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CONSKY: A Sky CCD Integration Simulation

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owlice
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CONSKY: A Sky CCD Integration Simulation

Postby owlice » Tue Jul 27, 2010 1:49 pm

CONSKY: A Sky CCD Integration Simulation

Abstract: This program addresses the question of what resources are needed to produce a continuous data record of the entire sky down to a given limiting visual magnitude. Toward this end, the program simulates a small camera/telescope or group of small camera/telescopes collecting light from a large portion of the sky. From a given stellar density derived from a Bahcall - Soneira Galaxy model, the program first converts star densities at visual magnitudes between 5 and 20 to number of sky pixels needed to monitor each star simultaneously. From pixels, the program converts input CCD parameters to needed telescope attributes, needed data storage space, and the length of time needed to accumulate data of photometric quality for stars of each limiting visual magnitude over the whole sky. The program steps though photometric integrations one second at a time and includes the contribution from a bright background, read noise, dark current, and atmospheric absorption.

Credit: Nemiroff, Robert J.; Rafert, J. Bruce

Site: http://dx.doi.org/10.20356/C4MW2H
http://adsabs.harvard.edu/abs/1999PASP..111..886N

Bibcode: 1999ascl.soft05001N

ID: ascl:9905.001
Last edited by Ada Coda on Mon May 30, 2016 2:13 am, edited 1 time in total.
Reason: Updated code entry.
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owlice
Guardian of the Codes
Posts: 1049
Joined: Wed Aug 04, 2004 4:18 pm
Location: Washington, DC

Re: CONSKY: A Sky CCD Integration Simulation

Postby owlice » Mon Oct 12, 2015 8:20 pm

Changed site URL from http://asterisk.apod.com/download/file.php?id=3369 to
http://asterisk.apod.com/library/ASCL/consky/consky.zip (change necessitated by retirement of old ASCL site)
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