Search Publications

Properties of the SCUBA-2 850 µm Sources in the Akari NEP-Deep Field
DOI: 10.5303/JKAS.2018.51.3.49 Bibcode: 2018JKAS...51...49S

Goto, Tomotsugu; Kim, Seong Jin; Pearson, Chris +15 more

We carry out the study of SMGs in the AKARI NEP-Deep field using James Clerk Maxwell Telescope (JCMT) SCUBA-2 850 µm source catalog released as a part of SCUBA-2 Cosmology Legacy Survey (S2CLS) program. The SCUBA-2 850 µm map has a root mean square (rms) noise of 1.2 mJy beam^{-1} and covers an area of 0.60 degree^{2}. We find 4 sub-mi…

2018 Journal of Korean Astronomical Society
AKARI 3
GIADA performance during Rosetta mission scientific operations at comet 67P
DOI: 10.1016/j.asr.2017.07.031 Bibcode: 2018AdSpR..62.1987S

Fulle, M.; Rodriguez, J.; Colangeli, L. +16 more

The Grain Impact Analyser and Dust Accumulator (GIADA) instrument onboard Rosetta studied the dust environment of comet 67P/Churyumov-Gerasimenko from 3.7 au inbound, through perihelion, to 3.8 au outbound, measuring the dust flow and the dynamic properties of individual particles. GIADA is composed of three subsystems: (1) Grain Detection System …

2018 Advances in Space Research
Rosetta 3
The LABOCA/ACT Survey of Clusters at All Redshifts: Multiwavelength Analysis of Background Submillimeter Galaxies
DOI: 10.3847/1538-4357/aaaab0 Bibcode: 2018ApJ...855...26A

Hilton, Matt; Bond, J. Richard; Dünner, Rolando +12 more

We present a multiwavelength analysis of 48 submillimeter galaxies (SMGs) detected in the Large APEX Bolometer Camera/Atacama Cosmology Telescope (ACT) Survey of Clusters at All Redshifts, LASCAR, which acquired new 870 µm and Australia Telescope Compact Array 2.1 GHz observations of 10 galaxy clusters detected through their Sunyaev-Zel’dovi…

2018 The Astrophysical Journal
Herschel 3
Search for companions in visual binary systems using precise radial-velocity measurements
DOI: 10.1093/pasj/psy054 Bibcode: 2018PASJ...70...60K

Sato, Bun'ei; Itoh, Yoichi; Katoh, Noriyuki

The frequency of triple and quadruple systems is considered to be high in the early phase of star formation. Some multiple systems decay in the pre-main-sequence phase. The multiplicity of main-sequence stars provides clues about the evolution of binary systems. This work searched for companions of five components of visual binary systems using pr…

2018 Publications of the Astronomical Society of Japan
Gaia 3
X-ray stars observed in LAMOST spectral survey
DOI: 10.1007/s10509-018-3328-8 Bibcode: 2018Ap&SS.363..104L

Shi, Jianrong; Han, Xianming L.; Lu, Hong-peng +1 more

X-ray stars have been studied since the beginning of X-ray astronomy. Investigating and studying the chromospheric activity from X-ray stellar optical spectra is highly significant in providing insights into stellar magnetic activity. The big data of LAMOST survey provides an opportunity for researching stellar optical spectroscopic properties of …

2018 Astrophysics and Space Science
XMM-Newton 3
Chromospheric Response during the Precursor and the Main Phase of a B6.4 Flare on 2005 August 20
DOI: 10.3847/1538-4357/aabd76 Bibcode: 2018ApJ...858...98A

Awasthi, Arun Kumar; Liu, Rui; Berlicki, Arkadiusz +2 more

Solar flare precursors depict a constrained rate of energy release, in contrast to the imminent rapid energy release, which calls for a different regime of plasma processes to be at play. Due to the subtle emission during the precursor phase, its diagnostics remain delusive, revealing either nonthermal electrons (NTEs) or thermal conduction to be …

2018 The Astrophysical Journal
SOHO 3
ALMA Observation of NGC 5135: The Circumnuclear CO (6-5) and Dust Continuum Emission at 45 pc Resolution
DOI: 10.3847/1538-4357/aae1f4 Bibcode: 2018ApJ...866..117C

Inami, Hanae; van der Werf, Paul; Gao, Yu +10 more

We present high-resolution (0.″17 × 0.″14) Atacama Large Millimeter/submillimeter Array (ALMA) observations of the CO (6-5) line and 435 µm dust continuum emission within a ∼9″ × 9″ area centered on the nucleus of the galaxy NGC 5135. NGC 5135 is a well-studied luminous infrared galaxy that also harbors a Compton-thick active galactic nucleu…

2018 The Astrophysical Journal
eHST 3
Discovery of two bright DO-type white dwarfs
DOI: 10.1093/mnras/sty1875 Bibcode: 2018MNRAS.480.1211R

Geier, S.; Reindl, Nicole; Østensen, R. H.

We discovered two bright DO-type white dwarfs, GALEX J053628.3+544854 (J0536+5448) and GALEX J231128.0+292935(J2311+2929), which rank among the eight brightest DO-type white dwarfs known. Our non-LTE model atmosphere analysis reveals effective temperatures and surface gravities of {T_eff} = 80000± 4600 K and log g = 8.25± 0.15 for J0536+5448 and {…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 3
XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster Cl J120958.9+495352 (z = 0.902)
DOI: 10.1051/0004-6361/201730913 Bibcode: 2018A&A...610A..71T

Thölken, Sophia; Schrabback, Tim; Reiprich, Thomas H. +6 more

Context. Observations of relaxed, massive, and distant clusters can provide important tests of standard cosmological models, for example by using the gas mass fraction. To perform this test, the dynamical state of the cluster and its gas properties have to be investigated. X-ray analyses provide one of the best opportunities to access this informa…

2018 Astronomy and Astrophysics
XMM-Newton eHST 3
Particles Co-orbital to Janus and to Epimetheus: A Firefly Planetary Ring
DOI: 10.3847/1538-4357/aa9c7f Bibcode: 2018ApJ...852...14W

Sfair, Rafael; Winter, Othon C.; Souza, Alexandre P. S. +3 more

The Cassini spacecraft found a new and unique ring that shares the trajectory of Janus and Epimetheus, co-orbital satellites of Saturn. Performing image analysis, we found this to be a continuous ring. Its width is between 30% and 50% larger than previously announced. We also verified that the ring behaves like a firefly. It can only be seen from …

2018 The Astrophysical Journal
Cassini 3