Zobrazeno 1 - 10
of 76
pro vyhledávání: '"Eilat Glikman"'
Autor:
Stephanie LaMassa, Alessandro Peca, C. Megan Urry, Eilat Glikman, Tonima Tasnim Ananna, Connor Auge, Francesca Civano, Aritra Ghosh, Allison Kirkpatrick, Michael J. Koss, Meredith Powell, Mara Salvato, Benny Trakhtenbrot
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 2, p 235 (2024)
We present the third catalog release of the wide-area (31.3 deg ^2 ) Stripe 82 X-ray survey. This catalog combines previously published X-ray source properties with multiwavelength counterparts and photometric redshifts, presents 343 new spectroscopi
Externí odkaz:
https://doaj.org/article/03f6b15bba1e449f8da5ed92e49b2a41
Autor:
Eilat Glikman, Rachel Langgin, Makoto A. Johnstone, Ilsang Yoon, Julia M. Comerford, Brooke D. Simmons, Hannah Stacey, Mark Lacy, John M. O’Meara
Publikováno v:
The Astrophysical Journal Letters, Vol 951, Iss 1, p L18 (2023)
We report the discovery of a candidate dual QSO at z = 1.889, a redshift that is in the era known as “cosmic noon” where most of the universe’s black hole and stellar mass growth occurred. The source was identified in Hubble Space Telescope WFC
Externí odkaz:
https://doaj.org/article/a0df07cdcdc949908ef43f1a116db20a
Autor:
Eilat Glikman, Cristian E. Rusu, Geoff C.-F. Chen, James Hung-Hsu Chan, Cristiana Spingola, Hannah Stacey, John McKean, Ciprian T. Berghea, S. G. Djorgovski, Matthew J. Graham, Daniel Stern, Tanya Urrutia, Mark Lacy, Nathan J. Secrest, John M. O’Meara
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 1, p 25 (2023)
We present the discovery of a gravitationally lensed dust-reddened QSO at z = 2.517, identified in a survey for QSOs by infrared selection. Hubble Space Telescope imaging reveals a quadruply lensed system in a cusp configuration, with a maximum image
Externí odkaz:
https://doaj.org/article/b9be94aa262c4a639e4bdeb0185ef880
The canonical picture of galaxy evolution invokes the injection of energy from supermassive black holes to reduce star formation efficiency in massive galaxies. This process can explain their observed scaling relations, which were already established
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b192a4922442c2e3299c64fd595e2c74
https://doi.org/10.21203/rs.3.rs-1355197/v1
https://doi.org/10.21203/rs.3.rs-1355197/v1
Autor:
Brandon Coleman, Allison Kirkpatrick, Kevin C Cooke, Eilat Glikman, Stephanie La Massa, Stefano Marchesi, Alessandro Peca, Ezequiel Treister, Connor Auge, C Megan Urry, Dave Sanders, Tracey Jane Turner, Tonima Tasnim Ananna
We aim to determine the intrinsic far-Infrared (far-IR) emission of X-ray-luminous quasars over cosmic time. Using a 16 deg^2 region of the Stripe 82 field surveyed by XMM-Newton and Herschel Space Observatory, we identify 2905 X-ray luminous (LX > 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd66d424c83abb311320ae023cec0568
Autor:
Gene C. K. Leung, Karen L. Masters, William C. Keel, Chris Lintott, Brooke Simmons, Jesse Carla Shanahan, Rebecca Smethurst, Eilat Glikman, Izzy Garland, Alison L. Coil
Recent observations and simulations have challenged the long-held paradigm that mergers are the dominant mechanism driving the growth of both galaxies and supermassive black holes (SMBH), in favour of non-merger (secular) processes. In this pilot stu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c03ee3da312f93a70c4796e3e7aed4e2
http://arxiv.org/abs/2108.05361
http://arxiv.org/abs/2108.05361
Autor:
Ashish Mahabal, Nicholas P. Ross, Barry McKernan, Eilat Glikman, K. E. Saavik Ford, Daniel Stern, S. G. Djorgovski, Andrew J. Drake, Eric Christensen, S. M. Larson, Matthew J. Graham
Publikováno v:
Graham, M J, Ross, N P, Stern, D, Drake, A J, McKernan, B, Ford, K E S, Djorgovski, S G, Mahabal, A, Glikman, E, Larson, S & Christensen, E 2020, ' Understanding extreme quasar optical variability with CRTS : II. Changing-state quasars ', Monthly Notices of the Royal Astronomical Society, vol. 491, no. 4, pp. 4925-4948 . https://doi.org/10.1093/mnras/stz3244
We present the results of a systematic search for quasars in the Catalina Real-time Transient Survey exhibiting both strong photometric and spectroscopic variability over a decadal baseline. We identify 73 sources with specific patterns of optical an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0276039ed2a465f5e44aff288d0f5144
http://arxiv.org/abs/1905.02262
http://arxiv.org/abs/1905.02262
Autor:
Michael Estrada, Brandon Coleman, Stephanie M. LaMassa, Kurt Hamblin, Jordan Johnson, Allison Kirkpatrick, Stefano Marchesi, Tonima Tasnim Ananna, Eilat Glikman, Jeyhan S. Kartaltepe, Ezequiel Treister, D. B. Sanders, Tracey Jane Turner, Meredith Powell, Jason Brewster, C. Megan Urry, Casey Carlile, Kevin C. Cooke
Quasars are the most luminous of active galactic nuclei (AGN), and are perhaps responsible for quenching star formation in their hosts. The Stripe 82X catalog covers 31.3 deg$^2$ of the Stripe 82 field, of which the 15.6 deg$^2$ covered with XMM-Newt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a99f1056f74f1808fb1bca362e84874e
Autor:
Jonathan R. Trump, Hugo Messias, Kevin C. Cooke, Allison Kirkpatrick, Alessandro Peca, Eilat Glikman, Stephanie M. LaMassa, T. K. Daisy Leung, Tracey Jane Turner, Michael Estrada, C. Megan Urry, Jason Brewster, Nico Cappelluti, Tonima Tasnim Ananna
Publikováno v:
The Astrophysical Journal. 903:106
Cold quasars are a rare subpopulation observed to host unobscured, X-ray luminous active galactic nuclei (AGN) while also retaining a cold gas supply fueling high star formation rates. These objects are interpreted as AGN early in their evolution. We
Autor:
S. S. Murray, Carol B. Hundal, H. Daniels-Koch, Mark Lacy, S. G. Djorgovski, Tanya Urrutia, Larson Lovdal, Stephanie M. LaMassa, Elinor L. Gates, Daniel Stern, Eilat Glikman, M. Crnogorcevic, Matthew J. Graham, Meg Urry
We present a spectroscopically complete sample of 147 infrared-color-selected AGN down to a 22 $��$m flux limit of 20 mJy over the $\sim$270 deg$^2$ of the SDSS Stripe 82 region. Most of these sources are in the QSO luminosity regime ($L_{\rm bol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b496361969a25fbd402ac1a9e5e10151