Zobrazeno 1 - 10
of 2 830
pro vyhledávání: '"So, An Kristen C."'
Autor:
Dage, Kristen C., Tremou, Evangelia, Otahola, Bolivia Cuevas, Koch, Eric W., Oh, Kwangmin, Plotkin, Richard M., Tang, Vivian L., Aldhalemi, Muhammad Ridha, Bustani, Zainab, Fawaz, Mariam Ismail, Harff, Hans J., Khalyleh, Amna, McBride, Timothy, Mason, Jesse, Preston, Anthony, Rinehart, Cortney, Vinson, Ethan, Anderson, Gemma, Cackett, Edward M., Fu, Shih Ching, Kamann, Sebastian, Panurach, Teresa, Pechetti, Renuka, Saikia, Payaswini, Sett, Susmita, Urquhart, Ryan, Usher, Christopher
Intermediate mass black holes (10^2 < M_BH< 10^5 Msun) are an open question in our understanding of black hole evolution and growth. They have long been linked to dense star cluster environments thanks to cluster dynamics, but there are a limited num
Externí odkaz:
http://arxiv.org/abs/2412.07284
Autor:
Wang, Ziteng, Rea, Nanda, Bao, Tong, Kaplan, David L., Lenc, Emil, Wadiasingh, Zorawar, Hare, Jeremy, Zic, Andrew, Anumarlapudi, Akash, Bera, Apurba, Beniamini, Paz, Cooper, A. J., Clarke, Tracy E., Deller, Adam T., Dawson, J. R., Glowacki, Marcin, Hurley-Walker, Natasha, McSweeney, S. J., Polisensky, Emil J., Peters, Wendy M., Younes, George, Bannister, Keith W., Caleb, Manisha, Dage, Kristen C., James, Clancy W., Kasliwal, Mansi M., Karambelkar, Viraj, Lower, Marcus E., Mori, Kaya, Ocker, Stella Koch, Pérez-Torres, Miguel, Qiu, Hao, Rose, Kovi, Shannon, Ryan M., Taub, Rhianna, Wang, Fayin, Wang, Yuanming, Zhao, Zhenyin, Bhat, N. D. R., Dobie, Dougal, Driessen, Laura N., Murphy, Tara, Jaini, Akhil, Deng, Xinping, Jahns-Schindler, Joscha N., Lee, Y. W. J., Pritchard, Joshua, Tuthill, John, Thyagarajan, Nithyanandan
Recently, a class of long-period radio transients (LPTs) has been discovered, exhibiting emission on timescales thousands of times longer than radio pulsars. Several models had been proposed implicating either a strong magnetic field neutron star, is
Externí odkaz:
http://arxiv.org/abs/2411.16606
Autor:
Panurach, Teresa, Dage, Kristen C., Urquhart, Ryan, Plotkin, Richard M., Paul, Jeremiah D., Bahramian, Arash, Brumback, McKinley C., Galvin, Timothy J., Molina, Isabella, Miller-Jones, James C. A., Saikia, Payaswini
Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve as potential candidates for (sub-Eddington) intermediate mass black h
Externí odkaz:
http://arxiv.org/abs/2410.23335
Autor:
Karam, Rawan, Dage, Kristen C., Tetarenko, Bailey E., Brumback, McKinley C., Haggard, Daryl, Bahramian, Arash, Hu, Chin-Ping, Neilsen, Joey, Altamirano, Diego, Athukoralalage, Wasundara, Charles, Philip A., Clarkson, William I., Hickox, Ryan C., Kennea, Jamie
The MOOSE (Monitoring Observations of SMC X-1 Excursions) program uses the Neutron Star Interior Composition Explorer Mission (NICER) to monitor the high mass X-ray binary SMC X-1 during its superorbital period excursions. Here we perform X-ray spect
Externí odkaz:
http://arxiv.org/abs/2410.17307
Ultraluminous X-ray binaries have challenged our assumptions of extreme accretion rates in X-ray binaries, and impact other subfields of astronomy, such as cosmology, gravitational wave sources and supernov{\ae}. Our understanding of ULXs has changed
Externí odkaz:
http://arxiv.org/abs/2407.01768
Autor:
Dage, Kristen C., Bahramian, Arash, Naoz, Smadar, Bobrick, Alexey, Athukoralalage, Wasundara, Brumback, McKinley C., Haggard, Daryl, Kundu, Arunav, Zepf, Stephen E.
Publikováno v:
2024MNRAS.tmp..625D
The globular cluster ultraluminous X-ray source, RZ2109, is a complex and unique system which has been detected at X-ray, ultra-violet, and optical wavelengths. Based on almost 20 years of Chandra and XMM-Newton observations, the X-ray luminosity exh
Externí odkaz:
http://arxiv.org/abs/2403.09525
Autor:
Pelisoli, Ingrid, Chomiuk, Laura, Strader, Jay, Marsh, T. R., Aydi, Elias, Dage, Kristen C., Kyer, Rebecca, Molina, Isabella, Panurach, Teresa, Urquhart, Ryan, Maccarone, Thomas J., Rich, R. Michael, Rodriguez, Antonio C., Breedt, E., Brown, A. J., Dhillon, V. S., Dyer, M. J., Gaensicke, Boris. T., Garbutt, J. A., Green, M. J., Kennedy, M. R., Kerry, P., Littlefair, S. P., Munday, James, Parsons, S. G.
Radio emission has been detected from tens of white dwarfs, in particular in accreting systems. Additionally, radio emission has been predicted as a possible outcome of a planetary system around a white dwarf. We searched for 3 GHz radio continuum em
Externí odkaz:
http://arxiv.org/abs/2402.11015
Autor:
Time-Domain, The AXIS, Group, Multi-Messenger Science Working, Arcodia, Riccardo, Bauer, Franz E., Cenko, S. Bradley, Dage, Kristen C., Haggard, Daryl, Ho, Wynn C. G., Kara, Erin, Koss, Michael, Liu, Tingting, Mallick, Labani, Negro, Michela, Pradhan, Pragati, Quirola-Vasquez, J., Reynolds, Mark T., Ricci, Claudio, Rothschild, Richard E., Sridhar, Navin, Troja, Eleonora, Yao, Yuhan
The Advanced X-ray Imaging Satellite (AXIS) promises revolutionary science in the X-ray and multi-messenger time domain. AXIS will leverage excellent spatial resolution (<1.5 arcsec), sensitivity (80x that of Swift), and a large collecting area (5-10
Externí odkaz:
http://arxiv.org/abs/2311.07658
Autor:
Matthew G. DeSaix, Christen M. Bossu, Julie C. Hagelin, Ryan J. Harrigan, James F. Saracco, Marius Somveille, Caz M. Taylor, Kristen C. Ruegg
Publikováno v:
Methods in Ecology and Evolution, Vol 15, Iss 12, Pp 2216-2225 (2024)
Abstract A prominent challenge for managing migratory species is the development of conservation plans that accommodate spatiotemporally varying distributions throughout the year. Migratory networks are spatially‐explicit models that incorporate mi
Externí odkaz:
https://doaj.org/article/b5714d6b086a440c950b707392cc0375
Autor:
Dage, Kristen C., Bahramian, Arash, James, Clancy W., Kundu, Arunav, Rhode, Katherine L., Strader, Jay, Vesperini, Enrico, Zepf, Stephen E.
We use multiband archival HST observations to measure the photometric and structural parameters of the M81 globular cluster that hosts the Fast Radio Burst FRB 20200120E. Our best-fitting King model has an effective radius $r_h = 3.06$ pc with a mode
Externí odkaz:
http://arxiv.org/abs/2310.10328