Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Lou Strolger"'
Autor:
Brenda L. Frye, Massimo Pascale, Justin Pierel, Wenlei Chen, Nicholas Foo, Reagen Leimbach, Nikhil Garuda, Seth H. Cohen, Patrick S. Kamieneski, Rogier A. Windhorst, Anton M. Koekemoer, Pat Kelly, Jake Summers, Michael Engesser, Daizhong Liu, Lukas J. Furtak, Maria del Carmen Polletta, Kevin C. Harrington, S. P. Willner, Jose M. Diego, Rolf A. Jansen, Dan Coe, Christopher J. Conselice, Liang Dai, Hervé Dole, Jordan C. J. D’Silva, Simon P. Driver, Norman A. Grogin, Madeline A. Marshall, Ashish K. Meena, Mario Nonino, Rafael Ortiz III, Nor Pirzkal, Aaron Robotham, Russell E. Ryan Jr., Lou Strolger, Scott Tompkins, Christopher N. A. Willmer, Haojing Yan, Min S. Yun, Adi Zitrin
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 2, p 171 (2024)
A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three d
Externí odkaz:
https://doaj.org/article/6cc49a5947ac4a70931e819d2c75b613
Autor:
Danial Langeroodi, Jens Hjorth, Wenlei Chen, Patrick L. Kelly, Hayley Williams, Yu-Heng Lin, Claudia Scarlata, Adi Zitrin, Tom Broadhurst, Jose M. Diego, Xiaosheng Huang, Alexei V. Filippenko, Ryan J. Foley, Saurabh Jha, Anton M. Koekemoer, Masamune Oguri, Ismael Perez-Fournon, Justin Pierel, Frederick Poidevin, Lou Strolger
Publikováno v:
The Astrophysical Journal, Vol 957, Iss 1, p 39 (2023)
A tight positive correlation between the stellar mass and the gas-phase metallicity of galaxies has been observed at low redshifts. The redshift evolution of this correlation can strongly constrain theories of galaxy evolution. The advent of JWST all
Externí odkaz:
https://doaj.org/article/3cb13063226a48b495670a59566bfd80
Autor:
Lou Strolger
Most resource allocation for observatory time (or money) is done through peer review processes that can be time consuming and prone to bias. STScI has pioneered a dual-anonymous reviewing process, and implemented new tools to attempt toreduce bias. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e68dbc05af5ef358f107b92a3cd55a0
Autor:
Hayley Williams, Patrick L. Kelly, Wenlei Chen, Gabriel Brammer, Adi Zitrin, Tommaso Treu, Claudia Scarlata, Anton M. Koekemoer, Masamune Oguri, Yu-Heng Lin, Jose M. Diego, Mario Nonino, Jens Hjorth, Danial Langeroodi, Tom Broadhurst, Noah Rogers, Ismael Perez-Fournon, Ryan J. Foley, Saurabh Jha, Alexei V. Filippenko, Lou Strolger, Justin Pierel, Frederick Poidevin, Lilan Yang
Ultraviolet light from early galaxies is thought to have ionized gas in the intergalactic medium. However, there are few observational constraints on this epoch because of the faintness of those galaxies and the redshift of their optical light into t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf96c3eeb2a8bd9016639bc92006a7bc
http://arxiv.org/abs/2210.15699
http://arxiv.org/abs/2210.15699
Autor:
Ori D. Fox, Schuyler D. Van Dyk, Benjamin F. Williams, Maria Drout, Emmanouil Zapartas, Nathan Smith, Dan Milisavljevic, Jennifer E. Andrews, K. Azalee Bostroem, Alexei V. Filippenko, Sebastian Gomez, Patrick L. Kelly, S. E. de Mink, Justin Pierel, Armin Rest, Stuart Ryder, Niharika Sravan, Lou Strolger, Qinan Wang, Kathryn E. Weil
This Letter presents the detection of a source at the position of the Type Ib/c supernova (SN) 2013ge more than four years after the radioactive component is expected to have faded. This source could mark the first post-SN direct detection of a survi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c2276fd75f7f41321248c503502690c
https://resolver.caltech.edu/CaltechAUTHORS:20220414-26670000
https://resolver.caltech.edu/CaltechAUTHORS:20220414-26670000
Autor:
Schuyler D. Van Dyk, David Rubin, O. D. Fox, Chadwick Casper, Lou Strolger, Tamás Szalai, Gary Z. Li, Lee Armus, Michael F. Skrutskie, Alexei V. Filippenko, H.G. Khandrika
Supernova (SN) rates serve as an important probe of star-formation models and initial mass functions. Near-infrared seeing-limited ground-based surveys typically discover a factor of 3-10 fewer SNe than predicted from far-infrared (FIR) luminosities
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92a959a7982d59bc21c92cea7a58ca4d
http://arxiv.org/abs/2106.09733
http://arxiv.org/abs/2106.09733
Autor:
Alice Jacques, R. C. Steele, John F. Kielkopf, Benne W. Holwerda, Shawn Knabel, W. Roemer, Lou Strolger
The Transiting Exoplanet Survey Satellite (TESS) is the latest observational effort to find exoplanets and map bright transient optical phenomena. Supernovae (SN) are particularly interesting as cosmological standard candles for cosmological distance
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1de734372b04b01420cd0bfbf83c5a7