Galaxy counts at 24 μm in the SWIRE fields (2008)
Shupe, David L., Rowan-Robinson, Michael, Lonsdale, Carol J., Masci, Frank, Evans, Tracey, Fang, Fan, ...
This paper presents galaxy source counts at 24 μm in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts in other fields, and to model...
Galaxy Counts at 24 Microns in the SWIRE Fields (2007)
Shupe, David L., Rowan-Robinson, Michael, Lonsdale, Carol J., Masci, Frank, Evans, Tracey, Fang, Fan, ...
This paper presents galaxy source counts at 24 microns in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts in other fields, and to model...
Parametric modelling of the 3.6um to 8um colour distributions of galaxies in the SWIRE Survey (2006)
Davoodi, Payam, Oliver, Seb, Polletta, Maria Del Carmen, Rowan-Robinson, Michael, Savage, Richard S., Waddington, Ian, ...
We fit a parametric model comprising a mixture of multi-dimensional Gaussian functions to the 3.6 to 8um colour and optical photo-z distribution of galaxy populations in the ELAIS-N1 and Lockman...
The First Measurements of Galaxy Clustering from IRAC Data of the Spitzer First Look Survey (2004)
Fang, Fan, Shupe, David L., Wilson, Gillian, Lacy, Mark, Fadda, Dario, Jarrett, Tom, ...
We present the first results of the angular auto-correlation function of the galaxies detected by the Infrared Array Camera (IRAC) instrument in the First Look Survey (FLS) of the Spitzer Space...
Models for Multiband IR Surveys (2000)
Xu, Cong, Lonsdale, Carol J., Shupe, David L., O'Linger, JoAnn, Masci, Frank
Empirical 'backward' galaxy evolution models for IR-bright galaxies are constrained using multiband IR surveys. A new Monte-Carlo algorithm is developed for this task. It exploits a large library of...
Emission Features and Source Counts of Galaxies in Mid-Infrared (1998)
Xu, Cong, Hacking, Perry B., Fang, Fan, Shupe, David L., Lonsdale, Carol J., Lu, Nanyao Y., ...
In this work we incorporate the newest ISO results on the mid-infrared spectral-energy-distributions (MIR SEDs) of galaxies into models for the number counts and redshift distributions of MIR...
The Local Luminosity Function at 25 Microns (1998)
Shupe, David L., Fang, Fan, Hacking, Perry B., Huchra, John P.
The local luminosity function at 25 $\mu$m provides the basis for interpreting the results of deep mid-infrared surveys planned or in progress with space astrophysics missions including ISO, WIRE and...