Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Bangale, Priyadarshini"'
Autor:
Reynolds, Stephen, An, Hongjun, Abdelmaguid, Moaz, Alford, Jason, Fryer, Chris L., Mori, Kaya, Nynka, Melania, Park, Jaegeun, Terada, Yukikatsu, Woo, Jooyun, Bamba, Aya, Bangale, Priyadarshini, Diesing, Rebecca, Eagle, Jordan, Gabici, Stefano, Gelfand, Joseph, Grefenstette, Brian, Garcia, Javier, Kim, Chanho, Kumar, Sajan, Mac Intyre, Brydyn, Madsen, Kristin, Manconi, Silvia, Motogami, Yugo, Ohsumi, Hayato, Olmi, Barbara, Sato, Toshiki, Shang, Ruo-Yu, Stern, Daniel, Tsuji, Naomi, Younes, George, Zoglauer, Andreas
HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging ($<10"$ full width at half maximum) and broad spectral coverage (0.2--80 keV) with an effective area far superior to current facilities (including XMM-Newt
Externí odkaz:
http://arxiv.org/abs/2311.04952
Autor:
Mori, Kaya, Reynolds, Stephen, An, Hongjun, Bamba, Aya, Krivonos, Roman, Tsuji, Naomi, Abdelmaguid, Moaz, Alford, Jason, Bangale, Priyadarshini, Celli, Silvia, Diesing, Rebecca, Eagle, Jordan, Fryer, Chris L., Gabici, Stefano, Gelfand, Joseph, Grefenstette, Brian, Garcia, Javier, Kim, Chanho, Kumar, Sajan, Kuznetsova, Ekaterina, Mac Intyre, Brydyn, Madsen, Kristin, Manconi, Silvia, Motogami, Yugo, Ohsumi, Hayato, Olmi, Barbara, Park, Jaegeun, Ponti, Gabriele, Sato, Toshiki, Shang, Ruo-Yu, Stern, Daniel, Terada, Yukikatsu, Woo, Jooyun, Younes, George, Zoglauer, Andreas
HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging (<10" FWHM) and broad spectral coverage (0.2-80 keV) with an effective area far superior to current facilities (including XMM-Newton and NuSTAR) to enable
Externí odkaz:
http://arxiv.org/abs/2311.04851
Autor:
Acharyya, Atreya, Adams, Colin, Archer, Avery, Bangale, Priyadarshini, Batista, Pedro, Benbow, Wystan, Brill, Aryeh, Capasso, M, Errando, Manel, Falcone, Abraham, Feng, Qi, Finley, John, Foote, Gregory, Fortson, Lucy, Furniss, Amy, Griffin, Sean, Hanlon, William, Hanna, David, Hervet, Olivier, Hinrichs, Claire, Hoang, John, Holder, Jamie, Humensky, T., Jin, Weidong, Kaaret, Philip, Kertzman, Mary P., Kherlakian, Maria, Kieda, David, Kleiner, Tobias, Korzoun, Nikolas, Kumar, Sajan, Lang, Mark, Lundy, Matthew, Maier, Gernot, McGrath, Conor, Millard, Matthew, Miller, Hayden, Millis, John, Mooney, Connor, Moriarty, Patrick, Mukherjee, Reshmi, O'Brien, Stephan, Ong, Rene A., Pohl, Martin, Pueschel, Elisa, Quinn, John, Ragan, Kenneth J., Reynolds, Paul, Ribeiro, Deivid, Roache, Emmet Thomas, Ryan, Jamie, Sadeh, Iftach, Saha, Lab, Santander, Marcos, Sembroski, Glenn H, Shang, Ruo, Tak, Donggeun, Talluri, Anjana, Tucci, James, Vazquez, Nico, Williams, David, Wong, Sam, Woo, Jooyun, DeBoer, David, Isaacson, Howard, de Pater, Imke, Price, Danny, Siemion, Andrew
The Breakthrough Listen Initiative is conducting a program using multiple telescopes around the world to search for "technosignatures": artificial transmitters of extraterrestrial origin from beyond our solar system. The VERITAS Collaboration joined
Externí odkaz:
http://arxiv.org/abs/2306.17680
Autor:
Acharyya, Atreya, Adams, Colin, Archer, Avery, Bangale, Priyadarshini, Benbow, Wystan, Brill, Aryeh, Christiansen, Jodi, Chromey, Alisha, Errando, Manel, Falcone, Abe, Feng, Qi, Finley, John, Foote, Gregory, Fortson, Lucy, Furniss, Amy, Gallagher, Greg, Hanlon, William, Hanna, David, Hervet, Olivier, Hinrichs, Claire, Hoang, John, Holder, Jamie, Jin, Weidong, Johnson, Madalyn, Kaaret, Philip, Kertzman, Mary P., Kieda, David, Kleiner, Tobias, Korzoun, Nikolas, Krennrich, Frank, Lang, Mark, Lundy, Matthew, Maier, Gernot, McGrath, Conor, Millard, Matthew, Millis, John, Mooney, Connor, Moriarty, Patrick, Mukherjee, Reshmi, O'Brien, Stephan, Ong, Rene A., Pohl, Martin, Pueschel, Elisa, Quinn, John, Ragan, Kenneth J., Reynolds, Paul, Ribeiro, Deivid, Roache, Emmet Thomas, Sadeh, Iftach, Sadun, Alberto, Saha, Lab, Santander, Marcos, Sembroski, Glenn, Shang, Ruo, Splettstoesser, Megan, Talluri, Anjana, Tucci, James, Vassiliev, Vladimir, Williams, David, Wong, Sam, Hovatta, Talvikki, Jorstad, Svetlana, Kiehlmann, Sebastian, Lahteenmaki, Anne, Liodakis, Ioannis, Marscher, Alan, Max-Moerbeck, Walter, Readhead, Anthony, Reeves, Rodrigo, Smith, Paul S, Tornikoski, Merja
We report the detection of very high energy gamma-ray emission from the blazar S3 1227+25 (VER J1230+253) with the Very Energetic Radiation Imaging Telescope Array System (VERITAS). VERITAS observations of the source were triggered by the detection o
Externí odkaz:
http://arxiv.org/abs/2305.02860
Autor:
Korngut, Phillip, Kim, Min Gyu, Arai, Toshiaki, Bangale, Priyadarshini, Bock, James, Cooray, Asantha, Cheng, Yun Ting, Feder, Richard, Hristov, Viktor, Lanz, Alicia, Levenson, Louis, Matsumoto, Toshio, Matsuura, Shuji, Nguyen, Chi, Sano, Kei, Tsumura, Kohji, Zemcov, Michael
Scattered sunlight from the interplanetary dust (IPD) cloud in our Solar system presents a serious foreground challenge for spectro-photometric measurements of the Extragalactic Background Light (EBL). In this work, we report on measurements of the a
Externí odkaz:
http://arxiv.org/abs/2104.07104
Autor:
Cheng, Yun-Ting, Arai, Toshiaki, Bangale, Priyadarshini, Bock, James J., Chang, Tzu-Ching, Cooray, Asantha, Feder, Richard M., Korngut, Phillip M., Lee, Dae Hee, Liu, Lunjun, Matsumoto, Toshio, Matsuura, Shuji, Nguyen, Chi H., Sano, Kei, Tsumura, Kohji, Zemcov, Michael
We study the stellar halos of $0.2\lesssim z \lesssim 0.5$ galaxies with stellar masses spanning $M_*\sim 10^{10.5}$ to $10^{12}M_\odot$ (approximately $L_*$ galaxies at this redshift) using imaging data from the Cosmic Infrared Background Experiment
Externí odkaz:
http://arxiv.org/abs/2103.03882
Autor:
Mazin, Daniel, Bangale, Priyadarshini, Sitarek, Julian, Cortina, Juan, Fink, David, Hose, Jürgen, Illa, Jose Maria, Lorenz, Eckart, Martínez, Manel, Menzel, Uta, Mirzoyan, Razmik, Teshima, Masahiro
So far the current ground-based Imaging Atmospheric Cherenkov Telescopes (IACTs) have energy thresholds in the best case in the range of ~30 to 50 GeV (H.E.S.S. II and MAGIC telescopes). Lowest energy gamma-ray showers produce low light intensity ima
Externí odkaz:
http://arxiv.org/abs/1410.5070
Autor:
Hessels, Jason W. T., Roberts, Mallory S. E., McLaughlin, Maura A., Ray, Paul S., Bangale, Priyadarshini, Ransom, Scott M., Kerr, Matthew, Camilo, Fernando, DeCesar, Megan E., Consortium, Fermi Pulsar Search
We have used the Green Bank Telescope at 350MHz to search 50 faint, unidentified Fermi Gamma-ray sources for radio pulsations. So far, these searches have resulted in the discovery of 10 millisecond pulsars, which are plausible counterparts to these
Externí odkaz:
http://arxiv.org/abs/1101.1742
Autor:
Reynolds, Stephen, An, Hongjun, Abdelmaguid, Moaz, Alford, Jason, Fryer, Chris, Mori, Kaya, Nynka, Melania, Park, Jaegeun, Terada, Yukikatsu, Woo, Jooyun, Bamba, Aya, Bangale, Priyadarshini, Diesing, Rebecca, Eagle, Jordan, Gabici, Stefano, Gelfand, Joseph, Grefenstette, Brian, Garcia, Javier, Kim, Chanho, Kumar, Sajan
Publikováno v:
Frontiers in Astronomy & Space Sciences; 2024, p1-21, 21p