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
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
Smithsonian Astrophysical Observatory Telescope Data Center Dataset Delivery
Short Name:
SAO TDC DL
Date:
17 Mar 2021 09:32:35
Publisher:
Smithsonian Astrophysical Observatory Telescope Data Center
Description:
This service delivers (most of) the datasets held at
Smithsonian Astrophysical Observatory Telescope Data Center. In addition to the default (nonstandard)
way of just appending accrefs to the get access URL, there is also a
very simple datalink service here that, for each dataset, essentially
just gives the dataset itself and possibly a preview. More advanced
datalink services might be available.
Some datasets may be embargoed, in which case the access yields a 403.
Credentials for individual files may be obtained by contacting the
site operators.
Catalogues of solar observations held at MSSL/UCL. Datasets available are SOHO CDS, SOHO EIT, Yohkoh SXT. URL links to data files are provided (EIT data files provided by SDAC, NASA). Reference: http://www.mssl.ucl.ac.uk/www_solar/surfindex.html
Solar Radio Emission Observations at “Orbita” Radio Polygon
Short Name:
solar_flux data
Date:
12 Dec 2024 19:58:36
Publisher:
Fesenkov Astrophysical Institute
Description:
The “Orbita” Radio Polygon at an altitude of 2750 meters conducts solar radio emission observations using state-of-the-art equipment. This includes instruments for monitoring solar radio flux at frequencies of 1 GHz and 2.8 GHz, as well as the Callisto solar radio spectrograph, which is part of the international e-Callisto network. These tools enable the detection of solar radio bursts of types II, III, IV, and V, and provide valuable insights for forecasting the geo-effectiveness of solar flare activity.
The provided dataset consists of daily tables, where each table corresponds to a single observation day. The data includes two columns:
- **timestamp**: The time of observation at the detector.
- **SFU**: The solar flux unit measurement, representing the intensity of solar radio emission in SFU (Solar Flux Units).
The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).
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
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>`_.
