1. The time-domain spectroscopic survey: Understanding the optically variable sky with sequels in SDSS-III
- Author
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Ruan, JJ, Anderson, SF, Green, PJ, Morganson, E, Eracleous, M, Myers, AD, Badenes, C, Bershady, MA, Brandt, WN, Chambers, KC, Davenport, JRA, Dawson, KS, Flewelling, H, Heckman, TM, Isler, JC, Kaiser, N, Kneib, JP, MacLeod, CL, Paris, I, Ross, NP, Runnoe, JC, Schlafly, EF, Schmidt, SJ, Schneider, DP, Schwope, AD, Shen, Y, Stassun, KG, Szkody, P, Waters, CZ, and York, DG
- Subjects
quasars: general ,stars: variables: general ,surveys ,astro-ph.GA ,astro-ph.CO ,astro-ph.SR ,Astronomy & Astrophysics ,Astronomical and Space Sciences ,Atomic ,Molecular ,Nuclear ,Particle and Plasma Physics ,Physical Chemistry ,Atomic ,Molecular ,Nuclear ,Particle and Plasma Physics ,Physical Chemistry (incl. Structural) - Abstract
The Time-Domain Spectroscopic Survey (TDSS) is an SDSS-IV eBOSS subproject primarily aimed at obtaining identification spectra of ∼220,000 optically variable objects systematically selected from SDSS/Pan-STARRS1 multi-epoch imaging. We present a preview of the science enabled by TDSS, based on TDSS spectra taken over ∼320 deg2 of sky as part of the SEQUELS survey in SDSS-III, which is in part a pilot survey for eBOSS in SDSS-IV. Using the 15,746 TDSS-selected single-epoch spectra of photometrically variable objects in SEQUELS, we determine the demographics of our variability-selected sample and investigate the unique spectral characteristics inherent in samples selected by variability. We show that variability-based selection of quasars complements color-based selection by selecting additional redder quasars and mitigates redshift biases to produce a smooth quasar redshift distribution over a wide range of redshifts. The resulting quasar sample contains systematically higher fractions of blazars and broad absorption line quasars than from color-selected samples. Similarly, we show that M dwarfs in the TDSS-selected stellar sample have systematically higher chromospheric active fractions than the underlying M-dwarf population based on their Hα emission. TDSS also contains a large number of RR Lyrae and eclipsing binary stars with main-sequence colors, including a few composite-spectrum binaries. Finally, our visual inspection of TDSS spectra uncovers a significant number of peculiar spectra, and we highlight a few cases of these interesting objects. With a factor of ∼15 more spectra, the main TDSS survey in SDSS-IV will leverage the lessons learned from these early results for a variety of time-domain science applications.
- Published
- 2016