Subject: spectroscopy / Content Level: General / Validation Level: 2

ID:: ivo://vopdc.obspm/lesia/BeStars
Title:: Be Stars Database
Short Name:: BeStars
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre - LESIA
Description:: The BeStars project contains (1) the complete catalogue of classical Be stars, BeSC, with some of their fundamental stellar parameters, and (2) a database, BeSS, which assembles classical Be star spectra obtained by professional and amateur astronomers at any wavelength, epoch, and spectral resolution.

ID:: ivo://vopdc.obspm/lesia/BeStars/BeSS
Title:: Be Stars Spectra
Short Name:: BeSS
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre - LESIA
Description:: The BeSS database assembles classical Be star spectra obtained by professional and amateur astronomers at any wavelength, epoch, and spectral resolution.

ID:: ivo://padc.obspm.planeto/vims_satellites/q/epn_core
Title:: Cassini VIMS
Short Name:: VIMS satellites
Date:: 04 Feb 2024 04:04:45
Publisher:: Paris Astronomical Data Centre
Description:: The Visual and Infrared Mapping Spectrometer (VIMS) instrument onboard the Cassini spacecraft observed the system of Saturn, acquiring spectral cubes in the range 0.4-5.2 microns. This service focuses on Saturn satellites, and provides access to calibrated and ancillary data, computed as described here: https://vims.univ-nantes.fr/info/isis-calibration. It also provides direct links to a larger web site with previews.

ID:: ivo://vopdc.obspm/dfbs
Title:: Digitized First Byurakan Survey
Short Name:: DFBS
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre
Description:: The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.

ID:: ivo://padc.obspm.planeto/iks/q/epn_core
Title:: IKS
Short Name:: IKS
Date:: 23 Nov 2022 16:32:49
Publisher:: Paris Astronomical Data Centre - LESIA
Description:: Measurements of comet Halley in the spectral channel of IKS on board the Vega-1 spacecraft. Data are retrieved from the PDS Small Bodies Node data set (2011 reformatted version) and updated. The data set consists in 101 tables providing the radiance spectrum of comet Halley from various distances, plus two composite spectra. For details and further references, see: Combes M. et al., 1988, The 2.5-12 micron Spectrum of Comet Halley from the IKS-VEGA Experiment, Icarus, 76, 404-436 [1988Icar...76..404C]

ID:: ivo://bira-iasb/nomad/q/epn_core
Title:: Mars atmospheric profiles - From NOMAD/TGO
Short Name:: nomad.epn_core
Date:: 28 Oct 2023 16:48:34
Publisher:: Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
Description:: Profiles of pressure, temperature and species of the Martian atmosphere derived from measurements of the NOMAD instrument on board ESA's Trace Gas Orbiter. See paper https://doi.org/10.1007/s11214-018-0517-2

ID:: ivo://padc.obspm.planeto/m4ast/q/epn_core
Title:: M4AST
Short Name:: M4AST
Date:: 23 Nov 2022 16:33:33
Publisher:: Paris Astronomical Data Centre - IMCCE
Description:: compiled database for asteroid spectra in the visible and NIR regions

ID:: ivo://bira-iasb/soir/soir_q/epn_core
Title:: SOIR
Short Name:: soir.epn_core
Date:: 28 Oct 2023 16:49:38
Publisher:: Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
Description:: Profiles of species in Venus atmosphere terminator. Data retrieved from calibrated spectra obtained with the SPICAV-SOIR instrument on board the Venus Express spacecraft. These spectra can be checked on the ESA PSA repository. See: A.C. Vandaele et al., Contribution from SOIR/VEX to the updated Venus International Reference Atmosphere (VIRA), Adv. Space Res. (2015), http://dx.doi.org/10.1016/j.asr:2015.08.012.

ID:: ivo://padc.obspm.planeto/basecom/q/epn_core
Title:: The Nançay Cometary Database
Short Name:: basecom.epn_core
Date:: 02 May 2024 18:54:10
Publisher:: Paris Astronomical Data Centre
Description:: Since 1973, the 18-cm lines of the OH radical have been systematically observed in a number of comets with the Nançay radio telescope. This allowed an evaluation of the cometary water production rates and their evolution with time, as well as a study of several physical processes: the excitation mechanisms of the OH radio lines, the expansion of the cometary atmospheres, their anisotropy in relation with non-gravitational forces, the Zeeman effect in relation with the cometary magnetic field. The Nançay observations of 53 cometary apparitions between 1982 and 2009 are now organized in this database.

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