Zobrazeno 1 - 10
of 934
pro vyhledávání: '"D C Murphy"'
Autor:
Dan Kocevski, Michelle Huig, Sean Griffin, Brad Cenko, C. A. Wilson-Hodge, Carolyn Kierans, Alexey Uliyanov, Sarah Walsh, J. McEnery, Lorraine Hanlon, D. C. Murphy, Jeremy S. Perkins, Peter Shawhan, Amy Liend, J. L. Racusin, Antonino Cucchiara, J.R. Smith, Dieter H. Hartmann, Alessandro Bruno, Georgia A. de Nolfo, Eric Burns, Alyson Joens, David Morris, Michael S. Briggs, Sheila McBreen, John Krizmanic, Teresa Tatoli, Lee J. Mitchell, Regina Caputo
Publikováno v:
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019).
The first simultaneous detection of a short gamma-ray burst (SGRB) with a gravitational-wave (GW) signal ushered in a new era of multi-messenger astronomy. In order to increase the number of SGRB-GW simultaneous detections, we need full sky coverage
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aea431a7d7667eacb2b9425776fe4ea8
https://doi.org/10.22323/1.358.0604
https://doi.org/10.22323/1.358.0604
Autor:
Albert Harding, Randy Hammond, Jennifer L. Marshall, A. Uomoto, E. Koch, D. C. Murphy, Joe D. Orndorff, D. D. Kelson, Stephen A. Smee, Christoph Birk, Andy Monson, Gregg Scharfstein, S. E. Persson, Patrick J. McCarthy, Robert H. Barkhouser, Stephen A. Shectman
Publikováno v:
Publications of the Astronomical Society of the Pacific. 125:654-682
The FourStar Infrared Camera is a 4 K × 4 K near-infrared (1.0-2.4 μm) imager built for the Magellan 6.5 m Baade Telescope at Las Campanas Observatory, Chile. FourStar has an all-refractive optical system, four HAWAII-2RG detectors, and Teledyne el
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::30a5b998150a8e91e992db63dfa3e0bb
https://doi.org/10.1086/671164
https://doi.org/10.1086/671164
Publikováno v:
The Astronomical Journal. 128:2239-2264
Near-infrared J, H, and Ks photometric measurements of 92 Cepheids in the Large Magellanic Cloud are presented. The stars are spread over the face of the Cloud, their periods range from 3 to 100 days, and their light curves are sampled at an average
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7f8e8867bce885fb80922fdb83ae2459
https://doi.org/10.1086/424934
https://doi.org/10.1086/424934
Autor:
Rachel S. Somerville, A. Oemler, Patrick J. McCarthy, S. E. Persson, John Wilson, C. N. Sabbey, Richard S. Ellis, Craig D. Mackay, O. Lahav, Heidi Chen, R. O. Marzke, Andrew E. Firth, M. G. Beckett, Raymond G. Carlberg, James R. Lewis, R. G. McMahon, Roberto G. Abraham, D. C. Murphy
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 332:617-646
The LCIR Survey, using the Cambridge IR Survey Instrument (CIRSI), reaches H \~ 20-21 over ~1 deg^2. We present results for 744 arcmin^2 in which public UBVRI data exist. We compare optical-IR colours with predictions of a semi-analytic hierarchical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::262915e2f4318d805ea45814146b76be
https://doi.org/10.1046/j.1365-8711.2002.05297.x
https://doi.org/10.1046/j.1365-8711.2002.05297.x
Autor:
Patrick J. McCarthy, Richard G. McMahon, Martin G. Beckett, Ofer Lahav, C. N. Sabbey, Richard S. Ellis, Augustus Oemler, Ronald O. Marzke, James R. Lewis, Roberto Abraham, Raymond G. Carlberg, Andrew E. Firth, Rachel S. Somerville, John Wilson, S. E. Persson, Hsiao-Wen Chen, Craig D. Mackay, D. C. Murphy, Paul Martini
Publikováno v:
The Astrophysical Journal. 570:54-74
(Abridged) The Las Campanas Infrared Survey, based on broad-band optical and near-infrared photometry, is designed to robustly identify a statistically significant and representative sample of evolved galaxies at redshifts z>1. We have completed an H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1152fabc919c528e85710560a598e525
https://doi.org/10.1086/339426
https://doi.org/10.1086/339426
The Las Campanas Infrared Survey: Early-Type Galaxy Progenitors beyond [CLC][ITAL]z[/ITAL][/CLC] = 1
Autor:
C. N. Sabbey, Patrick J. McCarthy, Roberto Abraham, Craig D. Mackay, D. C. Murphy, Richard S. Ellis, Andrew E. Firth, M. G. Beckett, O. Lahav, Paul Martini, R. G. McMahon, Ronald O. Marzke, James R. Lewis, Rachel S. Somerville, John Wilson, Augustus Oemler, S. E. Persson, Hsiao-Wen Chen, Raymond G. Carlberg
Publikováno v:
The Astrophysical Journal. 560:L131-L134
(Abridged) We have identified a population of faint red galaxies from a 0.62 square degree region of the Las Campanas Infrared Survey whose properties are consistent with their being the progenitors of early-type galaxies. The optical and IR colors,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::53a795bf4f2f08d0848402be535fb73d
https://doi.org/10.1086/323971
https://doi.org/10.1086/323971
Publikováno v:
The Astronomical Journal. 116:2475-2488
A new grid of 65 faint near-infrared standard stars is presented. They are spread around the sky, lie between 10th and 12th magnitude at K, and are measured in most cases to precisions better than 0.001 mag in the J, H, K, and Ks bands; the latter is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e938d0602ed7e2a066d8f8cc6e33e0d2
https://doi.org/10.1086/300607
https://doi.org/10.1086/300607
Autor:
D. C. Murphy, M. Hossein Safizadeh
Publikováno v:
International Journal of Production Research. 30:2921-2939
This study examines the relationship between the introduction of new products and R&D process and product expenditures of 15 industries. The objective is to determine the degree to which product and process R&D expenditures, uniquely or jointly, cont
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce2ec0274386286c390f4382a2b2b3e6
https://doi.org/10.1080/00207549208948199
https://doi.org/10.1080/00207549208948199
Autor:
Maximilian Stritzinger, Gastón Folatelli, Mark Sullivan, Christophe Balland, Peter M. Garnavich, P. Wyatt, E. Sergio Gonzalez, John Marriner, D. Hardin, Daniel D. Kelson, Julien Guy, Mario Hamuy, Nicholas B. Suntzeff, A. Conley, Mark M. Phillips, Hubert Lampeitl, Luis Boldt, D. Andrew Howell, Christopher R. Burns, Carlos Contreras, Pierre Astier, Nidia Morrell, Masao Sako, Reynald Pain, Barry F. Madore, Wendy L. Freedman, Bruce A. Bassett, Raymond G. Carlberg, Eric Hsiao, Adam G. Riess, D. C. Murphy, Laura Sturch, Joshua A. Frieman, Michael Wood-Vasey, Donald P. Schneider, Richard Kessler, Miguel Roth, S. E. Persson, Nicolas Regnault, Kathy Perrett
Publikováno v:
Astrophysical Journal
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2009, 704, pp.1036-1058. ⟨10.1088/0004-637X/704/2/1036⟩
The Astrophysical Journal, 2009, 704, pp.1036-1058. ⟨10.1088/0004-637X/704/2/1036⟩
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2009, 704, pp.1036-1058. ⟨10.1088/0004-637X/704/2/1036⟩
The Astrophysical Journal, 2009, 704, pp.1036-1058. ⟨10.1088/0004-637X/704/2/1036⟩
The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supernovae (SNe Ia) as a function of redshift, and to set observational constraints on the dark energy contribution to the total energy content of the Uni
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f91f1c61a777fc394e14b744df0c708
