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Article
Strong gravitational lensing by AGNs as a probe of the quasar–host relations in the distant Universe
The tight correlations found between the mass of supermassive black holes and the luminosities, stellar masses and velocity dispersions of their host galaxies are often interpreted as a sign of their co-evolut...
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Article
Author Correction: A fast radio burst source at a complex magnetized site in a barred galaxy
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Article
A fast radio burst source at a complex magnetized site in a barred galaxy
Fast radio bursts (FRBs) are highly dispersed, millisecond-duration radio bursts1–3. Recent observations of a Galactic FRB4–8 suggest that at least some FRBs originate from magnetars, but the origin of cosmologic...
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Article
A fast radio burst localized to a massive galaxy
Intense, millisecond-duration bursts of radio waves (named fast radio bursts) have been detected from beyond the Milky Way1. Their dispersion measures—which are greater than would be expected if they had propagat...
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Article
A possible close supermassive black-hole binary in a quasar with optical periodicity
A search of a data set of light curves for 247,000 known, spectroscopically confirmed quasars with a temporal baseline of about 9 years reveals a strong, smooth periodic signal in the optical variability of qu...
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Article
Data challenges of time domain astronomy
Astronomy has been at the forefront of the development of the techniques and methodologies of data intensive science for over a decade with large sky surveys and distributed efforts such as the Virtual Observa...
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Article
New cataclysmic variable 1RXS J073346.0+261933 in Gemini
In the course of our search for the optical identifications of ROSAT X-ray sources, we have found a highly variable object with a very unusual behavior on long time scales, rare color indices, and a high X-ray...
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Chapter and Conference Paper
Exploring the Use of Virtual Worlds as a Scientific Research Platform: The Meta-Institute for Computational Astrophysics (MICA)
We describe the Meta-Institute for Computational Astrophysics (MICA), the first professional scientific organization based exclusively in virtual worlds (VWs). The goals of MICA are to explore the utility of t...
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Article
The bright optical afterglow of the nearby γ-ray burst of 29 March 2003
Past studies of cosmological γ-ray bursts (GRBs) have been hampered by their extreme distances, resulting in faint afterglows. A nearby GRB could potentially shed much light on the origin of these events, but ...
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Article
Early optical emission from the γ-ray burst of 4 October 2002
Observations of the long-lived emission—or ‘afterglow’—of long-duration γ-ray bursts place them at cosmological distances, but the origin of these energetic explosions remains a mystery. Observations of optica...
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Chapter
The Roles of Small Telescopes in a Virtual Observatory Environment
The advent of the Virtual Observatory (VO) concept signals a paradigm shift in the way astronomy will be done in the era of information abundance and ubiquitous networking. Small telescopes will be playing a n...
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Chapter and Conference Paper
Challenges for Cluster Analysis in a Virtual Observatory
There has been an unprecedented and continuing growth in the volume, quality, and complexity of astronomical data sets over the past few years, mainly through large digital sky surveys. Virtual Observatory (VO...
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Article
The evolutionary history of early-type galaxies as derived from the fundamental plane
The fundamental plane (FP) scaling relations and their evolution are a powerful tool for studying the global properties of early-type galaxies and their evolutionary history. The form of the FP, as derived by ...
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Chapter and Conference Paper
The GRB Host Galaxies and Redshifts
Based in part on the observations obtained at the W.M. Keck Observatory, operated by the California Association for Research in Astronomy, a scientific partnership among Caltech, the Univ. of California and NASA; and with the NASA/ESA Hubble Space Telescope, operated by the AURA, Inc., under a contract with NASA.
Observations of GRB host galaxies and their environments in general can provide valuable clues about the nature of progenitors. Bursts are associated with faint,
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Chapter and Conference Paper
Exploration of Large Digital Sky Surveys
We review some of the scientific opportunities and technical challenges posed by the exploration of the large digital sky surveys, in the context of a Virtual Observatory (VO). The VO paradigm will profoundly ...
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Article
The unusual afterglow of the γ-ray burst of 26 March 1998 as evidence for a supernova connection
Cosmic γ-ray bursts have now been firmly established as one of the most powerful phenomena in the Universe, releasing almost the rest-mass energy of a neutron star within the space of a few seconds (ref. 1). The...
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Article
The afterglow, redshift and extreme energetics of the γ-ray burst of 23 January 1999
Long-lived emission, known as afterglow, has now been detected from about a dozen γ-ray bursts. Distance determinations place the bursts at cosmological distances, with redshifts, z, ranging from ∼1 to 3. The ene...
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Article
Identification of a host galaxy at redshift z = 3.42 for the γ-ray burst of 14 December 1997
Knowledge of the properties of γ-ray bursts has increased substantially following recent detections of counterparts at X-ray, optical and radio wavelengths. But the nature of the underlying physical mechanism ...
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Article
The energetic afterglow of the γ-ray burst of 14 December 1997
The discovery of fading but relatively long-lived X-ray emission1 accompanying γ-ray bursts has revolutionized the study of these objects. This ‘afterglow’ is most easily explained by models2,3,4 similar to those...
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Chapter and Conference Paper
Cataloging of the Digitized POSS-II: Initial Scientific Results
The Second Palomar Sky Survey (POSS-II) is now nearing completion. It will cover the entire northern sky with 894 fields (6.5° square) at 5° spacings, with no gaps in the coverage. Plates are taken in three ba...