Search Publications

ALMA + VLT observations of a damped Lyman-α absorbing galaxy: massive, wide CO emission, gas-rich but with very low SFR
DOI: 10.1093/mnras/stx2845 Bibcode: 2018MNRAS.474.4039M

Fynbo, J. P. U.; Dessauges-Zavadsky, M.; Christensen, L. +7 more

We are undertaking an Atacama Large Millimeter Array survey of molecular gas in galaxies selected for their strong H I absorption, so-called damped Lyα absorber (DLA)/sub-DLA galaxies. Here, we report CO(2-1) detection from a DLA galaxy at z = 0.716. We also present optical and near-infrared (NIR) spectra of the galaxy revealing [O II], Hα, and [N…

2018 Monthly Notices of the Royal Astronomical Society
Herschel eHST 29
A Galaxy Redshift Survey Near HST/COS AGN Sight Lines
DOI: 10.3847/1538-4365/aac727 Bibcode: 2018ApJS..237...11K

Savage, Blair D.; Shull, J. Michael; Danforth, Charles W. +8 more

To establish the connection between galaxies and UV-detected absorption systems in the local universe, a deep (g ≤ 20) and wide (∼20‧ radius) galaxy redshift survey is presented around 47 sight lines to UV-bright AGNs observed by the Cosmic Origins Spectrograph (COS). Specific COS science team papers have used this survey to connect absorbers to g…

2018 The Astrophysical Journal Supplement Series
eHST 29
On the Rate and on the Gravitational Wave Emission of Short and Long GRBs
DOI: 10.3847/1538-4357/aabee4 Bibcode: 2018ApJ...859...30R

Rodriguez, J.; Wang, Y.; Barres de Almeida, U. +13 more

On the ground of the large number of gamma-ray bursts (GRBs) detected with cosmological redshift, we classified GRBs in seven subclasses, all with binary progenitors which emit gravitational waves (GWs). Each binary is composed of combinations of carbon-oxygen cores (COcore), neutron stars (NSs), black holes (BHs), and white dwarfs (WDs…

2018 The Astrophysical Journal
INTEGRAL 29
Towards a census of high-redshift dusty galaxies with Herschel. A selection of "500 µm-risers"
DOI: 10.1051/0004-6361/201731888 Bibcode: 2018A&A...614A..33D

Buat, V.; Pappalardo, C.; Alvarez-Marquez, J. +6 more

Context. Over the last decade a large number of dusty star-forming galaxies has been discovered up to redshift z = 2 - 3 and recent studies have attempted to push the highly confused Herschel SPIRE surveys beyond that distance. To search for z ≥ 4 galaxies they often consider the sources with fluxes rising from 250 µm to 500 µm (so-cal…

2018 Astronomy and Astrophysics
Herschel 29
RELICS: Strong Lensing Analysis of the Galaxy Clusters Abell S295, Abell 697, MACS J0025.4-1222, and MACS J0159.8-0849
DOI: 10.3847/1538-4357/aad2d3 Bibcode: 2018ApJ...863..145C

Ouchi, Masami; Mahler, Guillaume; Bradač, Maruša +37 more

We present a strong lensing analysis of four massive galaxy clusters imaged with the Hubble Space Telescope in the Reionization Lensing Cluster Survey. We use a light-traces-mass technique to uncover sets of multiple images and constrain the mass distribution of the clusters. These mass models are the first published for Abell S295 and MACS J0159.…

2018 The Astrophysical Journal
eHST 29
The supermassive black hole coincident with the luminous transient ASASSN-15lh
DOI: 10.1051/0004-6361/201731773 Bibcode: 2018A&A...610A..14K

Kim, S.; Krühler, T.; Nicuesa Guelbenzu, A. +11 more

The progenitors of astronomical transients are linked to a specific stellar population and galactic environment, and observing their host galaxies hence constrains the physical nature of the transient itself. Here, we use imaging from the Hubble Space Telescope, and spatially resolved, medium-resolution spectroscopy from the Very Large Telescope o…

2018 Astronomy and Astrophysics
Gaia eHST 29
On the Dynamic Nature of a Quiescent Prominence Observed by IRIS and MSDP Spectrographs
DOI: 10.3847/1538-4357/aada08 Bibcode: 2018ApJ...865..123R

Schmieder, Brigitte; Chen, Yao; Labrosse, Nicolas +4 more

Quiescent solar prominences are generally considered to have a stable large-scale structure. However, they consist of multiple small-scale structures that are often significantly dynamic. To understand the nature of prominence plasma dynamics we use the high spatial, temporal, and spectral resolution observations obtained by Interface Region Imagi…

2018 The Astrophysical Journal
IRIS 29
The Temporal Development of Dust Formation and Destruction in Nova Sagittarii 2015#2 (V5668 SGR): A Panchromatic Study
DOI: 10.3847/1538-4357/aaba81 Bibcode: 2018ApJ...858...78G

Krautter, Joachim; Gehrz, R. D.; Shore, S. N. +15 more

We present 5-28 µm SOFIA FORECAST spectroscopy complemented by panchromatic X-ray through infrared observations of the CO nova V5668 Sgr documenting the formation and destruction of dust during ∼500 days following outburst. Dust condensation commenced by 82 days after outburst at a temperature of ∼1090 K. The condensation temperature indicat…

2018 The Astrophysical Journal
eHST 29
Anomalies in Time Delays of Lensed Gravitational Waves and Dark Matter Substructures
DOI: 10.3847/1538-4357/aae30f Bibcode: 2018ApJ...867...69L

Ding, Xuheng; Biesiada, Marek; Zhu, Zong-Hong +2 more

Cold dark matter scenarios of hierarchical large-scale structure formation predict the existence of abundant subhalos around large galaxies. However, the number of observed dwarf galaxies is far from this theoretical prediction, suggesting that most of the subhalos could be dark or quite faint. Gravitational lensing is a powerful tool to probe the…

2018 The Astrophysical Journal
eHST 29
Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps
DOI: 10.1088/1475-7516/2018/04/020 Bibcode: 2018JCAP...04..020D

Boulanger, F.; Ashdown, M.; Banday, A. J. +124 more

We discuss the potential of a next generation space-borne Cosmic Microwave Background (CMB) experiment for studies of extragalactic sources. Our analysis has particular bearing on the definition of the future space project, CORE, that has been submitted in response to ESA's call for a Medium-size mission opportunity as the successor of the Planck …

2018 Journal of Cosmology and Astroparticle Physics
Planck 29