Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Ben L. Tatton"'
Autor:
Vincenzo Ripepi, Y. Choi, Smitha Subramanian, Valentin D. Ivanov, Steven R. Majewski, Gisella Clementini, Jacco Th. van Loon, Dennis Zaritsky, Angus H. Wright, S. Rubele, Samyaday Choudhury, Ricardo R. Muñoz, Richard de Grijs, Clara M. Pennock, Florian Niederhofer, Noelia E. D. Noël, David Martínez-Delgado, Knut Olsen, Maria-Rosa L. Cioni, Pol Massana, Cameron P. M. Bell, David L. Nidever, A. Katherina Vivas, Joana M. Oliveira, Marcella Marconi, Ben L. Tatton
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
We present a map of the total intrinsic reddening across similar or equal to 34 deg(2) of the Small Magellanic Cloud (SMC) derived using optical (ugriz) and near-infrared (IR; YJK(s)) spectral energy distributions (SEDs) of background galaxies. The r
Autor:
Cameron P. M. Bell, Valentin D. Ivanov, David L. Nidever, Dennis Zaritsky, Samyaday Choudhury, Maria-Rosa L. Cioni, A. H. Wright, Knut Olsen, Smitha Subramanian, Jacco Th. van Loon, Joana M. Oliveira, Florian Niederhofer, Richard de Grijs, Y. Choi, Ben L. Tatton, Clara M. Pennock, David Martinez-Delgado, S. Rubele, Ricardo R. Muñoz
Publikováno v:
Monthly Notices of the Royal Astronomical Society
We present a method to map the total intrinsic reddening of a foreground extinguishing medium via the analysis of spectral energy distributions (SEDs) of background galaxies. In this pilot study, we implement this technique in two distinct regions of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e14bcbaafeb719bf5a83a912bc2a9879
http://arxiv.org/abs/1908.07538
http://arxiv.org/abs/1908.07538
Autor:
Marco Gullieuszik, M. I. Moretti, Vincenzo Ripepi, J. Th. van Loon, Jim Emerson, R. de Grijs, Gisella Clementini, Martin Groenewegen, Valentin D. Ivanov, Léo Girardi, Maria-Rosa L. Cioni, Stefano Rubele, Ben L. Tatton
Context: The details of how galaxies have evolved are imprinted in their star formation history, chemical enrichment and morpho-kinematic structure. Parameters behind these can be measured by combining photometric techniques with modelling. However,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ecefd885538542cd19b0d9ff07ac27c
Autor:
Marco Gullieuszik, Jim Emerson, Stefano Rubele, Léo Girardi, Ben L. Tatton, Martin Groenewegen, Maria-Rosa L. Cioni, Paola Marigo, Leandro Kerber, Joana M. Oliveira, Brent Miszalski, R. de Grijs, Kenji Bekki, Simone Zaggia, Valentin D. Ivanov, J. Th. van Loon
We derive the star formation history for several regions of the LMC, using deep near-infrared data from the VISTA near-infrared YJKs survey of the Magellanic system (VMC). The regions include three almost-complete 1.4 sqdeg tiles located 3.5 deg away
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95ef2e30b4d2cffb4d1c7c05811f19e9
http://hdl.handle.net/11577/2488459
http://hdl.handle.net/11577/2488459
Autor:
Marcella Marconi, Stefano Rubele, Vincenzo Ripepi, Valentin D. Ivanov, Ben L. Tatton, Jacco Th. van Loon, Smitha Subramanian, Joana M. Oliveira, Cameron P. M. Bell, Andrés E. Piatti, Richard de Grijs, Ning-Chen Sun, Kenji Bekki, Maria-Rosa L. Cioni
Publikováno v:
The Astrophysical Journal
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Star formation is a hierarchical process, forming young stellar structures of star clusters, associations, and complexes over a wide scale range. The star-forming complex in the bar region of the Large Magellanic Cloud is investigated with upper main
Autor:
Ning-Chen Sun, Richard de Grijs, Smitha Subramanian, Kenji Bekki, Cameron P. M. Bell, Maria-Rosa L. Cioni, Valentin D. Ivanov, Marcella Marconi, Joana M. Oliveira, Andrés E. Piatti, Vincenzo Ripepi, Stefano Rubele, Ben L. Tatton, Jacco Th. van Loon
Publikováno v:
Astrophysical Journal; 11/10/2017, Vol. 849 Issue 2, p1-1, 1p