Search Results - "Nagao, T."
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THE FMOS-COSMOS SURVEY OF STAR-FORMING GALAXIES AT z ∼ 1.6. IV. EXCITATION STATE AND CHEMICAL ENRICHMENT OF THE INTERSTELLAR MEDIUM
Published in The Astrophysical journal (20-01-2017)“…ABSTRACT We investigate the physical conditions of ionized gas in high-z star-forming galaxies using diagnostic diagrams based on the rest-frame optical…”
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SEARCH FOR HYPERLUMINOUS INFRARED DUST-OBSCURED GALAXIES SELECTED WITH WISE AND SDSS
Published in The Astrophysical journal (20-03-2016)“…ABSTRACT We aim to search for hyperluminous infrared (IR) galaxies (HyLIRGs) with IR luminosity > 1013 L☉ by applying the selection method of dust-obscured…”
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Early light curves of Type II supernovae interacting with a circumstellar disc
Published in Monthly notices of the Royal Astronomical Society (01-10-2020)“…ABSTRACT Type II supernovae (SNe) interacting with disc-like circumstellar matter (CSM) have been suggested as an explanation of some unusual Type II SNe, e.g…”
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A prospective phase II study of combined androgen blockade in patients with androgen receptor-positive metastatic or locally advanced unresectable salivary gland carcinoma
Published in Annals of oncology (01-04-2018)“…There is no standard first-line chemotherapy for recurrent/metastatic (RM) or unresectable locally advanced (LA) salivary gland carcinoma (SGC). We conducted a…”
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Evidence for Merger-driven Growth in Luminous, High-z, Obscured AGNs in the CANDELS/COSMOS Field
Published in The Astrophysical journal (20-01-2018)“…While major mergers have long been proposed as a driver of both active galactic nucleus (AGN) activity and the relation, studies of moderate to high-redshift…”
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Evidence for multiple origins of fast declining Type II supernovae from spectropolarimetry of SN 2013ej and SN 2017ahn
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT The origin of the diverse light-curve shapes of Type II supernovae (SNe), and whether they come from similar or distinct progenitors, has been…”
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A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys
Published in Monthly notices of the Royal Astronomical Society (11-08-2013)“…We present an investigation into how well the properties of the accretion flow on to a supermassive black hole may be coupled to those of the overlying hot…”
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The aspherical explosion of the Type IIP SN 2017gmr
Published in Monthly notices of the Royal Astronomical Society (01-10-2019)“…ABSTRACT Type IIP supernovae (SNe IIP), which represent the most common class of core-collapse (CC) SNe, show a rapid increase in continuum polarization just…”
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Aerosol data assimilation using data from Himawari‐8, a next‐generation geostationary meteorological satellite
Published in Geophysical research letters (16-06-2016)“…Himawari‐8, a next‐generation geostationary meteorological satellite, was launched on 7 October 2014 and became operational on 7 July 2015. The advanced imager…”
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Effective decoration of Pd nanoparticles on the surface of SnO2 nanowires for enhancement of CO gas-sensing performance
Published in Journal of hazardous materials (30-01-2014)“…Decoration of noble metal nanoparticles (NPs) on the surface of semiconducting metal oxide nanowires (NWs) to enhance material characteristics,…”
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Changes in Seismicity Pattern Due to the 2016 Kumamoto Earthquakes Identify a Highly Stressed Area on the Hinagu Fault Zone
Published in Geophysical research letters (28-08-2019)“…A highly stressed area where eventual ruptures have often been observed to nucleate is characterized by low b values of earthquake frequency‐size distribution…”
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Late-time H/He-poor Circumstellar Interaction in the Type Ic Supernova SN 2021ocs: An Exposed Oxygen–Magnesium Layer and Extreme Stripping of the Progenitor
Published in Astrophysical journal. Letters (01-12-2022)“…Abstract Supernova (SN) 2021ocs was discovered in the galaxy NGC 7828 ( z = 0.01911) within the interacting system Arp 144 and subsequently classified as a…”
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THE FMOS-COSMOS SURVEY OF STAR-FORMING GALAXIES AT z ~ 1.6. II. THE MASS-METALLICITY RELATION AND THE DEPENDENCE ON STAR FORMATION RATE AND DUST EXTINCTION
Published in The Astrophysical journal (01-09-2014)“…We investigate the relationships between stellar mass, gas-phase oxygen abundance (metallicity), star formation rate (SFR), and dust content of star-forming…”
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Orbital lymphoproliferative disorders (OLPDs): value of MR imaging for differentiating orbital lymphoma from benign OPLDs
Published in American journal of neuroradiology : AJNR (01-10-2014)“…Accurate discrimination of orbital lymphoma from benign orbital lymphoproliferative disorders is crucial for treatment planning. We evaluated MR imaging…”
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The Molecular Gas Content and Fuel Efficiency of Starbursts at z ∼ 1.6 with ALMA
Published in The Astrophysical journal (10-11-2018)“…We present an analysis of the molecular gas properties, based on CO (2−1) emission, of 12 starburst galaxies at z ∼ 1.6 selected by having a boost ( 4×) in…”
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EVOLUTION OF THE QUASAR LUMINOSITY FUNCTION OVER 3 < z < 5 IN THE COSMOS SURVEY FIELD
Published in The Astrophysical journal (20-08-2012)“…We investigate the high-redshift quasar luminosity function (QLF) down to an apparent magnitude of I sub(AB) = 25 in the Cosmic Evolution Survey (COSMOS)…”
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Chemically synthesized nanowire TiO2/ZnO core-shell p-n junction array for high sensitivity ultraviolet photodetector
Published in Applied physics letters (04-11-2013)“…A sol-gel-based ultrathin TiO2 lamination coating was adapted to a hydrothermally grown ZnO nanowire array to realize an all-oxide ultra-sensitive p-n…”
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A Catastrophic Failure to Build a Massive Galaxy around a Supermassive Black Hole at z = 3.84
Published in The Astrophysical journal (20-08-2019)“…We present observations of the stellar and molecular gas mass of SDSS J163909+282447.1, a luminous quasar at z = 3.84 with an extreme mass for a supermassive…”
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Concurrent Starbursts in Molecular Gas Disks within a Pair of Colliding Galaxies at z = 1.52
Published in The Astrophysical journal (20-11-2018)“…We report on the discovery of a merger-driven starburst at z = 1.52, PACS-787, based on high signal-to-noise ALMA observations. CO(5-4) and continuum emission…”
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