The Atacama Pathfinder EXperiment (APEX) : a new submillimeter facility for southern skies

By R. Güsten, L. Nyman, Peter Schilke, K. Menten, C. Cesarsky, R. Booth. 2006

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View Paper: https://www.semanticscholar.org/paper/aa684b6531c1f60c8dbcdb2e0ae5620d34659e28

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In Astronomy and Astrophysics

Citations in the corpus

THE LARGE APEX BOLOMETER CAMERA SURVEY OF THE EXTENDED CHANDRA DEEP FIELD SOUTH (2009, methodology): “Our SMG sample comes from the survey of the ECDFS using the Large APEX BOlometer CAmera (Siringo et al. 2009, LABOCA) on the Atacama Pathfinder EXperiment (Güsten et al. 2006, APEX) 12-m telescope (the LABOCA ECDFS Submillimetre Survey, or LESS; Weiß et al. 2009).”
GAS AND DUST IN A SUBMILLIMETER GALAXY AT z = 4.24 FROM THE HERSCHEL ATLAS (2011, neutral): “The total integrated intensity of the [C ii] line is 2.64 ± 0.41 K km s−1 or 107 ± 17 Jy km s−1 (Table 2)—at 362 GHz, the gain of the APEX is 40.7 Jy K−1 in converting T ∗a to flux density (Güsten et al. 2006).”
The ATLASGAL survey: a catalog of dust condensations in the Galactic plane (2013, neutral): “…of Galactic plane surveys The ATLASGAL survey1(Schuller et al. 2009) imaged the Galactic plane between Galactic longitude,−60◦ ≤ ℓ ≤ +60◦ and Galactic latitude−1.5◦ ≤ b ≤ +1.5◦ at 870µm with the LABOCA camera (Siringo et al. 2009) on the APEX Telescope (Güsten et al. 2006) in its first campaign.”
The LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxies (2011, methodology): “…G A N D G A L A X Y S A M P L E S Our SMG sample comes from the survey of the ECDFS using the Large APEX Bolometer Camera (LABOCA; Siringo et al. 2009) on the Atacama Pathfinder Experiment (APEX; Güsten et al. 2006) 12-m telescope [the LABOCA ECDFS Submillimetre Survey (LESS); Weiß et al. 2009].”
ATLASGAL - properties of a complete sample of Galactic clumps (2017, methodology): “The data were obtained between June and November 2016 at the 12 m diameter Atacama Pathfinder Experiment telescope (APEX, Güsten et al. 2006), using the low frequency module of the Swedish Heterodyne Facility Instrument (SHeFI, Vassilev et al. 2008) receiver.”
Volatile carbon locking and release in protoplanetary disks. A study of TW Hya and HD 100546 (2016, methodology): “This publication is based on data acquired with the Atacama Pathfinder Experiment (APEX), proposals 093.”
The Atacama Large Millimeter/Submillimeter Array (2009, methodology): “In fact, the APEX telescope [10], a modified version of the Vertex design for the ALMA prototype, has operated on the site since 2005 and has observed in the 1.”
The LABOCA survey of the Extended Chandra Deep Field South: A photometric redshift survey of submillimetre galaxies (2010, methodology): “…to study SMGs detected in the Extended Chandra Deep Field-South (ECDF-S) by the Large APEX BOlometer CAmera (LABOCA; Siringo et al. 2009) on the Atacama Pathfinder EXperiment (APEX; Güsten et al. 2006) 12-m telescope as part of the LABOCA ECDF-S Submillimetre Survey (LESS; Weiß et al. 2009).”
The large APEX bolometer camera LABOCA (2008, background): “The APEX telescope (Güsten et al. 2006), as the name implies, serves as a pathfinder for the future large-scale (sub)millimeter wavelength and (far)infrared missions, namely the Atacama Large Millimeter Array (ALMA), the Herschel Space Observatory and the Stratospheric Observatory for Infrared…”
ATLASGAL - The APEX telescope large area survey of the galaxy at 870 μm (2009, background): “On an excellent 5100 m high site and at a latitude of−23◦, the 12 m diameter APEX telescope (Güsten et al. 2006a,b) is ideally located to make sensitive observations of the two inner quadrants of the Galactic Plane.”