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18 papers · 2 filters
Probing High-Redshift Galaxy Formation at the Highest Luminosities: New Insights from DEIMOS Spectroscopy
Kyoung-Soo Lee, Arjun Dey, Michael C. Cooper +2
We present DEIMOS spectroscopic observations of the most UV-luminous star-forming galaxies at 3.2<z<4.6. Our sample contains galaxies with luminosities of L*<L<7L* and is one of th…
The Clustering of Extremely Red Objects
David P. Palamara, Michael J. I. Brown, Buell T. Jannuzi +10
We measure the clustering of Extremely Red Objects (EROs) in ~8 deg^2 of the NOAO Deep Wide Field Survey Boötes field in order to establish robust links between ERO z~1.2 and local…
A Successful Broad-band Survey for Giant Lya Nebulae II: Spectroscopic Confirmation
Moire K. M. Prescott, Arjun Dey, Buell T. Jannuzi
Using a systematic broad-band search technique, we have carried out a survey for large Lya nebulae (or Lya "blobs") at 2<z<3 within 8.5 square degrees of the NOAO Deep Wide-Field S…
PAH Emission in Powerful High-Redshift Radio Galaxies
Jason Ian Rawlings, Nicholas Seymour, Mathew Page +15
We present the mid-infrared spectra of seven of the most powerful radio-galaxies known to exist at 1.5 < z < 2.6. The radio emission of these sources is dominated by the AGN with 5…
Addressing Decadal Survey Science through Community Access to Highly Multiplexed Spectroscopy with BigBOSS on the KPNO Mayall Telescope
Caty Pilachowski, Carles Badenes, Stephen Bailey +87
This document summarizes the results of a community-based discussion of the potential science impact of the Mayall+BigBOSS highly multiplexed multi-object spectroscopic capability.…
Evidence for a wide range of UV obscuration in z ~ 2 dusty galaxies from the GOODS-Herschel survey
Kyle Penner, Mark Dickinson, Alexandra Pope +20
Dusty galaxies at z ~ 2 span a wide range of relative brightness between rest-frame mid-infrared (8um) and ultraviolet wavelengths. We attempt to determine the physical mechanism r…
Herschel Detection of Dust Emission from UV-Luminous Star-Forming Galaxies at 3.3<z<4.3
Kyoung-Soo Lee, Stacey Alberts, David Atlee +5
We report the Herschel SPIRE detection of dust emission arising from UV-luminous (L>~L*) star-forming galaxies at 3.3<z<4.3. Our sample of 1,913 Lyman Break Galaxy (LBG) candidates…
A UV Ultra-luminous Lyman Break Galaxy at Z=2.78 in NDWFS Bootes Field
Fuyan Bian, Xiaohui Fan, Linhua Jiang +7
We present one of the most ultraviolet (UV) luminous Lyman Break Galaxies (LBGs) (J1432+3358) at z=2.78, discovered in the NOAO Deep Wide-Field Survey (NDWFS) Bootes field. The R-b…
IDCS J1433.2+3306: An IR-Selected Galaxy Cluster at z = 1.89
Gregory R. Zeimann, S. A. Stanford, Mark Brodwin +6
We report the discovery of an IR-selected galaxy cluster in the IRAC Distant Cluster Survey (IDCS). New data from the Hubble Space Telescope spectroscopically confirm IDCS J1433.2+…
Assembly of the Red Sequence in Infrared-Selected Galaxy Clusters from the IRAC Shallow Cluster Survey
Gregory F. Snyder, Mark Brodwin, Conor M. Mancone +9
We present results for the assembly and star formation histories of massive (~L*) red sequence galaxies in 11 spectroscopically confirmed, infrared-selected galaxy clusters at 1.0…
Rapid Coeval Black Hole and Host Galaxy Growth in MRC 1138-262: The Hungry Spider
N. Seymour, B. Altieri, C. De Breuck +30
We present a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC 1138-26 at z = 2.156, also known as the Spiderweb Galaxy. By combinin…
IDCS J1426.5+3508: Cosmological implications of a massive, strong lensing cluster at Z = 1.75
Anthony H. Gonzalez, S. A. Stanford, Mark Brodwin +6
The galaxy cluster IDCS J1426.5+3508 at z = 1.75 is the most massive galaxy cluster yet discovered at z > 1.4 and the first cluster at this epoch for which the Sunyaev-Zel'Dovich e…
IDCS J1426.5+3508: Sunyaev-Zel'dovich Measurement of a Massive IR-selected Cluster at z=1.75
M. Brodwin, A. H. Gonzalez, S. A. Stanford +14
We report 31 GHz CARMA observations of IDCS J1426.5+3508, an infrared-selected galaxy cluster at z = 1.75. A Sunyaev-Zel'dovich decrement is detected towards this cluster, indicati…
IDCS J1426+3508: Discovery of a Massive, IR-Selected Galaxy Cluster at z = 1.75
S. A. Stanford, M. Brodwin, Anthony H. Gonzalez +6
We report the discovery of an IR-selected massive galaxy cluster in the IRAC Distant Cluster Survey (IDCS). We present new data from the Hubble Space Telescope and the W. M. Keck O…
Mid-Infrared Selection of AGN with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-Selected AGN in COSMOS
Daniel Stern, Roberto J. Assef, Dominic J. Benford +15
The Wide-field Infrared Survey Explorer (WISE) is an extremely capable and efficient black hole finder. We present a simple mid-infrared color criterion, W1-W2 \geq 0.8 (i.e., [3.4…
CO J=2-1 line emission in cluster galaxies at z~1: fueling star formation in dense environments
Jeff Wagg, Alexandra Pope, Stacey Alberts +9
We present observations of CO J=2-1 line emission in infrared-luminous cluster galaxies at z~1 using the IRAM Plateau de Bure Interferometer. Our two primary targets are optically…
The Spectral Energy Distributions and Infrared Luminosities of z \approx 2 Dust Obscured Galaxies from Herschel and Spitzer
J. Melbourne, B. T. Soifer, Vandana Desai +6
Dust-obscured galaxies (DOGs) are a subset of high-redshift (z \approx 2) optically-faint ultra-luminous infrared galaxies (ULIRGs, e.g. L_{IR} > 10^{12} Lsun). We present new far-…
The Galaxy Optical Luminosity Function from the AGN and Galaxy Evolution Survey (AGES)
Richard J. Cool, Daniel J. Eisenstein, Christopher S. Kochanek +9
We present the galaxy optical luminosity function for the redshift range 0.05<z<0.75 from the AGN and Galaxy Evolution Survey (AGES), a spectroscopic survey of 7.6 sq. deg. in the…