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Open Astronomy

formerly Baltic Astronomy

Editor-in-Chief: Barbuy, Beatriz


IMPACT FACTOR 2018: 0.350

CiteScore 2018: 0.24

SCImago Journal Rank (SJR) 2018: 0.202
Source Normalized Impact per Paper (SNIP) 2018: 0.144

ICV 2018: 120.66

Open Access
Online
ISSN
2543-6376
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Volume 21, Issue 1-2

Issues

Characterizing the Photometric Response of the ANS Collaboration Monitoring Program

U. Munari / S. Moretti
Published Online: 2017-03-23 | DOI: https://doi.org/10.1515/astro-2017-0354

Abstract

the ANS Collaboration uses the UBV RCIC filters from various commercial manufacturers (Omega Optical, Custom Scientific, Schuler, Optec, Astrodon) for its ongoing photometric monitoring of symbiotic stars. We measured their transmittance profiles over the range 2000 Å to 1.1 μm for various operating conditions, and we are monitoring their evolution over time. Their field performance in terms of color equations has been evaluated by analyzing the transformations from local to standard system of the 14602 observing runs so far collected on symbiotic stars with the ANS Collaboration telescopes. Ageing effects, red leaks and transmittance vs. angle of incidence are also evaluated.

Keywords: stars; symbiotic binaries; novae; photometry

References

About the article

Received: 2011-12-02

Accepted: 2011-12-15

Published Online: 2017-03-23

Published in Print: 2012-06-01


Citation Information: Open Astronomy, Volume 21, Issue 1-2, Pages 22–31, ISSN (Online) 2543-6376, DOI: https://doi.org/10.1515/astro-2017-0354.

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© 2017. This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License. BY-NC-ND 4.0

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[1]
Ulisse Munari and Sergio Dallaporta
New Astronomy, 2014, Volume 27, Page 25

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