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Maintained by LG |
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Outside ResponsibilitiesCo-Investigator, Far Ultraviolet Spectroscopic Explorer Honors and AwardsFellow of the Royal Society of the United Kingdom, 2004 Selected Recent PublicationsThe Cosmic Evolution of Hard X-Ray-selected Active Galactic Nuclei An
850 Micron SCUBA Survey of the Hubble Deep Field-North GOODS
Region The Evolution of the Ultraluminous Infrared Galaxy Population
from Redshift
0 to 1.5 Faint 6.7 Micron Galaxies and Their Contributions to the
Stellar Mass
Density in the Universe The Evolution of the Ultraluminous Infrared Galaxy
Population from Redshift
0 to 1.5 The
Luminosity Function of Lyα Emitters
at Redshift z ~ 5.7 A Deep Wide-Field, Optical, and Near-Infrared
Catalog of a Large Area
around the Hubble Deep Field North The
Changing
Active
Galactic
Nucleus
Population Optical
and
Infrared
Properties
of
the
2 Ms
Chandra
Deep
Field
North
X-Ray
Sources The
Chandra
Deep
Field
North
Survey.
XIII.
2 Ms
Point-Source
Catalogs A
Deep
6.7 µm
Survey
in
the
SSA13
Field
with
ISO A
Submillimeter
and
Radio
Survey
of
Gamma-Ray
Burst
Host
Galaxies:
A Glimpse
into
the
Future
of
Star
Formation
Studies Astronomy:
Wrestling
Monsters
in
Deep
Space Imaging
Large-Scale
Structure
in
the
X-Ray
Sky The
Properties
of
Microjansky
Radio
Sources
in
the
Hubble
Deep
Field-North,
SSA
13,
and
SSA
22
Fields Very
High
Redshift
X-Ray-selected
Active
Galactic
Nuclei
in
the
Chandra
Deep
Field-North The
Redshift
Evolution
of
the
2-8
keV
X-Ray
Luminosity
Function The
Hawaii+Anglo-Australian
Observatory
K-Band
Galaxy
Redshift
Survey.
I.
The
Local
K-Band
Luminosity
Function Mid-Infrared
Identification
of
Faint
Submillimeter
Sources X-Ray,
Optical,
and
Infrared
Imaging
and
Spectral
Properties
of
the
1 Ms
Chandra
Deep
Field
North
Sources Faint
Submillimeter
Counts
from
Deep
850
Micron
Observations
of
the
Lensing
Clusters
A370,
A851,
and
A2390 Approaching
Reionization:
The
Evolution
of
the
Ly-alpha
Forest
from z =
4 to z =
6 A
Redshift z =
6.56
Galaxy
behind
the
Cluster
Abell
370 The
2-8
keV
X-Ray
Number
Counts
Determined
from
Chandra
Blank
Field Observations Star
Formation
History
since z =
1.5
as
Inferred
from
Rest-Frame
Ultraviolet
Luminosity
Density
Evolution Supermassive
Black
Hole
Accretion
History
Inferred
from
a Large
Sample
of
Chandra
Hard
X-Ray
Sources Submillimeter
Properties
of
the
1 Ms
Chandra
Deep
Field-North
X-Ray
Sample Resolving
the
Structure
of
Ionized
Helium
in
the
Intergalactic
Medium
with
the
Far
Ultraviolet
Spectroscopic
Explorer FUSE
Observations
of
Cooling-Flow
Gas
in
the
Galaxy
Clusters
A1795
and
A2597 Galaxy
Halo
Masses
from
Galaxy-Galaxy
Lensing The
Chandra
Deep
Survey
of
the
Hubble
Deep
Field
North
Area.
II.
Results
from
the
Caltech
Faint
Field
Galaxy
Redshift
Survey
Area Detecting
High-Redshift
Evolved
Galaxies
as
the
Hosts
of
Optically
Faint
Hard
X-Ray
Sources The
Nature
of
the
Hard
X-Ray
Background
Sources:
Optical,
Near-Infrared,
Submillimeter,
and
Radio
Properties
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