Zobrazeno 1 - 10
of 3 172
pro vyhledávání: '"Thompson, T A"'
Autor:
Thompson, T. Ben, Sklar, Michael
Many publicly available language models have been safety tuned to reduce the likelihood of toxic or liability-inducing text. To redteam or jailbreak these models for compliance with toxic requests, users and security analysts have developed adversari
Externí odkaz:
http://arxiv.org/abs/2407.17447
Feature visualization, also known as "dreaming", offers insights into vision models by optimizing the inputs to maximize a neuron's activation or other internal component. However, dreaming has not been successfully applied to language models because
Externí odkaz:
http://arxiv.org/abs/2402.01702
Autor:
Desai, D. D., Kochanek, C. S., Shappee, B. J., Jayasinghe, T., Stanek, K. Z., Holoien, T. W. -S., Thompson, T. A., Ashall, C., Beacom, J. F., Do, A., Dong, S., Prieto, J. L.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 530, Issue 4, Pages 5016-5029, June 2024
We present the volumetric rates and luminosity functions (LFs) of Type Ia supernovae (SNe Ia) from the $V$-band All-Sky Automated Survey for Supernovae (ASAS-SN) catalogues spanning discovery dates from UTC 2014-01-26 to UTC 2017-12-29. Our standard
Externí odkaz:
http://arxiv.org/abs/2306.11100
Autor:
Hart, K., Shappee, B. J., Hey, D., Kochanek, C. S., Stanek, K. Z., Lim, L., Dobbs, S., Tucker, M., Jayasinghe, T., Beacom, J. F., Boright, T., Holoien, T., Ong, J. M. Joel, Prieto, J. L., Thompson, T. A., Will, D.
The All-Sky Automated Survey for Supernovae (ASAS-SN) began observing in late-2011 and has been imaging the entire sky with nightly cadence since late 2017. A core goal of ASAS-SN is to release as much useful data as possible to the community. Workin
Externí odkaz:
http://arxiv.org/abs/2304.03791
Simulation can evaluate a statistical method for properties such as Type I Error, FDR, or bias on a grid of hypothesized parameter values. But what about the gaps between the grid-points? Continuous Simulation Extension (CSE) is a proof-by-simulation
Externí odkaz:
http://arxiv.org/abs/2212.10042
Autor:
Neumann, K. D., Holoien, T. W. -S., Kochanek, C. S., Stanek, K. Z., Vallely, P. J., Shappee, B. J., Prieto, J. L., Pessi, T., Jayasinghe, T., Brimacombe, J., Bersier, D., Aydi, E., Basinger, C., Beacom, J. F., Bose, S., Brown, J. S., Chen, P., Clocchiatti, A., Desai, D. D., Dong, Subo, Falco, E., Holmbo, S., Morrell, N., Shields, J. V., Sokolovsky, K. V., Strader, J., Stritzinger, M. D., Swihart, S., Thompson, T. A., Way, Z., Aslan, L., Bishop, D. W., Bock, G., Bradshaw, J., Cacella, P., Castro-Morales, N., Conseil, E., Cornect, R., Cruz, I., Farfan, R. G., Fernandez, J. M., Gabuya, A., Gonzalez-Carballo, J. -L., Kendurkar, M. R., Kiyota, S., Koff, R. A., Krannich, G., Marples, P., Masi, G., Monard, L. A. G., Muñoz, J. A., Nicholls, B., Post, R. S., Pujic, Z., Stone, G., Tomasella, L., Trappett, D. L., Wiethoff, W. S.
Publikováno v:
MNRAS, 520, 4356 (2023)
We catalog the 443 bright supernovae discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN) in $2018-2020$ along with the 519 supernovae recovered by ASAS-SN and 516 additional $m_{peak}\leq18$ mag supernovae missed by ASAS-SN. Our stati
Externí odkaz:
http://arxiv.org/abs/2210.06492
Autor:
Kawash, A., Chomiuk, L., Strader, J., Sokolovsky, K. V., Aydi, E., Kochanek, C. S., Stanek, K. Z., Kostrzewa-Rutkowska, Z., Hodgkin, S. T., Mukai, K., Shappee, B., Jayasinghe, T., Smith, M. Rizzo, Holoien, T. W. -S., Prieto, J. L., Thompson, T. A.
We present the first estimate of the Galactic nova rate based on optical transient surveys covering the entire sky. Using data from the All-Sky Automated Survey for Supernovae (ASAS-SN) and \textit{Gaia} -- the only two all-sky surveys to report clas
Externí odkaz:
http://arxiv.org/abs/2206.14132
Autor:
Christy, C. T., Jayasinghe, T., Stanek, K. Z., Kochanek, C. S., Thompson, T. A., Shappee, B. J., Holoien, T. W. -S., Prieto, J. L., Dong, Subo, Giles, W.
The All-Sky Automated Survey for Supernovae (ASAS-SN) is the first optical survey to monitor the entire sky, currently with a cadence of $\lesssim 24$ hours down to $g \lesssim 18.5$ mag. ASAS-SN has routinely operated since 2013, collecting $\sim$ 2
Externí odkaz:
http://arxiv.org/abs/2205.02239
Autor:
Christy, C. T., Jayasinghe, T., Stanek, K. Z., Kochanek, C. S., Way, Z., Prieto, J. L., Shappee, B. J., Holoien, T. W. -S., Thompson, T. A., Schneider, A.
We present the first results from Citizen ASAS-SN, a citizen science project for the All-Sky Automated Survey for Supernovae (ASAS-SN) hosted on the Zooniverse platform. Citizen ASAS-SN utilizes the newer, deeper, higher cadence ASAS-SN $g$-band data
Externí odkaz:
http://arxiv.org/abs/2111.02415
Autor:
Kawash, A., Chomiuk, L., Rodriguez, J. A., Strader, J., Sokolovsky, K. V., Aydi, E., Kochanek, C. S., Stanek, K. Z., Mukai, K., De, K., Shappee, B., Holoien, T. W. -S., Prieto, J. L., Thompson, T. A.
There is a longstanding discrepancy between the observed Galactic classical nova rate of $\sim 10$ yr$^{-1}$ and the predicted rate from Galactic models of $\sim 30$--50 yr$^{-1}$. One explanation for this discrepancy is that many novae are hidden by
Externí odkaz:
http://arxiv.org/abs/2105.13893