A Caltech Library Service

Items where Person is "Noble-A-G"

Up a level
Export as [feed] Atom [feed] RSS 1.0 [feed] RSS 2.0
Group by: Date | Item Type | First Author | No Grouping
Jump to: 2018 | 2017 | 2016 | 2015 | 2012
Number of items: 7.


Foltz, R. and Wilson, G. and Muzzin, A. et al. (2018) Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population. Astrophysical Journal, 866 (2). Art. No. 136. ISSN 1538-4357.


Bonaventura, N. R. and Webb, T. M. A. and Muzzin, A. et al. (2017) Red but not dead: unveiling the star-forming far-infrared spectral energy distribution of SpARCS brightest cluster galaxies at 0 < z < 1.8. Monthly Notices of the Royal Astronomical Society, 469 (2). pp. 1259-1281. ISSN 0035-8711.

Delahaye, A. G. and Webb, T. M. A. and Nantais, J. et al. (2017) Galaxy Merger Candidates in High-redshift Cluster Environments. Astrophysical Journal, 843 (2). Art. No. 126. ISSN 1538-4357.


Noble, A. G. and Webb, T. M. A. and Yee, H. K. C. et al. (2016) The Phase Space of z ~ 1.2 SpARCS Clusters: Using Herschel to Probe Dust Temperature as a Function of Environment and Accretion History. Astrophysical Journal, 816 (2). Art. No. 48. ISSN 0004-637X.


Webb, Tracy M. A. and Muzzin, Adam and Noble, Alison et al. (2015) The Star-Formation History of BCGs to z = 1.8 from the SpARCS/SWIRE Survey: Evidence for significant in-situ star formation at high-redshift. Astrophysical Journal, 814 (2). Art. No. 96. ISSN 0004-637X.

Webb, Tracy and Noble, Allison and DeGroot, Andrew et al. (2015) An Extreme Starburst in the Core of a Rich Galaxy Cluster at z = 1.7. Astrophysical Journal, 809 (2). Art. No. 173. ISSN 0004-637X.


Lidman, C. and Suherli, J. and Wilson, G. et al. (2012) Evidence for significant growth in the stellar mass of brightest cluster galaxies over the past 10 billion years. Monthly Notices of the Royal Astronomical Society, 427 (1). pp. 550-568. ISSN 0035-8711.

This list was generated on Tue Aug 11 15:28:32 2020 PDT.