Physiology & Behavior, ISSN 0031-9384, 2016
Abstract Aberrant glucocorticoid secretion is implicated in the pathophysiology of stress-related disorders (i.e., depression, anxiety). Glucocorticoids exert...
Psychiatry
Psychiatry
Journal Article
Physiology and Behavior, ISSN 0031-9384, 12/2017, Volume 182, pp. 62 - 68
Hypoxia-induced neurocognitive impairments have been of clinical interest for centuries. The mechanisms responsible for these neurocognitive impairments at...
Cerebrovasculature | High altitude | Hypoxia | Neurocognition | Neurovascular coupling | VELOCITY CHANGES | COGNITIVE PERFORMANCE | 30-PERCENT OXYGEN | HUMANS | ACUTE-HYPOXIA | ALTITUDE | LATERALIZATION | ACCLIMATIZATION | BEHAVIORAL SCIENCES | PSYCHOLOGY, BIOLOGICAL | CEREBRAL-BLOOD-FLOW | VISUOSPATIAL PERFORMANCE | Physiological aspects | Neurosciences
Cerebrovasculature | High altitude | Hypoxia | Neurocognition | Neurovascular coupling | VELOCITY CHANGES | COGNITIVE PERFORMANCE | 30-PERCENT OXYGEN | HUMANS | ACUTE-HYPOXIA | ALTITUDE | LATERALIZATION | ACCLIMATIZATION | BEHAVIORAL SCIENCES | PSYCHOLOGY, BIOLOGICAL | CEREBRAL-BLOOD-FLOW | VISUOSPATIAL PERFORMANCE | Physiological aspects | Neurosciences
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 05/2019, Volume 876, Issue 2, p. 127
We have searched for short periodicities in the light curves of stars with T-eff cooler than 4000 K made from 2-minute cadence data obtained in Transiting...
DWARF | stars: variables: general | LOW-MASS STARS | FIELD | starspots | stars: flare | stars: pre-main sequence | DUST | RADIUS | circumstellar matter | ASTRONOMY & ASTROPHYSICS | stars: low-mass | SCALE
DWARF | stars: variables: general | LOW-MASS STARS | FIELD | starspots | stars: flare | stars: pre-main sequence | DUST | RADIUS | circumstellar matter | ASTRONOMY & ASTROPHYSICS | stars: low-mass | SCALE
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2013, Volume 779, Issue 2, pp. 91 - 12
We analyze the planetary microlensing event MOA-2010-BLG-328. The best fit yields host and planetary masses of M-h = 0.11 +/- 0.01 M-circle dot and M-p = 9.2...
gravitational lensing: micro | planetary systems | EXTRASOLAR PLANETS | EARTH-MASS | SNOW LINE | MAGNIFICATION MICROLENSING EVENTS | JUPITER/SATURN ANALOG | OPTICAL DEPTH | GALACTIC BULGE | DIFFERENCE IMAGE-ANALYSIS | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE STARS | MASS PLANET | Orbitals | Separation | Planets | Planetary mass | Parallax | Red dwarf stars | Ambiguity | Physics - Earth and Planetary Astrophysics | MATHEMATICAL SOLUTIONS | GRAVITATIONAL LENSES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MASS | RESOLUTION | DWARF STARS | NEPTUNE PLANET
gravitational lensing: micro | planetary systems | EXTRASOLAR PLANETS | EARTH-MASS | SNOW LINE | MAGNIFICATION MICROLENSING EVENTS | JUPITER/SATURN ANALOG | OPTICAL DEPTH | GALACTIC BULGE | DIFFERENCE IMAGE-ANALYSIS | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE STARS | MASS PLANET | Orbitals | Separation | Planets | Planetary mass | Parallax | Red dwarf stars | Ambiguity | Physics - Earth and Planetary Astrophysics | MATHEMATICAL SOLUTIONS | GRAVITATIONAL LENSES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MASS | RESOLUTION | DWARF STARS | NEPTUNE PLANET
Journal Article
Astrophysical Journal, ISSN 0004-637X, 05/2015, Volume 804, Issue 1, pp. 33 - 12
We report the discovery of a Jupiter-mass planet orbiting an M-dwarf star that gave rise to the microlensing event OGLE-2011-BLG-0265. Such a system is very...
gravitational lensing: micro | planetary systems | OGLE-III | SNOW LINE | GIANT PLANETS | JUPITER/SATURN ANALOG | GALACTIC BULGE | SURFACE BRIGHTNESS RELATIONS | ANGULAR SIZES | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | STARS | MASS PLANET | Planets | Planet formation | Extrasolar planets | Stars | Galactic bulge | Mathematical models | Light curve | Planetary systems | Physics - Earth and Planetary Astrophysics
gravitational lensing: micro | planetary systems | OGLE-III | SNOW LINE | GIANT PLANETS | JUPITER/SATURN ANALOG | GALACTIC BULGE | SURFACE BRIGHTNESS RELATIONS | ANGULAR SIZES | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | STARS | MASS PLANET | Planets | Planet formation | Extrasolar planets | Stars | Galactic bulge | Mathematical models | Light curve | Planetary systems | Physics - Earth and Planetary Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 529, p. A102
Aims. We report the discovery of a planet with a high planet-to-star mass ratio in the microlensing event MOA-2009-BLG-387, which exhibited pronounced...
gravitational lensing: micro | instrumentation: adaptive optics | instrumentation: photometers | methods: data analysis | methods: numerical | planets and satellites: detection | LUMINOSITY | MASSES | SNOW LINE | JUPITER/SATURN ANALOG | GALACTIC BULGE | DISCOVERY | MICROLENSING EVENTS | PHOTOMETRY | COOL | ASTRONOMY & ASTROPHYSICS | STARS | Physics - Earth and Planetary Astrophysics
gravitational lensing: micro | instrumentation: adaptive optics | instrumentation: photometers | methods: data analysis | methods: numerical | planets and satellites: detection | LUMINOSITY | MASSES | SNOW LINE | JUPITER/SATURN ANALOG | GALACTIC BULGE | DISCOVERY | MICROLENSING EVENTS | PHOTOMETRY | COOL | ASTRONOMY & ASTROPHYSICS | STARS | Physics - Earth and Planetary Astrophysics
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 04/2019, Volume 624, p. A132
Context. The Andromeda (M31) galaxy subtends nearly 100 square degrees on the sky. Any study of its halo must therefore account for the severe contamination...
galaxies: individual: M31 | POPULATION | planetary nebulae: general | O-III | GLOBULAR-CLUSTER SYSTEM | IDENTIFICATION | LUMINOSITY FUNCTION | galaxies: halos | GALAXY | ASTRONOMY & ASTROPHYSICS | REGIONS | STARS | STANDARD CANDLES | RADIAL-VELOCITIES
galaxies: individual: M31 | POPULATION | planetary nebulae: general | O-III | GLOBULAR-CLUSTER SYSTEM | IDENTIFICATION | LUMINOSITY FUNCTION | galaxies: halos | GALAXY | ASTRONOMY & ASTROPHYSICS | REGIONS | STARS | STANDARD CANDLES | RADIAL-VELOCITIES
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 547, p. A55
Context. Caustic crossing is the clearest signature of binary lenses in microlensing. In the present context, this signature is diluted by the large source...
Gravitational lensing: micro | Binaries: general | Stars: individual: MOA 2009-BLG-411L | CLUMP ABSOLUTE MAGNITUDE | MAGNIFICATION MICROLENSING EVENTS | CENTRAL PERTURBATIONS | PLANETARY | stars: individual: MOA 2009-BLG-411L | gravitational lensing: micro | BINARY INTERPRETATIONS | INTERSTELLAR EXTINCTION | OGLE | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | STARS | binaries: general | BULGE
Gravitational lensing: micro | Binaries: general | Stars: individual: MOA 2009-BLG-411L | CLUMP ABSOLUTE MAGNITUDE | MAGNIFICATION MICROLENSING EVENTS | CENTRAL PERTURBATIONS | PLANETARY | stars: individual: MOA 2009-BLG-411L | gravitational lensing: micro | BINARY INTERPRETATIONS | INTERSTELLAR EXTINCTION | OGLE | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | STARS | binaries: general | BULGE
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 08/2019, Volume 628, p. A39
We report the detection of a transiting Earth-size planet around GJ 357, a nearby M2.5 V star, using data from the Transiting Exoplanet Survey Satellite...
SKY | stars: individual: G1 357 | EXOPLANET | techniques: radial velocities | techniques: photometric | SEARCH | GIANT PLANETS | PRECISION | planetary systems | stars: late-type | ASTRONOMY & ASTROPHYSICS | MASS | STARS | ECHELLE SPECTROMETER | ERROR-CORRECTION | BAYESIAN-INFERENCE | Terrestrial planets | Spectroscopy | Extrasolar planets | Terrestrial environments | Orbits | Planetary mass | Circumstellar habitable zone | Periodic variations | Periodicities | Transit | Earth | Satellites | Planets | Planet detection | Radial velocity | Photometry | Planetary systems
SKY | stars: individual: G1 357 | EXOPLANET | techniques: radial velocities | techniques: photometric | SEARCH | GIANT PLANETS | PRECISION | planetary systems | stars: late-type | ASTRONOMY & ASTROPHYSICS | MASS | STARS | ECHELLE SPECTROMETER | ERROR-CORRECTION | BAYESIAN-INFERENCE | Terrestrial planets | Spectroscopy | Extrasolar planets | Terrestrial environments | Orbits | Planetary mass | Circumstellar habitable zone | Periodic variations | Periodicities | Transit | Earth | Satellites | Planets | Planet detection | Radial velocity | Photometry | Planetary systems
Journal Article
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Full Text
Mechanical dissociation of the M-band titin/obscurin complex is directionally dependent
FEBS Letters, ISSN 0014-5793, 07/2015, Volume 589, Issue 15, pp. 1735 - 1739
Titin and obscurin, two giant muscle proteins, bind to each other in an antiparallel Ig–Ig fashion at the M-band. This interaction must be able to withstand...
Steered molecular dynamic | Peeling | M10 | Shearing | Muscular dystrophy | GIANT MUSCLE PROTEINS | STEERED MOLECULAR-DYNAMICS | TITIN | BIOCHEMISTRY & MOLECULAR BIOLOGY | PULLING GEOMETRY | SIMULATION | THICK FILAMENTS | CELL BIOLOGY | SKELETAL-MUSCLE | BIOPHYSICS | SARCOMERE | OBSCURIN | MICROSCOPE | Hydrophobic and Hydrophilic Interactions | Connectin - chemistry | Muscle Proteins - chemistry | Hydrogen Bonding | Molecular Dynamics Simulation
Steered molecular dynamic | Peeling | M10 | Shearing | Muscular dystrophy | GIANT MUSCLE PROTEINS | STEERED MOLECULAR-DYNAMICS | TITIN | BIOCHEMISTRY & MOLECULAR BIOLOGY | PULLING GEOMETRY | SIMULATION | THICK FILAMENTS | CELL BIOLOGY | SKELETAL-MUSCLE | BIOPHYSICS | SARCOMERE | OBSCURIN | MICROSCOPE | Hydrophobic and Hydrophilic Interactions | Connectin - chemistry | Muscle Proteins - chemistry | Hydrogen Bonding | Molecular Dynamics Simulation
Journal Article