I. Oteo
Spanish National Research Council
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Featured researches published by I. Oteo.
Astronomy and Astrophysics | 2013
I. Oteo; J. Cepa; A. Bongiovanni; A.M. Pérez‐García; Bernabe Cedres; H. Dominguez Sanchez; A. Ederoclite; M. Sánchez-Portal; I. Pintos-Castro; R. Pérez-Martínez
Lyman break galaxies (LBGs) represent one of the kinds of star-forming galaxies that are found in the high-redshift universe. The detection of LBGs in the FIR domain can provide very important clues on their dust attenuation and total SFR, allowing a more detailed study than those performed so far. In this work we explore the FIR emission of a sample of 16 LBGs at z ~ 3 in the GOODS-North and GOODS-South fields that are individually detected in PACS-100um or PACS-160um. These detections demonstrate the possibility of measuring the dust emission of LBGs at high redshift. We find that PACS-detected LBGs at z ~ 3 are highly obscured galaxies which belong to the Ultra luminous IR galaxies or Hyper luminous IR galaxies class. Their total SFR cannot be recovered with the dust attenuation factors obtained from their UV continuum slope or their SED-derived dust attenuation employing Bruzual & Charlot (2003) templates. Both methods underestimate the results for most of the galaxies. Comparing with a sample of PACS-detected LBGs at z ~ 1 we find evidences that the FIR emission of LBGs might have changed with redshift in the sense that the dustiest LBGs found at z ~ 3 have more prominent FIR emission, are dustier for a given UV slope, and have higher SFR for a given stellar mass than the dustiest LBGs found at z ~ 1.
Astronomy and Astrophysics | 2012
I. Oteo; A. Bongiovanni; A. M. Pérez García; J. Cepa; A. Ederoclite; M. Sanchez-Portal; I. Pintos-Castro; R. Perez-Martinez; S. Berta; B. Magnelli; P. Popesso; F. Pozzi; A. Poglitsch; D. Lutz; R. Genzel; L. J. Tacconi; N. M. Förster Schreiber; E. Sturm; D. Elbaz; H. Aussel; E. Daddi; P. Andreani; A. Cimatti; R. Maiolino; B. Altieri; I. Valtchanov
In this work we analyze the physical properties of a sample of 56 spectroscopically selected star-forming (SF) Ly
Astronomy and Astrophysics | 2010
A. Bongiovanni; I. Oteo; J. Cepa; A. M. Pérez García; M. Sánchez-Portal; A. Ederoclite; J. A. L. Aguerri; E. J. Alfaro; B. Altieri; P. Andreani; M. T. Aparicio-Villegas; H. Aussel; N. Benítez; S. Berta; Tom Broadhurst; J. Cabrera-Caño; Francisco J. Castander; A. Cava; M. Cerviño; H. Chulani; A. Cimatti; D. Cristóbal-Hornillos; E. Daddi; H. Dominguez; D. Elbaz; Alberto Fernandez-Soto; N. M. Förster Schreiber; R. Genzel; M. F. Gómez; R. M. González Delgado
alpha
Monthly Notices of the Royal Astronomical Society | 2014
I. Oteo; A. Bongiovanni; G. Magdis; A.M. Pérez‐García; J. Cepa; H. Dominguez Sanchez; A. Ederoclite; M. Sanchez-Portal; I. Pintos-Castro
emitting galaxies at 2.0
Monthly Notices of the Royal Astronomical Society | 2014
H. Dominguez Sanchez; A. Bongiovanni; M. A. Lara-Lopez; I. Oteo; J. Cepa; A. M. Pérez García; M. Sánchez-Portal; A. Ederoclite; D. Lutz; G. Cresci; I. Delvecchio; S. Berta; B. Magnelli; P. Popesso; F. Pozzi; L. Riguccini
lesssim
Monthly Notices of the Royal Astronomical Society | 2013
M. Pović; M. Huertas-Company; J. A. L. Aguerri; I. Márquez; J. Masegosa; C. Husillos; A. Molino; D. Cristóbal-Hornillos; J. Perea; N. Benítez; A. del Olmo; Alberto Fernandez-Soto; Y. Jimenez-Teja; M. Moles; E. J. Alfaro; T. Aparicio-Villegas; Begoña Ascaso; Tom Broadhurst; J. Cabrera-Caño; Francisco J. Castander; J. Cepa; M. Fernández Lorenzo; M. Cerviño; R. M. González Delgado; L. Infante; C. López-Sanjuan; V. J. Martínez; I. Matute; I. Oteo; A. M. Pérez-García
z
Astronomy and Astrophysics | 2013
I. Pintos-Castro; M. Sanchez-Portal; J. Cepa; J. S. Santos; B. Altieri; R. Pérez Martínez; E. J. Alfaro; A. Bongiovanni; D. Coia; L. Conversi; H. Dominguez-Sanchez; A. Ederoclite; J. I. González-Serrano; L. Metcalfe; I. Oteo; A. M. Pérez García; J. Polednikova; T. D. Rawle; I. Valtchanov
lesssim
Monthly Notices of the Royal Astronomical Society | 2013
I. Oteo; D. Lutz; G. Magdis; F. Prada; J. Perea; M. Sánchez-Portal; A. M. Pérez-García; A. Poglitsch; Francisco J. Castander; B. Magnelli; P. Andreani; Alberto Fernandez-Soto; J. M. Quintana; M. Moles; I. Márquez; L. Infante; J. Cepa; I. Valtchanov; I. Matute; T. Aparicio-Villegas; F. Pozzi; R. Maiolino; Tom Broadhurst; J. Polednikova; E. Sturm; J. Cabrera-Caño; D. Elbaz; A. Bongiovanni; A. Ederoclite; C. Husillos
3.5 using both a spectral energy distribution (SED) fitting procedure from rest-frame UV to mid-IR and direct 160
Monthly Notices of the Royal Astronomical Society | 2013
I. Oteo; A. Bongiovanni; J. Cepa; A. M. Pérez-García; A. Ederoclite; M. Sánchez-Portal; I. Pintos-Castro; R. Pérez-Martínez; J. Polednikova; J. A. L. Aguerri; E. J. Alfaro; T. Aparicio-Villegas; N. Benítez; Tom Broadhurst; J. Cabrera-Caño; Francisco J. Castander; M. Cerviño; D. Cristóbal-Hornillos; Alberto Fernandez-Soto; R. M. Gonzalez-Delgado; C. Husillos; L. Infante; V. J. Martínez; I. Márquez; J. Masegosa; I. Matute; M. Moles; A. Molino; A. del Olmo; J. Perea
mu
The Astrophysical Journal | 2011
I. Oteo; A. Bongiovanni; A. M. Pérez García; J. Cepa; A. Ederoclite; M. Sanchez-Portal; I. Pintos-Castro; D. Lutz; S. Berta; E. Le Floc'h; B. Magnelli; P. Popesso; F. Pozzi; L. Riguccini; B. Altieri; P. Andreani; H. Aussel; A. Cimatti; E. Daddi; D. Elbaz; N. M. Förster Schreiber; R. Genzel; R. Maiolino; A. Poglitsch; E. Sturm; L. J. Tacconi; I. Valtchanov
m observations taken with the Photodetector Array Camera & Spectrometer (PACS) instrument onboard emph{Herschel Space Observatory}. We define LAEs as those Ly
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