Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Sipple, Jackson"'
In fuzzy dark matter (FDM) cosmologies, the dark matter consists of ultralight bosons ($m\lesssim10^{-20}$ eV). The astrophysically large de Broglie wavelengths of such particles hinder the formation of low-mass dark matter halos. This implies a test
Externí odkaz:
http://arxiv.org/abs/2407.17059
Autor:
Kittiwisit, Piyanat, Murray, Steven G., Garsden, Hugh, Bull, Philip, Cain, Christopher, Parsons, Aaron R., Sipple, Jackson, Abdurashidova, Zara, Adams, Tyrone, Aguirre, James E., Alexander, Paul, Ali, Zaki S., Baartman, Rushelle, Balfour, Yanga, Beardsley, Adam P., Berkhout, Lindsay M., Bernardi, Gianni, Billings, Tashalee S., Bowman, Judd D., Bradley, Richard F., Burba, Jacob, Carey, Steven, Carilli, Chris L., Chen, Kai-Feng, Cheng, Carina, Choudhuri, Samir, DeBoer, David R., Acedo, Eloy de Lera, Dexter, Matt, Dillon, Joshua S., Dynes, Scott, Eksteen, Nico, Ely, John, Ewall-Wice, Aaron, Fagnoni, Nicolas, Fritz, Randall, Furlanetto, Steven R., Gale-Sides, Kingsley, Gehlot, Bharat Kumar, Ghosh, Abhik, Glendenning, Brian, Gorce, Adelie, Gorthi, Deepthi, Greig, Bradley, Grobbelaar, Jasper, Halday, Ziyaad, Hazelton, Bryna J., Hewitt, Jacqueline N., Hickish, Jack, Huang, Tian, Jacobs, Daniel C., Josaitis, Alec, Julius, Austin, Kariseb, MacCalvin, Kern, Nicholas S., Kerrigan, Joshua, Kim, Honggeun, Kohn, Saul A., Kolopanis, Matthew, Lanman, Adam, La Plante, Paul, Liu, Adrian, Loots, Anita, Ma, Yin-Zhe, MacMahon, David H. E., Malan, Lourence, Malgas, Cresshim, Malgas, Keith, Marero, Bradley, Martinot, Zachary E., Mesinger, Andrei, Molewa, Mathakane, Morales, Miguel F., Mosiane, Tshegofalang, Neben, Abraham R., Nikolic, Bojan, Nunhokee, Chuneeta Devi, Nuwegeld, Hans, Pascua, Robert, Patra, Nipanjana, Pieterse, Samantha, Qin, Yuxiang, Rath, Eleanor, Razavi-Ghods, Nima, Riley, Daniel, Robnett, James, Rosie, Kathryn, Santos, Mario G., Sims, Peter, Singh, Saurabh, Storer, Dara, Swarts, Hilton, Tan, Jianrong, Thyagarajan, Nithyanandan, van Wyngaarden, Pieter, Williams, Peter K. G., Xu, Zhilei, Zheng, Haoxuan
Detection of the faint 21 cm line emission from the Cosmic Dawn and Epoch of Reionisation will require not only exquisite control over instrumental calibration and systematics to achieve the necessary dynamic range of observations but also validation
Externí odkaz:
http://arxiv.org/abs/2312.09763
Autor:
Murphy, Geoff G., Bull, Philip, Santos, Mario G., Abdurashidova, Zara, Adams, Tyrone, Aguirre, James E., Alexander, Paul, Ali, Zaki S., Baartman, Rushelle, Balfour, Yanga, Beardsley, Adam P., Bernardi, Gianni, Billings, Tashalee, Bowman, Judd D., Bradley, Richard F., Burba, Jacob, Cain, Christopher, Carey, Steven, Carilli, Chris L., Cheng, Carina, DeBoer, David R., Acedo, Eloy de Lera, Dexter, Matt, Dillon, Joshua S., Eksteen, Nico, Ely, John, Ewall-Wice, Aaron, Fagnoni, Nicolas, Fritz, Randall, Furlanetto, Steven R., Gale-Sides, Kingsley, Glendenning, Brian, Gorthi, Deepthi, Greig, Bradley, Grobbelaar, Jasper, Halday, Ziyaad, Hazelton, Bryna J., Hewitt, Jacqueline N., Hickish, Jack, Jacobs, Daniel C., Julius, Austin, Kariseb, MacCalvin, Kern, Nicholas S., Kerrigan, Joshua, Kittiwisit, Piyanat, Kohn, Saul A., Kolopanis, Matthew, Lanman, Adam, La Plante, Paul, Liu, Adrian, Loots, Anita, MacMahon, David Harold Edward, Malan, Lourence, Malgas, Cresshim, Malgas, Keith, Marero, Bradley, Martinot, Zachary E., Mesinger, Andrei, Molewa, Mathakane, Morales, Miguel F., Mosiane, Tshegofalang, Murray, Steven G., Neben, Abraham R., Nikolic, Bojan, Nuwegeld, Hans, Parsons, Aaron R., Patra, Nipanjana, Pieterse, Samantha, Razavi-Ghods, Nima, Robnett, James, Rosie, Kathryn, Sims, Peter, Sipple, Jackson, Smith, Craig, Swarts, Hilton, Thyagarajan, Nithyanandan, van Wyngaarden, Pieter, Williams, Peter K. G., Zheng, Haoxuan
Observations with radio arrays that target the 21-cm signal originating from the early Universe suffer from a variety of systematic effects. An important class of these are reflections and spurious couplings between antennas. We apply a Hamiltonian M
Externí odkaz:
http://arxiv.org/abs/2312.03697
Autor:
Sipple, Jackson, Lidz, Adam
A recent ultraviolet luminosity function (UVLF) analysis in the Hubble Frontier Fields, behind foreground lensing clusters, has helped solidify estimates of the faint-end of the $z \sim 5-9$ UVLF at up to five magnitudes fainter than in the field. Th
Externí odkaz:
http://arxiv.org/abs/2306.12087
Autor:
Zheng, WeiKang, Stahl, Benjamin E., de Jaeger, Thomas, Filippenko, Alexei V., Wang, Shan-Qin, Gan, Wen-Pei, Brink, Thomas G., Altunin, Ivan, Baer-Way, Raphael, Bigley, Andrew, Blanchard, Kyle, Blanchard, Peter K., Bradley, James, Cargill, Samantha K., Casper, Chadwick, Chapman, Teagan, Chander, Vidhi, Channa, Sanyum, Choi, Byung Yun, Choksi, Nick, Chu, Matthew, Clubb, Kelsey I., Cohen, Daniel P., Dalba, Paul A., deGraw, Asia, de Kouchkovsky, Maxime, Ellison, Michael, Falcon, Edward, Fox, Ori D., Fuller, Kiera, Ganeshalingam, Mohan, Girish, Nachiket, Gould, Carolina, Halevi, Goni, Halle, Andrew, Hayakawa, Kevin T., Hardy, Romain, Hestenes, Julia, Hoffman, Andrew M., Hyland, Michael, Jeffers, Benjamin T., Jennings, Connor, Kandrashoff, Michael T., Khodanian, Anthony, Kim, Minkyu, Kim, Haejung, Kislak, Michelle E., Krishnan, Daniel, Kumar, Sahana, Kumar, Snehaa Ganesh, Leja, Joel, Leonard, Erin J., Li, Gary Z., Li, Weidong, Lian, Ji-Shun, Liu, Evelyn, Lowe, Thomas B., Lu, Philip, Ma, Emily, Mason, Michelle N., May, Michael, McAllister, Kyle, McGinness, Emma, Modak, Shaunak, Molloy, Jeffrey, Murakami, Yukei S., Nayak, Omnarayani, Perera, Derek, Pina, Kenia, Punjabi, Druv, Rikhter, Andrew, Ross, Timothy W., Sipple, Jackson, Soler, Costas, Stegman, Samantha, Stephens, Haynes, Sunseri, James, Tang, Kevin, Taylor, Stephen, Thrasher, Patrick, Van Dyk, Schuyler D., Wang, Xiang-Gao, Wayland, Jeremy, Wilkins, Andrew, Yagubyan, Abel, Yuk, Heechan, Yunus, Sameen, Zhang, Keto D.
We present BVRI and unfiltered Clear light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search (LOSS) follow-up program. Our SESN sample consists of 19 spectroscopically normal
Externí odkaz:
http://arxiv.org/abs/2203.05596
Publikováno v:
ApJ 928 162, 2022
We explore a new approach for extracting reionization-era contributions to the kinetic Sunyaev-Zel'dovich (kSZ) effect. Our method utilizes the cross-power spectrum between filtered and squared maps of the cosmic microwave background (CMB) and photom
Externí odkaz:
http://arxiv.org/abs/2111.13717
Akademický článek
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Akademický článek
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Publikováno v:
Astrophysical Journal; 3/24/2022, Vol. 928 Issue 2, p1-14, 14p
