Zobrazeno 1 - 10
of 3 817
pro vyhledávání: '"Jordán, D."'
Autor:
Sinclair, Adrian K., Burgoyne, James, Huber, Anthony I., Murphy, Colin, Choi, Steve K., Duell, Cody J., Huber, Zachary B., Li, Yaqiong, Chapman, Scott C., Niemack, Michael D., Nikola, Thomas, Vavagiakis, Eve M., Walker, Samantha, Wheeler, Jordan D., Austermann, Jason, Lin, Lawrence, Xie, Ruixuan, Zou, Bugao, Mauskopf, Philip D.
The Fred Young Submillimeter Telescope (FYST), on Cerro Chajnantor in the Atacama desert of Chile, will conduct wide-field and small deep-field surveys of the sky with more than 100,000 detectors on the Prime-Cam instrument. Kinetic inductance detect
Externí odkaz:
http://arxiv.org/abs/2406.14892
Autor:
Macgregor, Peter. J., Norris, Ray P., O'Brien, Andrew, Akhlaghi, Mohammad, Anderson, Craig, Collier, Jordan D., Crawford, Evan J., Duchesne, Stefan W., Filipović, Miroslav D., Koribalski, Bärbel S., Pacaud, Florian, Reiprich, Thomas H., Riseley, Christopher J., Rudnick, Lawrence, Vernstrom, Tessa, Hopkins, Andrew. M., Johnston-Hollitt, Melanie, Marvil, Josh, Whiting, Matthew, Tingay, Steven
We present radio observations of the galaxy cluster Abell S1136 at 888 MHz, using the Australian Square Kilometre Array Pathfinder radio telescope, as part of the Evolutionary Map of the Universe Early Science program. We compare these findings with
Externí odkaz:
http://arxiv.org/abs/2406.09709
Autor:
Cook, Robin H. W., Davies, Luke J. M., Rhee, Jonghwan, Hale, Catherine L., Bellstedt, Sabine, Thorne, Jessica E., Delvecchio, Ivan, Collier, Jordan D., Dodson, Richard, Driver, Simon P., Holwerda, Benne W., Jarvis, Matt J., Knowles, Kenda, Lagos, Claudia, Maddox, Natasha, Meyer, Martin, Robotham, Aaron S. G., Roychowdhury, Sambit, Rozgonyi, Kristof, Seymour, Nicholas, Siudek, Malgorzata, Whiting, Matthew, Whittam, Imogen
The tight relationship between infrared luminosity (L$_\mathrm{TIR}$) and 1.4 GHz radio continuum luminosity (L$_\mathrm{1.4GHz}$) has proven useful for understanding star formation free from dust obscuration. Infrared emission in star-forming galaxi
Externí odkaz:
http://arxiv.org/abs/2405.00337
Autor:
Sinigaglia, Francesco, Rodighiero, Giulia, Elson, Ed, Bianchetti, Alessandro, Vaccari, Mattia, Maddox, Natasha, Ponomareva, Anastasia A., Frank, Bradley S., Jarvis, Matt J., Catinella, Barbara, Cortese, Luca, Roychowdhury, Sambit, Baes, Maarten, Collier, Jordan D., Ilbert, Olivier, Khostovan, Ali A., Kurapati, Sushma, Pan, Hengxing, Prandoni, Isabella, Rajohnson, Sambatriniaina H. A., Salvato, Mara, Sekhar, Srikrishna, Sharma, Gauri
We present the first measurement of HI mass of star-forming galaxies in different large scale structure environments from a blind survey at $z\sim 0.37$. In particular, we carry out a spectral line stacking analysis considering $2875$ spectra of colo
Externí odkaz:
http://arxiv.org/abs/2403.00734
Autor:
The BLAST Observatory Collaboration, Coppi, Gabriele, Dicker, Simon, Aguirre, James E., Austermann, Jason E., Beall, James A., Clark, Susan E., Cox, Erin G., Devlin, Mark J., Fissel, Laura M., Galitzki, Nicholas, Hensley, Brandon S., Hubmayr, Johannes, Molinari, Sergio, Nati, Federico, Novak, Giles, Schisano, Eugenio, Soler, Juan D., Tucker, Carole E., Ullom, Joel N., Vaskuri, Anna, Vissers, Michael R., Wheeler, Jordan D., Zannoni, Mario
Publikováno v:
2024 PASP 136 035003
Sensitive wide-field observations of polarized thermal emission from interstellar dust grains will allow astronomers to address key outstanding questions about the life cycle of matter and energy driving the formation of stars and the evolution of ga
Externí odkaz:
http://arxiv.org/abs/2401.14370
Autor:
Payne, Daniel E., Chambers, Jordan D., Burkitt, Anthony, Cook, Mark J., Kuhlman, Levin, Freestone, Dean R., Grayden, David B.
Objective: Forecasting epileptic seizures can reduce uncertainty for patients and allow preventative actions. While many models can predict the occurrence of seizures from features of the EEG, few models incorporate changes in features over time. Lon
Externí odkaz:
http://arxiv.org/abs/2309.09471
Autor:
Woodland, Leonie, Macdougal, David, Cabrera, Ivelisse M., Thompson, Jordan D., Prabhakaran, D., Bewley, Robert I., Coldea, Radu
Publikováno v:
Phys. Rev. B 108, 184416 (2023)
The Ising chain realizes the fundamental paradigm of spin fractionalization, where locally flipping a spin creates two domain walls (spinons) that can separate apart at no energy cost. In a quasi-one-dimensional system, the mean-field effects of the
Externí odkaz:
http://arxiv.org/abs/2308.07699
Autor:
Ponomareva, Anastasia A., Jarvis, Matt J., Pan, Hengxing, Maddox, Natasha, Jones, Michael G., Frank, Bradley S., Rajohnson, Sambatriniaina H. A., Mulaudzi, Wanga, Meyer, Martin, Adams, Elizabeth A. K., Baes, Maarten, Hess, Kelley M., Kurapati, Sushma, Prandoni, Isabella, Sinigaglia, Francesco, Spekkens, Kristine, Tudorache, Madalina, Heywood, Ian, Collier, Jordan D., Sekhar, Srikrishna
We present the first measurement of the HI mass function (HIMF) using data from MeerKAT, based on 276 direct detections from the MIGHTEE Survey Early Science data covering a period of approximately a billion years ($0 \leq z \leq 0.084 $). This is th
Externí odkaz:
http://arxiv.org/abs/2304.13051
The one-sided and full Hilbert transforms are evaluated exactly by means of the method of finite-part integration [E.A. Galapon, \textit{Proc. Roy. Soc. A} \textbf{473}, 20160567 (2017)]. In general, the result consists of two terms -- the first is a
Externí odkaz:
http://arxiv.org/abs/2210.14462
Autor:
Pan, Hengxing, Jarvis, Matt J., Santos, Mario G., Maddox, Natasha, Frank, Bradley S., Ponomareva, Anastasia A., Prandoni, Isabella, Kurapati, Sushma, Baes, Maarten, Piña, Pavel E. Mancera, Rodighiero, Giulia, Meyer, Martin J., Davé, Romeel, Sharma, Gauri, Rajohnson, Sambatriniaina H. A., Adams, Nathan J., Bowler, Rebecca A. A., Sinigaglia, Francesco, van der Hulst, Thijs, Hatfield, Peter W., Sekhar, Srikrishna, Collier, Jordan D.
We study the $M_{\rm HI}-M_{\star}$ relation over the last billion years using the MIGHTEE-HI sample. We first model the upper envelope of the $M_{\rm HI}-M_{\star}$ relation with a Bayesian technique applied to a total number of 249 HI-selected gala
Externí odkaz:
http://arxiv.org/abs/2210.04651