This service publishes plate scans of the Palomar-Leiden Troian
surveys conducted between 1960 and 1977. The surveys led to the
discovery of more than 2,000 asteroids (1,800 with orbital information),
with another 2,400 asteroids, including 19 Trojans, found after further
analysis of the plates.
Note that because of the large size of the plates, in this service each
original plate is contained in two parts, marked with "_1" and "_2",
respectively. The central parts
of the two parts overlap.
The resource contains the recommendations and requirements for ALMA
FITS products of the Inter-ARC ALMA Science Archive Working Group
(ASAWG) with the view to including a metadataset that is complete and
easily accessible by the ChiVO Data Provider (CDP).
SMAKCED H-band images of Early-Type Virgo Dwarf Galaxies
Short Name:
smakced H images
Date:
23 Mar 2022 13:13:18
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
The The VO @ ASTRON's sitewide SIAP version 2 service
publishes all the images published through the site. For more advanced
queries including uploads, all this data is also available through
ObsTAP.
These are 1.4GHz Very Long Baseline Interferometry images of 532
radio sources with a flux density exceeding 100uJy as determined by
Ibar et al. (2009, MNRAS, 397, 281), obtained between 2010-06-03 and
2010-09-03.
For all fields, we give frames processed using natural weighting to
preserve maximal sensitivity. For the 65 detected sources, we
additionally give frames processed using uniform weighting to suppress
sidelobes (see Middelberg et al. 2013, A&A 551, 97 for details) in
flux density measurements. Some sources have larger images to cover a
larger area because the initial coordinates were not sufficiently
accurate.