Bibcode
DOI
Mauduit, J.-C.; Lacy, M.; Farrah, D.; Surace, J. A.; Jarvis, M.; Oliver, S.; Maraston, C.; Vaccari, M.; Marchetti, L.; Zeimann, G.; Gonzáles-Solares, E. A.; Pforr, J.; Petric, A. O.; Henriques, B.; Thomas, P. A.; Afonso, J.; Rettura, A.; Wilson, G.; Falder, J. T.; Geach, J. E.; Huynh, M.; Norris, R. P.; Seymour, N.; Richards, G. T.; Stanford, S. A.; Alexander, D. M.; Becker, R. H.; Best, P. N.; Bizzocchi, L.; Bonfield, D.; Castro-Rodríguez, N.; Cava, A.; Chapman, S.; Christopher, N.; Clements, D. L.; Covone, G.; Dubois, N.; Dunlop, J. S.; Dyke, E.; Edge, A.; Ferguson, H. C.; Foucaud, S.; Franceschini, A.; Gal, R. R.; Grant, J. K.; Grossi, M.; Hatziminaoglou, E.; Hickey, S.; Hodge, J. A.; Huang, J.-S.; Ivison, R. J.; Kim, M.; LeFevre, O.; Lehnert, M.; Lonsdale, C. J.; Lubin, L. M.; McLure, R. J.; Messias, H.; Martínez-Sansigre, A.; Mortier, A. M. J.; Nielsen, D. M.; Ouchi, M.; Parish, G.; Pérez-Fournon, I.; Pierre, M.; Rawlings, S.; Readhead, A.; Ridgway, S. E.; Rigopoulou, D.; Romer, A. K.; Rosebloom, I. G.; Rottgering, H. J. A.; Rowan-Robinson, M.; Sajina, A.; Simpson, C. J.; Smail, I.; Squires, G. K.; Stevens, J. A.; Taylor, R.; Trichas, M.; Urrutia, T.; van Kampen, E.; Verma, A.; Xu, C. K.
Referencia bibliográfica
Publications of the Astronomical Society of the Pacific, Volume 124, issue 917, pp.714-736
Fecha de publicación:
7
2012
Número de citas
168
Número de citas referidas
149
Descripción
We present the Spitzer Extragalactic Representative Volume Survey
(SERVS), an 18 deg2 medium-deep survey at 3.6 and 4.5 μm
with the postcryogenic Spitzer Space Telescope to ≈2 mJy (AB=23.1)
depth of five highly observed astronomical fields (ELAIS-N1, ELAIS-S1,
Lockman Hole, Chandra Deep Field South, and XMM-LSS). SERVS is designed
to enable the study of galaxy evolution as a function of environment
from z˜5 to the present day and is the first extragalactic survey
that is both large enough and deep enough to put rare objects such as
luminous quasars and galaxy clusters at z≳1 into their cosmological
context. SERVS is designed to overlap with several key surveys at
optical, near- through far-infrared, submillimeter, and radio
wavelengths to provide an unprecedented view of the formation and
evolution of massive galaxies. In this article, we discuss the SERVS
survey design, the data processing flow from image reduction and
mosaicking to catalogs, and coverage of ancillary data from other
surveys in the SERVS fields. We also highlight a variety of early
science results from the survey.
Proyectos relacionados
Formación y Evolución de Galaxias: Observaciones Infrarrojas y en otras Longitudes de Onda
Este grupo desarrolla varios proyectos extragalácticos en diferentes rangos del espectro electromagnético utilizando satélites y telescopios en tierra para estudiar la evolución cosmológica de las galaxias y el origen de la actividad nuclear en galaxias activas. En el aspecto instrumental, el grupo forma parte del consorcio internacional que ha
Ismael
Pérez Fournon