Search Publications

Starbursts in and out of the star-formation main sequence
DOI: 10.1051/0004-6361/201732370 Bibcode: 2018A&A...616A.110E

Daddi, E.; Elbaz, D.; Franco, M. +13 more


Aims: We use high-resolution continuum images obtained with the Atacama Large Millimeter Array (ALMA) to probe the surface density of star formation in z ~ 2 galaxies and study the different physical properties between galaxies within and above the star-formation main sequence of galaxies.
Methods: We use ALMA images at 870 µm with…

2018 Astronomy and Astrophysics
AKARI Herschel eHST 166
Rotation of Low-mass Stars in Upper Scorpius and ρ Ophiuchus with K2
DOI: 10.3847/1538-3881/aab605 Bibcode: 2018AJ....155..196R

Rebull, L. M.; Stauffer, J. R.; Cody, A. M. +3 more

We present an analysis of K2 light curves (LCs) for candidate members of the young Upper Sco (USco) association (∼8 Myr) and the neighboring ρ Oph embedded cluster (∼1 Myr). We establish ∼1300 stars as probable members, ∼80% of which are periodic. The phased LCs have a variety of shapes which can be attributed to physical causes ranging from stell…

2018 The Astronomical Journal
AKARI Gaia 134
The State-of-Play of Anomalous Microwave Emission (AME) research
DOI: 10.1016/j.newar.2018.02.001 Bibcode: 2018NewAR..80....1D

Leahy, J. P.; Paladini, R.; Poidevin, F. +30 more

Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10-60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997. Since then, AME has been observed by a range of experiments and in a variety of environments. AME is spatially correlated wit…

2018 New Astronomy Reviews
AKARI 97
Orbital properties of binary post-AGB stars
DOI: 10.1051/0004-6361/201833816 Bibcode: 2018A&A...620A..85O

Manick, Rajeev; Van Winckel, Hans; Kamath, Devika +5 more

Binary post-asymptotic giant branch (post-AGB) stars are thought to be the products of a strong but poorly understood interaction during the AGB phase. The aim of this contribution is to update the orbital elements of a sample of galactic post-AGB binaries observed in a long-term radial-velocity monitoring campaign by analysing these systems in a …

2018 Astronomy and Astrophysics
AKARI Gaia Herschel 86
Planck's view on the spectrum of the Sunyaev-Zeldovich effect
DOI: 10.1093/mnras/sty327 Bibcode: 2018MNRAS.476.3360E

Bertoldi, Frank; Chluba, Jens; Basu, Kaustuv +1 more

We present a detailed analysis of the stacked frequency spectrum of a large sample of galaxy clusters using Planck data, together with auxiliary data from the AKARI and IRAS missions. Our primary goal is to search for the imprint of relativistic corrections to the thermal Sunyaev-Zeldovich effect (tSZ) spectrum, which allow to measure the temperat…

2018 Monthly Notices of the Royal Astronomical Society
AKARI Planck 68
The Spectrum of the Universe
DOI: 10.1177/0003702818767133 Bibcode: 2018ApSpe..72..663H

Hill, Ryley; Masui, Kiyoshi W.; Scott, Douglas

The cosmic background (CB) radiation, encompassing the sum of emission from all sources outside our own Milky Way galaxy across the entire electromagnetic spectrum, is a fundamental phenomenon in observational cosmology. Many experiments have been conceived to measure it (or its constituents) since the extragalactic Universe was first discovered; …

2018 Applied Spectroscopy
AKARI INTEGRAL ISO Planck 63
Polar Dust, Nuclear Obscuration, and IR SED Diversity in Type-1 AGNs
DOI: 10.3847/1538-4357/aae075 Bibcode: 2018ApJ...866...92L

Lyu, Jianwei; Rieke, George H.

Despite the hypothesized similar face-on viewing angles, the infrared emission of type-1 active galactic nuclei (AGNs) has diverse spectral energy distribution (SED) shapes that deviate substantially from the well-characterized quasar templates. Motivated by the commonly seen UV-optical obscuration and the discovery of parsec-scale mid-IR polar du…

2018 The Astrophysical Journal
AKARI 61
The second-closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environment
DOI: 10.1051/0004-6361/201629942 Bibcode: 2018A&A...616A.169M

Gentile, Gianfranco; Paragi, Zsolt; Fynbo, Johan P. U. +17 more

We report the detection of the radio afterglow of a long gamma-ray burst (GRB) 111005A at 5-345 GHz, including very long baseline interferometry observations with a positional error of 0.2 mas. The afterglow position is coincident with the disc of a galaxy ESO 58049 at z = 0.01326 (∼1″ from its centre), which makes GRB 111005A the second-closest G…

2018 Astronomy and Astrophysics
AKARI eHST 58
New polarimetric and spectroscopic evidence of anomalous enrichment in spinel-bearing calcium-aluminium-rich inclusions among L-type asteroids
DOI: 10.1016/j.icarus.2017.12.026 Bibcode: 2018Icar..304...31D

Surdej, J.; Tanga, P.; Carry, B. +14 more

Asteroids can be classified into several groups based on their spectral reflectance. Among these groups, the one belonging to the L-class in the taxonomic classification based on visible and near-infrared spectra exhibit several peculiar properties. First, their near-infrared spectrum is characterized by a strong absorption band interpreted as the…

2018 Icarus
AKARI 43
The AKARI IRC asteroid flux catalogue: updated diameters and albedos
DOI: 10.1051/0004-6361/201731806 Bibcode: 2018A&A...612A..85A

Müller, T. G.; Usui, F.; Alí-Lagoa, V. +1 more

The AKARI IRC all-sky survey provided more than twenty thousand thermal infrared observations of over five thousand asteroids. Diameters and albedos were obtained by fitting an empirically calibrated version of the standard thermal model to these data. After the publication of the flux catalogue in October 2016, our aim here is to present the AKAR…

2018 Astronomy and Astrophysics
AKARI 40