Drift-Phoenix is a computer code that simulates the structure of an atmosphere including the formation of clouds. The code is part of the Phoenix-code family. Drift describes the formation of mineral clouds and allows to predict cloud details, like the size of the cloud particles and their composition.
The science archive of the ELODIE spectrograph contains all the spectra collected by the instrument between 1993 and 2006 (total life time of the instrument). ELODIE is an echelle spectrograph providing a resolution R=42000 in the spectral range 390-680 nm. The web interface of the archive distribute a variety of products, and the SSA service gives the reconnected 1D spectra in instrumental flux (not physical). This service is given for test: The spectra cannot be viewved with VOSpec because they are not flux-calibrated.
Epic Spectra SSAP of the SSC Interface for the 4XMM Catalogue
Short Name:
4XMM-SSA
Date:
07 Apr 2021 13:40:35
Publisher:
Observatory of Strasbourg, SSC Team
Description:
The 4XMM-DR10 catalogue contains source detections drawn from 11647 XMM-Newton EPIC observations,
covering an energy interval from 0.2 keV to 12 keV. These observations were made between 2000 February 3
and 2019 December 14 and all datasets were publicly available by 2020 December 10,
but not all public observations are included in this catalogue .
This version of the XMM-Newton EPIC Serendipitous Source Catalogue,
4XMM-DR10 includes 748670 clean detections which relate to 575158 unique
sources from 11647 observations that were public by 2020 December 10.
3XMM-DR7 covers a total sky area of ~1192 square degrees if overlaps
are taken into account, where some
regions of the sky have been pointed as many as 50 times.
The median flux in the total photon energy band (0.2 - 12 keV) of the
catalogue detections is ~ 8.3 × 10-14 erg cm-2 s-1; in the soft energy band (0.2 - 2 keV)
the median flux is ~ 5.3 × 10-15, and in the hard band (2 - 12 keV) it is ~ 1.2 × 10-14.
About 23% of the sources have total fluxes below 1 × 10-14 erg cm-2 s-1.
The ESO Simple Spectral Access service provides access to the 1D reduced spectra generated either by the principal investigators of ESO observations, or by an unattended ESO processing-pipeline that makes use of certified master calibrations. The spectra are FITS files adhering to the ESO Science Data Product standard, based on the Virtual Observatory Spectral Data Model standard (v1.0 for some spectra, and v2.0 for some others, use the VOCLASS FITS keyword to discern the two).
Science spectra from the HST collection hosted at ESAC/ESA. All public HST observations in calibrated and science-ready form are synchronised with the MAST services for HST reprocessed public data and corresponding metadata. The European HST archive interface can be accessed at https://hst.esac.esa.int/ehst
The Extreme Ultraviolet Explorer (EUVE) was a NASA-funded satellite
launched in June 1992 which obtained extreme ultraviolet spectra (70 - 760 Angstroms)
of over 350 unique astronomical targets. The science payload, was designed and built
at the Space Sciences Laboratory at the University of California, Berkeley, under
the direction of Dr. Roger F. Malina. The program ended in January, 2001. These
particular spectra were extracted by Damian Christian, formerly of the EUVE project,
and reformatted by MAST staff.