Search Publications

A NuSTAR study of the 55 ks hard X-ray pulse-phase modulation in the magnetar 4U 0142+61
DOI: 10.1093/pasj/psy129 Bibcode: 2019PASJ...71...15M

Enoto, Teruaki; Makishima, Kazuo; Nakazawa, Kazuhiro +1 more

Archival NuSTAR data of the magnetar 4U 0142+61, acquired in 2014 March for a total time span of 258 ks, were analyzed. This is to reconfirm the 55 ks modulation in the hard X-ray pulse phases of this source, found with a Suzaku observation in 2009 (Makishima et al., 2014, Phys. Rev. Lett., 112, 171102). Indeed, the 10-70 keV X-ray pulsation, dete…

2019 Publications of the Astronomical Society of Japan
Suzaku 20
An 11 Earth-mass, Long-period Sub-Neptune Orbiting a Sun-like Star
DOI: 10.3847/1538-3881/ab3e2f Bibcode: 2019AJ....158..165M

López-Morales, Mercedes; Latham, David W.; Mayo, Andrew W. +27 more

Although several thousands of exoplanets have now been detected and characterized, observational biases have led to a paucity of long-period, low-mass exoplanets with measured masses and a corresponding lag in our understanding of such planets. In this paper we report the mass estimation and characterization of the long-period exoplanet Kepler-538…

2019 The Astronomical Journal
Gaia 20
Dust production in the debris disk around HR 4796 A
DOI: 10.1051/0004-6361/201935998 Bibcode: 2019A&A...630A.142O

Ménard, F.; Augereau, J. -C.; Bayo, A. +21 more

Context. Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from the grinding down of bigger planetesimals.
Aims: High angular resolution observations at optical wavelengths can provide key constraints on the radial and…

2019 Astronomy and Astrophysics
Gaia eHST 20
Investigating dynamical properties of evolved Galactic open clusters
DOI: 10.1051/0004-6361/201832702 Bibcode: 2019A&A...624A...8A

Corradi, W. J. B.; Santos, J. F. C.; Maia, F. F. S. +1 more

Context. The stellar content of Galactic open clusters is gradually depleted during their evolution as a result of internal relaxation and external interactions. The final residues of the long-term evolution of open clusters are called open cluster remnants. These are sparsely populated structures that can barely be distinguished from the field. <…

2019 Astronomy and Astrophysics
Gaia 20
Infrared luminosity functions based on 18 mid-infrared bands: revealing cosmic star formation history with AKARI and Hyper Suprime-Cam*
DOI: 10.1093/pasj/psz009 Bibcode: 2019PASJ...71...30G

Momose, Rieko; Hashimoto, Tetsuya; Goto, Tomotsugu +21 more

Much of star formation is obscured by dust. For a complete understanding of the cosmic star formation history (CSFH), infrared (IR) census is indispensable. AKARI carried out deep mid-infrared observations using its continuous nine-band filters in the North Ecliptic Pole (NEP) field (5.4 deg2). This took a significant amount of the sate…

2019 Publications of the Astronomical Society of Japan
AKARI 20
Constraining models of activity on comet 67P/Churyumov-Gerasimenko with Rosetta trajectory, rotation, and water production measurements
DOI: 10.1051/0004-6361/201834415 Bibcode: 2019A&A...630A..18A

Jorda, L.; Kührt, E.; Mottola, S. +11 more


Aims: We use four observational data sets, mainly from the Rosetta mission, to constrain the activity pattern of the nucleus of comet 67P/Churyumov-Gerasimenko (67P).
Methods: We developed a numerical model that computes the production rate and non-gravitational acceleration of the nucleus of comet 67P as a function of time, taking into …

2019 Astronomy and Astrophysics
Rosetta 20
Fluctuation of the background sky in the Hubble Extremely Deep Field (XDF) and its origin
DOI: 10.1093/pasj/psz070 Bibcode: 2019PASJ...71...88M

Matsumoto, Toshio; Tsumura, Kohji

We performed a fluctuation analysis of the Hubble Extremely Deep Field (XDF) at four optical wavelength bands and found large fluctuations that are significantly brighter than those expected for ordinary galaxies. Good cross-correlations with flat spectra are found down to {0{^''.}2}, indicating the existence of a spatial structure even…

2019 Publications of the Astronomical Society of Japan
eHST 20
Plasma properties of suprathermal electrons near comet 67P/Churyumov-Gerasimenko with Rosetta
DOI: 10.1051/0004-6361/201834964 Bibcode: 2019A&A...630A..42M

Henri, P.; Goldstein, R.; Galand, M. +6 more

Context. The Rosetta spacecraft escorted comet 67P/Churyumov-Gerasimenko from 2014 to September 2016. The mission provided in situ observations of the cometary plasma during different phases of the cometary activity, which enabled us to better understand its evolution as a function of heliocentric distance.
Aims: In this study, different elec…

2019 Astronomy and Astrophysics
Rosetta 20
Speckle Observations and Orbits of Multiple Stars
DOI: 10.3847/1538-3881/ab4137 Bibcode: 2019AJ....158..167T

Torres, Guillermo; Latham, David W.; Tokovinin, Andrei +2 more

We report results of speckle-interferometric monitoring of visual hierarchical systems using the newly commissioned instrument NN-EXPLORE Exoplanet and Stellar Speckle Imager at the 3.5 m WIYN telescope. During one year, 390 measurements of 129 resolved subsystems were made, while some targets were unresolved. Using our astrometry and archival dat…

2019 The Astronomical Journal
Gaia Hipparcos 20
Constraining the Johannsen deformation parameter ɛ3 with black hole x-ray data
DOI: 10.1103/PhysRevD.99.083001 Bibcode: 2019PhRvD..99h3001T

Tripathi, Ashutosh; Abdikamalov, Askar B.; Ayzenberg, Dimitry +2 more

We extend our previous work on tests of the Kerr black hole hypothesis using x-ray reflection spectroscopy and we infer observational constraints on the Johannsen deformation parameter ɛ3 . We analyze a NuSTAR observation of the stellar-mass black hole in GS 1354-645, Suzaku data of the supermassive black holes in Ark 564, 1H0419-577, a…

2019 Physical Review D
Suzaku XMM-Newton 20