NOVA (Nuevo Observatorio Virtual Argentino) is the Argentina's Virtual Observatory. It provides the astronomical community with a data center, software tools, data interoperability standards and resources coordination with the aim of making more efficient and productive the access, handling and analysis of multi-wavelength astronomical data collected by Institutes of Astronomy in Argentina.This is public information and it could be used by astronomy researchers, researchers of other fields, students and the general public.
Information gathered from HIPASS, LVHIS, THINGS, VLA-ANGST, Little
THINGS, FIGGS and WHISP. This is an extension for Martin, M. C
Catalogue (1998).
CHIPA was built to provide the most relevant parameters derived from
the HI line emission and high resolution HI interferometer maps for
galaxies published since 1953 until today. The new catalogue contains
more about a hundred galaxies from both hemispheres including
different morphological types.
High-resolution optical spectra of HD165052 (Ferrero+, 2013) at NOVA
Short Name:
NOVA HD 165052
Date:
14 Aug 2014 17:03:24
Publisher:
Nova
Description:
This is a set of high-resolution high-S/N optical spectra of the
massive binary star HD 165 052 (O7Vz + O7.5Vz) taken between 2008
April and 2011 May with echelle spectrographs at CASLEO (mainly), LCO
and ESO. Each one covers the spectral range 3700-6000 A with a
resolution varying between ~13000 and ~45000 @ 5000A according to the
instrument. Originally, the spectra were secured for radial velocity
measurements. More details about observations, instrument
configurations and reduction process can be found in documentation
section.
This collection is comprised of spectra from many different
researchers, observatories and instrumental configurations. Most of
them were used in publications (bibcode indicated at column "Ref.").
Band merged JHKs catalogue for first epoch data from CASU v1.3. VVV
DR1, corrected for header errors (Mike Irwin, Private Communication).
Release of the Milky Way bulge and southern plane from the
near-infrared ESO public survey VISTA variables in the Vía Láctea.
