Crowded-field image simulator for WSO-UV/ISSIS: first functional version developed by the Glendama team
Abstract
We are developing a web-based interactive software to simulate crowded-field imaging with the Imaging and Slitless Spectrograph Instrument for Surveys (ISSIS) on board the future World Space Observatory - Ultraviolet (WSO-UV). This new tool is aimed to prepare WSO-UV/ISSIS proposals to observe multicomponent targets and dense fields. For a given combination of UV channel, filters and exposure time, the user creates a set of point-like and extended sources (source model). This source model produces a final image, which takes into account a pixelated field of view, a realistic conversion between physical flux and counts per second, the convolution with the expected point spread function, a sky background and noise fluctuations. The current version of the simulator is available at the Gravitational LENses and DArk MAtter (Glendama) website, and it allows users to specify all relevant parameters of each point-like or extended source, drag-and-drop sources by using a mouse or a fingertip/stylus on a touchscreen, change the frame size or the brightness scale, etc.
Keywords
Cite
@article{arxiv.1409.5416,
title = {Crowded-field image simulator for WSO-UV/ISSIS: first functional version developed by the Glendama team},
author = {Vyacheslav N. Shalyapin and Luis J. Goicoechea},
journal= {arXiv preprint arXiv:1409.5416},
year = {2014}
}
Comments
5 pages, 4 figures, accepted for publication in ApSS (Special Issue UV Astronomy 3). The Crowded-field Image Simulator (CIS) for ISSIS is freely available at http://grupos.unican.es/glendama (see also http://grupos.unican.es/glendama/Granada.pdf for simulations of gravitationally lensed AGN)