411 datasets found

Keywords: m stars

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  • 2MASS view of Sgr dSph. VII. Kinematics

    We have assembled a large-area spectroscopic survey of giant stars in the Sagittarius (Sgr) dwarf galaxy core. Using medium resolution (R~15000), multifiber spectroscopy we have...
  • The AstraLux Large M-dwarf Survey

    These tables contain the results from a multiplicity survey of 701 M-type and 60 K-type stars (among which 182 new and 37 previously known companions were detected in 205...
  • K-band spectra for 133 nearby M dwarfs

    We present K-band spectra for 133 nearby (d < 33 pc) M dwarfs, including 18 M dwarfs with reliable metallicity estimates (as inferred from an FGK type companion), 11 M dwarf...
  • Transit light curves of GJ1214

    The super-Earth GJ1214b transits a nearby M dwarf that exhibits a 1% intrinsic variability in the near-infrared. Here, we analyze new observations to refine the physical...
  • HIRES radial velocities of GJ 581

    We present 11 years of HIRES precision radial velocities (RVs) of the nearby M3V star Gliese 581, combining our data set of 122 precision RVs with an existing published 4.3-year...
  • Photometry of polar CV* 1RXS J173006.4+033813

    We report the discovery of 1RXS J173006.4+033813, a polar cataclysmic variable with a period of 120.21 minutes. The white dwarf primary has a magnetic field of B=42^+6^-5_MG and...
  • A 2MASS view of the Sgr dSph. VI.

    We present high-resolution spectroscopic measurements of the abundances of the {alpha} element titanium (Ti) and s-process elements yttrium (Y) and lanthanum (La) for 59...
  • Photometry and spectroscopy in IC 2391

    We present the stellar and substellar mass function (MF) of the open cluster IC 2391, plus its radial dependence, and use this to put constraints on the formation mechanism of...
  • Radio interferometric planet search. I.

    Radio astrometry of nearby, low-mass stars has the potential to be a powerful tool for the discovery and characterization of planetary companions. We present a Very Large Array...
  • Young M dwarfs within 25pc. I.

    We have completed a high-resolution (R~60000) optical spectroscopic survey of 185 nearby M dwarfs identified using ROSAT data to select active, young objects with fractional...
  • M giant stars in the Sagittarius dwarf galaxy. V.

    We present reliable measurements of the metallicity distribution function (MDF) at different points along the tidal stream of the Sagittarius (Sgr) dwarf spheroidal (dSph)...
  • M dwarfs flares timing & energy from TESS & Swift

    Ultraviolet flare emission can drive photochemistry in exoplanet atmospheres and even serve as the primary source of uncertainty in atmospheric retrievals. Additionally, flare...
  • TOI-1450 radial velocities & activity indicators

    M-dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUnting for M Dwarf Rocky planets Using MAROON-X (HUMDRUM) survey uses the MAROON-X...
  • Phot. & RVs for 6 giant planets around cool dwarfs

    Transiting giant exoplanets around M-dwarf stars (GEMS) are rare, owing to the low-mass host stars. However, the all-sky coverage of TESS has enabled the detection of an...
  • Coronographic observations for M dwarfs companions

    We present Super-RDI, a unique framework for the application of reference star differential imaging (RDI) to Keck/NIRC2 high-contrast imaging observations with the vortex...
  • Ultracool dwarf candidates from machine-learning

    We present the discovery of 118 new ultracool dwarf candidates, discovered using a new machine-learning tool, named SMDET, applied to time-series images from the Wide-field...
  • TOI-762 and TIC 46432937: LCs data

    We present the discovery of TOI 762 A b and TIC 46432937 b, two giant planets transiting M-dwarf stars. Transits of both systems were first detected from observations by the...
  • High resolution spectroscopic obs. of TOI-6255

    TOI-6255 b (GJ 4256) is an Earth-sized planet (1.079+/-0.065R_{Earth}) with an orbital period of only 5.7hr. With the newly commissioned Keck Planet Finder and CARMENES...
  • Transit time for planets in LHS 1678 System

    The nearby LHS-1678 (TOI-696) system contains two confirmed planets and a wide-orbit, likely brown-dwarf companion, which orbit an M2 dwarf with a unique evolutionary history....
  • The solar neighborhood LI. RECONS & TESS obs.

    We present the optical photometric variability of 32 planet-hosting M dwarfs within 25pc over timescales of months to decades. The primary goal of this project-A Trail to Life...
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