Visible spectroscopy in the neighborhood of 2003EL{61}
Context: The recent discovery of a group of trans-neptunian objects (TNOs) in a narrow region of the orbital parameter space and with surfaces composed of...
Visible spectroscopy of 2003 UB313: evidence for N2 ice on the surface of the largest TNO?
Context: .The recent discovery of two large trans-Neptunian objects (TNOs) 2003 UB313 and 2005 FY9, with surface properties similar to those of Pluto, provides...
Visible spectroscopy of the Polana-Eulalia family complex: Spectral homogeneity
The Polana-Eulalia family complex is located in the inner part of the asteroid belt, bounded by the ν6 and the 3:1 resonances, where we can find another three...
Visible spectroscopy of the Sulamitis and Clarissa primitive families: a possible link to Erigone and Polana
The low-inclination (i 8∘) primitive asteroid families in the inner main belt, that is, Polana-Eulalia, Erigone, Sulamitis, and Clarissa, are considered to be...
Visible-near-infrared observations of organics and carbonates on (101955) Bennu: Classification method and search for surface context
The OSIRIS-REx Visible and InfraRed Spectrometer (OVIRS) onboard the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer...
VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way
We describe the public ESO near-IR variability survey (VVV) scanning the Milky Way bulge and an adjacent section of the mid-plane where star formation activity...
Visual Determination of the Mean Effective Chromospheric Thickness
IN the course of taking submillimetre chromospheric data from Concorde 001 during the eclipse of June 30 (ref. 1), it proved possible to record information on...
VLA and ALMA observations of the lensed radio-quiet quasar SDSS J0924+0219: a molecular structure in a 3 μJy radio source
We present Karl G. Jansky Very Large Array (VLA) and Atacama Large Millimetre Array (ALMA) observations of SDSS J0924+0219, a z = 1.524 radio-quiet lensed...