Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Kip Kuntz"'
Autor:
Mayura Balakrishnan, Paul A. Draghis, Jon M. Miller, Joe Bright, Robert Fender, Mason Ng, Edward Cackett, Andrew Fabian, Kip Kuntz, James C. A. Miller-Jones, Daniel Proga, Paul S. Ray, John Raymond, Mark Reynolds, Abderahmen Zoghbi
Publikováno v:
The Astrophysical Journal, Vol 947, Iss 1, p 38 (2023)
A number of neutron stars have been observed within the remnants of the core-collapse supernova explosions that created them. In contrast, black holes are not yet clearly associated with supernova remnants (SNRs). Indeed, some observations suggest th
Externí odkaz:
https://doaj.org/article/a45583cd7918437fa6a5203d06529ca5
Autor:
Catriana K. Paw U., Brian Walsh, Kip Kuntz, Rousseau Nutter, Cadin M. Connor, Samantha Busk, Vadim Burwitz, Gisela Hartner, Thomas Müller, Surangkhana Rukdee, Thomas Schmidt, Emil Atz, Norman Dobson, Dennis Chornay, Frederick S. Porter, Kenneth M. Simms, Van Naldoza, Steven Sembay, David G. Sibeck, Nick Thomas
Publikováno v:
Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4e547c93116ce68bd04c875a03a6ac42
https://doi.org/10.1117/12.2629503
https://doi.org/10.1117/12.2629503
Autor:
Emil Atz, Brian Walsh, Connor O’Brien, Michael Collier, Ariel Berman, Lisa Billingsley, J. Bernard Blake, Jeffery Broll, Dennis Chornay, William Crain, Thompson Cragwell, Norman Dobson, Joseph Kujawski, Kip Kuntz, Van Naldoza, Rousseau Nutter, F. Scott Porter, David Sibeck, Kenneth Simms, Nicholas Thomas, Drew Turner, Allan Weatherwax, Ajmal Yousuff, Aleks Zosuls
Publikováno v:
The Review of scientific instruments. 93(6)
The Cusp Plasma Imaging Detector (CuPID) CubeSat observatory is a 6U CubeSat designed to observe solar wind charge exchange in magnetospheric cusps to test competing theories of magnetic reconnection at the Earth’s magnetopause. The CuPID is equipp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bcc5d5526b3c45d86eb974687b9f3a7e
https://pubmed.ncbi.nlm.nih.gov/35778053
https://pubmed.ncbi.nlm.nih.gov/35778053
Publikováno v:
NATURE. 363(6425)
THE monochromatic luminosities of high-redshift (z > 3) radio galaxies rise steeply between wavelengths of about 2,000 and 5,000 A, to form a characteristic 'red bump'1–6. It is usually assumed that this bump arises from the photospheric emission o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a18ae1ef5ae270e7ba241358966aafb3
http://ora.ox.ac.uk/objects/uuid:7c70afd1-eb9e-4b77-9488-0973432b5669
http://ora.ox.ac.uk/objects/uuid:7c70afd1-eb9e-4b77-9488-0973432b5669