Zobrazeno 1 - 10
of 2 423
pro vyhledávání: '"Schneider Benjamin"'
Autor:
Grant, Catherine E., Bautz, Marshall W., Miller, Eric D., Foster, Richard F., LaMarr, Beverly, Malonis, Andrew, Prigozhin, Gregory, Schneider, Benjamin, Leitz, Christopher, Falcone, Abraham D.
The Arcus Probe mission concept provides high-resolution soft X-ray and UV spectroscopy to reveal feedback-driven structure and evolution throughout the universe with an agile response capability ideal for probing the physics of time-dependent phenom
Externí odkaz:
http://arxiv.org/abs/2412.16344
Non-small cell lung cancer (NSCLC) is often intrinsically resistant to several first- and second-line therapeutics and can rapidly acquire further resistance after a patient begins receiving treatment. Treatment outcomes are therefore significantly i
Externí odkaz:
http://arxiv.org/abs/2410.16967
Autor:
Schneider, Benjamin, Prigozhin, Gregory, Foster, Richard F., Bautz, Marshall W., Fu, Hope, Grant, Catherine E., Heine, Sarah, Juneau, Jill, LaMarr, Beverly, Limousin, Olivier, Lourie, Nathan, Malonis, Andrew, Miller, Eric D.
The advent of back-illuminated complementary metal-oxide-semiconductor (CMOS) sensors and their well-known advantages over charge-coupled devices (CCDs) make them an attractive technology for future X-ray missions. However, numerous challenges remain
Externí odkaz:
http://arxiv.org/abs/2409.05954
Autor:
Heine, Sarah N. T., Marshall, Herman L., Schneider, Benjamin, Lamar, Beverly, Kothnur, Nithya, Garner, Alan
The MIT X-ray Polarimetry Beamline is a facility that we developed for testing components for possible use in X-ray polarimetry. Over the past few years, we have demonstrated that the X-ray source can generate nearly 100% polarized X-rays at various
Externí odkaz:
http://arxiv.org/abs/2408.11168
Autor:
Sarkar, Arnab, Chakraborty, Priyanka, Vogelsberger, Mark, McDonald, Michael, Torrey, Paul, Garcia, Alex M., Khullar, Gourav, Ferland, Gary J., Forman, William, Wolk, Scott, Schneider, Benjamin, Bautz, Mark, Miller, Eric, Grant, Catherine, ZuHone, John
We present star formation rates (SFR), the mass-metallicity relation (MZR), and the SFR-dependent MZR across redshifts 4 to 10 using 81 star-forming galaxies observed by the JWST NIRSpec employing both low-resolution PRISM and medium-resolution grati
Externí odkaz:
http://arxiv.org/abs/2408.07974
Autor:
Poliszczuk, Artem, Wilkins, Dan, Allen, Steven W., Miller, Eric D., Chattopadhyay, Tanmoy, Schneider, Benjamin, Darve, Julien Eric, Bautz, Marshall, Falcone, Abe, Foster, Richard, Grant, Catherine E., Herrmann, Sven, Kraft, Ralph, Morris, R. Glenn, Nulsen, Paul, Orel, Peter, Schellenberger, Gerrit, Stueber, Haley R.
Traditional cosmic ray filtering algorithms used in X-ray imaging detectors aboard space telescopes perform event reconstruction based on the properties of activated pixels above a certain energy threshold, within 3x3 or 5x5 pixel sliding windows. Th
Externí odkaz:
http://arxiv.org/abs/2407.16768
Autor:
Miller, Eric D., Gregory, James A., Bautz, Marshall W., Clark, Harry R., Cooper, Michael, Donlon, Kevan, Foster, Richard F., Grant, Catherine E., Jensen, Mallory, LaMarr, Beverly, Lambert, Renee, Leitz, Christopher, Malonis, Andrew, Neak, Mo, Prigozhin, Gregory, Ryu, Kevin, Schneider, Benjamin, Warner, Keith, Young, Douglas J., Zhang, William W.
Future X-ray astrophysics missions will survey large areas of the sky with unparalleled sensitivity, enabled by lightweight, high-resolution optics. These optics inherently produce curved focal surfaces with radii as small as 2 m, requiring a large a
Externí odkaz:
http://arxiv.org/abs/2406.18753
Autor:
Chakraborty, Priyanka, Sarkar, Arnab, Wolk, Scott, Schneider, Benjamin, Brickhouse, Nancy, Lanzetta, Kenneth, Foster, Adam, Smith, Randall
We report the detection of seven new galaxy candidates with redshift $z$ $>$ 11 within the JWST Advanced Deep Extragalactic Survey (JADES) GOODS-S and GOODS-N fields. These new candidates are detected through meticulous analysis of NIRCam photometry
Externí odkaz:
http://arxiv.org/abs/2406.05306
Autor:
Sarkar, Arnab, Grant, Catherine E., Miller, Eric D., Bautz, Mark, Schneider, Benjamin, Foster, Rick F., Schellenberger, Gerrit, Allen, Steven, Kraft, Ralph P., Wilkins, Dan, Falcone, Abe, Ptak, Andrew
Galactic cosmic ray (GCR) particles have a significant impact on the particle-induced background of X-ray observatories, and their flux exhibits substantial temporal variability, potentially influencing background levels. In this study, we present on
Externí odkaz:
http://arxiv.org/abs/2405.06602
Autor:
Levan, Andrew J., Jonker, Peter G., Saccardi, Andrea, Malesani, Daniele Bjørn, Tanvir, Nial R., Izzo, Luca, Heintz, Kasper E., Sánchez, Daniel Mata, Quirola-Vásquez, Jonathan, Torres, Manuel A. P., Vergani, Susanna D., Schulze, Steve, Rossi, Andrea, D'Avanzo, Paolo, Gompertz, Benjamin, Martin-Carrillo, Antonio, Postigo, Antonio de Ugarte, Schneider, Benjamin, Yuan, Weimin, Ling, Zhixing, Zhang, Wenjie, Mao, Xuan, Liu, Yuan, Sun, Hui, Xu, Dong, Zhu, Zipei, Fernández, José Feliciano Agüí, Amati, Lorenzo, Bauer, Franz E., Campana, Sergio, Carotenuto, Francesco, Chrimes, Ashley, van Dalen, Joyce N. D., D'Elia, Valerio, Della Valle, Massimo, De Pasquale, Massimiliano, Dhillon, Vikram S., Galbany, Lluís, Gaspari, Nicola, Gianfagna, Giulia, Gomboc, Andreja, Habeeb, Nusrin, van Hoof, Agnes P. C., Hu, Youdong, Jakobsson, Pall, Julakanti, Yashaswi, Korth, Judith, Kouveliotou, Chryssa, Laskar, Tanmoy, Littlefair, Stuart P., Maiorano, Elisabetta, Mao, Jirong, Melandri, Andrea, Miller, M. Coleman, Mukherjee, Tamal, Oates, Samantha R., O'Brien, Paul, Palmerio, Jesse T., Parviainen, Hannu, Pieterse, Daniëlle L. A., Piranomonte, Silvia, Piro, Luigi, Pugliese, Giovanna, Ravasio, Maria E., Rayson, Ben, Salvaterra, Ruben, Sánchez-Ramírez, Rubén, Sarin, Nikhil, Shilling, Samuel P. R., Starling, Rhaana L. C., Tagliaferri, Gianpiero, Thakur, Aishwarya Linesh, Thöne, Christina C., Wiersema, Klaas, Worssam, Isabelle, Zafar, Tayyaba
The nature of the minute-to-hour long Fast X-ray Transients (FXTs) localised by telescopes such as Chandra, Swift, and XMM-Newton remains mysterious, with numerous models suggested for the events. Here, we report multi-wavelength observations of EP24
Externí odkaz:
http://arxiv.org/abs/2404.16350