Rodighiero, G., Vaccari, M., Franceschini, A., Tresse, L., Fevre, O. Le, Brun, V. Le, ...
[Abridged]We exploit a large homogeneous dataset to derive a self-consistent picture of IR emission based on the time-dependent 24, 15, 12 and 8micron monochromatic and bolometric IR luminosity...
Mid-infrared spectroscopy of infrared-luminous galaxies at z~0.5-3 (2009)
Hernan-Caballero, A., Perez-Fournon, I., Hatziminaoglou, E., Afonso-Luis, A., Rowan-Robinson, M., Rigopoulou, D., ...
We present results on low-resolution mid-infrared (MIR) spectra of 70 infrared-luminous galaxies obtained with the Infrared Spectrograph (IRS) onboard Spitzer. We selected sources from the European...
MAMBO 1.2mm observations of luminous starbursts at z~2 in the SWIRE fields (2008)
Lonsdale, C. J., Polletta, M., Omont, A., Shupe, D., Berta, S., Zylka, R., ...
We report on--off pointed MAMBO observations at 1.2 mm of 61 Spitzer-selected star-forming galaxies from the SWIRE survey. The sources are selected on the basis of bright 24um fluxes (f_24um>0.4mJy)...
Berta, S., Rubele, S., Franceschini, A., Held, E. V., Rizzi, L., Rodighiero, G., ...
Context. The ESO-Spitzer Imaging extragalactic Survey (ESIS) is the optical follow up of the Spitzer Wide-area Infra-Red Extragalactic survey (SWIRE) in the ELAIS-S1 region of the sky. Aims. In the...
Real-Time Calibration of the Murchison Widefield Array (2008)
Mitchell, D. A., Greenhill, L. J., Wayth, R. B., Sault, R. J., Lonsdale, C. J., Cappallo, R. J., ...
The interferometric technique known as peeling addresses many of the challenges faced when observing with low-frequency radio arrays, and is a promising tool for the associated calibration systems....
Berta, S., Rubele, S., Franceschini, A., Held, E., Rizzi, L., Rodighiero, G., ...
(abridged) The ESIS survey is the optical follow up of the SWIRE/Spitzer in the ELAIS-S1 region of the sky. In the era of observational cosmology, the main efforts are focused on the study of galaxy...
Clements, D. L., Vaccari, M., Babbedge, T., Oliver, S., Rowan-Robinson, M., Davoodi, P., ...
We present the optical-to-submillimetre spectral energy distributions (SEDs) for 33 radio and mid-infrared (mid-IR) identified submillimetre galaxies discovered via the SHADES 850-μm SCUBA imaging...
Obscuration in extremely luminous quasars (2008)
Polletta, M., Weedman, D., Hönig, S., Lonsdale, C. J., Smith, H. E., Houck, J.
The SEDs and IR spectra of a remarkable sample of obscured AGNs selected in the MIR are modeled with recent clumpy torus models. The sample contains 21 AGNs at z = 1.3–3 discovered in the largest...
The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function (2007)
Berta, S., Lonsdale, C. J., Polletta, M., Savage, R. S., Franceschini, A., Buttery, H., ...
Context. In the last couple of years a population of very massive (M_* > 10^(11) M_⊙), high-redshift (z ≥ 2) galaxies has been identified, but its role in galaxy evolution has not yet been fully...
Waddington, I., Oliver, S. J., Babbedge, T. S. R., Fang, F., Farrah, D., Franceschini, A., ...
We investigate the clustering of galaxies selected in the 3.6 micron band of the Spitzer Wide-area Infrared Extragalactic (SWIRE) legacy survey. The angular two-point correlation function is...
The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function (2007)
Berta, S., Lonsdale, C. J., Polletta, M., Savage, R. S., Franceschini, A., Buttery, H., ...
(Abridged) We selected high-z massive galaxies at 5.8 microns, in the SWIRE ELAIS-S1 field (1 sq. deg.). Galaxies with the 1.6 microns stellar peak redshifted into the IRAC bands (z~1-3, called...
Keck spectroscopy of z = 1-3 ULIRGs from the Spitzer SWIRE survey (2007)
Berta, S., Lonsdale, C. J., Siana, B., Farrah, D., Smith, H. E., Polletta, M. C., ...
Context. High-redshift ultra luminous infrared galaxies contribute the bulk of the cosmic IR background and are the best candidates for very massive galaxies in formation at z > 1.5. Aims. It is...
Keck spectroscopy of z=1-3 ULIRGs from the Spitzer SWIRE survey (2007)
Berta, S., Lonsdale, C. J., Siana, B., Farrah, D., Smith, H. E., Polletta, M., ...
(Abridged) High-redshift ultra luminous infrared galaxies contribute the bulk of the cosmic IR background and are the best candidates for very massive galaxies in formation at z>1.5. We present...
The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function (2007)
Berta, S., Lonsdale, C. J., Polletta, M., Savage, R. S., Franceschini, A., Buttery, H., ...
Polletta, M, Tajer, M, Maraschi, L, Trinchieri, G, Lonsdale, C J, Chiappetti, L, ...
We present the SEDs of a hard X-ray selected sample containing 136 sources with F[SUB]2-10keV[/SUB]>10[SUP]-14[/SUP] erg cm[SUP]-2[/SUP] s[SUP]-1[/SUP] 132 are AGNs. The sources are detected in a 1...
Weedman, D., Polletta, M., Lonsdale, C. J., Wilkes, B. J., Siana, B., Houck, J. R., ...
Spectra have been obtained with the Infrared Spectrograph (IRS) on the Spitzer Space Telescope for 20 sources in the Lockman Hole field of the SWIRE survey. The sample is divided between sources with...
Babbedge, T. S. R., Rowan-Robinson, M., Vaccari, M., Surace, J. A., Lonsdale, C. J., Clement, D. L., ...
We construct rest-frame luminosity functions at 3.6, 4.5, 5.8, 8 and 24 microns over the redshift range 0
Berta, S., Rubele, S., Franceschini, A., Held, E. V., Rizzi, L., Lonsdale, C. J., ...
The ESO-Spitzer extragalactic Imaging Survey (ESIS) is the optical follow up of the Spitzer Wide-Area InfraRed Extragalactic (SWIRE) survey in the ELAIS-S1 area. This paper presents B, V, R Wide...
The Two Micron All Sky Survey (1994)
Kleinmann, S. G., Lysaght, M. G., Pughe, W. L., Schneider, S. E., Skrutskie, M. F., Weinberg, M. D., ...
Peer Reviewed
The two micron all sky survey (1994)
Kleinmann, S. G., Lysaght, M. G., Pughe, W. L., Schneider, S. E., Skrutskie, M. F., Weinberg, M. D., ...
This paper describes the design, expectations, and prototyping of a new allsky survey, called 2MASS (Two Micron All Sky Survey) to be carried out with the new generation of infrared array detectors.