Search Results - "IZUMIURA, HIDEYUKI"
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The Seimei telescope project and technical developments
Published in Publications of the Astronomical Society of Japan (01-06-2020)“…ABSTRACT An overview of the Seimei telescope, a 3.8 m optical infrared telescope located on Mt. Chikurinji in the Okayama prefecture of Japan, is presented…”
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Optical spectroscopic observations of a symbiotic star MWC 560 in the mass accumulation phase
Published in Publications of the Astronomical Society of Japan (01-12-2021)“…Abstract There are about a dozen symbiotic stars known to produce high-velocity jets during outbursts. MWC 560 (V694 Mon) is a symbiotic star that seems to…”
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Near-IR Spectroscopy of Luminous LoBAL Quasars at 1 < z < 2.5
Published in The Astrophysical journal (20-10-2017)“…We present near-IR spectroscopy of 22 luminous low-ionization broad absorption line quasars (LoBAL QSOs) at redshift , with 12 objects at z ∼ 1.5 and 10 at z ∼…”
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Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate
Published in Publications of the Astronomical Society of Japan (01-02-2022)“…Abstract We report the detection of radial velocity (RV) variations in nine evolved G- and K-type giant stars. The observations were conducted at Okayama…”
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Long-term Near-infrared Brightening of Nonvariable OH/IR Stars
Published in The Astrophysical journal (01-07-2020)“…Nonvariable OH/IR stars are thought to have just left the asymptotic giant branch (AGB) phase. In this conventional picture, they must still show strong…”
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Two Long-period Giant Planets around Two Giant Stars: HD 112570 and HD 154391
Published in The Astronomical journal (01-02-2024)“…Abstract We present the discoveries of two giant plants orbiting the red-giant-branch star HD 112570 and the red-clump star HD 154391, based on the…”
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OISTER OPTICAL AND NEAR-INFRARED OBSERVATIONS OF TYPE Iax SUPERNOVA 2012Z
Published in The Astrophysical journal (20-06-2015)“…We report observations of the Type Iax supernova (SN Iax) 2012Z at optical and near-infrared (NIR) wavelengths from immediately after the explosion until ~260…”
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Optical spectroscopic monitoring of the symbiotic star MWC 560 before and after the 2018 unpredicted brightening
Published in Publications of the Astronomical Society of Japan (01-06-2021)“…Abstract MWC 560 (V694 Mon) is classified as a symbiotic binary consisting of a white dwarf and an M5III red giant. In this object, a very- high-speed…”
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Okayama Astrophysical Observatory Wide-Field Camera
Published in Publications of the Astronomical Society of Japan (01-12-2019)“…Abstract We report on the development of a wide-field near-infrared (0.9–2.5$\, \mu$m) camera built as a renewal of the existing classical Cassegrain 0.91 m…”
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Dust and Chemical Abundances of the Sagittarius Dwarf Galaxy Planetary Nebula Hen2-436
Published in The Astrophysical journal (01-03-2011)“…We have estimated elemental abundances of the planetary nebula (PN) Hen2-436 in the Sagittarius (Sgr) spheroidal dwarf galaxy using ESO/VLT FORS2,…”
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OISTER optical and near-infrared observations of the super-Chandrasekhar supernova candidate SN 2012dn: Dust emission from the circumstellar shell
Published in Publications of the Astronomical Society of Japan (01-10-2016)“…Abstract We present extensively dense observations of the super-Chandrasekhar supernova (SC SN) candidate SN 2012dn from −11 to +140 d after the date of its…”
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OPTICAL-TO-NEAR-INFRARED SIMULTANEOUS OBSERVATIONS FOR THE HOT URANUS GJ3470b: A HINT OF A CLOUD-FREE ATMOSPHERE
Published in The Astrophysical journal (20-06-2013)“…(ProQuest: ... denotes formulae and/or non-USASCII text omitted) We present optical (g' R sub(c) and I sub(c)) to near-infrared (J) simultaneous photometric…”
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A DOUBLE PLANETARY SYSTEM AROUND THE EVOLVED INTERMEDIATE-MASS STAR HD 4732
Published in The Astrophysical journal (01-01-2013)“…We report the detection of a double planetary system orbiting around the evolved intermediate-mass star HD 4732 from precise Doppler measurements at Okayama…”
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High Dispersion Spectrograph (HDS) for the Subaru Telescope
Published in Publications of the Astronomical Society of Japan (25-12-2002)“…We present the design and performance of the High Dispersion Spectrograph (HDS) of the Subaru Telescope. HDS is an echelle spectrograph located at the Nasmyth…”
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The nearby evolved stars survey – I. JCMT/SCUBA-2 submillimetre detection of the detached shell of U Antliae
Published in Monthly notices of the Royal Astronomical Society (01-11-2019)“…ABSTRACT We present the highest resolution single-dish submillimetre observations of the detached shell source U Antliae to date. The observations were…”
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A PAIR OF GIANT PLANETS AROUND THE EVOLVED INTERMEDIATE-MASS STAR HD 47366: MULTIPLE CIRCULAR ORBITS OR A MUTUALLY RETROGRADE CONFIGURATION
Published in The Astrophysical journal (01-03-2016)“…ABSTRACT We report the detection of a double planetary system around the evolved intermediate-mass star HD 47366 from precise radial-velocity measurements at…”
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Surface brightness correction for compact extended sources observed by the AKARI Far-Infrared Surveyor in the slow-scan mode
Published in Publications of the Astronomical Society of Japan (01-02-2017)“…Abstract We present a general surface brightness correction method for compact extended sources imaged in the slow-scan pointed observation mode of the…”
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Three-dimensional Atmospheric Dynamics of Jupiter from Ground-based Doppler Imaging Spectroscopy in the Visible
Published in The planetary science journal (16-04-2024)“…We present three-dimensional (3D) maps of Jupiter’s atmospheric circulation at cloud-top level from Doppler-imaging data obtained in the visible domain with…”
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A Substellar Companion to the Intermediate-Mass Giant 11 Comae
Published in The Astrophysical journal (01-01-2008)“…We report the detection of a substellar companion orbiting the intermediate-mass giant star 11 Com (G8 III). Precise Doppler measurements of the star from…”
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Detection of Fluorine in the Halo Planetary Nebula BoBn 1: Evidence for a Binary Progenitor Star
Published in The Astrophysical journal (01-08-2008)“…We have found the fluorine lines [F IV] lambda lambda 3996.92, 4059.90 in the extremely metal-poor ([Ar/H] = -2.10 plus or minus 0.21) halo planetary nebula…”
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