Atmosphere Extinction at the ORM on La Palma: A 20 yr Statistical Database Gathered at the Carlsberg Meridian Telescope
A. Garcia-Gil, C. Munoz-Tunon, A.M. Varela

TL;DR
This study analyzes 20 years of atmospheric extinction data at ORM using photometric measurements, revealing seasonal variations, the impact of volcanic eruptions, and no significant long-term changes in sky transparency.
Contribution
It provides the longest homogeneous in situ database on atmospheric extinction at ORM, including volcanic impact analysis and seasonal variation insights.
Findings
Median extinction coefficient kV is 0.13 mag/airmass.
Summer months show higher dust and cirrus impact (~29%).
No significant secular changes in atmospheric extinction over 20 years.
Abstract
The Observatorio del Roque de los Muchachos (ORM), in the Canary Islands (Spain), was one of the candidates to host the future European Extremely Large Telescope (E-ELT) and is the site of the Gran Telescopio Canarias (GTC), the largest optical infrared facility to date. Sky transparency is a key parameter as it defines the quality of the photometry to be acquired in the astronomical observations. We present a study of the atmosphere extinction at the ORM, carried out after analysis of a database spanning more than 20 yr, to our knowledge, the longest and most complete and homogeneous in situ database available for any observatory. It is based on photometric measurements in the V band and r' band (transformed to the V -band extinction coefficient kV) using the Carlsberg Meridian Telescope (CMT). Clear seasonal variations that repeat yearly are observed. The median value of kV is 0.13…
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