User: Juandesant

Name: Juandesant

Joined: Wednesday 25 January 2012 16:55:07 (UTC)

Last seen: Friday 30 January 2015 14:54:55 (UTC)

Email (public): jdsant [at] iaa.es

Website: http://amiga.iaa.es/p/49-juan-de-dios-santander.htm

Location: Granada, Spain

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1 Group (admin)

2 Groups (member)

1 Workflows

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Juandesant has been credited 3 times

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Being in the web since always, now using it to provide astronomical content and methodologies.

Other contact details:

Not specified

Interests:

big data, virtual observatory, e-Science

Field/Industry: Astronomy

Occupation/Role(s): VIA-SKA Project Manager / AMIGA DB Radio Astronomer

Organisation(s):

Instituto de Astrofísica de Andalucía (IAA-CSIC)
Wf4Ever Project

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Workflow

Taverna 2

Uploader

Juandesant

CSV to VOTable importer (2)

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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: Juandesant AMIGA Wf4Ever

Workflow

Taverna 2

Uploader

Jose Enrique Ruiz

Environment (2)

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From a previously selected cube of galaxies residing in a remote database, we provide extragalactic environment parameters for all galaxies sample. This workflow takes as input the path of the tabular *.pckl Python pickle dataset created in the previous workflow, as well as the database connection settings and several criteria on how to filter the potential companions of the target galaxies. It provides a file with the SDSS identifiers of each target galaxy of the sample, environmental estim...

Created: 2013-01-04 | Last updated: 2013-01-14

Credits: Juandesant Jsm

Workflow

Taverna 2

Uploader

Jose Enrique Ruiz

Intialize Sample (2)

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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: Juandesant Jsm

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