Zobrazeno 1 - 10
of 17
pro vyhledávání: '"E C, Moran"'
Autor:
R J Smethurst, B D Simmons, C J Lintott, J Shanahan, A L Coil, W C Keel, E Glikman, E C Moran, K L Masters, M Urry, K Willett
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:3419-3420
Autor:
Sophia R Flury, E. C. Moran
The Sloan Digital Sky Survey (SDSS) has proved to be a powerful resource for understanding the physical properties and chemical composition of star-forming galaxies in the local universe. The SDSS population of active galactic nuclei (AGN) remains as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::01bcd9beafaf6f63e7f26316248ba8dd
http://arxiv.org/abs/2006.01113
http://arxiv.org/abs/2006.01113
Publikováno v:
The Astrophysical Journal. 647:140-160
Using archival Chandra observations of 19 LINERs we explore the X-ray properties of their inner kiloparsec to determine the origin of their nuclear X-ray emission, to investigate the presence of an AGN, and to identify the power source of the optical
Publikováno v:
The Astrophysical Journal. 515:L61-L64
Optical spectropolarimetry of the nucleus of the LINER NGC 1052, obtained at the Keck Observatory, reveals a rise in polarization in the wings of the H-alpha line profile. The polarization vector of H-alpha is offset by 67 degrees from the parsec-sca
Autor:
C. Megan Urry, Sugata Kaviraj, Karen L. Masters, Kyle W. Willett, E. C. Moran, Steven P. Bamford, Anna Han, Chris Lintott, Robert C. Nichol, Brooke Simmons, Kevin Schawinski
The growth of supermassive black holes appears to be driven by galaxy mergers, violent merger-free processes and/or `secular' processes. In order to quantify the effects of secular evolution on black hole growth, we study a sample of active galactic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa7a099a393718392c8495d2b365226c
Autor:
E C, Moran, J E, Harvey
Publikováno v:
Applied optics. 27(8)
In Wolter type I grazing incidence telescopes, ghost images result whenever unreflected xrays or singly reflected x rays pass through the telescope and impinge on the focal plane. These ghost images degrade imagequality and can bo eliminated by appro
Autor:
George D. Becker, Ryan J. Foley, A. L. Malec, Thea N. Steele, W. H. de Vries, Alexei V. Filippenko, George H Marion, Ray W. Russell, Weidong Li, Charles E. Woodward, Maryam Modjaz, Peter M. Garnavich, R. J. Rudy, Ryan Chornock, Arthur M. Wolfe, A. Stockton, David K. Lynch, Jeffrey M. Silverman, Marc Rafelski, Michael T. Murphy, E. C. Moran, Regina A. Jorgenson
Supernova (SN) 2008ax in NGC 4490 was discovered within hours after shock breakout, presenting the rare opportunity to study a core-collapse SN beginning with the initial envelope-cooling phase immediately following shock breakout. We present an exte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6e3bba7d565cec5513bf2929f59a65a
http://arxiv.org/abs/1001.2775
http://arxiv.org/abs/1001.2775
We have compared the X-ray--to--optical flux ratios (F_x/F_opt) of absorbed active galactic nuclei (AGNs) in the Chandra Deep Field North (CDF-N) with those of nearby, optically classified Seyfert 2 galaxies. The comparison provides an opportunity to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16b8bc7b6343f11d79893aa914558bf5
Autor:
Stephanie M. LaMassa, E. C. Moran, Michael Eracleous, Luigi C. Gallo, Adam D. Myers, C. Megan Urry, Gordon T. Richards, Sabrina Cales, Timothy M. Heckman
Publikováno v:
The Astrophysical Journal. 800:144
SDSS J015957.64+003310.5 is an X-ray selected, z = 0.31 active galactic nucleus (AGN) from the Stripe 82X survey that transitioned from a Type 1 quasar to a Type 1.9 AGN between 2000 and 2010. This is the most distant AGN, and first quasar, yet obser
Autor:
Alexei V. Filippenko, Mohan Ganeshalingam, Brandon J. Swift, Ari Laor, E. C. Moran, Louis-Benoit Desroches, Kirpal Nandra, Weidong Li, Misty C. Bentz, P. M. O'Neill, Dan Maoz, Shai Kaspi, Bradley M. Peterson, Luis C. Ho
We present optical observations of the low-luminosity Seyfert 1 nucleus of NGC 4395, as part of a multiwavelength reverberation-mapping program. Observations were carried out over two nights in 2004 April at Lick, Wise, and Kitt Peak Observatories. W
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ffe5424d4c449b03744928701f86cf9
http://arxiv.org/abs/astro-ph/0606494
http://arxiv.org/abs/astro-ph/0606494