Zobrazeno 1 - 10
of 109
pro vyhledávání: '"N. Castro Rodríguez"'
Autor:
N. Castro-Rodríguez, M. E. Camisassa, Mark Hollands, Detlev Koester, Tim Cunningham, A. T. Knowles, Roberto Raddi, Pier-Emmanuel Tremblay, Alberto Rebassa-Mansergas, Santiago Torres, Jinwei Ren, Matthew J. Hoskin, Jesus Maldonado, Boris T. Gänsicke
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The age-metallicity relation is a fundamental tool for constraining the chemical evolution of the Galactic disc. In this work we analyse the observational properties of this relation using binary stars that have not interacted consisting of a white d
Autor:
H. Bouy, M. Tamura, D. Barrado, K. Motohara, N. Castro Rodríguez, N. Miret-Roig, M. Konishi, S. Koyama, H. Takahashi, N. Huélamo, E. Bertin, J. Olivares, L. M. Sarro, A. Berihuete, J.-C. Cuillandre, P. A. B. Galli, Y. Yoshii, T. Miyata
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 664, ⟨10.1051/0004-6361/202243850⟩
Astronomy and Astrophysics-A&A, 2022, 664, ⟨10.1051/0004-6361/202243850⟩
Context: A rich population of low-mass brown dwarfs and isolated planetary mass objects has been reported recently in the Upper Scorpius and Ophiuchus star forming complex. Aims: We investigate the membership, nature and properties of 17 of these iso
Autor:
Pablo Rodríguez-Gil, Mark Hollands, Roi Alonso, N. Castro-Rodríguez, Nicolas Lodieu, Paula Izquierdo, A. Cabrera-Lavers, Hans J. Deeg, D. Reverte-Payá, F. M. Pérez-Toledo
The cool white dwarf WD 1856+534 was found to be transited by a Jupiter-sized object with a mass at or below 14 M$_{\rm{Jup}}$. We used the GTC telescope to obtain and analyse photometry and low resolution spectroscopy of six transits of WD 1856+534
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81219b933afc05deca961ea25053d759
http://arxiv.org/abs/2103.15720
http://arxiv.org/abs/2103.15720
Akademický článek
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Autor:
Fernando Selman, Paul A. Crowther, N. Castro-Rodríguez, Jorge Melnick, Chris Evans, Jorick S. Vink, Jonathan Mackey, Nuno Filipe Castro
We introduce VLT-MUSE observations of the central 2$'\times2'$ (30$\times$30 pc) of the Tarantula Nebula in the Large Magellanic Cloud. The observations provide an unprecedented spectroscopic census of the massive stars and ionised gas in the vicinit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::00c697d9d3c38b96c6626e50f4b5553b
http://arxiv.org/abs/1802.01597
http://arxiv.org/abs/1802.01597
Akademický článek
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Autor:
N. Castro-Rodríguez, Antonio Marín-Franch, J. M. Rodríguez Espinosa, Itziar Aretxaga, A. Herrero, Rafael Guzman, Roberto Terlevich, J. M. Mas-Hesse, Alberto Manrique, Jesús Gallego, Eleazar R. Carrasco, R. Calvi, Elena Terlevich, Eduard Salvador-Solé, K. Chanchaiworawit
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Recercat. Dipósit de la Recerca de Catalunya
instname
E-Prints Complutense. Archivo Institucional de la UCM
Dipòsit Digital de la UB
Universidad de Barcelona
Universidad Complutense de Madrid
Recercat. Dipósit de la Recerca de Catalunya
instname
E-Prints Complutense. Archivo Institucional de la UCM
Dipòsit Digital de la UB
Universidad de Barcelona
We present the results of our search near the end of the Reionization Epoch for faint galaxies. This has been done using very deep OSIRIS images obtained at the Gran Telescopio Canarias (GTC). Our observations focus around two close, massive Lyman al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c9861c925ae2e80630bd1305f22c021
http://hdl.handle.net/2445/112624
http://hdl.handle.net/2445/112624
CONTEXT. A set of 20 extremely red galaxies at 2.5
Comment: 14 pages, published in A&A. v2: Erratum correction of a factor (1+z)^4 in the luminosity of Figs. 5, 6, A.1
Comment: 14 pages, published in A&A. v2: Erratum correction of a factor (1+z)^4 in the luminosity of Figs. 5, 6, A.1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ccae94e171887aaa72cd91364ca5255a
http://arxiv.org/abs/1702.00380
http://arxiv.org/abs/1702.00380
Autor:
J. A. L. Aguerri, Walter Boschin, C. del Burgo, A. Kundert, Enrico Maria Corsini, Jairo Méndez-Abreu, Elena D'Onghia, R. Barrena, S. Zarattini, N. Castro-Rodríguez, Rubén Sánchez-Janssen, Marisa Girardi
Fossil groups are expected to be the final product of galaxy merging within galaxy groups. In simulations, they are predicted to assemble their mass at high redshift. This early formation allows for the innermost $M^\ast$ galaxies to merge into a mas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::134bef4d7f1f29183fa8e2027cc54a9c
https://hdl.handle.net/11368/2867127
https://hdl.handle.net/11368/2867127
Autor:
Eli Dwek, Bruno Maffei, Giulia Rodighiero, Duncan Farrah, Mat Page, Julie Wardlow, Hien Nguyen, Michael Zemcov, A. Amblard, David L. Clements, Matthew Joseph Griffin, Antonio Cava, C. K. Xu, Stephen Anthony Eales, Edo Ibar, N. Lu, Rob Ivison, Pasquale Panuzzo, David Elbaz, Pierre Chanial, Ivan Valtchanov, G. Marsden, Kate Gudrun Isaak, J. I. Rawlings, D. Rizzo, S. C. Madden, L. R. Levenson, Anthony J. Smith, Thomas R. Greve, G. Mainetti, Lucia Marchetti, Michael Rowan-Robinson, Gillian S. Wright, Asantha Cooray, Robbie Richard Auld, Edward L. Chapin, N. Castro-Rodríguez, Glenn Morrison, Drew Brisbin, Nick Seymour, Gwenifer Raymond, Andrew Blain, James J. Bock, Markos Trichas, A. Conley, Joaquin Vieira, Mark Halpern, Marco P. Viero, Bernhard Schulz, Guilaine Lagache, V. Arumugam, Denis Burgarella, J. S. Dunlop, D. L. Shupe, L. Conversi, Herve Aussel, Isaac Roseboom, Lian-Tao Wang, Alain Omont, Jamie Stevens, Evanthia Hatziminaoglou, C. P. Pearson, A. M. J. Mortier, Andreas Papageorgiou, Douglas Scott, Scott Chapman, B. O'Halloran, Jason Glenn, C. D. Dowell, M. Symeonidis, Ismael Perez-Fournon, Alberto Franceschini, Dimitra Rigopoulou, Mattia Vaccari, Alessandro Boselli, Matthieu Béthermin, K. E. Tugwell, Michael Pohlen, V. Buat, S. J. Oliver, L. Vigroux
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 419:2758-2773
We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500 {\mu}m by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm-sources with