PI: J Allyn Smith, Austin Peay State U., firstname.lastname@example.org
Address: Physics Department, 601 College St.; P.O. Box 4608, Clarksville, TN 37044 USA
CoI: Douglas Tucker, FNAL
CoI: Sahar Allam, FNAL
CoI: Deborah J Gulledge, Austin Peay State U.
CoI: William Wester, FNAL
CoI: Jacob M Robertson, Austin Peay State U.
Title: Targeted Samples of the Hot Stellar Content in the Southern Sky
Abstract: This proposal is a continuation of our program to identify the hot stellar component -- in particular, pure-hydrogen-atmosphere (``DA'') white dwarfs -- in the Southern sky. These objects will be vital for the absolute color calibration of future Southern Sky CCD-based imaging surveys and facilities, such as the Dark Energy Survey (DES) and the Large Synoptic Survey Telescope. Previously, we focused on identifying candidate hot stars by performing $u,g$-band imaging within the Blanco Cosmology Survey and PreCam Survey fields. Here, we continue to expand our program in two ways: (1) using the CTIO-0.9m telescope to obtain full $ugriz$ imaging for potentially hot WDs from the SuperCOSMOS survey (Rowell & Hambly, 2011) within the DES footprint; and (2) performing medium-resolution spectroscopy with the SOAR telescope to classify our candidates from our previous imaging runs, as well as candidates from other sources (e.g. the McCook & Sion WD Catalog and the SDSS DR-10 catalog), and determine their effective surface temperatures and surface gravities. In addition to providing calibration stars for future surveys and facilities, this data set will permit studies of the white dwarf luminosity function and of Galactic structure.
Program Type: Standard/Galactic
Run 1 (2016B): CT-0.9m/CFIM -- 5n on Oct 03 - Oct 07 2016
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360