Publisher: The GAVO DC team - STScI NAVO Directory Search Results

ID:: ivo://org.gavo.dc/elsnersim/q/s
Title:: Simulated non-Gaussian CMB maps
Short Name:: cmb_ng
Date:: 27 Dec 2024 08:31:03
Publisher:: The GAVO DC team
Description:: Simulated non-Gaussian temperature and polarization CMB maps. The non-Gaussian simulations have been generated using the algorithm described in :bibcode:`2009ApJS..184..264E` up to a multipole moment of l_max = 1024. The transfer functions were computed with CAMB version February 2009 and RECFAST 1.5.

ID:: ivo://org.gavo.dc/smakced/q/cat
Title:: SMAKCED Census of Structure in Early-type Dwarf Galaxies
Short Name:: smakced census
Date:: 27 Dec 2024 08:31:13
Publisher:: The GAVO DC team
Description:: The Stellar content, MAss and Kinematics of Cluster Early-type Dwarf galaxies (SMAKCED_) project is a survey of 121 Virgo cluster early type galaxies. This service publishes deep near-infrared (H band) images obtained by SMAKCED together with `resulting decompositions`_ and other properties of the galaxies in the sample. .. _SMAKCED: http://smakced.net .. _resulting decompositions: http://smakced.net/data.html

ID:: ivo://org.gavo.dc/smakced/q/im
Title:: SMAKCED H-band images of Early-Type Virgo Dwarf Galaxies
Short Name:: smakced H images
Date:: 27 Dec 2024 08:31:13
Publisher:: The GAVO DC team
Description:: The Stellar content, MAss and Kinematics of Cluster Early-type Dwarf galaxies (SMAKCED_) project is a survey of 121 Virgo cluster early type galaxies. This service publishes deep near-infrared (H band) images obtained by SMAKCED together with `resulting decompositions`_ and other properties of the galaxies in the sample. .. _SMAKCED: http://smakced.net .. _resulting decompositions: http://smakced.net/data.html

ID:: ivo://org.gavo.dc/sp_ace/q/c
Title:: SP_ACE spectral analysis tool
Short Name:: sp_ace
Date:: 27 Dec 2024 08:31:01
Publisher:: The GAVO DC team
Description:: SP_ACE computes stellar parameters (gravity, temperature) and element abundances from optical stellar spectra (`sample spectrum`_). It employs 1D stellar atmosphere models in Local Thermodynamic Equilibrium (LTE). The present service does not offer all the options available for SP_Ace as documented in `the tutorial`_. All options are available if running SP_Ace locally (cf. `download page`_). This service exposes an updated version containing some bug fixes with respect to the one described in the paper. .. _the tutorial: http://dc.g-vo.org/sp_ace/q/dist/static/tutorial.pdf .. _download page: http://dc.g-vo.org/sp_ace/q/dist/static .. _sample spectrum: http://dc.g-vo.org/sp_ace/q/c/static/fast_spectrum.txt

ID:: ivo://org.gavo.dc/mlqso/q/q
Title:: Spectra of lensed QSOs (SSAP)
Short Name:: mlqso bidi ssa
Date:: 27 Dec 2024 08:31:12
Publisher:: The GAVO DC team
Description:: An archive of optical and near-infrared spectra of strongly lensed quasars and the lensing galaxies. The spectra are resolved to about a few Ångstroms and are flux-calibrated. The spectra resulted from deblending the lensed images in bidimensional spectra available from the SSAP service for `ivo://org.gavo.dc/mlqso/q/s <http://dc.g-vo.org/mlqso/q/s/info>`_.

ID:: ivo://org.gavo.dc/casa_lines/q/line_tap
Title:: Splatalogue CASA LineTAP
Short Name:: Spltlg radio
Date:: 27 Dec 2024 08:31:05
Publisher:: The GAVO DC team
Description:: This is a rendering of the `CASA Offline Splatalogue`_ in a draft LineTAP, mainly intended to enable verification of the standard. This is not recommended for production yet. In particular, many InChIs are known wrong, and we have skipped several hundred lines because we did have no InChIs for their species at all. .. _CASA Offline Splatalogue: https://safe.nrao.edu/wiki/bin/view/ALMA/CASA_Offline_Splat_list

ID:: ivo://edu.gavo.org/eurovo/cosadie_star_clusters
Title:: Star clusters
Date:: 27 Dec 2024 08:31:13
Publisher:: The GAVO DC team
Description:: Within this use case you learn about the difference between intrinsic linear size and apparent angular size, a difference that is frequently at the center of astronomical problems. Star clusters are the objects used to illustrate this difference. You also learn some basic facts about star clusters, whose distribution in space has helped us to understand the structure of our Milky Way. Thanks to Aladin, you will be able to explore their distribution on the sky on your own.

ID:: ivo://org.gavo.dc/stctrans/q/utypes
Title:: STC utype generator
Short Name:: stcs to utype
Date:: 27 Dec 2024 08:31:05
Publisher:: The GAVO DC team
Description:: This services converts the representations of STC objects in XML, utypes, and STC-S into each other.

ID:: ivo://edu.gavo.org/eurovo/cosadie_stellarium
Title:: Stellarium for Beginners
Date:: 27 Dec 2024 08:31:12
Publisher:: The GAVO DC team
Description:: Within this use case you learn about Stellarium's main features, each presented with examples taken from its most common use.

ID:: ivo://org.gavo.dc/gcpms/q/data
Title:: Stellar Proper Motions in the Ogle II Galactic Bulge Fields
Short Name:: gcpms.data
Date:: 27 Dec 2024 08:31:03
Publisher:: The GAVO DC team
Description:: A proper-motion catalogue of 5080236 stars in 49 OGLE-II Galactic bulge (GB) fields, covering a range of -11°<l<11° and -6°<b<3°. Some columns have been left out from the original source.

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