LOFAR calibration and wide-field imaging
Artikel i vetenskaplig tidskrift, 2012

LOFAR is a revolutionary instrument, operating at low frequencies (nu less than or similar to 240 MHz). It will drive major breakthroughs in the area of observational cosmology, but its use requires the development of challenging techniques and algorithms. Since its field of view and sensitivity are increased by orders of magnitude as compared to the older generation of instruments, new technical problems have to be addressed. The LOFAR survey team is in charge of commissioning the first LOFAR data produced in the imager mode as part of building the imaging pipeline. We are developing algorithms to tackle the problems associated with calibration (ionosphere, beam, etc.) and wide-field imaging for the achievement of the deep extragalactic surveys. New types of problems arise in that context, and notions such as algorithmic complexity and parallelism become fundamental.

LOFAR

Interferometry

Imaging

Calibration

Författare

C. Tasse

Observatoire de Paris-Meudon

G. van Diepen

Netherlands Institute for Radio Astronomy (ASTRON)

S. van der Tol

Universiteit Leiden

R. J. van Weeren

Universiteit Leiden

J. E. van Zwieten

Universiteit Leiden

Fabien Batejat

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

S. Bhatnagar

National Radio Astronomy Observatory Socorro

I. van Bemmel

Netherlands Institute for Radio Astronomy (ASTRON)

L. Birzan

Universiteit Leiden

A. Bonafede

Istituto di Radioastronomia

John Conway

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

C. Ferrari

Observatoire de la Cote d'Azur

F. De Gasperin

Max Planck-institutet

K. Golap

National Radio Astronomy Observatory Socorro

G. Heald

Netherlands Institute for Radio Astronomy (ASTRON)

N. Jackson

University of Manchester

G. Macario

Observatoire de la Cote d'Azur

J. McKean

Netherlands Institute for Radio Astronomy (ASTRON)

N. R. Mohan

Universiteit Leiden

E. Orru

Rijksuniversiteit Groningen

R. Pizzo

Netherlands Institute for Radio Astronomy (ASTRON)

D. Rafferty

Universiteit Leiden

U. Rau

National Radio Astronomy Observatory Socorro

H. Rottgering

Universiteit Leiden

A. Shulevski

Rijksuniversiteit Groningen

Comptes Rendus Physique

1631-0705 (ISSN)

Vol. 13 28-32

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1016/j.crhy.2011.10.006