Search Publications

NOEMA redshift measurements of bright Herschel galaxies
DOI: 10.1051/0004-6361/201936988 Bibcode: 2020A&A...635A...7N

Berta, S.; Omont, A.; Lagache, G. +31 more

Using the IRAM NOrthern Extended Millimeter Array (NOEMA), we conducted a program to measure redshifts for 13 bright galaxies detected in the Herschel Astrophysical Large Area Survey with S500 µm ≥ 80 mJy. We report reliable spectroscopic redshifts for 12 individual sources, which are derived from scans of the 3 and 2 mm bands, co…

2020 Astronomy and Astrophysics
Herschel 41
The Breakthrough Listen Search for Intelligent Life: A 3.95-8.00 GHz Search for Radio Technosignatures in the Restricted Earth Transit Zone
DOI: 10.3847/1538-3881/ab9361 Bibcode: 2020AJ....160...29S

Kalas, Paul; Gajjar, Vishal; Isaacson, Howard +5 more

We report on a search for artificial narrowband signals of 20 stars within the restricted Earth Transit Zone (rETZ) as a part of the ten-year Breakthrough Listen (BL) search for extraterrestrial intelligence (ETI). The rETZ is the region of the sky from which an observer would see Earth transit the Sun with an impact parameter of less than 0.5. Th…

2020 The Astronomical Journal
Gaia 41
NuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario
DOI: 10.1051/0004-6361/201936486 Bibcode: 2020A&A...634A..92U

Bianchi, S.; Cappi, M.; Ponti, G. +11 more


Aims: We test the two-corona accretion scenario for active galactic nuclei in the case of the "bare" Seyfert 1 galaxy HE 1143-1810.
Methods: We perform a detailed study of the broad-band UV-X-ray spectral properties and of the short-term variability of HE 1143-1810. We present results of a joint XMM-Newton and NuSTAR monitoring of the so…

2020 Astronomy and Astrophysics
XMM-Newton 41
Monitoring of the radio galaxy M 87 during a low-emission state from 2012 to 2015 with MAGIC
DOI: 10.1093/mnras/staa014 Bibcode: 2020MNRAS.492.5354M

Maraschi, L.; Covino, S.; Antonelli, L. A. +186 more

M 87 is one of the closest (z = 0.004 36) extragalactic sources emitting at very high energies (VHE, E > 100 GeV). The aim of this work is to locate the region of the VHE gamma-ray emission and to describe the observed broad-band spectral energy distribution (SED) during the low VHE gamma-ray state. The data from M 87 collected between 2012 and…

2020 Monthly Notices of the Royal Astronomical Society
eHST 41
The Fornax 3D project: Non-linear colour-metallicity relation of globular clusters
DOI: 10.1051/0004-6361/202037686 Bibcode: 2020A&A...637A..27F

Viaene, S.; Hilker, M.; Pinna, F. +15 more

Globular cluster (GC) systems of massive galaxies often show a bimodal colour distribution. This has been interpreted as a metallicity bimodality, created by a two-stage galaxy formation where the red, metal-rich GCs were formed in the parent halo and the blue metal-poor GCs were accreted. This interpretation, however, crucially depends on the ass…

2020 Astronomy and Astrophysics
eHST 41
Origins of Type Ibn SNe 2006jc/2015G in interacting binaries and implications for pre-SN eruptions
DOI: 10.1093/mnras/stz3431 Bibcode: 2020MNRAS.491.6000S

Sun, Ning-Chen; Crowther, Paul A.; Podsiadlowski, Philipp +2 more

Type Ibn supernovae (SNe Ibn) are intriguing stellar explosions whose spectra exhibit narrow helium lines with little hydrogen. They trace the presence of circumstellar material (CSM) formed via pre-SN eruptions of their stripped-envelope progenitors. Early work has generally assumed that SNe Ibn come from massive Wolf-Rayet (WR) stars via single-…

2020 Monthly Notices of the Royal Astronomical Society
eHST 41
A Catalog of M-dwarf Flares with ASAS-SN
DOI: 10.3847/1538-4357/ab793a Bibcode: 2020ApJ...892..144R

Holoien, Thomas W. -S.; Auchettl, Katie; Kochanek, Christopher S. +5 more

We analyzed the light curves of 1376 early-to-late, nearby M dwarfs to search for white-light flares using photometry from the All-Sky Automated Survey for Supernovae. We identified 480 M dwarfs with at least one potential flare employing a simple statistical algorithm that searches for sudden increases in V-band flux. After more detailed evaluati…

2020 The Astrophysical Journal
Gaia 41
First direct observation of a torsional Alfvén oscillation at coronal heights
DOI: 10.1051/0004-6361/201937144 Bibcode: 2020A&A...633L...6K

Kohutova, P.; Verwichte, E.; Froment, C.

Context. Torsional Alfvén waves are promising candidates for the transport of energy across different layers of the solar atmosphere. They have been predicted theoretically for decades. Previous detections of Alfvén waves so far have however mostly relied on indirect signatures.
Aims: We present the first direct observational evidence of a fu…

2020 Astronomy and Astrophysics
IRIS 40
Dissecting the Phase Space Snail Shell
DOI: 10.3847/1538-4357/ab6b21 Bibcode: 2020ApJ...890...85L

Shen, Juntai; Li, Zhao-Yu

The ongoing vertical phase-mixing, manifesting itself as a snail shell in the $Z-{V}_{Z}$ phase space, has been discovered with Gaia DR2 data. To better understand the origin and properties of the phase-mixing process, we study the vertical phase-mixing signatures in arches (including the classical "moving groups") of the ${V}_{R}-{V}_{\phi }$ pha…

2020 The Astrophysical Journal
Gaia 40
AstroSat detection of Lyman continuum emission from a z = 1.42 galaxy
DOI: 10.1038/s41550-020-1173-5 Bibcode: 2020NatAs...4.1185S

Verhamme, Anne; Inoue, Akio K.; Schaerer, Daniel +10 more

One of the outstanding problems of current observational cosmology is to understand the nature of sources that produced the bulk of the ionizing radiation after the Cosmic Dark Age. Direct detection of these reionization sources1 is practically infeasible at high redshift (z) due to the steep decline of intergalactic medium transmission…

2020 Nature Astronomy
eHST 40