The Pan-STARRS wide-field optical/NIR imaging survey

By N. Kaiser, W. Burgett, K. Chambers, Larry Denneau, Jim Heasley, Robert Jedicke, E. Magnier, J. Morgan, P. Onaka, J. Tonry. Astronomical Telescopes + Instrumentation, 2010

411 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

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Citations in the corpus

THE Pan-STARRS1 PHOTOMETRIC SYSTEM (2012, background): “The Pan-STARRS1 system is a 1.8 m aperture, f/4.4 telescope (Hodapp et al. 2004) illuminating a 1.4 Gpixel detector spanning a 3.3◦ field of view (Tonry et al. (2008) and Onaka et al. (2008)), located on Haleakala (Kaiser et al. (2010)), and dedicated to sky survey observations (Chambers et al. (in ”
The Zwicky Transient Facility: System Overview, Performance, and First Results (2018, background): “Subsequently the pipeline fits a zeropoint and color term to photometrically calibrate the quadrant to PanSTARRS 1 (Chambers et al. 2016).”
Galaxy Groups Within 3500 km s−1 (2017, background): “The situation could be vastly improved in the future with systematic incorporation of deep infrared or optical photometry from, for example, WISE, the Wide-field Infrared Survey Explorer (Wright et al. 2010) or Pan-STARRS (Kaiser et al. 2010).”
The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample (2017, background): “The description of the PS1 survey is given in Kaiser et al. (2010).”
The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release (2020, methodology): “SDSS-IV/eBOSS used the same DR8 imaging as SDSS-III/ BOSS, but leveraged new photometric calibrations using the “uber-calibration” method of Padmanabhan et al. (2008), updated by Schlafly et al. (2012) to be pinned to PanSTARRS imaging (Kaiser et al. 2010).”
The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole? (2018, methodology): “We also perform our own photometry using images from the Pan-STARRS 3pi survey (Kaiser et al. 2010), the Two Micron All-Sky Survey (2MASS; Huchra et al. 2012) and the Wide-field Infrared Survey Explorer (WISE; Wright et al. 2010).”
The Sloan Digital Sky Survey Reverberation Mapping Project: Sample Characterization (2018, methodology): “Started in 2014, SDSS-RM will continue through 2020 to build a spectroscopic time baseline of seven years, and a photometric time baseline of a decade when combining dedicated SDSS-RM imaging (2014-2020) with earlier (2010-2013) imaging from the Pan-STARRS 1 (PS1, Kaiser et al. 2010) survey.”
A LARGE CATALOG OF ACCURATE DISTANCES TO MOLECULAR CLOUDS FROM PS1 PHOTOMETRY (2014, methodology): “We have developed a related technique: we simultaneously infer the distance and reddening to stars from their PanSTARRS1 (Kaiser et al. 2010, PS1) photometry and bracket clouds between foreground unreddened stars and background reddened stars.”
The Dark Energy Survey Image Processing Pipeline (2018, background): “03 17 data.1 DES is one in a series of large optical surveys that includes the Sloan Digital Sky Survey (SDSS; York et al. 2000), the Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS1 or PS1; Kaiser et al. 2010), Kilo Degree Survey (KiDS; de Jong et al. 2013), the Hyper Suprime-Cam”
COSMOLOGICAL CONSTRAINTS FROM MEASUREMENTS OF TYPE Ia SUPERNOVAE DISCOVERED DURING THE FIRST 1.5 yr OF THE Pan-STARRS1 SURVEY (2013, background): “A more complete description of the Pan-STARRS1 system, both hardware and software, is provided by Kaiser et al. (2010).”
PHOTOMETRIC CALIBRATION OF THE FIRST 1.5 YEARS OF THE PAN-STARRS1 SURVEY (2012, background): “The Pan-STARRS1 System and Surveys The Pan-STARRS1 system is a wide-field optical imager devoted to survey operations (Kaiser et al. 2010).”
The Dark Energy Survey: Data Release 1 (2018, background): “…including the Sloan Digital Sky Survey (SDSS; York et al. 2000), the Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS1 or PS1; Kaiser et al. 2010), the Kilo Degree Survey (KiDS; de Jong et al. 2013), the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP; Aihara et al.…”
SUBARU HIGH-z EXPLORATION OF LOW-LUMINOSITY QUASARS (SHELLQs). I. DISCOVERY OF 15 QUASARS AND BRIGHT GALAXIES AT 5.7 < z < 6.9 (2016, positive): “New optical widefield surveys such as the Panoramic Survey Telescope & Rapid Response System 1 (Pan-STARRS1; Kaiser et al. 2010) 3π survey and the Dark Energy Survey (Dark Energy Survey Collaboration 2016) are equipped with a y-band filter centered at 9500 – 10000 Å, and are starting to deliver…”
MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARS (2013, background): “Advances in optical detector technology, computer processing power, and data storage capability have enabled new sky surveys (e.g., the Sloan Digital Sky Survey; York et al. 2000); triggered many new optical transient surveys, such as the Palomar Transient Factory (Law et al. 2009) and Pan-STARRS1 (”
THE PAN-STARRS1 DISTANT z > 5.6 QUASAR SURVEY: MORE THAN 100 QUASARS WITHIN THE FIRST GYR OF THE UNIVERSE (2016, background): “Over the last years, we have been searching for highredshift quasars in the PS1 survey (Kaiser et al. 2002, 2010), which has imaged the whole sky above a declination of −30◦ for about four years in five filters (gP1, rP1, iP1, zP1, yP1).”
Cosmic X-ray surveys of distant active galaxies (2015, background): “…the coverage down to optical magnitudes of 23–24 in five optical bands over practically the entire sky: for example, the SDSS (e.g., York et al 2000; Aihara et al 2011), VST ATLAS (e.g., Shanks et al 2013), PanSTARRS (e.g., Kaiser et al 2010; Magnier et al 2013), and DES (e.g., Flaugher 2005).”
RAPIDLY EVOLVING AND LUMINOUS TRANSIENTS FROM PAN-STARRS1 (2014, background): “Located on Haleakala, Hawaii, it possesses a 1.8-m diameter primary mirror and a 3◦.3 diameter field of view (Kaiser et al. 2010).”
PERIODOGRAMS FOR MULTIBAND ASTRONOMICAL TIME SERIES (2015, background): “For surveys that obtain multiband data one band at a time, such as Pan-STARRS (Kaiser et al. 2010) and DES (Flaugher 2008), and for future multicolor surveys such as LSST (Ivezić et al. 2008), this ad hoc approach is not optimal.”
THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: TECHNICAL OVERVIEW (2014, background): “Kaiser et al. (2010) describe the overall PS1 system, including hardware and software.”