Workflows

Search filter terms
Filter by type
Filter by tag
Filter by user
Filter by licence
Filter by group
Results per page:
Sort by:
Showing 47 results. Use the filters on the left and the search box below to refine the results.
Tag: astrotaverna

Workflow Astronomical object name to equatorial coo... (1)

Thumb
 Resolve equatorial coordinates of a list of objects (names) with AstroTaverna plugin

Created: 2012-06-30 | Last updated: 2012-07-01

Credits: User Jose Enrique Ruiz

Workflow VOTable of NED Images from a List of Objects (1)

Thumb
Extraction of metadata using NED Image Virtual Observatory Service into a single VOTable, providing a list of objects and the width for each field in arcmin. Among the most relevant metadata are the URL link to the FITS images. This Wf makes use of a Tool developed as an internal pyhton script file.

Created: 2012-07-01 | Last updated: 2012-07-01

Credits: User Jose Enrique Ruiz

Attributions: Workflow Astronomical object name to equatorial coordinates Resolver

Workflow Extract a column from a VOTable into a List (3)

Thumb
Snippet showing how to use AstroTaverna tool for extracting a column from a VOTable into a single List.

Created: 2013-03-08 | Last updated: 2013-04-22

Credits: User Julian Garrido User Susana

Workflow Discovery of Brown Dwarfs mining the 2MASS... (1)

Thumb
Brown dwarfs are objects occupying the gap between the least massive stars and the most massive planets. They are intrinsically faint objects so their detection is not straighforward and, in fact, was almost impossible until the advent of global surveys at deep optical and near-infrared bands like SDSS, 2MASS or DENIS among others. Here we propose to mine the SDSS and 2MASS databases to identify T-type brown dwarfs through an appropriate combination of colours in the optical and the infra-red...

Created: 2013-04-12

Credits: User Jose Enrique Ruiz

Workflow Crossmatching VOTables (2)

Thumb
Snippet showing how to use AstroTaverna tool for crossmatching two VOTables VOTable samples may be downloaded from MyExperiment http://www.myexperiment.org/files/911/versions/1/download/SDSS7.vot http://www.myexperiment.org/files/910/versions/1/download/2MASS.vot

Created: 2013-04-12 | Last updated: 2013-04-22

Credits: User Jose Enrique Ruiz

Workflow Retrieving information from HST ConeSearch... (1)

Thumb
This workflow retieves information from Hubble Space Telescope VO Services in the form of VOTables. The input of the workflow is an ASCII file with a list of source names. This file is converted to a VOTable, and coordinates added with an extra-column needed to query SIAP Image service. The final result are two different VOTables issued as the response of both VO Services, Images VOTable has been previously filtered.

Created: 2013-04-12

Workflow Table format coversion: ASCII to VOTable (2)

Thumb
Snippet showing how to use AstroTaverna tool for table format conversion

Created: 2013-04-12 | Last updated: 2013-04-12

Workflow Find asteroids in images from CAHA observa... (1)

Thumb
It analyzes images from CAFOS instrument in Calar Alto Observatory. It uses SkyBot catalog in order to identify objects in the Solar System. It includes a double check to avoid objets that are not asteroids (comparing with USNO and 2MASS catalogs). The result is a VOTable of asteroids

Created: 2013-07-17

Credits: User Julian Garrido

Attributions:

Workflow CSV to VOTable importer (2)

Thumb
This module provides a VOTable representation of the CSV file being pointed by the csv_file_path, either as a POSIX local file path, or a URL.

Created: 2013-07-29 | Last updated: 2013-07-29

Credits: User Juandesant Network-member AMIGA Network-member Wf4Ever

Workflow Intialize Sample (2)

Thumb
This workflow saves a tabular *.pckl Python pickle dataset in the local file system, containing values calculated on physical parameters associated to potential companions of a sample of target galaxies. These original physical parameters are extracted from a postgreSQL database, containing information of all galaxies covered by the SDSS spectroscopic survey. The workflow first access the external database located in the AMIGA server and selects the target galaxies from the sample (those havi...

Created: 2013-01-04 | Last updated: 2013-01-05

Credits: User Juandesant User Jsm

Results per page:
Sort by: