Zobrazeno 1 - 10
of 69
pro vyhledávání: '"Vestrand, W. Thomas"'
Autor:
Korobkin, Oleg, Hungerford, Aimee M., Fryer, Christopher L., Mumpower, Matthew R., Misch, G. Wendell, Sprouse, Trevor M., Lippuner, Jonas, Surman, Rebecca, Couture, Aaron J., Bloser, Peter F., Shirazi, Farzane, Even, Wesley P., Vestrand, W. Thomas, Miller, Richard S.
Publikováno v:
The Astrophysical Journal, Volume 889, Issue 2, id.168, 2020
The mergers of compact binaries with at least one neutron star component are the potential leading sites of the production and ejection of $r$-process elements. Discoveries of galactic binary pulsars, short gamma-ray bursts, and gravitational-wave de
Externí odkaz:
http://arxiv.org/abs/1905.05089
Autor:
Wollaeger, Ryan T., Fryer, Chris L., Fontes, Christopher J., Lippuner, Jonas, Vestrand, W. Thomas, Mumpower, Matthew R., Korobkin, Oleg, Hungerford, Aimee L., Even, Wesley P.
We explore the impact of pulsar electromagnetic dipole and fallback accretion emission on the luminosity of a suite of kilonova models. The pulsar models are varied over pulsar magnetic field strength, pulsar lifetime, ejecta mass, and elemental abun
Externí odkaz:
http://arxiv.org/abs/1904.05934
Autor:
Kierans, Carolyn A., Beacom, John F., Boggs, Steve, Buckley, Matthew, Caputo, Regina, Crocker, Roland, De Becker, Michael, Diehl, Roland, Fryer, Chris L., Griffin, Sean, Hartmann, Dieter, Hays, Elizabeth, Jean, Pierre, Krause, Martin G. H., Linden, Tim, Marcowith, Alexandre, Martin, Pierrick, Moiseev, Alexander, Oberlack, Uwe, Orlando, Elena, Panther, Fiona, Prantzos, Nikos, Rothschild, Richard, Seitenzahl, Ivo, Shrader, Chris, Siegert, Thomas, Strong, Andy, Tomsick, John, Vestrand, W. Thomas, Zoglauer, Andreas
The 511 keV line from positron annihilation in the Galaxy was the first $\gamma$-ray line detected to originate from outside our solar system. Going into the fifth decade since the discovery, the source of positrons is still unconfirmed and remains o
Externí odkaz:
http://arxiv.org/abs/1903.05569
Autor:
Bellm, Eric C., Kulkarni, Shrinivas R., Graham, Matthew J., Dekany, Richard, Smith, Roger M., Riddle, Reed, Masci, Frank J., Helou, George, Prince, Thomas A., Adams, Scott M., Barbarino, C., Barlow, Tom, Bauer, James, Beck, Ron, Belicki, Justin, Biswas, Rahul, Blagorodnova, Nadejda, Bodewits, Dennis, Bolin, Bryce, Brinnel, Valery, Brooke, Tim, Bue, Brian, Bulla, Mattia, Burruss, Rick, Cenko, S. Bradley, Chang, Chan-Kao, Connolly, Andrew, Coughlin, Michael, Cromer, John, Cunningham, Virginia, De, Kishalay, Delacroix, Alex, Desai, Vandana, Duev, Dmitry A., Eadie, Gwendolyn, Farnham, Tony L., Feeney, Michael, Feindt, Ulrich, Flynn, David, Franckowiak, Anna, Frederick, S., Fremling, C., Gal-Yam, Avishay, Gezari, Suvi, Giomi, Matteo, Goldstein, Daniel A., Golkhou, V. Zach, Goobar, Ariel, Groom, Steven, Hacopians, Eugean, Hale, David, Henning, John, Ho, Anna Y. Q., Hover, David, Howell, Justin, Hung, Tiara, Huppenkothen, Daniela, Imel, David, Ip, Wing-Huen, Ivezić, Željko, Jackson, Edward, Jones, Lynne, Juric, Mario, Kasliwal, Mansi M., Kaspi, S., Kaye, Stephen, Kelley, Michael S. P., Kowalski, Marek, Kramer, Emily, Kupfer, Thomas, Landry, Walter, Laher, Russ R., Lee, Chien-De, Lin, Hsing Wen, Lin, Zhong-Yi, Lunnan, Ragnhild, Mahabal, Ashish, Mao, Peter, Miller, Adam A., Monkewitz, Serge, Murphy, Patrick, Ngeow, Chow-Choong, Nordin, Jakob, Nugent, Peter, Ofek, Eran, Patterson, Maria T., Penprase, Bryan, Porter, Michael, Rauch, Ludwig, Rebbapragada, Umaa, Reiley, Dan, Rigault, Mickael, Rodriguez, Hector, van Roestel, Jan, Rusholme, Ben, van Santen, Jakob, Schulze, S., Shupe, David L., Singer, Leo P., Soumagnac, Maayane T., Stein, Robert, Surace, Jason, Sollerman, Jesper, Szkody, Paula, Taddia, F., Terek, Scott, Van Sistine, Angela, van Velzen, Sjoert, Vestrand, W. Thomas, Walters, Richard, Ward, Charlotte, Ye, Quan-Zhi, Yu, Po-Chieh, Yan, Lin, Zolkower, Jeffry
Publikováno v:
Publications of the Astronomical Society of the Pacific, Volume 131, Issue 995, pp. 018002 (2019)
The Zwicky Transient Facility (ZTF) is a new optical time-domain survey that uses the Palomar 48-inch Schmidt telescope. A custom-built wide-field camera provides a 47 deg$^2$ field of view and 8 second readout time, yielding more than an order of ma
Externí odkaz:
http://arxiv.org/abs/1902.01932
Autor:
Graham, Matthew J., Kulkarni, S. R., Bellm, Eric C., Adams, Scott M., Barbarino, Cristina, Blagorodnova, Nadejda, Bodewits, Dennis, Bolin, Bryce, Brady, Patrick R., Cenko, S. Bradley, Chang, Chan-Kao, Coughlin, Michael W., De, Kishalay, Eadie, Gwendolyn, Farnham, Tony L., Feindt, Ulrich, Franckowiak, Anna, Fremling, Christoffer, Gal-yam, Avishay, Gezari, Suvi, Ghosh, Shaon, Goldstein, Daniel A., Golkhou, V. Zach, Goobar, Ariel, Ho, Anna Y. Q., Huppenkothen, Daniela, Ivezic, Zeljko, Jones, R. Lynne, Juric, Mario, Kaplan, David L., Kasliwal, Mansi M., Kelley, Michael S. P., Kupfer, Thomas, Lee, Chien-De, Lin, Hsing Wen, Lunnan, Ragnhild, Mahabal, Ashish A., Miller, Adam A., Ngeow, Chow-Choong, Nugent, Peter, Ofek, Eran O., Prince, Thomas A., Rauch, Ludwig, van Roestel, Jan, Schulze, Steve, Singer, Leo P., Sollerman, Jesper, Taddia, Francesco, Yan, Lin, Ye, Quan-Zhi, Yu, Po-Chieh, Andreoni, Igor, Barlow, Tom, Bauer, James, Beck, Ron, Belicki, Justin, Biswas, Rahul, Brinnel, Valery, Brooke, Tim, Bue, Brian, Bulla, Mattia, Burdge, Kevin, Burruss, Rick, Connolly, Andrew, Cromer, John, Cunningham, Virginia, Dekany, Richard, Delacroix, Alex, Desai, Vandana, Duev, Dmitry A., Hacopians, Eugean, Hale, David, Helou, George, Henning, John, Hover, David, Hillenbrand, Lynne A., Howell, Justin, Hung, Tiara, Imel, David, Ip, Wing-Huen, Jackson, Edward, Kaspi, Shai, Kaye, Stephen, Kowalski, Marek, Kramer, Emily, Kuhn, Michael, Landry, Walter, Laher, Russ R., Mao, Peter, Masci, Frank J., Monkewitz, Serge, Murphy, Patrick, Nordin, Jakob, Patterson, Maria T., Penprase, Bryan, Porter, Michael, Rebbapragada, Umaa, Reiley, Dan, Riddle, Reed, Rigault, Mickael, Rodriguez, Hector, Rusholme, Ben, van Santen, Jakob, Shupe, David L., Smith, Roger M., Soumagnac, Maayane T., Stein, Robert, Surace, Jason, Szkody, Paula, Terek, Scott, van Sistine, Angela, van Velzen, Sjoert, Vestrand, W. Thomas, Walters, Richard, Ward, Charlotte, Zhang, Chaoran, Zolkower, Jeffry
The Zwicky Transient Facility (ZTF), a public-private enterprise, is a new time domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg$^2$ field of view and 8 second readout time. It is well positioned in th
Externí odkaz:
http://arxiv.org/abs/1902.01945
Observatories are complex scientific and technical institutions serving diverse users and purposes. Their telescopes, instruments, software, and human resources engage in interwoven workflows over a broad range of timescales. These workflows have bee
Externí odkaz:
http://arxiv.org/abs/1407.7552
Publikováno v:
Astrophys.J.639:377-381,2006
We report on the first XMM-Newton observation of the Vela-like pulsar PSR B2334+61. Spectral analysis reveals soft X-ray emission, with the bulk of the photons emitted at energies below ~1.5 keV. We find that the spectrum has a thermal origin and is
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508439
Autor:
McConnell, Mark L., Bloser, Peter F., Case, Gary, Cherry, Michael, Cravens, James, Guzik, T. Gregory, Hurley, Kevin, Kippen, R. Marc, Macri, John, Miller, Richard S., Paciesas, William, Ryan, James M., Schaefer, Bradley, Stacy, J. Gregory, Vestrand, W. Thomas, Wefel, John P.
The primary scientific mission of the Black Hole Finder Probe (BHFP), part of the NASA Beyond Einstein program, is to survey the local Universe for black holes over a wide range of mass and accretion rate. One approach to such a survey is a hard X-ra
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508313
Autor:
McGowan, Katherine E., Zane, Silvia, Cropper, Mark, Kennea, Jamie A., Cordova, France A., Ho, Cheng, Sasseen, Tim, Vestrand, W. Thomas
Publikováno v:
Astrophys.J.600:343-350,2004
We report on the XMM-Newton observations of the young, 102 ms pulsar PSR B1706-44. We have found that both a blackbody plus power-law and a magnetized atmospheric model plus power-law provide an excellent fit to the EPIC spectra. The two scenarios ar
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309445
Publikováno v:
Astrophys.J.641:756-762,2006
We report on our serendipitous discovery with the XMM-Newton Observatory of a luminous X-ray emitting cluster of galaxies that is located behind the Andromeda galaxy (M31). X-ray emission from the cluster was detected previously by ROSAT, and catalog
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307223