Zobrazeno 1 - 10
of 4 994
pro vyhledávání: '"Wagg, A."'
Autor:
Xu, Fuxiang, Wang, Ran, Li, Jianan, Neri, Roberto, Pensabene, Antonio, Decarli, Roberto, Shao, Yali, Bañados, Eduardo, Cox, Pierre, Bertoldi, Frank, Feruglio, Chiara, Walter, Fabian, Venemans, Bram P., Omont, Alain, Riechers, Dominik, Wagg, Jeff, Menten, Karl M., Fan, Xiaohui
We present NOrthern Extended Millimeter Array observations of CO(8-7), (9-8), and (10-9) lines, as well as the underlying continuum for two far-infrared luminous quasars: SDSS J2054-0005 at $\rm z=6.0389$ and SDSS J0129-0035 at $\rm z=5.7788$. Both q
Externí odkaz:
http://arxiv.org/abs/2411.01701
Autor:
Wainer, Tobin M., Davenport, James R. A., Mendoza, Guadalupe Tovar, Feinstein, Adina D., Wagg, Tom
We examine 4 years of Kepler 30-min data, and 5 Sectors of TESS 2-min data for the dM3 star KIC-8507979/TIC-272272592. This rapidly rotating (P=1.2 day) star has previously been identified as flare active, with a possible long-term decline in its fla
Externí odkaz:
http://arxiv.org/abs/2409.06631
We present cogsworth, an open-source Python tool for producing self-consistent population synthesis and galactic dynamics simulations. With cogsworth one can (1) sample a population of binaries and star formation history, (2) perform rapid (binary) s
Externí odkaz:
http://arxiv.org/abs/2409.04543
Autor:
Wagg, Tom, Juric, Mario, Yoachim, Peter, Kurlander, Jake, Cornwall, Sam, Moeyens, Joachim, Eggl, Siegfried, Jones, R. Lynne, Birtwhistle, Peter
We simulate and analyse the contribution of the Rubin Observatory Legacy Survey of Space and Time (LSST) to the rate of discovery of Near Earth Object (NEO) candidates, their submission rates to the NEO Confirmation page (NEOCP), and the resulting de
Externí odkaz:
http://arxiv.org/abs/2408.12517
Autor:
Zhou, Dazhi, Greve, Thomas R., Gullberg, Bitten, Lee, Minju M., Di Mascolo, Luca, Dicker, Simon R., Romero, Charles E., Chapman, Scott C., Chen, Chian-Chou, Cornish, Thomas, Devlin, Mark J., Ho, Luis C., Kohno, Kotaro, Lagos, Claudia D. P., Mason, Brian S., Mroczkowski, Tony, Wagg, Jeff F. W., Wang, Q. Daniel, Wang, Ran, Brinch, Malte., Dannerbauer, Helmut, Jiang, Xue-Jian, Lauritsen, Lynge R. B., Vijayan, Aswin P., Vizgan, David, Wardlow, Julie L., Sarazin, Craig L., Sarmiento, Karen P., Serjeant, Stephen, Bhandarkar, Tanay A., Haridas, Saianeesh K., Moravec, Emily, Orlowski-Scherer, John, Sievers, Jonathan L. R., Tanaka, Ichi, Wang, Yu-Jan, Zeballos, Milagros, Laza-Ramos, Andres, Liu, Yuanqi, Hassan, Mohd Shaiful Rizal, Jwel, Abdul Kadir Md, Nazri, Affan Adly, Lim, Ming-Kang, Ibrahim, Ungku Ferwani Salwa Ungku
High-redshift radio(-loud) galaxies (H$z$RGs) are massive galaxies with powerful radio-loud active galactic nuclei (AGNs) and serve as beacons for protocluster identification. However, the interplay between H$z$RGs and the large-scale environment rem
Externí odkaz:
http://arxiv.org/abs/2408.02177
Autor:
Cornish, Thomas M., Wardlow, Julie L., Greve, Thomas R., Chapman, Scott, Chen, Chian-Chou, Dannerbauer, Helmut, Goto, Tomotsugu, Gullberg, Bitten, Ho, Luis C., Jiang, Xue-Jian, Lagos, Claudia, Lee, Minju, Serjeant, Stephen, Shim, Hyunjin, Smith, Daniel J. B., Vijayan, Aswin, Wagg, Jeff, Zhou, Dazhi
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Vol. 533, Issue 1 (2024) pp. 1032-1044
Measuring the environments of massive galaxies at high redshift is crucial to understanding galaxy evolution and the conditions that gave rise to the distribution of matter we see in the Universe today. While high-$z$ radio galaxies (H$z$RGs) and qua
Externí odkaz:
http://arxiv.org/abs/2407.21099
Autor:
Wilson, James, Champneys, Max D., Tipuric, Matt, Mills, Robin, Wagg, David J., Rogers, Timothy J.
The use of measured vibration data from structures has a long history of enabling the development of methods for inference and monitoring. In particular, applications based on system identification and structural health monitoring have risen to promi
Externí odkaz:
http://arxiv.org/abs/2406.04943
Autor:
Wagg, Tom, Broekgaarden, Floor S.
Software is crucial for the advancement of astronomy especially in the context of rapidly growing datasets that increasingly require algorithm and pipeline development to process the data and produce results. However, software has not always been con
Externí odkaz:
http://arxiv.org/abs/2406.04405
Autor:
Stegmann, Jakob, Vigna-Gómez, Alejandro, Rantala, Antti, Wagg, Tom, Zwick, Lorenz, Renzo, Mathieu, van Son, Lieke A. C., de Mink, Selma E., White, Simon D. M.
Publikováno v:
Jakob Stegmann et al 2024 ApJL 972 L19
A substantial fraction of stars can be found in wide binaries with projected separations between $\sim10^2$ and $10^5\,\rm AU$. In the standard lore of binary physics, these would evolve as effectively single stars that remotely orbit one another on
Externí odkaz:
http://arxiv.org/abs/2405.02912
Local and distant measurements of the Hubble constant are in significant tension: local measurements of the Hubble constant appear to show a Universe that is significantly contracted when compared to distant measurements. From the point of view of an
Externí odkaz:
http://arxiv.org/abs/2403.19957