Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Galaxy and Mass Assembly: FUV, NUV, ugrizYJHK Petrosian, Kron and Sersic photometry

Thumbnail Image

Date

2011

Authors

Hill, David
Kelvin, Lee
Driver, Simon P
Robotham, Aaron
Cameron, Ewen
Cross, N J G
Andrae, Ellen
Baldry, I. K.
Liske, Jochen
Madore, Barry

Journal Title

Journal ISSN

Volume Title

Publisher

Blackwell Publishing Ltd

Abstract

In order to generate credible 0.1-2μm spectral energy distributions, the Galaxy and Mass Assembly (GAMA) project requires many gigabytes of imaging data from a number of instruments to be reprocessed into a standard format. In this paper, we discuss the

Description

Keywords

Keywords: Galaxies: fundamental parameters; Methods: data analysis; Methods: observational; Surveys; Techniques: image processing; Techniques: photometric

Citation

URI

http://hdl.handle.net/1885/78542

Collections

ANU Research Publications

Source

Monthly Notices of the Royal Astronomical Society

Type

Journal article

Book Title

Entity type

Access Statement

Open Access

License Rights

DOI

10.1111/j.1365-2966.2010.17950.x

Restricted until

Downloads

File
Description
01_Hill_Galaxy_and_Mass_Assembly:_FUV,_2011.pdf (7.35 MB)

DSpace software copyright © 2002-2026 LYRASIS

abcd