- Kim, AG;
- Padmanabhan, N;
- Aldering, G;
- Allen, SW;
- Baltay, C;
- Cahn, RN;
- D’Andrea, CB;
- Dalal, N;
- Dawson, KS;
- Denney, KD;
- Eisenstein, DJ;
- Finley, DA;
- Freedman, WL;
- Ho, S;
- Holz, DE;
- Kasen, D;
- Kent, SM;
- Kessler, R;
- Kuhlmann, S;
- Linder, EV;
- Martini, P;
- Nugent, PE;
- Perlmutter, S;
- Peterson, BM;
- Riess, AG;
- Rubin, D;
- Sako, M;
- Suntzeff, NV;
- Suzuki, N;
- Thomas, RC;
- Wood-Vasey, WM;
- Woosley, SE
This document presents the results from the Distances subgroup of the Cosmic Frontier Community Planning Study (Snowmass 2013). We summarize the current state of the field as well as future prospects and challenges. In addition to the established probes using Type Ia supernovae and baryon acoustic oscillations, we also consider prospective methods based on clusters, active galactic nuclei, gravitational wave sirens and strong lensing time delays.
