynamical state of 964 clusters observed by Chandra, we process the X-ray images for 1308 clusters from XMM-Newton archival data, together with the images of 22 clusters newly released by Chandra, and we e…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 28
The detailed chemical abundance patterns of accreted halo stars from the optical to infrared
DOI: 10.1093/mnras/stac518 Bibcode: 2022MNRAS.513.1557C

Hawkins, Keith; Lucey, Madeline; Jofré, Paula +3 more

Understanding the assembly of our Galaxy requires us to also characterize the systems that helped build it. In this work, we accomplish this by exploring the chemistry of accreted halo stars from Gaia-Enceladus/Gaia-Sausage (GES) selected in the infrared from the Apache Point Observatory Galactic Evolution Experiment (APOGEE) Data Release 16. We u…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 28
An Atmospheric Retrieval of the Brown Dwarf Gliese 229B
DOI: 10.3847/1538-4357/ac9cc9 Bibcode: 2022ApJ...940..164C

Faherty, Jacqueline K.; Calamari, Emily; Burningham, Ben +6 more

We present results from an atmospheric retrieval analysis of Gl 229B using the Brewster retrieval code. We find the best fit model to be cloud-free, consistent with the T dwarf retrieval work of Line et al.; Zalesky et al. and Gonzales et al. Fundamental parameters (mass, radius, log(L Bol /L Sun), log(g)) determined from our…

2022 The Astrophysical Journal
Gaia 28
The CARMENES search for exoplanets around M dwarfs. Benchmarking the impact of activity in high-precision radial velocity measurements
DOI: 10.1051/0004-6361/202141880 Bibcode: 2022A&A...663A..27J

Amado, P. J.; Caballero, J. A.; Czesla, S. +17 more

Context. Current exoplanet surveys using the radial velocity (RV) technique are targeting M dwarfs because any habitable zone terrestrial-mass planets will induce a high RV and orbit on shorter periods than for more massive stars. One of the main caveats is that M dwarfs show a wide range of activity levels from inactive to very active, which can …

2022 Astronomy and Astrophysics
Gaia 28
Dark matter in galaxy clusters: Parametric strong-lensing approach
DOI: 10.1051/0004-6361/202243278 Bibcode: 2022A&A...664A..90L

Jullo, Eric; Limousin, Marceau; Beauchesne, Benjamin

We present a parametric strong-lensing analysis of three massive galaxy clusters for which Hubble Space Telescope imaging is available, as well as spectroscopy of multiply imaged systems and galaxy cluster members. Our aim is to probe the inner shape of dark matter haloes, in particular the existence of a core. We adopted the following working hyp…

2022 Astronomy and Astrophysics
eHST 28
Surface and interior meridional circulation in the Sun
DOI: 10.1007/s41116-022-00034-7 Bibcode: 2022LRSP...19....3H

Hanasoge, Shravan M.

Solar meridional circulation is an axisymmetric flow system, extending from the equator to the poles (20 m/s at the surface, 1% of the mean solar rotation rate), plunging inwards and su…

2022 Living Reviews in Solar Physics
SOHO 28
The AGEL Survey: Spectroscopic Confirmation of Strong Gravitational Lenses in the DES and DECaLS Fields Selected Using Convolutional Neural Networks
DOI: 10.3847/1538-3881/ac7da2 Bibcode: 2022AJ....164..148T

Kewley, Lisa J.; Harshan, Anishya; Kacprzak, Glenn G. +13 more

We present spectroscopic confirmation of candidate strong gravitational lenses using the Keck Observatory and Very Large Telescope as part of our ASTRO 3D Galaxy Evolution with Lenses (AGEL) survey. We confirm that (1) search methods using convolutional neural networks (CNNs) with visual inspection successfully identify strong gravitational lenses…

2022 The Astronomical Journal
eHST 28
A New Iron Emission Template for Active Galactic Nuclei. I. Optical Template for the Hβ Region
DOI: 10.3847/1538-4365/ac3f3e Bibcode: 2022ApJS..258...38P

Laor, Ari; Ho, Luis C.; Barth, Aaron J. +1 more

We present a new empirical template for iron emission in active galactic nuclei (AGNs) covering the 4000-5600 Å range. The new template is based on a spectrum of the narrow-line Seyfert 1 galaxy Mrk 493 obtained with the Hubble Space Telescope. In comparison with the canonical iron template object I Zw 1, Mrk 493 has narrower broad-line widths, lo…

2022 The Astrophysical Journal Supplement Series
eHST 28