19.6k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of Hawaiʻi at MānoaUS4k papers
- California Institute of TechnologyUS1.2k papers
- Centre National de la Recherche ScientifiqueFR1.2k papers
- University of Science and Technology of ChinaCN1.1k papers
- Budker Institute of Nuclear PhysicsRU1.1k papers
- Institute of High Energy PhysicsCN1.1k papers
- Peking UniversityCN1k papers
- The University of TokyoJP955 papers
- Seoul National UniversityKR845 papers
- University of TurinIT772 papers
- Justus-Liebig-Universität GießenDE771 papers
- Chinese Academy of SciencesCN754 papers
86 papers · 2 filters
Optical and Near-Infrared Spectroscopy of a High-Redshift, Hard X-ray Emitting Spiral Galaxy
Steve Dawson, Nate McCrady, Daniel Stern +4
We present optical and near-infrared Keck spectroscopy of CXOHDFN J123635.6+621424 (hereafter HDFX28), a hard X-ray source at a redshift of z = 2.011 in the flanking fields of the…
Absorption Line Survey of H3+ toward the Galactic Center Sources I. GCS 3-2 and GC IRS3
M. Goto, B. J. McCall, T. R. Geballe +4
We present high-resolution (R = 20000) spectroscopy of H3+ absorption toward the luminous Galactic center sources GCS 3-2 and GC IRS 3. With the efficient wavelength coverage affor…
Zero-metallicity stars II. Evolution of very massive objects with mass loss
P. Marigo, C. Chiosi, R. -P. Kudritzki
We present evolutionary models of zero-metallicity very massive objects, with initial masses in the range 120 Msun -- 1000 Msun, covering their quiescent evolution up to central ca…
Cosmological constraints from evolution of cluster baryon mass function at z~0.5
A. Vikhlinin, A. Voevodkin, C. R. Mullis +8
We present a new method for deriving cosmological constraints based on the evolution of the baryon mass function of galaxy clusters, and implement it using 17 distant clusters from…
Deep Near-Infrared Observations and Identifications of Chandra Sources in the Orion Molecular Cloud 2 and 3
M. Tsujimoto, K. Koyama, N. Kobayashi +3
We conducted deep NIR imaging observations of the Orion molecular cloud 2 and 3 using QUIRC on the 88-inch telescope of the University of Hawaii. Our purposes are 1) to generate a…
SDSSp J104433.04012502.2 at is Gravitationally Magnified by an Intervening Galaxy
Yasuhiro Shioya, Yoshiaki Taniguchi, Takashi Murayama +15
During the course of our optical deep survey program on L emitters at in the sky area surrounding the quasar SDSSp J104433.04012502.2 at , we found th…
Astrophysics of Young Star Binaries
L. Prato, T. P. Greene, M. Simon
This paper describes our study of the astrophysics of individual components in close pre-main-sequence binaries. We observed both stars in 17 systems, located in 4 nearby star form…
A Method of Correcting Near-Infrared Spectra for Telluric Absorption
William D. Vacca, Michael C. Cushing, John T. Rayner
We present a method for correcting near-infrared medium-resolution spectra for telluric absorption. The method makes use of a spectrum of an A0V star, observed near in time and clo…
VLT and HST Observations of the Host Galaxy of GRB990705
E. Le Floc'h, P. -A. Duc, I. F. Mirabel +6
We present VLT spectroscopic observations of Gamma-Ray Burst (GRB) 990705 host galaxy and highlight the benefits provided by the prompt-phase features of GRBs to derive the redshif…
Correlations of Richness and Global Properties in Galaxy Clusters
H. K. C. Yee, E. Ellingson
We measure the optical richness of galaxy clusters from the CNOC1 cluster redshift survey using the galaxy-cluster center correlation amplitude B_gc. We show that the B_gc values m…
The Properties of Microjansky Radio Sources in the HDF-N, SSA13, and SSA22 Fields
S. C. Chapman, A. J. Barger, L. L. Cowie +9
(abridged) We present multiwavelength observations for a large sample of microjansky radio sources detected in ultradeep 1.4GHz maps centered on the Hubble Deep Field-North (HDF-N)…
Cosmological Perturbation Theory Using the Schrödinger Equation
Istvan Szapudi, Nick Kaiser
We introduce the theory of non-linear cosmological perturbations using the correspondence limit of the Schrödinger equation. The resulting formalism is equivalent to using the coll…
Jovian dust streams: Probes of the Io plasma torus
Harald Krueger, Mihaly Horanyi, Eberhard Gruen
Jupiter was discovered to be a source of high speed dust particles by the Ulysses spacecraft in 1992. These dust particles originate from the volcanic plumes on Io. They collect el…
A Survey for Circumstellar Disks Around Young Substellar Objects
Michael C. Liu, Joan Najita, Alan T. Tokunaga
(Abridged) We have completed the first systematic survey for disks around spectroscopically identified young brown dwarfs and very low mass stars. We have obtained L'-band (3.8 um)…
A Submillimeter and Radio Survey of Gamma-Ray Burst Host Galaxies: A Glimpse into the Future of Star Formation Studies
E. Berger, L. L. Cowie, S. R. Kulkarni +3
We present the first comprehensive search for submillimeter and radio emission from the host galaxies of twenty well-localized gamma-ray bursts (GRBs). With the exception of a sing…
Evolution of Elliptical Galaxies at z >~ 1 Revealed from a Large, Multicolor Sample of Extremely Red Objects
M. Miyazaki, K. Shimasaku, T. Kodama +23
We study the evolution of elliptical galaxies at z >~ 1 on the basis of a sample of 247 Extremely Red Objects (EROs) with R-Ks >= 3.35 (AB) and Ks <= 22.1 (AB) constructed from BVR…
Observations of [S IV] 10.5 micron and [Ne II] 12.8 micron in Two Halo Planetary Nebulae: Implications for Chemical Self-Enrichment
Harriet L. Dinerstein, Matthew J. Richter, John H. Lacy +1
We have detected the [S IV] 10.5 micron and [Ne II] 12.8 micron fine-structure lines in the halo population planetary nebula (PN) DdDm 1, and set upper limits on their intensities…
Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations
Joseph B. Jensen, John L. Tonry, Brian J. Barris +5
To empirically calibrate the IR surface brightness fluctuation (SBF) distance scale and probe the properties of unresolved stellar populations, we measured fluctuations in 65 galax…
Carbon Abundances of Faint Stars in M13 - Evidence for Two Abundance Altering Mechanisms
Michael M. Briley, Judith G. Cohen, Peter B. Stetson
We present an analysis of CH band strengths in Keck LRIS spectra of a sample of 81 stars in M13 within 2 magnitudes of the main-sequence turnoff. The subgiants clearly exhibit a su…
Mid-Infrared Identification of Faint Submillimeter Sources
Y. Sato, L. L. Cowie, K. Kawara +4
Faint submillimeter sources detected with the Submillimeter Common-User Bolometer Array on the James Clerk Maxwell Telescope have faced an identification problem due to the telesco…
The Hawaii-AAO K-band Galaxy Redshift Survey -- Paper I: The Local K-band Luminosity Function
J. -S. Huang, K. Glazebrook, L. L. Cowie +1
We present the K-band local luminosity function derived froma sample of 1056 bright (K<15) K-selected galaxies from the Hawaii-AAO K-band redshift survey. The Hawaii-AAO K-band red…
Science Objectives and Early Results of the DEEP2 Redshift Survey
Marc Davis, Sandra M. Faber, Jeffrey A. Newman +18
The DEIMOS spectrograph has now been installed on the Keck-II telescope and commissioning is nearly complete. The DEEP2 Redshift Survey, which will take approximately 120 nights at…
Data analysis methods for XMM-Newton observations of extended sources. Application to bright massive clusters of galaxies at z=0.2
Philippe B. Marty, Jean-Paul Kneib, Rachida Sadat +2
In this paper, a review is given of methods useful for XMM-Newton EPIC data analysis of extended sources, along with some applications to a bright massive cluster of galaxies at z=…
FeH Absorption in the Near-Infrared Spectra of Late M and L Dwarfs
M. C. Cushing, J. T. Rayner, S. P. Davis +1
We present medium-resolution z-, J-, and H-band spectra of four late-type dwarfs with spectral types ranging from M8 to L7.5. In an attempt to determine the origin of numerous weak…