827 citations · 2.1k across the 18 of their papers we have counts for
18 papers
The Host Galaxy of FRB 20190520B and Its Unique Ionized Gas Distribution
Xiang-Lei Chen, Chao-Wei Tsai, Daniel Stern +13
The properties of host galaxies associated with Fast Radio Bursts (FRBs) provide critical information for inferring the progenitors and radiation mechanisms of these bursts. We rep…
Discovery of a Low-Redshift Hot Dust-Obscured Galaxy
Guodong Li, Chao-Wei Tsai, Daniel Stern +10
We report the discovery of the hyperluminous, highly obscured AGN WISE J190445.04+485308.9 (W1904+4853 hereafter, ) at z=0.415. Its well-s…
An Exploration of How Training Set Composition Bias in Machine Learning Affects Identifying Rare Objects
Sean E. Lake, Chao-Wei Tsai
When training a machine learning classifier on data where one of the classes is intrinsically rare, the classifier will often assign too few sources to the rare class. To address t…
Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA
Tanio Diaz-Santos, Roberto J. Assef, Peter R. M. Eisenhardt +9
Hot, dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous obscured quasars identified by WISE. We present ALMA observations of the [CII] fine-structure line and und…
The Contribution of Galaxies to the Cosmic Infrared Background as Measured Using WISE
Sean E. Lake, Edward L. Wright, Roberto J. Assef +4
The study of the extragalactic background light (EBL) in the optical and near infrared has received a lot of attention in the last decade, especially near a wavelength of $λ\approx…
The role of the most luminous, obscured AGN in galaxy assembly at z~2
Duncan Farrah, Sara Petty, Brian Connolly +14
We present HST WFC3 F160W imaging and infrared spectral energy distributions for twelve extremely luminous, obscured AGN at , selected via "Hot, Dust Obscured" mid-infra…
The 2.4 m Galaxy Luminosity Function as Measured Using WISE. III. Measurement Results
S. E. Lake, E. L. Wright, R. J. Assef +5
The WISE satellite surveyed the entire sky multiple times in four infrared wavelengths (3.4, 4.6, 12, and m; Wright et al. 2010). The unprecedented combination of coverage a…
The 2.4 m Galaxy Luminosity Function as Measured Using WISE. II. Sample Selection
S. E. Lake, E. L. Wright, R. J. Assef +5
The WISE satellite surveyed the entire sky multiple times in four infrared (IR) wavelengths ( and m, Wright et al. 2010). This all-sky IR photometric surve…
The 2.4 m Galaxy Luminosity Function as Measured Using WISE. I. Measurement Techniques
S. E. Lake, E. L. Wright, C. -W. Tsai +1
The astronomy community has at its disposal a large back catalog of public spectroscopic galaxy redshift surveys that can be used for the measurement of luminosity functions. Utili…
-corrections: an Examination of their Contribution to the Uncertainty of Luminosity Measurements
Sean E. Lake, E. L. Wright
In this paper we provide formulae that can be used to determine the uncertainty contributed to a measurement by a -correction and, thus, valuable information about which flux me…
NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-Selected Quasars at z ~ 2
D. Stern, G. B. Lansbury, R. J. Assef +30
We report on a NuSTAR and XMM-Newton program that has observed a sample of three extremely luminous, heavily obscured WISE-selected AGN at z~2 in a broad X-ray band (0.1 - 79 keV).…
UV-bright nearby early type galaxies observed in the mid-infrared: evidence for a multi-stage formation history by way of WISE and GALEX imaging
S. M. Petty, J. D. Neill, T. H. Jarrett +9
In the local Universe, 10% of massive elliptical galaxies are observed to exhibit a peculiar property: a substantial excess of ultraviolet emission (UVX) over what is expected from…
Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas
T. H. Jarrett, F. Masci, C. W. Tsai +15
The Wide-field Infrared Survey Explorer (WISE) mapped the entire sky at mid-infrared wavelengths 3.4, 4.6, 12 and 22 microns. The mission was primarily designed to extract point so…
Submillimeter Follow-up of WISE-Selected Hyperluminous Galaxies
Jingwen Wu, Chao-Wei Tsai, Jack Sayers +20
We have used the Caltech Submillimeter Observatory (CSO) to follow-up a sample of WISE-selected, hyperluminous galaxies, so called W1W2-dropout galaxies. This is a rare (~ 1000 all…
Constructing a WISE High Resolution Galaxy Atlas
T. H. Jarrett, F. Masci, C. W. Tsai +16
After eight months of continuous observations, the Wide-field Infrared Survey Explorer (WISE) mapped the entire sky at 3.4 μm, 4.6 μm, 12 μm and 22 μm. We have begun a dedicated WI…
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…
Optical Spectroscopic Survey of High Latitude WISE Selected Sources
Sean E. Lake, Edward L. Wright, Sara Petty +5
We report on the results of an optical spectroscopic survey at high Galactic latitude (b\geq30°) of a sample of WISE-selected targets, grouped by WISE W1 (λ_eff = 3.4 \mum) flux, w…
The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)
J. Davy Kirkpatrick, Michael C. Cushing, Christopher R. Gelino +37
We present ground-based spectroscopic verification of six Y dwarfs (see Cushing et al), eighty-nine T dwarfs, eight L dwarfs, and one M dwarf identified by the Wide-field Infrared…