Hintze Centre for Astrophysical Surveys

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A Faint Progenitor System for the Faint Supernova 2024vjm

Authors:

Erez Zimmerman, Avishay Gal-Yam, Paul Groot, Eran Ofek, Jan van Roestel, Andrea Pastorello, Stefano Valenti, Aravind Ravi, Ping Chen, Steve Schulze, Nadejda Blagorodnova, Maxime Wavasseur, Marco Gómez-Muñoz, Hugo Tranin, Simon de Wet, Giorgos Leloudas, Paul Vreeswijk, Lindsey Kwok, Michaela Schwab, Saurabh Jha, Kate Maguire, David Sand, Eric Stringer, Thomas Kupfer, Tamar Faran, Joseph Anderson, Jennifer Andrews, Moira Andrews, Avshalom Badash, Steven Bloemen, K Bostroem, Ting-Wan Chen, Massimo Della Valle, Georgios Dimitriadis, Yize Dong, Joseph Farah, James Gillanders, Benjamin Godson, Mariusz Gromadzki, Daichi Hiramatsu, Emily Hoang, Dale Howell, Daryl Janzen, Hanindyo Kuncarayakti, Jiaxuan Li, Joe Lyman, Keiichi Maeda, Mark Magee, Darshana Mehta, Andrew Milligan, Shane Moran, Yuan Qi Ni, David O’Neill, Jeniveve Pearson, Daniëlle Pieterse, Giuliano Pignata, Andrea Reguitti, Daniel Reichart, Nicolas Meza Retamal, Rita Santos, Simone Scaringi, Manisha Shrestha, Shubham Srivastav, Fiorenzo Stoppa, Bhagya Subrayan, Giorgio Valerin, Xiaofeng Wang, Kathryn Wynn, Ofer Yaron, Weicheng Zang
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A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst

Authors:

Yu-Han Yang, Eleonora Troja, Brendan O'Connor, Chris Fryer, Myungshin Im, Joe Durbak, Gregory Paek, Roberto Ricci, Clécio De Bom, James Gillanders, Alberto Castro-Tirado, Zong-Kai Peng, Simone Dichiara, Geoffrey Ryan, Hendrik van Eerten, ZG Dai, Seo-Won Chang, Hyeonho Choi, Kishalay De, Youdong Hu, Charles Kilpatrick, Alexander Kutyrev, Mankeun Jeong, Chung-Uk Lee, Martin Makler, Felipe Navarrete, Ignacio Pérez-García
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A persistent ultraviolet outflow from the accretion disc in a transient neutron star binary

Authors:

Noel Castro Segura, Christian Knigge, Knox Long, Diego Altamirano, Montserrat Armas Padilla, Charles Bailyn, David Buckley, Douglas Buisson, Jorge Casares, Phil Charles, Jorge Combi, Virginia A Cúneo, Nathalie Degenaar, Santiago del Palacio, Maria Diaz Trigo, Rob Fender, Poshak Gandhi, Claudia Gutíerrez, Juan Hernández Santisteban, Felipe Jiménez Ibarra, James Matthews, Mariano Mendez, Matthew Middleton, Teo Muñoz Darias, Mehtap Özbey Arabaci, Mayukh Pahari, Lauren Rhodes, Thomas Russell, Simone Scaringi, Jakob van den Eijden, Georgios Vasilopolulos, Federico Vincentelli, Phil Wiseman
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Decadal pre-explosion activity and circumstellar interaction in a supernova

Authors:

Ting-Wan Chen, Amar Aryan, Sheng Yang, Stephen Smartt, Takashi Moriya, Se an Brennan, Maximilian Stritzinger, Bailey Martin, Matt Nicholl, Albert Kong, James Gillanders, Anirban Dutta, Brian Schmidt, Yu-Chi Cheng, Mark Huber, Cheng-Han Lai, Chien-Hsiu Lee, Yu-Hsing Lee, Chow-Choong Ngeow, Ken Smith, Christopher Ashall, Christopher R Burns, Kenneth Chambers, Zhi-Yue Chen, Thomas de Boer, Eric Y Hsiao, Khoa Ho, Willem Hoogendam, David Jones, Erkki Kankare, Tom Killestein, Hanindyo Kuncarayakti, Meng-Han Lee, Chuan-Jui Li, Chien-Cheng Lin, Christopher Lidman, Thomas Lowe, Eugene Magnier, Kyle Medler, Anais Möller, Thomas Moore, Nidia Morrell, Gregory Paek, Cameron Pfeffer, Da-Chun Qiang, Liana Rauf, Tom Reynolds, Aiswarya Sankar.K, Shubham Srivastav, Jack Tweddle, Richard Wainscoat, Ze-Ning Wang, Huangfei Xiao, Zong-Hong Zhu, Katie Auchettl, Yen-Chen Pan, Benjamin Shappee, Jie-Lin Yang
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Dynamical Modeling of SAURON Galaxies

Carnegie Observatories Centennial Symposium. 1. Coevolution of Black Holes and Galaxies

Authors:

M Cappellari, RCE van den Bosch, EK Verolme, R Bacon, M Bureau, Y Copin, RL Davies, E Emsellem, D Krajnovic, H Kuntschner, R McDermid, BW Miller, RF Peletier, PT de Zeeuw

Abstract:

We describe our program for the dynamical modeling of early-type galaxies observed with the panoramic integral-field spectrograph SAURON. We are using Schwarzschild's numerical orbit superposition method to reproduce in detail all kinematical and photometric observables, and recover the intrinsic orbital structure of the galaxies. Since catastrophes are the most prominent features in the orbital observables, two-dimensional kinematical coverage is essential to constrain the dynamical models.
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