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In the last decade, the development of information and communication technologies (ICTs) has impl... more In the last decade, the development of information and communication technologies (ICTs) has imply a significant change in the traditional distance learning and specifically in e-learning. The new tools developed are consolidating the online learning modality at the university level all over the world and in all disciplines.In this study, we present the case of the Master of Astronomy and Astrophysics which is running from 2010 in the Valencian International University (http://www.viu.es). Unlike other more consolidated distance universities in Spain, the teaching method which has opted in this case includes an element of presence via webcam. This method could be considered as a kind of blended learning, combining the advantages of traditional e-learning with the humanity of personal and direct contact with the students.The results of participation in the master beyond the initial expectations with 37 students enrolled, of which approximately 80% were Spanish and the other 20% were mostly from Latin American countries. The feedback provided by students in the first months of teaching appreciates favorably the presence component, while casting doubt on the usefulness of certain tools traditionally used in the field of e-learning.
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Papers by Vicent Martínez
Mètode: Revista de difusió de la investigació de la Universitat de Valencia, 2013
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Monthly Notices of the Royal Astronomical Society, 2021
This paper proposes a morphostatistical characterization of the galaxy distribution through spati... more This paper proposes a morphostatistical characterization of the galaxy distribution through spatial statistical modelling based on inhomogeneous Gibbs point processes. The galaxy distribution is supposed to exhibit two components. The first one is related to the major geometrical features exhibited by the observed galaxy field, here, its corresponding filamentary pattern. The second one is related to the interactions exhibited by the galaxies. Gibbs point processes are statistical models able to integrate these two aspects in a probability density, controlled by some parameters. Several such models are fitted to real observational data via the ABC shadow algorithm. This algorithm provides simultaneous parameter estimation and posterior-based inference, hence allowing the derivation of the statistical significance of the obtained results.
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A study of the galaxy distribution in the field of the elliptical galaxy NGC1600 has been underta... more A study of the galaxy distribution in the field of the elliptical galaxy NGC1600 has been undertaken. Although this galaxy is often classified as a member of a loose group, all the neighbouring galaxies are much fainter and could be taken as satellites of NGC1600. The number density profile of galaxies in the field of this galaxy shows a decline with radius, with evidence of a background at approximately 1.3 Mpc. The density and number density profile are consistent with that found for other isolated early-type galaxies. NGC1600 appears as an extended source in X-rays, and the center of the X-ray emission seems not to coincide with the center of the galaxy. The velocity distribution of neighbouring galaxies has been measured from optical spectroscopic observations and shows that the mean radial velocity is approximately 85 km s −1 less than that of NGC1600, indicating that the centre of mass could lie outside the galaxy. The velocity dispersion of the ‘group ’ is estimated at 429 ± ...
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Astronomy & Astrophysics, 2021
The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will scan thousa... more The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will scan thousands of square degrees of the northern sky with a unique set of 56 filters using the dedicated 2.55 m Javalambre Survey Telescope (JST) at the Javalambre Astrophysical Observatory. Prior to the installation of the main camera (4.2 deg2 field-of-view with 1.2 Gpixels), the JST was equipped with the JPAS-Pathfinder, a one CCD camera with a 0.3 deg2 field-of-view and plate scale of 0.23 arcsec pixel−1. To demonstrate the scientific potential of J-PAS, the JPAS-Pathfinder camera was used to perform miniJPAS, a ∼1 deg2 survey of the AEGIS field (along the Extended Groth Strip). The field was observed with the 56 J-PAS filters, which include 54 narrow band (FWHM ∼ 145 Å) and two broader filters extending to the UV and the near-infrared, complemented by the u, g, r, i SDSS broad band filters. In this miniJPAS survey overview paper, we present the miniJPAS data set (images and catalogs), as we hi...
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Metode Revista De Difusio De La Investigacio De La Universitat De Valencia, 2014
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Metode Revista De Difusio De La Investigacio De La Universitat De Valencia, 2010
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Metode Revista De Difusion De La Investigacion, 2011
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Metode Revista De Difusion De La Investigacion, 2010
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Metode Revista De Difusio De La Investigacio De La Universitat De Valencia, 2010
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Recovering the real-space correlation function from
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Astronomy & Astrophysics, 2015
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SPIE Proceedings, 2002
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Nuovo Cimento della Societa Italiana di Fisica B, 2007
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The Astrophysical Journal, 2009
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The Astrophysical Journal, 2005
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The Astrophysical Journal, 1999
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The Astrophysical Journal, 1994
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In the last decade, the development of information and communication technologies (ICTs) has impl... more In the last decade, the development of information and communication technologies (ICTs) has imply a significant change in the traditional distance learning and specifically in e-learning. The new tools developed are consolidating the online learning modality at the university level all over the world and in all disciplines.In this study, we present the case of the Master of Astronomy and Astrophysics which is running from 2010 in the Valencian International University (http://www.viu.es). Unlike other more consolidated distance universities in Spain, the teaching method which has opted in this case includes an element of presence via webcam. This method could be considered as a kind of blended learning, combining the advantages of traditional e-learning with the humanity of personal and direct contact with the students.The results of participation in the master beyond the initial expectations with 37 students enrolled, of which approximately 80% were Spanish and the other 20% were mostly from Latin American countries. The feedback provided by students in the first months of teaching appreciates favorably the presence component, while casting doubt on the usefulness of certain tools traditionally used in the field of e-learning.
Bookmarks Related papers MentionsView impact
Mètode: Revista de difusió de la investigació de la Universitat de Valencia, 2013
Bookmarks Related papers MentionsView impact
Monthly Notices of the Royal Astronomical Society, 2021
This paper proposes a morphostatistical characterization of the galaxy distribution through spati... more This paper proposes a morphostatistical characterization of the galaxy distribution through spatial statistical modelling based on inhomogeneous Gibbs point processes. The galaxy distribution is supposed to exhibit two components. The first one is related to the major geometrical features exhibited by the observed galaxy field, here, its corresponding filamentary pattern. The second one is related to the interactions exhibited by the galaxies. Gibbs point processes are statistical models able to integrate these two aspects in a probability density, controlled by some parameters. Several such models are fitted to real observational data via the ABC shadow algorithm. This algorithm provides simultaneous parameter estimation and posterior-based inference, hence allowing the derivation of the statistical significance of the obtained results.
Bookmarks Related papers MentionsView impact
A study of the galaxy distribution in the field of the elliptical galaxy NGC1600 has been underta... more A study of the galaxy distribution in the field of the elliptical galaxy NGC1600 has been undertaken. Although this galaxy is often classified as a member of a loose group, all the neighbouring galaxies are much fainter and could be taken as satellites of NGC1600. The number density profile of galaxies in the field of this galaxy shows a decline with radius, with evidence of a background at approximately 1.3 Mpc. The density and number density profile are consistent with that found for other isolated early-type galaxies. NGC1600 appears as an extended source in X-rays, and the center of the X-ray emission seems not to coincide with the center of the galaxy. The velocity distribution of neighbouring galaxies has been measured from optical spectroscopic observations and shows that the mean radial velocity is approximately 85 km s −1 less than that of NGC1600, indicating that the centre of mass could lie outside the galaxy. The velocity dispersion of the ‘group ’ is estimated at 429 ± ...
Bookmarks Related papers MentionsView impact
Bookmarks Related papers MentionsView impact
Bookmarks Related papers MentionsView impact
Astronomy & Astrophysics, 2021
The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will scan thousa... more The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will scan thousands of square degrees of the northern sky with a unique set of 56 filters using the dedicated 2.55 m Javalambre Survey Telescope (JST) at the Javalambre Astrophysical Observatory. Prior to the installation of the main camera (4.2 deg2 field-of-view with 1.2 Gpixels), the JST was equipped with the JPAS-Pathfinder, a one CCD camera with a 0.3 deg2 field-of-view and plate scale of 0.23 arcsec pixel−1. To demonstrate the scientific potential of J-PAS, the JPAS-Pathfinder camera was used to perform miniJPAS, a ∼1 deg2 survey of the AEGIS field (along the Extended Groth Strip). The field was observed with the 56 J-PAS filters, which include 54 narrow band (FWHM ∼ 145 Å) and two broader filters extending to the UV and the near-infrared, complemented by the u, g, r, i SDSS broad band filters. In this miniJPAS survey overview paper, we present the miniJPAS data set (images and catalogs), as we hi...
Bookmarks Related papers MentionsView impact
Metode Revista De Difusio De La Investigacio De La Universitat De Valencia, 2014
Bookmarks Related papers MentionsView impact
Metode Revista De Difusio De La Investigacio De La Universitat De Valencia, 2010
Bookmarks Related papers MentionsView impact
Metode Revista De Difusion De La Investigacion, 2011
Bookmarks Related papers MentionsView impact
Metode Revista De Difusion De La Investigacion, 2010
Bookmarks Related papers MentionsView impact
Metode Revista De Difusio De La Investigacio De La Universitat De Valencia, 2010
Bookmarks Related papers MentionsView impact
Recovering the real-space correlation function from
Bookmarks Related papers MentionsView impact
Astronomy & Astrophysics, 2015
Bookmarks Related papers MentionsView impact
SPIE Proceedings, 2002
Bookmarks Related papers MentionsView impact
Nuovo Cimento della Societa Italiana di Fisica B, 2007
Bookmarks Related papers MentionsView impact
The Astrophysical Journal, 2009
Bookmarks Related papers MentionsView impact
The Astrophysical Journal, 2005
Bookmarks Related papers MentionsView impact
The Astrophysical Journal, 1999
Bookmarks Related papers MentionsView impact
The Astrophysical Journal, 1994
Bookmarks Related papers MentionsView impact
The Astrophysical Journal, 2004
Bookmarks Related papers MentionsView impact