Kate Brand, Arjun Dey, Buell T. Jannuzi, Christopher S. Kochanek, Almus T. Kenter, ...
The XBoötes Survey is a 5-ks Chandra survey of the Boötes Field of the NOAO Deep Wide-Field Survey (NDWFS). This survey is unique in that it is the largest (9.3 deg2), contiguous region imaged in...
The Star Formation and Nuclear Accretion Histories of Normal Galaxies in the AGES Survey (2009)
Watson, Casey R., Kochanek, Christopher S., Forman, William R., Hickox, Ryan C., Jones, Christine J., Brown, Michael J. I., ...
We combine IR, optical and X-ray data from the overlapping, 9.3 square degree NOAO Deep Wide-Field Survey (NDWFS), AGN and Galaxy Evolution Survey (AGES), and XBootes Survey to measure the X-ray...
A Full Year's Chandra Exposure on SDSS Quasars from the Chandra Multiwavelength Project (2008)
Green, Paul J., Aldcroft, T. L., Richards, G. T., Barkhouse, W. A., Constantin, A., Haggard, D., ...
We study the spectral energy distributions and evolution of a large sample of optically selected quasars from the Sloan Digital Sky Survey (SDSS) that were observed in 323 Chandra images analyzed by...
John D. Silverman, Paul J. Green, Dong-woo Kim, Belinda J. Wilkes, Robert A, David Morris, ...
We present X-ray and optical observations of CXOMP J213945.0-234655, a high redshift (z = 4:93) quasar discovered through the Chandra Multiwavelength Project (ChaMP). This object is the most distant...
Chandra multiwavelength project X-ray point source catalog (2007)
Kim, Minsun, Kim, Dong-Woo, Wilkes, Belinda J., Green, Paul J., Kim, Eunhyeuk, Anderson, Craig S., ...
Kim, Minsun, Wilkes, Belinda J., Kim, Dong-Woo, Green, Paul J., Barkhouse, Wayne A., Lee, Myung Gyoon, ...
Chandra Multiwavelength Project X-ray Point Source Catalog (2006)
Kim, Minsun, Kim, Dong-Woo, Wilkes, Belinda J., Green, Paul J., Kim, Eunhyeuk, Anderson, Craig S., ...
We present the Chandra Multiwavelength Project (ChaMP) X-ray point source catalog with ~6,800 X-ray sources detected in 149 Chandra observations covering \~10 deg^2. The full ChaMP catalog sample is...
Kim, Minsun, Wilkes, Belinda J., Kim, Dong-Woo, Green, Paul J., Barkhouse, Wayne A., Lee, Myung Gyoon, ...
We present the Chandra Multiwavelength Project (ChaMP) X-ray point source number counts and the cosmic X-ray background (CXRB) flux densities in multiple energy bands. From the ChaMP X-ray point...
Lens-Aided Multi-Angle Spectroscopy (LAMAS) Reveals Small-Scale Outflow Structure in Quasars (2006)
Spectral differences between lensed quasar image components are common. Since lensing is intrinsically achromatic, these differences are typically explained as the effect of either microlensing, or...
Minsun Kim, Belinda J. Wilkes, Dong-woo Kim, Paul J. Green, Wayne A. Barkhouse, Myung Gyoon Lee, ...
We present the Chandra Multiwavelength Project (ChaMP) X-ray point source number counts and cosmic X-ray background (CXRB) flux densities in multiple energy bands. From the ChaMP X-ray point source...
Minsun Kim, Dong-woo Kim, Belinda J. Wilkes, Paul J. Green, Eunhyeuk Kim, Craig S. Anderson, ...
We present the Chandra Multiwavelength Project (ChaMP) X-ray point source catalog with 6800 X-ray sources detected in 149 Chandra observations covering 10 deg 2. The full ChaMP catalog sample is 7...
The Chandra XBootes Survey - III: Optical and Near-IR Counterparts (2005)
Brand, Kate, Brown, Michael J. I., Dey, Arjun, Jannuzi, Buell T., Kochanek, Christopher S., Kenter, Almus T., ...
The XBootes Survey is a 5-ks Chandra survey of the Bootes Field of the NOAO Deep Wide-Field Survey (NDWFS). This survey is unique in that it is the largest (9.3 deg^2), contiguous region imaged in...
Discovery of a Galaxy Cluster in the Foreground of the Wide-Separation Quasar Pair UM425 (2005)
Green, Paul J., Infante, Leopoldo, Lopez, Sebastian, Aldcroft, Thomas L., Winn, Josh N.
We report the discovery of a cluster of galaxies in the field of UM425, a pair of quasars separated by 6.5arcsec. Based on this finding, we revisit the long-standing question of whether this quasar...
XBootes: An X-Ray Survey of the NDWFS Bootes Field - Paper I Overview and Initial Results (2005)
Murray, Stephen S., Kenter, Almus, Forman, William R., Jones, Christine, Green, Paul J., Kochanek, Christopher S., ...
We obtained a 5 ksec deep Chandra X-ray Observatory ACIS-I map of the 9.3 square degree Bootes field of the NOAO Deep Wide-Field Survey. Here we describe the data acquisition and analysis strategies...
Tracing the Nuclear Accretion History of the Red Galaxy Population (2005)
Brand, Kate, Dey, Arjun, Brown, Michael J. I., Watson, Casey R., Jannuzi, Buell T., Najita, Joan R., ...
We investigate the evolution of the hard X-ray luminosity of the red galaxy population using a large sample of 3316 red galaxies selected over a wide range in redshift (0.3
X-ray emitting AGN unveiled by the Chandra Multiwavelength Project (2003)
Silverman, John D., Green, Paul J., Aldcroft, Thomas L., Kim, Dong-Woo, Barkhouse, Wayne, Cameron, Robert A., ...
We present an X-ray and optical analysis of a 2-8 keV flux limited (fx > 10e-14 erg s^-1 cm^-2) sample of 126 AGN detected in 16 Chandra fields. This work represents a small though significant subset...
The Chandra Multiwavelength Project: Optical Followup of Serendipitous Chandra Sources (2003)
Green, Paul J., Silverman, J. D., Cameron, R. A., Wilkes, B. J., Barkhouse, W. A., ...
We present followup optical g', r', and i', imaging and spectroscopy of serendipitous X-ray sources detected in 6 archival Chandra, images included in the Chandra, Multiwavelength Project (ChaMP). Of...
Chandra Observations of the QSO Pair Q2345+007: Binary Quasar or Massive Dark Lens? (2002)
Green, Paul J., Kochanek, Chris, Siemiginowska, Aneta, Kim, Dong-Woo, Markevitch, Maxim, Silverman, John, ...
The components of the wide (7.3") separation quasar pair Q2345+007A,B (z=2.15) have the most strikingly similar optical spectra seen to date (Steidel & Sargent 1991) yet no detected lensing mass,...
A Chandra Survey of Broad Absorption Line Quasars (2001)
Green, Paul J., Aldcroft, Thomas L., Mathur, Smita, Wilkes, Belinda J., Elvis, Martin
We have carried out a survey with the Chandra X-ray Observatory of a sample of 10 optically bright broad absorption line (BAL) QSOs. Eight out of ten sources are detected. The 6 brightest X-ray...
Quasar Evolution and the Baldwin Effect in the Large Bright Quasar Survey (2001)
Green, Paul J., Forster, Karl, Kuraszkiewicz, Joanna
From a large homogeneous sample of optical/UV emission line measurements for 993 quasars from the Large Bright Quasar Survey (LBQS), we study correlations between emission line equivalent width and...
Emission Line Properties of the Large Bright Quasar Survey (2000)
Forster, Karl, Green, Paul J., Aldcroft, Thomas L., Vestergaard, Marianne, Foltz, Craig B., Hewett, Paul C.
We present measurements of the optical/UV emission lines for a large homogeneous sample of 993 quasars from the Large Bright Quasar Survey. Our largely automated technique accounts for continuum...
Cool Companions to Hot White Dwarfs (2000)
Green, Paul J., Ali, Babar, Napiwotzki, Ralf
We describe a near-IR photometric search for cool red dwarf companions to hot EUV-detected white dwarfs (WDs). While some composite systems have been found optically among WDs detected in recent EUV...
A Comparative Study of the Mass Distribution of Extreme Ultraviolet-Selected White Dwarfs (1999)
Napiwotzki, Ralf, Green, Paul J., Saffer, Rex A.
We present new determinations of effective temperature, surface gravity, and masses for a sample of 46 hot DA white dwarfs selected from the EUVE and ROSAT Wide Field Camera bright source lists in...
Differences Between The Optical/Uv Spectra Of X-Ray Bright And X-Ray Faint QSOs (1998)
We contrast measurements of composite optical and ultraviolet (UV) spectra constructed from samples of QSOs defined by their soft X-ray brightness. X-ray bright (XB) composites show stronger emission...
Evidence Against BALS in the X-ray Bright QSO PG1416-129 (1997)
Green, Paul J., Aldcroft, Thomas L., Mathur, Smita, Schartel, Norbert
Recent results from the ROSAT All Sky Survey, and from deep ROSAT pointings reveal that broad absorption line quasars (BALQSOs) are weak in the soft X-ray bandpass (with optical-to-X-ray spectral...
Understanding the Elusive Dwarf Carbon Star (1996)
Most stars in our Galaxy with photospheric C/O>1 (carbon stars) are not giants but dwarfs. The newly-recognized class of dwarf carbon (dC) stars joins the growing family of stars with peculiar...
Schartel, Norbert, Green, Paul J., Anderson, Scott F., Hewett, Paul C., Foltz, Craig B., Margon, Bruce, ...
We develop and apply a novel method of analysis to study the X-ray spectral properties of 908 QSOs in the Large Bright Quasar Survey (LBQS) that were observed during the soft X-ray ROSAT All-Sky...
Quasar emission lines are sensitive to both the luminosity and shape of the quasars' high energy continuum - primarily in the soft X-ray and the (obscured) extreme ultraviolet. We initiate the first...
Broad Absorption Line QSOs Observed by the ROSAT PSPC (1995)
Recent results from the ROSAT All-Sky Survey (RASS) have shown that broad absorption line (BAL) QSOs are either highly absorbed or underluminous in the soft X-ray bandpass. Here, we extend this work...
Faint high latitude carbon stars / (1992)
Thesis (Ph. D.)--University of Washington, 1992.
NUCLEAR QUADRUPOLE RESONANCE ZEEMAN STUDY OF POLYCRYSTALLINE GROUP IVA CHLORIDES. (1967)
Green, Paul J., Graybeal, Jack D.
Author Institution: Department of Chemistry, West Virginia University