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Publications of the Astronomical Society of Australia Publications of the Astronomical Society of Australia Society
Publications of the Astronomical Society of Australia
RESEARCH ARTICLE

Optimal Multiwavelength Source Detection: Experience Gained from the WISE Mission

K. A. Marsh A B and T. H. Jarrett A
+ Author Affiliations
- Author Affiliations

A Infrared Processing and Analysis Center, California Institute of Technology 100–22, Pasadena, CA 91125, USA

B Corresponding author. Email: kam@ipac.caltech.edu

Publications of the Astronomical Society of Australia 29(3) 269-275 https://doi.org/10.1071/AS11043
Submitted: 8 September 2011  Accepted: 30 November 2011   Published: 19 December 2011

Abstract

We discuss the optimal detection of point sources from multiwavelength imaging data using an approach, referred to as MDET, which requires no prior knowledge of the source spectrum. MDET may be regarded as a somewhat more general version of the so-called ‘chi-squared’ technique. We describe the theoretical basis of the technique, and show examples of its performance with four-channel infrared broad-band imaging data from the WISE mission. We also discuss the potential benefits of applying it to the multifrequency data cubes of the ASKAP surveys, and suggest that it could increase the detection sensitivity of searches for neutral hydrogen emission at moderately high redshifts.

Keywords: methods: data analysis — methods: observational — techniques: image processing


References

Chang, T.-C., Pen, U.-L., Bandura, K. and Peterson, J. B., 2010, Nature, 466, 463
Crossref | GoogleScholarGoogle Scholar | 1:CAS:528:DC%2BC3cXptFKjsbg%3D&md5=c7647d1b698e7605e5ad4b1f4e688e28CAS |

Cutri, R. M. et al., 2011, Explanatory Supplement to the WISE Preliminary Release, available at http://wise2.ipac.caltech.edu/docs/release/prelim/expsup

Jarrett, T. H. et al., 2011, ApJ, 735, 112
Crossref | GoogleScholarGoogle Scholar |

Johnston, S. et al., 2008, Science With ASKAP (arXiv:0810.5187)

Johnston, S., Feain, I. J. and Gupta, N., 2009, ASPC, 407, 446
| 1:CAS:528:DC%2BD1MXhsVOgsb7K&md5=0e39f5e4e991f0f47cb68880225ba21fCAS |

Khandai, N., Sethi, S. K., Di Matteo, T., Croft, R. A. C., Springel, V., Jana, A. and Gardner, J. P., 2011, MNRAS, 415, 2580
Crossref | GoogleScholarGoogle Scholar | 1:CAS:528:DC%2BC3MXhtFyqu73E&md5=529ddf43f3709531c0bfcf0984c56ccfCAS |

Koribalski, B., 1996, ASPC, 106, 238
| 1:CAS:528:DyaK2sXjtVylu7s%3D&md5=25715cc7e88734683a460dbfdcaabc30CAS |

Mainzer, A. et al., 2011, ApJ, 726, 30
Crossref | GoogleScholarGoogle Scholar |

Rawlings, S., Abdalla, F. B., Bridle, S. L., Blake, C. A., Baugh, C. M., Greenhill, L. J. & van der Hulst, J. M., 2004, in Science with the Square Kilometre Array, ed. C. Carilli & S. Rawlings, New Astronomy Reviews, Vol. 48 (Elsevier)

Szalay, A. S., Connolly, A. J. and Szololy, G. P., 1999, AJ, 117, 68

Wright, E. L. et al., 2010, AJ, 140, 1868

Zwaan, M., 2006, in Cosmology, Galaxy Formation and Astroparticle Physics on the Pathway to the SKA, ed. H.-R. Klöckner, M. Jarvis & S. Rawlings (Oxford, UK: ASTRON)