1 The Palomar - Quest ( PQ ) Survey : The Science Case
نویسنده
چکیده
3.1 The Large QSO Survey. The principal effort of the Yale group is a search for QSOs using both colors and variability as selection criteria. Different combinations of UBRIriz colors can be used to select QSOs out to z ~ 6, with a majority at z ~ 2 ± 1. Variability is essentially redshift-independent selection method. For a demonstration of the methodology, see, e.g., Rengstorf et al. (2003). Over the survey area of 15,000 deg, we expect to detect ~ 300,000 QSOs down to our flux limits. We plan to obtain spectroscopic redshifts for ~ 1,000 of them, mainly to calibrate the selection functions and photometric redshifts (which we believe we can estimate from colors with a typical accuracy Δz ≈ 0.2). We note that many of the 2dFQz survey spectroscopically identified QSOs, as well as many QSOs from SDSS and other surveys will be within our area; we will make a full use of this external information. The resulting unprecedented QSO sample will be used for several projects, as follows:
منابع مشابه
The Palomar-Quest Digital Synoptic Sky Survey
We describe briefly the Palomar-Quest (PQ) digital synoptic sky survey, including its parameters, data processing, status, and plans. Exploration of the time domain is now the central scientific and technological focus of the survey. To this end, we have developed a real-time pipeline for detection of transient sources. We describe some of the early results, and lessons learned which may be use...
متن کاملNew Approaches to Object Classification in Synoptic Sky Surveys
Digital synoptic sky surveys pose several new object classification challenges. In surveys where real-time detection and classification of transient events is a science driver, there is a need for an effective elimination of instrument-related artifacts which can masquerade as transient sources in the detection pipeline, e.g., unremoved large cosmic rays, saturation trails, reflections, crossta...
متن کاملQuasars as Probes of Late Reionization and Early Structure Formation
Observations of QSOs at z ∼ 5.7 − 6.4 show the appearance of Gunn-Peterson troughs around z ∼ 6, and a change in the slope of the IGM optical depth τ(z) near z ∼ 5.5. These results are interpreted as a signature of the end of the reionization era, which probably started at considerably higher redshifts. However, there also appears to be a substantial cosmic variance in the transmission of the I...
متن کاملCoordination in CE Systems: An Approach Based on the Management of Dependences between Activities
the Management of Dependences between Activities Sylvain Lizotte & Brahim Chaib-draa Computer Science Department, Laval University, Ste-Foy, PQ, Canada, G1K 7P4 e-mail: {lizotte,chaib}@ift.ulaval.ca Short form of the title: Coordination = Management of Dependences Author to whom correspondence should be sent: B. Chaib-draa Mailing address: Département Informatique, Pav. Pouliot, Université Lava...
متن کاملThe QUEST Large Area CCD Camera
We have designed, constructed, and put into operation a very large area CCD camera that covers the field of view of the 1.2 m Samuel Oschin Schmidt Telescope at the Palomar Observatory. The camera consists of 112 CCDs arranged in a mosaic of four rows with 28 CCDs each. The CCDs are pixel Sarnoff 600 # 2400 thinned, back-illuminated devices with pixels. The camera covers an area of on the 13 mm...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2005