Survey and Other Telescope Technologies and Discoveries

By J. Tyson, S. Wolff. 2002

276 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/bfd85fd7b5c97241e48f89b7669806410c07e9fb

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Citations in the corpus

FIRST RESULTS FROM THE CATALINA REAL-TIME TRANSIENT SURVEY (2008, methodology): “For this reason subtraction has been particularly successful for dense stellar fields observed in supernova searches such used by the SNfactory (Aldering et al. 2002).”
The WFCAM Science Archive (2006, background): “Key words: astronomical databases – surveys: infrared – stars: general – galaxies: general – cosmology: observations”
Large Synoptic Survey Telescope: From Science Drivers to Reference Design (2008, methodology): “The large LSST étendue is achieved in a novel three-mirror design (modified Paul-Baker, Davison and Angel 2002) with a very fast f/1.25 beam.”
The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution (2005, background): “A further major leap forward will be enabled by upcoming deep synoptic sky surveys, such as Pan-STARRS (Kaiser et al. 2002) andLSST (Tyson 2002).”
THE GALAXY CONTENT OF SDSS CLUSTERS AND GROUPS (2007, unknown): “37 80 v1 [ as tr oph ] 2 2 O ct 2 00 7 tions”
PHYSICS OF ECLIPSING BINARIES. II. TOWARD THE INCREASED MODEL FIDELITY (2016, methodology): “This decade has provided us with a range of ground-breaking surveys and missions: MOST (Walker et al. 2003), CoRoT (Baglin 2003), Kepler (Borucki et al. 2010), Pan-Starrs (Kaiser et al. 2002), Gaia (de Bruijne 2012), and LSST (Tyson & LSST 2002), to name just a few.”
EFFICIENT PHOTOMETRIC SELECTION OF QUASARS FROM THE SLOAN DIGITAL SKY SURVEY. II. ∼1, 000, 000 QUASARS FROM DATA RELEASE 6 (2004, unknown): “On the other hand, large-scale synoptic surveys such as the Large Synoptic Survey Telescope (LSST; Tyson 2002), the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS; Kaiser et al. 2002), and the Dark Energy Survey (DES; The Dark Energy Survey Collaboration 2005) will, in the next dec”
Wide field aplanatic two-mirror telescopes for ground-based γ-ray astronomy (2006, background): “(17) Again, the parameter Y1 = 1/4 is chosen by convention.”
SDSS data management and photometric quality assessment (2004, background): “The success of SDSS provides encouragement that even more ambitious surveys, such as LSST (Tyson 2002), which is expected to produce and immediately process 20 TB of data per observing night, may also be successful endeavors.”