The LABOCA survey of the Extended Chandra Deep Field-South – radio and mid-infrared counterparts to submillimetre galaxies

AD Biggs, RJ Ivison, E Ibar, JL Wardlow… - Monthly Notices of …, 2011 - academic.oup.com
We present radio and infrared (3.6–24 μm) counterparts to submillimetre galaxies (SMGs)
detected in the Extended Chandra Deep Field-South with the Large APEX Bolometer …

A Multiply Imaged Luminous Infrared Galaxy Behind the Bullet Cluster (1E0657-56)

AH Gonzalez, D Clowe, M Bradač… - The Astrophysical …, 2009 - iopscience.iop.org
We present evidence for a Spitzer-selected luminous infrared galaxy (LIRG) behind the
Bullet Cluster (1E0657-56). The galaxy, originally identified as a multiply imaged source …

A bright submillimeter source in the bullet cluster (1e0657-56) field detected with blast

M Rex, PAR Ade, I Aretxaga, JJ Bock… - The Astrophysical …, 2009 - iopscience.iop.org
ABSTRACT We present the 250, 350, and 500 μm detection of bright submillimeter emission
in the direction of the Bullet Cluster measured by the Balloon-borne Large-Aperture …

Spitzer 24 μm Time Series Observations of the Eclipsing M Dwarf Binary GU Boötis

K von Braun, GT van Belle, DR Ciardi… - The Astrophysical …, 2008 - iopscience.iop.org
We present a set of Spitzer 24 μm MIPS time series observations of the M dwarf eclipsing
binary star GU Boötis. Our data cover three secondary eclipses of the system: two …

Deconvolving infrared telescope images as point sources on a grid

DG Elliott - IR Space Telescopes and Instruments, 2003 - spiedigitallibrary.org
Deconvolution of infrared telescope images can partially recover the distribution of light in
the sky. The light from point sources and extended sources is modeled as a grid of closely …

Spitzer 24-micron Time-Series Observations of the Eclipsing M-dwarf Binary GU Bootis

K von Braun, GT van Belle, DR Ciardi… - arXiv preprint arXiv …, 2007 - arxiv.org
We present a set of {\it Spitzer} 24$\mu $ m MIPS time series observations of the M-dwarf
eclipsing binary star GU Bo\" otis. Our data cover three secondary eclipses of the system …