@booklet {41742,
	title = {STROBE-X: X-ray Timing and Spectroscopy on Dynamical Timescales from Microseconds to Years},
	year = {2019},
	month = {2019/03/1},
	pages = {arXiv:1903.03035},
	abstract = {We present the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X), a probe-class mission concept selected for study by NASA. It combines huge collecting area, high throughput, broad energy coverage, and excellent spectral and temporal resolution in a single facility. STROBE-X offers an enormous increase in sensitivity for X-ray spectral timing, extending these techniques to extragalactic targets for the first time. It is also an agile mission capable of rapid response to transient events, making it an essential X-ray partner facility in the era of time-domain, multi-wavelength, and multi-messenger astronomy. Optimized for study of the most extreme conditions found in the Universe, its key science objectives include: (1) Robustly measuring mass and spin and mapping inner accretion flows across the black hole mass spectrum, from compact stars to intermediate-mass objects to active galactic nuclei. (2) Mapping out the full mass-radius relation of neutron stars using an ensemble of nearly two dozen rotation-powered pulsars and accreting neutron stars, and hence measuring the equation of state for ultradense matter over a much wider range of densities than explored by NICER. (3) Identifying and studying X-ray counterparts (in the post-Swift era) for multiwavelength and multi-messenger transients in the dynamic sky through cross-correlation with gravitational wave interferometers, neutrino observatories, and high-cadence time-domain surveys in other electromagnetic bands. (4) Continuously surveying the dynamic X-ray sky with a large duty cycle and high time resolution to characterize the behavior of X-ray sources over an unprecedentedly vast range of time scales. STROBE-X{\textquoteright}s formidable capabilities will also enable a broad portfolio of additional science.},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics},
	url = {https://ui.adsabs.harvard.edu/abs/2019arXiv190303035R},
	author = {Ray, Paul S. and Arzoumanian, Zaven and Ballantyne, David and Bozzo, Enrico and Brandt, Soren and Brenneman, Laura and Chakrabarty, Deepto and Christophersen, Marc and DeRosa, Alessandra and Feroci, Marco and Gendreau, Keith and Goldstein, Adam and Hartmann, Dieter and Hernanz, Margarita and Jenke, Peter and Kara, Erin and Maccarone, Tom and McDonald, Michael and Nowak, Michael and Phlips, Bernard and Remillard, Ron and Stevens, Abigail and Tomsick, John and Watts, Anna and Wilson-Hodge, Colleen and Wood, Kent and Zane, Silvia and Ajello, Marco and Alston, Will and Altamirano, Diego and Antoniou, Vallia and Arur, Kavitha and Ashton, Dominic and Auchettl, Katie and Ayres, Tom and Bachetti, Matteo and Balokovic, Mislav and Baring, Matthew and Baykal, Altan and Begelman, Mitch and Bhat, Narayana and Bogdanov, Slavko and Briggs, Michael and Bulbul, Esra and Bult, Petrus and Burns, Eric and Cackett, Ed and Campana, Riccardo and Caspi, Amir and Cavecchi, Yuri and Chenevez, Jerome and Cherry, Mike and Corbet, Robin and Corcoran, Michael and Corsi, Alessandra and Degenaar, Nathalie and Drake, Jeremy and Eikenberry, Steve and Enoto, Teruaki and Fragile, Chris and Fuerst, Felix and Gandhi, Poshak and Garcia, Javier and Goldstein, Adam and Gonzalez, Anthony and Grefenstette, Brian and Grinberg, Victoria and Grossan, Bruce and Guillot, Sebastien and Guver, Tolga and Haggard, Daryl and Heinke, Craig and Heinz, Sebastian and Hemphill, Paul and Homan, Jeroen and Hui, Michelle and Huppenkothen, Daniela and Ingram, Adam and Irwin, Jimmy and Jaisawal, Gaurava and Jaodand, Amruta and Kalemci, Emrah and Kaplan, David and Keek, Laurens and Kennea, Jamie and Kerr, Matthew and van der Klis, Michiel and Kocevski, Daniel and Koss, Mike and Kowalski, Adam and Lai, Dong and Lamb, Fred and Laycock, Silas and Lazio, Joseph and Lazzati, Davide and Longcope, Dana and Loewenstein, Michael and Maitra, Dipankair and Majid, Walid and Maksym, W. Peter and Malacaria, Christian and Margutti, Raffaella and Martindale, Adrian and McHardy, Ian and Meyer, Manuel and Middleton, Matt and Miller, Jon and Miller, Cole and Motta, Sara and Neilsen, Joey and Nelson, Tommy and Noble, Scott and O{\textquoteright}Brien, Paul and Osborne, Julian and Osten, Rachel and Ozel, Feryal and Palliyaguru, Nipuni and Pasham, Dheeraj and Patruno, Alessandro and Pelassa, Vero and Petropoulou, Maria and Pilia, Maura and Pohl, Martin and Pooley, David and Prescod-Weinstein, Chanda and Psaltis, Dimitrios and Raaijmakers, Geert and Reynolds, Chris and Riley, Thomas E. and Salvesen, Greg and Santangelo, Andrea and Scaringi, Simone and Schanne, Stephane and Schnittman, Jeremy and Smith, David and Smith, Krista Lynne and Snios, Bradford and Steiner, Andrew and Steiner, Jack and Stella, Luigi and Strohmayer, Tod and Sun, Ming and Tauris, Thomas and Taylor, Corbin and Tohuvavohu, Aaron and Vacchi, Andrea and Vasilopoulos, Georgios and Veledina, Alexandra and Walsh, Jonelle and Weinberg, Nevin and Wilkins, Dan and Willingale, Richard and Wilms, Joern and Winter, Lisa and Wolff, Michael and in {\textquoteright}t Zand, Jean and Zezas, Andreas and Zhang, Bing and Zoghbi, Abdu}
}
