Search Publications

Estimate of the carbon footprint of astronomical research infrastructures
DOI: 10.1038/s41550-022-01612-3 Bibcode: 2022NatAs...6..503K

Hughes, Annie; Martin, Pierrick; Knödlseder, Jürgen +4 more

The carbon footprint of astronomical research is an increasingly topical issue with first estimates of research institute and national community footprints having recently been published. As these assessments have typically excluded the contribution of astronomical research infrastructures, we complement these studies by providing an estimate of t…

2022 Nature Astronomy
XMM-Newton 37
Intracluster Magnetic Filaments and an Encounter with a Radio Jet
DOI: 10.3847/1538-4357/ac7c76 Bibcode: 2022ApJ...935..168R

Brunetti, G.; Forman, W.; Jones, T. W. +6 more

Thin synchrotron-emitting filaments are increasingly seen in the intracluster medium (ICM). We present the first example of a direct interaction between a magnetic filament, a radio jet, and a dense ICM clump in the poor cluster A194. This enables the first exploration of the dynamics and possible histories of magnetic fields and cosmic rays in su…

2022 The Astrophysical Journal
XMM-Newton 37
BASS XXXII: Studying the Nuclear Millimeter-wave Continuum Emission of AGNs with ALMA at Scales ≲100-200 pc
DOI: 10.3847/1538-4357/ac8794 Bibcode: 2022ApJ...938...87K

Baba, Shunsuke; Imanishi, Masatoshi; Ueda, Yoshihiro +25 more

To understand the origin of nuclear (≲100 pc) millimeter-wave (mm-wave) continuum emission in active galactic nuclei (AGNs), we systematically analyzed subarcsecond resolution Band-6 (211-275 GHz) Atacama Large Millimeter/submillimeter Array data of 98 nearby AGNs (z < 0.05) from the 70 month Swift/BAT catalog. The sample, almost unbiased for o…

2022 The Astrophysical Journal
AKARI Herschel 37
VIA MACHINAE: Searching for stellar streams using unsupervised machine learning
DOI: 10.1093/mnras/stab3372 Bibcode: 2022MNRAS.509.5992S

Buckley, Matthew R.; Shih, David; Necib, Lina +1 more

We develop a new machine learning algorithm, VIA MACHINAE, to identify cold stellar streams in data from the Gaia telescope. VIA MACHINAE is based on ANODE, a general method that uses conditional density estimation and sideband interpolation to detect local overdensities in the data in a model agnostic way. By applying ANODE to the positions, prop…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 37
ALMA Observations of NGC 6334S. II. Subsonic and Transonic Narrow Filaments in a High-mass Star Formation Cloud
DOI: 10.3847/1538-4357/ac3df8 Bibcode: 2022ApJ...926..165L

Sanhueza, Patricio; Smith, Howard A.; Qiu, Keping +21 more

We present a study of narrow filaments toward a massive infrared dark cloud, NGC 6334S, using the Atacama Large Millimeter/submillimeter Array. Thirteen gas filaments are identified using the H13CO+ line, while a single continuum filament is revealed by the continuum emission. The filaments present a compact radial distributi…

2022 The Astrophysical Journal
Herschel 37
Chemo-kinematics of the Milky Way spiral arms and bar resonances: Connection to ridges and moving groups in the solar vicinity
DOI: 10.1051/0004-6361/202141836 Bibcode: 2022A&A...663A..38K

Gerhard, Ortwin; Khoperskov, Sergey

Making use of a new high-resolution spiral galaxy simulation as well as Gaia DR2 and EDR3 data complemented by chemical abundances from the Galah DR3, APOGEE DR16, and LAMOST DR5 surveys, we explore the possible link between the Milky Way (MW) spiral arms, (R, vϕ) ridges, and moving groups in local vR-vϕ space. We …

2022 Astronomy and Astrophysics
Gaia 37
Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency
DOI: 10.1093/mnras/stac1137 Bibcode: 2022MNRAS.513.3587Z

Zorotovic, Monica; Schreiber, MatthiasR

Common envelope evolution is a fundamental ingredient in our understanding of the formation of close binary stars containing compact objects that include the progenitors of type Ia supernovae, short gamma-ray bursts, and most stellar gravitational wave sources. To predict the outcome of common envelope evolution, we still rely to a large degree on…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 37
Radio footprints of a minor merger in the Shapley Supercluster: From supercluster down to galactic scales
DOI: 10.1051/0004-6361/202142048 Bibcode: 2022A&A...660A..81V

Di Gennaro, G.; Diego, J. M.; Rossetti, M. +29 more

Context. The Shapley Supercluster (⟨z⟩≈0.048) contains several tens of gravitationally bound clusters and groups, making it an ideal subject for radio studies of cluster mergers.
Aims: We used new high sensitivity radio observations to investigate the less energetic events of mass assembly in the Shapley Supercluster from supercluster down to…

2022 Astronomy and Astrophysics
XMM-Newton 37
First Peek with JWST/NIRCam Wide-field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O III]/Hα Emitter at z = 6.11
DOI: 10.3847/2041-8213/ac8938 Bibcode: 2022ApJ...936L...8S

Koekemoer, Anton M.; Pirzkal, Nor; Gennaro, Mario +16 more

We report the serendipitous discovery of an [O III] λ λ4959/5007 and Hα line emitter in the Epoch of Reionization (EoR) with the James Webb Space Telescope (JWST) commissioning data taken in the NIRCam wide-field slitless spectroscopy (WFSS) mode. Located ~55″ away from the flux calibrator P330-E, this galaxy exhibits bright [O III] λ λ4959/5007 a…

2022 The Astrophysical Journal
Gaia JWST 37
Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-sized Exoplanet HD 106315c
DOI: 10.3847/1538-3881/ac85be Bibcode: 2022AJ....164..124K

Gorjian, Varoujan; Fortney, Jonathan J.; Mikal-Evans, Thomas +27 more

We present a transmission spectrum for the Neptune-sized exoplanet HD 106315c from optical to infrared wavelengths based on transit observations from the Hubble Space Telescope/Wide Field Camera 3, K2, and Spitzer. The spectrum shows tentative evidence for a water absorption feature in the 1.1-1.7 µm wavelength range with a small amplitude o…

2022 The Astronomical Journal
eHST 37