GLAST large area telescope multiwavelength planning     

O. Reimer  P. F. Michelson  R. A. Cameron  S. W. Digel  D. J. Thompson  K. S. Wood 《Astrophysics and Space Science》2007,309(1-4):523-526

Gamma-ray astrophysics depends in many ways on multiwavelength studies. The Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT) Collaboration has started multiwavelength planning well before the scheduled 2007 launch of the observatory. Some of the high-priority multiwavelength needs include: (1) availability of contemporaneous radio and X-ray timing of pulsars; (2) expansion of blazar catalogs, including redshift measurements; (3) improved observations of molecular clouds, especially at high galactic latitudes; (4) simultaneous broad-band blazar monitoring; (5) characterization of gamma-ray transients, including gamma ray bursts; (6) radio, optical, X-ray and TeV counterpart searches for reliable and effective sources identification and characterization. Several of these activities are needed to be in place before launch.   相似文献   

The galaxy luminosity–size relation and selection biases in the Hubble Ultra Deep Field     

E. Cameron †  S. P. Driver 《Monthly notices of the Royal Astronomical Society》2007,377(2):523-534

We use the Hubble Ultra Deep Field to study the galaxy luminosity–size  ( M – R _e )  distribution. With a careful analysis of selection effects due to both detection completeness and measurement reliability, we identify bias-free regions in the   M – R _e   plane for a series of volume-limited samples. By comparison to a nearby survey also having well-defined selection limits, namely the Millennium Galaxy Catalogue, we present clear evidence for evolution in surface brightness since   z ∼ 0.7  . Specifically, we demonstrate that the mean, rest-frame B -band  〈μ〉 _e   for galaxies in a sample spanning 8 mag in luminosity between   M _B =−22  and −14 mag increases by ∼1.0 mag arcsec⁻² from   z ∼ 0.1  to 0.7. We also highlight the importance of considering surface brightness-dependent measurement biases in addition to incompleteness biases. In particular, the increasing, systematic underestimation of Kron fluxes towards low surface brightnesses may cause diffuse, yet luminous, systems to be mistaken for faint, compact objects.  相似文献   

WASP-1b and WASP-2b: two new transiting exoplanets detected with SuperWASP and SOPHIE   总被引：1，自引：0，他引：1  

A. Collier Cameron  F. Bouchy  G. Hébrard  P. Maxted  D. Pollacco  F. Pont  I. Skillen  B. Smalley  R. A. Street  R. G. West  D. M. Wilson  S. Aigrain  D. J. Christian  W. I. Clarkson  B. Enoch  A. Evans  A. Fitzsimmons  M. Fleenor  M. Gillon  C. A. Haswell  L. Hebb  C. Hellier  S. T. Hodgkin  K. Horne  J. Irwin  S. R. Kane  F. P. Keenan  B. Loeillet  T. A. Lister  M. Mayor  C. Moutou  A. J. Norton  J. Osborne  N. Parley  D. Queloz  R. Ryans  A. H. M. J. Triaud  S. Udry  P. J. Wheatley 《Monthly notices of the Royal Astronomical Society》2007,375(3):951-957

We have detected low-amplitude radial-velocity variations in two stars, USNO-B1.0 1219–0005465 (GSC  02265–00107 = WASP–1  ) and USNO-B1.0 0964–0543604 (GSC  00522–01199 = WASP–2  ). Both stars were identified as being likely host stars of transiting exoplanets in the 2004 SuperWASP wide-field transit survey. Using the newly commissioned radial-velocity spectrograph SOPHIE at the Observatoire de Haute-Provence, we found that both objects exhibit reflex orbital radial-velocity variations with amplitudes characteristic of planetary-mass companions and in-phase with the photometric orbits. Line-bisector studies rule out faint blended binaries as the cause of either the radial-velocity variations or the transits. We perform preliminary spectral analyses of the host stars, which together with their radial-velocity variations and fits to the transit light curves yield estimates of the planetary masses and radii. WASP-1b and WASP-2b have orbital periods of 2.52 and 2.15 d, respectively. Given mass estimates for their F7V and K1V primaries, we derive planet masses 0.80–0.98 and 0.81–0.95 times that of Jupiter, respectively. WASP-1b appears to have an inflated radius of at least 1.33 R _Jup, whereas WASP-2b has a radius in the range 0.65–1.26 R _Jup.  相似文献   

Cultural and economic residential sorting of Auckland’s population, 1991–2013: an entropy approach     

Mondal  Mohana  Cameron  Michael P.  Poot  Jacques 《Journal of Geographical Systems》2021,23(2):291-330

Journal of Geographical Systems - Auckland, the largest city of New Zealand, is one of the most diverse cities in the world, with more than 40% of its population born abroad, more than 200...  相似文献   

Benefits of greenhouse gas mitigation on the supply,management, and use of water resources in the United States     

K. Strzepek  J. Neumann  J. Smith  J. Martinich  B. Boehlert  M. Hejazi  J. Henderson  C. Wobus  R. Jones  K. Calvin  D. Johnson  E. Monier  J. Strzepek  J.-H. Yoon 《Climatic change》2015,132(1):127-141

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Cloud computing and virtualization within the regional climate model and evaluation system     

Chris A. Mattmann  Duane Waliser  Jinwon Kim  Cameron Goodale  Andrew Hart  Paul Ramirez  Dan Crichton  Paul Zimdars  Maziyar Boustani  Kyo Lee  Paul Loikith  Kim Whitehall  Chris Jack  Bruce Hewitson 《Earth Science Informatics》2014,7(1):1-12

The Regional Climate Model Evaluation System (RCMES) facilitates the rapid, flexible inclusion of NASA observations into climate model evaluations. RCMES provides two fundamental components. A database (RCMED) is a scalable point-oriented cloud database used to elastically store remote sensing observations and to make them available using a space time query interface. The analysis toolkit (RCMET) is a Python-based toolkit that can be delivered as a cloud virtual machine, or as an installer package deployed using Python Buildout to users in order to allow for temporal and spatial regridding, metrics calculation (RMSE, bias, PDFs, etc.) and end-user visualization. RCMET is available to users in an “offline”, lone scientist mode based on a virtual machine dynamically constructed with model outputs and observations to evaluate; or on an institution’s computational cluster seated close to the observations and model outputs. We have leveraged RCMES within the content of the Coordinated Regional Downscaling Experiment (CORDEX) project, working with the University of Cape Town and other institutions to compare the model output to NASA remote sensing data; in addition we are also working with the North American Regional Climate Change Assessment Program (NARCCAP). In this paper we explain the contribution of cloud computing to RCMES’s specifically describing studies of various cloud databases we evaluated for RCMED, and virtualization toolkits for RCMET, and their potential strengths in delivering user-created dynamic regional climate model evaluation virtual machines for our users.  相似文献   

Flow,frequency, and uncertainty estimation for an extreme historical flood event in the Highlands of Scotland,UK     

David Cameron 《水文研究》2007,21(11):1460-1470

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Bistable profile illumination in pulsars B0919+06 and B1859+07     

Joanna M. Rankin  Cameron Rodriguez  Geoffrey A. E. Wright 《Monthly notices of the Royal Astronomical Society》2006,370(2):673-680

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Review     

Hugh Cameron 《大气与海洋》2013,51(1):17-20

PHYSICS IN CANADA ‐ SURVEY AND OUTLOOK ‐ PREPARED BY A STUDY GROUP OF THE CANADIAN ASSOCIATION OF PHYSICISTS HEADED BY DR. D.C. ROSE, AND PUBLISHED IN MAY, 1967.  相似文献   

The Millennium Galaxy Catalogue: bulge–disc decomposition of 10 095 nearby galaxies     

Paul D. Allen  Simon P. Driver  Alister W. Graham  Ewan Cameron  Jochen Liske  Roberto De Propris 《Monthly notices of the Royal Astronomical Society》2006,371(1):2-18

We present near-infrared (NIR) adaptive optics-assisted spectroscopic observations of the  CO (Δμ= 2)  absorption bands towards the centre of the giant elliptical galaxy NGC 1399. The observations were made with NAOS-CONICA (on the European Southern Observatory's Very Large Telescope) and have a full width at half-maximum resolution of 0.15 arcsec (14 pc). Kinematic analysis of the observations reveals a decoupled core and strongly non-Gaussian line-of-sight velocity profiles in the central 0.2 arcsec (19 pc). NIR imaging also indicates an asymmetric elongation of the central isophotes in the same region.
We use spherical orbit-superposition models to interpret the kinematics, using a set of orthogonal 'eigen-velocity profiles' that allow us to fit models directly to spectra. The models require a central black hole of mass  1.2^+0.5_−0.6× 10⁹ M_⊙  , with a strongly tangentially biased orbit distribution in the inner 40 pc.  相似文献