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1. ALHAMBRA Final Catalogue
ID:
ivo://svo.cab/alhambra
Title:
ALHAMBRA Final Catalogue
Short Name:
ALHAMBRA
Date:
03 Jun 2020 15:33:39
Publisher:
SVO CAB
Description:
This data server provides access to the ALHAMBRA Final Catalogue. The ALHAMBRA (Advance Large Homogeneous Area Medium Band Redshift Astronomical) survey (Moles et al. 2008) has observed 8 different regions of the sky, including sections of the COSMOS, DEEP2, ELAIS, GOODS-N, SDSS and Groth fields using a new photometric system with 20 contiguous, non-overlapping, equal width (~ 300A) filters, covering the optical range (3500A-9700A), plus the standard broadband NIR J, H and Ks filters. The observations were carried out with the Calar Alto (CAHA) 3.5m telescope using the wide field, 0.25 deg2 FOV optical camera LAICA and the NIR instrument Omega-2000. The ALHAMBRA survey dataset represents a ~700hrs of total exposure time, gathered in between the 2005 and 2012.Further information on the project can be found at the ALHAMBRA web page.
2. ASK Classification
ID:
ivo://svo.cab/ask
Title:
ASK Classification
Short Name:
ASK
Date:
14 Mar 2019 08:42:54
Publisher:
SVO CAB
Description:
Access to the results of the unsupervised classification of all galaxy spectra in the seventh and final Sloan Digital Sky Survey data release (SDSS/DR7) as described in Sanchez Almeida et al. (2010 ApJ 714,487S). 99% of the galaxies can be assigned to only 17 major classes, with 11 additional minor classes including the remaining 1%.
3. CMC15, Carlsberg Meridian Catalogue
ID:
ivo://svo.cab/cmc15
Title:
CMC15, Carlsberg Meridian Catalogue
Short Name:
CMC15
Date:
03 Jun 2020 15:34:50
Publisher:
SVO CAB
Description:
CMC15 is an astrometric and photometric catalogue of more than 122.7 million stars in the magnitude range 9 < r' (SDSS) < 17. With a positional accuracy to about 35 mas, the catalogue covers the declination range -40deg to 50deg. The current release comprises all the observations made between March 1999 and March 2011. The catalogue fills the gap between 5h 30m and 10h 30m for declinations south of -15deg of the CMC14 and adds the bans -30deg to -40deg. Some zones north of -30deg have also been re-observed in order to improve their internal errors.
5. Spitzer Taurus conesearch
ID:
ivo://svo.cab/spitzertaurus
Title:
Spitzer Taurus conesearch
Short Name:
Spitzer Taurus
Date:
14 Mar 2019 08:20:19
Publisher:
SVO CAB
Description:
Spitzer Taurus access
6. Stars with Debris Disks and Planets
ID:
ivo://svo.cab/debris
Title:
Stars with Debris Disks and Planets
Date:
23 Jan 2017 10:09:28
Publisher:
SVO CAB
Description:
Planetary systems are built by planets and planetesimals formed in circumstellar disks surrounding young pre-main sequence stars. Once in the main-sequence collisions of planetesimals produce small dust particles giving rise to the so-called debris disks. The mutual interaction among planets, planetesimals and debris disks, and with their host stars determines the fate of planetary systems. Currently thousands of main-sequence stars are known to host planets and debris disks. The Solar System with its peculiarities is just one of such planetary systems. However, only few tens of stars are known to host simultaneously both planets and debris disks. Therefore, the study of those systems is particularly valuable to widen our knowledge of planetary systems and their evolution. This page just collects some of the properties of the known, to our knowledge, solar-type stars hosting both planets and debris disk.
7. TESELA
ID:
ivo://svo.cab/tesela
Title:
TESELA
Short Name:
TESELA
Date:
14 Mar 2019 08:20:45
Publisher:
SVO CAB
Description:
The most important advantage of widefield cameras is, precisely, the "widefield", since this offers the observers the possibility of obtaining vast amounts of data in a much shorter observing time. However, for a reliable data interpretation, it is necessary a proper data calibration. Concerning the flatfielding of images, many times it is required to obtain several integrations in blank regions (sky patches without bright sources) nearby to the science target areas. TESELA is a service developed to provide access to a catalogue of blank regions, based on the application of the Delaunay triangulation of the sky. The present implementation of TESELA uses as source for the star coordinates the Tycho-2 Catalogue (Hog et al. 2000). The system has been jointly developed by the Department of Astrophysics of the Universidad Complutense de Madrid and CAB (INTA-CSIC) and is maintained at CAB (INTA-CSIC). If you use TESELA in your research, please include the following acknowledgement in any resulting publications: "This publication makes use of TESELA, developed under the Spanish Virtual Observatory project supported from the Spanish MICINN through grant AyA2008-02156." "Partially funded by the Spanish MICINN under the Consolider-Ingenio 2010 Program grant CSD2006-00070: First Science with the GTC"