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The Atacama Desert has long been established as an excellent site for submillimeter observations. Yet identifying potentially optimal locations for a new facility within this region can require long field campaigns that rely on the…

天体物理仪器与方法 · 物理学 2022-03-08 Pablo Gómez Toribio , Tony Mroczkowski , Anna Cabré , Carlos De Breuck , Ricardo Bustos , Rodrigo Reeves

In this study we describe an innovative method to determine potential sites for optical and infrared astronomical observations in the Andes region of northern South America. The method computes the Clear sky fraction (CSF) from…

天体物理仪器与方法 · 物理学 2015-04-24 G. Pinzón , D. González , J. Hernández

Atmospheric water vapor is the main limiting factor of atmospheric transparency in the mm and submm wavelength spectral windows. Thus, dry sites are needed for the installation and successful operation of radio astronomy observatories…

We report precipitable water vapor (PWV) measurements made at Las Campanas Observatory using optical spectra of H2O lines obtained with the Magellan echelle spectrograph, and calculated using a robust technique that is accurate to 5-10%.…

The Himalayan plateau region of Ladakh, India, is a potential host for a science-class submillimeter observatory, building on existing astronomical infrastructure near Hanle and Merak. Using the fifth-generation European Centre for…

天体物理仪器与方法 · 物理学 2026-04-16 Tanmay Singh , Mayuri Sathyanarayana Rao , Ritoban Basu Thakur

The most important limitation for ground-based submillimetre (submm) astronomy is the broad-band absorption of the total water vapour in the atmosphere above an observation site, often expressed as the Precipitable Water Vapour (PWV). A…

天体物理仪器与方法 · 物理学 2015-06-11 P. Tremblin , N. Schneider , V. Minier , G. Al. Durand , J. Urban

Aims: We studied the precipitable water vapour (PWV) content near Cerro Armazones and discuss the potential use of our technique of modelling the telluric absorbtion lines for the investigation of other molecular layers. The site is…

天体物理仪器与方法 · 物理学 2016-03-16 Masha Lakicevic , Stefan Kimeswenger , Stefan Noll , Wolfgang Kausch , Stefanie Unterguggenberger , Florian Kerber

The reliability of astronomical observations at millimeter and sub-millimeter wavelengths closely depends on a low vertical content of water vapor as well as on high atmospheric emission stability. Although Concordia station at Dome C…

天体物理仪器与方法 · 物理学 2015-06-04 S. De Gregori , M. De Petris , B. Decina , L. Lamagna , J. R. Pardo , B. Petkov , C. Tomasi , L. Valenziano

We discuss properties of the atmospheric water vapor above the high Andean plateau region known as the Llano de Chajnantor, in the Atacama Desert of northern Chile. A combination of radiometric and radiosonde measurements indicate that the…

Consistently superb observing conditions are crucial for achieving the scientific objectives of a telescope. Submillimeter astronomy is possible only at a few exceptionally dry sites, notably Mauna Kea, the Antarctic plateau, and the…

天体物理仪器与方法 · 物理学 2016-03-01 Simon J. E. Radford

The space-temporal evaluation to characterize meteorological droughts was based on data accumulated monthly precipitation between 1996-2005 from 20 meteorological stations distributed in the Coello River basin. Data precipitation was…

地球物理 · 物理学 2017-03-08 Cruz Roa AF , Miguel Barrios

Sites for next-generation telescopes are chosen decades before the first light of a telescope. Site selection is usually based on recent measurements over a period that is too short to account for long-term changes in observing conditions…

天体物理仪器与方法 · 物理学 2022-09-28 C. Haslebacher , M. -E. Demory , B. -O. Demory , M. Sarazin , P. L. Vidale

Climate change is affecting and will increasingly affect astronomical observations. In this paper, we investigated the role some key weather parameters play in the quality of astronomical observations, and analysed their long-term trends…

In a radio interferometer, the determination of geometrical antenna positions relies on accurate calibration of the dry and wet delay of the atmosphere above each antenna. For the Atacama Large Millimeter/Submillimeter Array (ALMA), which…

Precipitable water vapour (PWV) strongly affects the quality of data obtained from millimetre- and submillimetre-wave astronomical observations, such as those for cosmic microwave background measurements. Some of these observatories have…

天体物理仪器与方法 · 物理学 2024-02-16 Junna Sugiyama , Haruki Nishino , Akito Kusaka

Radiative transfer models explain and predict interaction between solar radiation and the different elements present in the atmosphere, which are responsible for energy attenuation. In Colombia there have been neither measurements nor…

大气与海洋物理 · 物理学 2012-07-31 Camilo Delgado-Correal , Jorge Hernández , Gabriel Castaño

In this work, we present results from a long-term precipitable water vapor (PWV) study in the Chajnantor area, in northern Chile. Data from several instruments located at relevant sites for sub-millimeter and mid-infrared astronomy were…

天体物理仪器与方法 · 物理学 2016-09-07 Fernando Cortés , Rodrigo Reeves , Ricardo Bustos

Accurate determination of the geothermal gradient is critical for assessing the geothermal energy potential of a given region. Of particular interest is the case of Colombia, a country with abundant geothermal resources. A history of active…

地球物理 · 物理学 2025-10-03 Juan Camilo Mejía-Fragoso , Manuel A. Florez , Rocío Bernal-Olaya

Over the past few years a major effort has been put into the exploration of potential sites for the deployment of submillimetre astronomical facilities. Amongst the most important sites are Dome C and Dome A on the Antarctic Plateau, and…

Thanks to the first mm studies on the territory of the former USSR in the early 1960s and succeeding sub-mm measurements in the 1970s - early 1980s at wavelengths up to 0.34 mm, a completely unique astroclimate was revealed in the Eastern…

天体物理仪器与方法 · 物理学 2020-12-10 Alexander V. Lapinov , Svetlana A. Lapinova , Leonid Yu. Petrov , Daniel Ferrusca
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