Design of the Pan‐STARRS telescopes

By K. Hodapp, N. Kaiser, H. Aussel, W. Burgett, K. Chambers, M. Chun, T. Dombeck, A. Douglas, D. Hafner, Jim Heasley and 21 more. 2004

140 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/554f4dd45ad99ac4f7ce1ec1fe17007e499a1d22

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In Astronomy and Astrophysics

Citations in the corpus

Light-curve modelling of superluminous supernova 2006gy: collision between supernova ejecta and a dense circumstellar medium (2012, background): “…surveys such as the Texas Supernova Search (Quimby 2006a), Palomar Transient Factory (Law et al. 2009; Rau et al. 2009), Catarina Real-time Transient Survey (Drake et al. 2009) and the Panoramic Survey Telescope & Rapid Response System (Hodapp et al. 2004) discovered new kinds of supernovae (SNe).”
Distant radio galaxies and their environments (2008, methodology): “Presently combination of the new radio surveys with planned new deep optical and infrared wide-field surveys, such as PAN-STARRS (Hodapp et al 2004) and those with the VST and VISTA (Arnaboldi et al 2007) will be used to identify HzRGs and provide photometric data.”
FIRST RESULTS FROM THE CATALINA REAL-TIME TRANSIENT SURVEY (2008, background): “Several large experiments (LSST, Ivezic et al. 2008; PanSTARRS, Hodapp et al. 2004; SkyMapper, Keller et al. 2007) are set to make a major impact in the near future by covering thousands of square degrees with targets ranging from distant supernovae to near earth asteroids.”
A LARGE CATALOG OF ACCURATE DISTANCES TO MOLECULAR CLOUDS FROM PS1 PHOTOMETRY (2014, methodology): “The 1.8 m telescope has a 3◦ field of view outfitted with the 1.4 billion pixel GPC1 camera (Hodapp et al. 2004; Tonry & Onaka 2009; Onaka et al. 2008).”
The Optical to Mid-infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS, and WISE Surveys (2019, background): “The Pan-STARRS1 survey (Hodapp et al. 2004) images the sky in five broadband filters, g, r, i, z, y, covering from 400 nm to 1 μm(Stubbs et al. 2010).”
PHOTOMETRIC CALIBRATION OF THE FIRST 1.5 YEARS OF THE PAN-STARRS1 SURVEY (2012, background): “The approximately one trillion pixels per night are processed in a massively parallel fashion at the Maui High Performance Computer Center.”
The Pan-STARRS1 Database and Data Products (2016, methodology): “The wide-field optical design of the telescope (Hodapp et al. 2004) allowed PS1 to observe most of the 3πSurvey area in each of five filters (gP1, rP1, iP1, zP1, yP1) between 10 and 15 times.”