Search Publications

UV slope of z ∼ 3 bright (L > L*) Lyman-break galaxies in the COSMOS field
DOI: 10.1051/0004-6361/201834442 Bibcode: 2019A&A...626A..45P

Castellano, M.; Pentericci, L.; Santini, P. +7 more

Context. The analysis of the UV slope β of Lyman-break galaxies (LBG) at different luminosities and redshifts is fundamental for understanding their physical properties, and in particular, their dust extinction.
Aims: We analyse a unique sample of 517 bright (L > L*) LBGs at redshift z ∼ 3 in order to characterise the distributi…

2019 Astronomy and Astrophysics
eHST 5
Tiny grains shining bright in the gaps of Herbig Ae transitional discs
DOI: 10.1093/mnras/stz1061 Bibcode: 2019MNRAS.486.3721B

Monnier, John D.; Kraus, Stefan; Federrath, Christoph +7 more

This work presents a study of two Herbig Ae transitional discs, Oph IRS 48 and HD 169142; which both have reported rings in their dust density distributions. We use Keck-II/NIRC2 adaptive optics imaging observations in the L' filter (3.8 µm) to probe the regions of these discs inwards of {∼ }20 au from the star. We introduce our method for i…

2019 Monthly Notices of the Royal Astronomical Society
Gaia IUE 5
Galaxy rotation curve from classical Cepheids
DOI: 10.1002/asna.201913655 Bibcode: 2019AN....340..787G

Gnaciński, Piotr

The galaxy rotation curve is usually assumed to be flat. However, some galaxies have rotation curves that are lower than the flat rotation curve. In our galaxy, the Keplerian rotation of interstellar clouds in the galactic longitude l = 135° was observed. We use a kinematic approach to derive the rotational velocity of classical Cepheids. The rota…

2019 Astronomische Nachrichten
Gaia 5
Revised wavelength and spectral response calibrations for AKARI near-infrared grism spectroscopy: Post-cryogenic phase
DOI: 10.1093/pasj/psy131 Bibcode: 2019PASJ...71....2B

Nakagawa, Takao; Baba, Shunsuke; Onaka, Takashi +2 more

We present a new calibration for the second-order light contamination in the near-infrared grism spectroscopy with the Infrared Camera aboard AKARI, specifically for the post-cryogenic phase of the satellite (Phase 3). Following our previous work on the cryogenic phase (Phases 1 and 2), the wavelength and spectral response calibrations were revise…

2019 Publications of the Astronomical Society of Japan
AKARI 5
Active galactic nucleus selection in the AKARI NEP-Deep field with the fuzzy support vector machine algorithm
DOI: 10.1093/pasj/psz043 Bibcode: 2019PASJ...71...65P

Goto, Tomotsugu; Matsuhara, Hideo; Poliszczuk, Artem +15 more

The aim of this work is to create a new catalog of reliable active galactic nucleus (AGN) candidates selected from the AKARI NEP-Deep field. Selection of the AGN candidates was done by applying a fuzzy support vector machine algorithm, which allows the incorporation of measurement uncertainties into the classification process. The training dataset…

2019 Publications of the Astronomical Society of Japan
AKARI 5
Wave Activity in Jupiter's North Equatorial Belt From Near-Infrared Reflectivity Observations
DOI: 10.1029/2018GL081858 Bibcode: 2019GeoRL..46.1232G

Wong, Michael H.; Irwin, Patrick G. J.; Orton, Glenn S. +4 more

High spatial resolution images of Jupiter at 1.58-2.28 µm are used to track and characterize a wave pattern observed in 2017 at a planetocentric latitude of 14°N. The wave pattern has a wave number of 18 and spans ∼5° in latitude. One bright crest remains stationary in System III longitude, while the remaining crests move slowly westward. Th…

2019 Geophysical Research Letters
eHST 5
QSO2 outflow characterization using data obtained with OSIRIS at the Gran Telescopio Canarias
DOI: 10.1051/0004-6361/201935270 Bibcode: 2019A&A...626A..89B

Cabrera-Lavers, Antonio; Bellocchi, Enrica; Emonts, Bjorn +1 more

Context. Ionized outflows are ubiquitous in non-radio-loud obscured quasars (QSO2s) at different redshifts. However, the actual size of the outflows and their efficiency for gas ejection and star formation truncation are controversial. Large-scale (exceeding several kiloparsec) extended radio structures might be necessary to identify (even to trig…

2019 Astronomy and Astrophysics
eHST 5
Shape evolution of cometary nuclei via anisotropic mass loss
DOI: 10.1051/0004-6361/201834806 Bibcode: 2019A&A...622L...5V

Vavilov, D. E.; Eggl, S.; Medvedev, Yu. D. +1 more

Context. Breathtaking imagery recorded during the European Space Agency Rosetta mission confirmed the bilobate nature of the nucleus of comet 67P/Churyumov-Gerasimenko. The peculiar appearance of the nucleus is not unique among comets. The majority of cometary cores imaged at high resolution exhibit a similar build. Various theories have been brou…

2019 Astronomy and Astrophysics
Rosetta 5
Triangulum-Andromeda Overdensity: a Region with a Complex Stellar Population
DOI: 10.3847/1538-4357/ab4ada Bibcode: 2019ApJ...886..113S

Souto, Diogo; Cunha, K.; Majewski, S. R. +4 more

The Triangulum-Andromeda (TriAnd) overdensity is a distant structure of the Milky Way located in the second Galactic quadrant well below the Galactic plane. Since its discovery, its nature has been under discussion, whether it could be old perturbations of the Galactic disk or the remains of a disrupted former dwarf galaxy. In this study, we inves…

2019 The Astrophysical Journal
Gaia 5
Prospects for detecting the astrometric signature of Barnard's Star b
DOI: 10.1051/0004-6361/201834643 Bibcode: 2019A&A...623A..10T

Zucker, S.; Reiners, A.; Ribas, I. +2 more

A low-amplitude periodic signal in the radial velocity (RV) time series of Barnard's Star was recently attributed to a planetary companion with a minimum mass of 3.2 M at an orbital period of 233 days. The relatively long orbital period and the proximity of Barnard's Star to the Sun raises the question whether the true mass of the plan…

2019 Astronomy and Astrophysics
Gaia 5