activity
19952007
most citedFirst Space-Based Microlens Parallax Measurement: Spitzer Observations of OGLE-2005-SMC-001

143 citations · 143 across the 1 of their papers we have counts for

collaborators
Showing astro-phShow all

8 papers · 1 filter

astro-ph2007143 cited

First Space-Based Microlens Parallax Measurement: Spitzer Observations of OGLE-2005-SMC-001

Subo Dong, A. Udalski, A. Gould +20

We combine Spitzer and ground-based observations to measure the microlens parallax of OGLE-2005-SMC-001, the first such space-based determination since S. Refsdal proposed the idea…

astro-ph2000

The extragalactic background and its fluctuations in the far-infrared wavelengths

G. Lagache, J-L. Puget, A. Abergel +22

A Cosmic Far-InfraRed Background (CFIRB) has long been predicted that would traces the intial phases of galaxy formation. It has been first detected by Puget et al.(1996) using COB…

astro-ph1999

First detections of FIRBACK sources with SCUBA

Douglas Scott, Guilaine Lagache, Colin Borys +10

The FIRBACK (Far InfraRed BACKground) survey represents the deepest extensive 170 micron images obtained by the ISO satellite. The sources detected comprise about 10% of the Cosmic…

astro-ph1999

FIRBACK Far Infrared Survey with ISO: Data Reduction, Analysis and First Results

Herve Dole, Guilaine Lagache, Jean-Loup Puget +19

FIRBACK is one of the deepest cosmological surveys performed in the far infrared, using ISOPHOT. We describe this survey, its data reduction and analysis. We present the maps of fi…

astro-ph1999

A Deep 12 Micron Survey with ISO

D. L. Clements, F-X. Desert, A. Franceschini +4

We present the first results of a study of faint 12 micron sources detected with the Infrared Space Observatory (ISO) in four deep, high galactic latitude fields. The sample includ…

astro-ph1998

FIRBACK: I. A deep survey at 175 m with ISO, preliminary results

J. L. Puget, G. Lagache, D. L Clements +10

FIRBACK is a deep survey conducted with the ISOPHOT instrument aboard the Infrared Space Observatory (ISO) at an effective wavelength of 175 m. We present here results we have o…