Publication type: Non-refereed

  • Publication
    Near-infrared Spectra of Two Asteroids with Low Tisserand Invariant
    We present near-infrared reflectance spectra of two asteroids with low Tisserand invariant, 2906 Caltech and 1373 Cincinnati. The Tisserand invariant is a...
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    Near-infrared spectroscopic survey of B-type asteroids: compositional analysis
    We present near-infrared spectra of 23 B-type asteroids obtained with the NICS cameraspectrograph at the 3.56 m Telescopio Nazionale Galileo. We also include...
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    Near-infrared Spectroscopy of Brown Dwarf and Planetary-Mass Members in Upper Scorpius
    In these proceedings, I present new VLT/X-shooter near-infrared spectroscopy of brown dwarf and planetary-mass candidates with masses below 30 Jupiter masses...
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    Near-infrared spectroscopy of Seyfert and spiral galaxies
    We present near-infrared long-slit spectroscopy of matched samples of nearby Seyfert and normal spiral galaxies. The central molecular content in Seyferts type...
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    Near-infrared Spectroscopy of Three Nearby L Dwarfs
    Not Available Based on observations collected at the European Southern Observatory.
  • Publication
    Near-infrared Spectroscopy of Three Nearby L Dwarfs
    Not Available Based on observations collected at the European Southern Observatory.
  • Publication
    Near-IR and Optical Observations of the Ongoing Outburst of SAX J1808.4-3658
    Following the report of a new outburst of the accreting millisecond pulsar SAX J1808.4-3658 by Markwardt and Swank (ATel #1728), the source was observed using...
  • Publication
    Near-IR brightening of the blazar CTA 102 (2230+114) observed by the GASP
    The GLAST-AGILE Support Program (GASP) of the Whole Earth Blazar Telescope (WEBT) reports on the recent observation of a strong near-IR brightening of the gamma...
  • Publication
    Near-IR Imaging of Star-forming Regions with IRAF
    We report on our ongoing project ``Infrared Study of Hii Regions Associated with Small Clouds.'' Several tasks are being developed under the IRAF environment...