Zobrazeno 1 - 10
of 108
pro vyhledávání: '"Ressler, Michael E."'
Autor:
Rose, Sam, Lau, Ryan M., Jencson, Jacob E., Kasliwal, Mansi M., De, Kishalay, Ressler, Michael E., Fox, Ori D., Hankins, Matthew J.
The James Webb Space Telescope (JWST) has opened up a new window to study highly reddened explosive transients. We present results from late-time (1421 days post-explosion) JWST follow-up spectroscopic observations with NIRSpec and MIRI LRS of the in
Externí odkaz:
http://arxiv.org/abs/2407.20430
Autor:
Izumi, Natsuko, Ressler, Michael E., Lau, Ryan M., Koch, Patrick M., Saito, Masao, Kobayashi, Naoto, Yasui, Chikako
The extreme outer Galaxy (EOG), which we define as the region of the Milky Way with a galactocentric radius of more than 18 kpc, provides an excellent opportunity to study star formation in an environment significantly different from that in the sola
Externí odkaz:
http://arxiv.org/abs/2407.07822
Autor:
Mainzer, A. K., Masiero, Joseph R., Abell, Paul A., Bauer, J. M., Bottke, William, Buratti, Bonnie J., Carey, Sean J., Cotto-Figueroa, D., Cutri, R. M., Dahlen, D., Eisenhardt, Peter R. M., Fernandez, 6 Y. R., Furfaro, Roberto, Grav, Tommy, Hoffman, T. L., Kelley, Michael S., Kim, Yoonyoung, Kirkpatrick, J. Davy, Lawler, Christopher R., Lilly, Eva, Liu, X., Marocco, Federico, Marsh, K. A., Masci, Frank J., McMurtry, Craig W., Pourrahmani, Milad, Reinhart, Lennon, Ressler, Michael E., Satpathy, Akash, Schambeau, C. A., Sonnett, S., Spahr, Timothy B., Surace, Jason A., Vaquero, Mar, Wright, E. L., Zengilowski, Gregory R., Team, NEO Surveyor Mission
The Near-Earth Object (NEO) Surveyor mission is a NASA observatory designed to discover and characterize near-Earth asteroids and comets. The mission's primary objective is to find the majority of objects large enough to cause severe regional impact
Externí odkaz:
http://arxiv.org/abs/2310.12918
Autor:
Morrison, Jane, Dicken, Daniel, Argyriou, Ioannis, Ressler, Michael E., Gordon, Karl D., Regan, Michael W., Cracraft, Misty, Rieke, George H., Engesser, Michael, Alberts, Stacey, Alvarez-Marquez, Javier, Colbert, James W., Fox, Ori D., Gasman, Danny, Law, David R., Marin, Macarena Garcia, Gaspar, Andras, Guillard, Pierre, Kendrew, Sarah, Labiano, Alvaro, Laine, Seppo, Noriega-Crespo, Alberto, Shivaei, Irene, Sloan, Greg
Publikováno v:
Publications of the Astronomical Society of the Pacific, Volume 135, Number 1049, 2023
The detectors in the Mid-Infrared Instrument (MIRI) of the James Webb Space Telescope (JWST) are arsenic-21 doped silicon impurity band conduction (Si:As IBC) devices and are direct descendants of the Spitzer IRAC22 long wavelength arrays (channels 3
Externí odkaz:
http://arxiv.org/abs/2308.16327
Autor:
Argyriou, Ioannis, Lage, Craig, Rieke, George H., Gasman, Danny, Bouwman, Jeroen, Morrison, Jane, Libralato, Mattia, Dicken, Daniel, Brandl, Bernhard R., Álvarez-Márquez, Javier, Labiano, Alvaro, Regan, Michael, Ressler, Michael E.
Publikováno v:
A&A 680, A96 (2023)
The Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope (JWST) uses three Si:As impurity band conduction (IBC) detector arrays. The output voltage level of each MIRI detector pixel is digitally recorded by sampling-up-the-ramp. For
Externí odkaz:
http://arxiv.org/abs/2303.13517
Galaxy and occupies perhaps a quarter of the volume of the Galactic disk. Decoding the spectrum of the Galactic diffuse ionizing field is of fundamental interest. This can be done via direct measurements of ionization fractions of various elements. B
Externí odkaz:
http://arxiv.org/abs/2303.02193
Autor:
Lau, Ryan M., Kasliwal, Mansi M., Bond, Howard E., Smith, Nathan, Fox, Ori D., Carlon, Robert, Cody, Ann Marie, Contreras, Carlos, Dykhoff, Devin, Gehrz, Robert, Hsiao, Eric, Jencson, Jacob, Khan, Rubab, Masci, Frank, Monard, L. A. G., Monson, Andrew J., Morrell, Nidia, Phillips, Mark, Ressler, Michael E.
We present multi-epoch mid-infrared (IR) photometry and the optical discovery observations of the "impostor" supernova (SN) 2010da in NGC. 300 using new and archival Spitzer Space Telescope images and ground-based observatories. The mid-infrared coun
Externí odkaz:
http://hdl.handle.net/10150/624070
http://arizona.openrepository.com/arizona/handle/10150/624070
http://arizona.openrepository.com/arizona/handle/10150/624070
Autor:
Jones, O. C., Álvarez-Márquez, J., Sloan, G. C., Kavanagh, P. J., Argyriou, I., Labiano, A., Law, D. R., Patapis, P., Mueller, Michael, Larson, Kirsten L., Bright, Stacey N., Klaassen, P. D., Fox, O. D., Gasman, Danny, Geers, V. C., Glauser, Adrian M., Guillard, Pierre, Nayak, Omnarayani, Noriega-Crespo, A., Ressler, Michael E., Sargent, B., Temim, T., Vandenbussche, B., Marín, Macarena García
During the commissioning of {\em JWST}, the Medium-Resolution Spectrometer (MRS) on the Mid-Infrared Instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large Magellanic Cloud. The MRS was designed to provide medium resolution (R = $\l
Externí odkaz:
http://arxiv.org/abs/2301.13233
Autor:
Sahai, Raghvendra, Bujarrabal, Valentin, Quintana-Lacaci, Guillermo, Reindl, Nicole, Van de Steene, Griet, Contreras, Carmen Sánchez, Ressler, Michael E.
The planetary nebula (PN) NGC3132 is a striking example of the dramatic but poorly understood, mass-loss phenomena that (1-8) Msun stars undergo during their death throes as they evolve into white dwarfs (WDs). From an analysis of JWST multiwavelengt
Externí odkaz:
http://arxiv.org/abs/2211.16741
Autor:
Lau, Ryan M., Hankins, Matthew J., Han, Yinuo, Argyriou, Ioannis, Corcoran, Michael F., Eldridge, Jan J., Endo, Izumi, Fox, Ori D., Marin, Macarena Garcia, Gull, Theodore R., Jones, Olivia C., Hamaguchi, Kenji, Lamberts, Astrid, Law, David R., Madura, Thomas, Marchenko, Sergey V., Matsuhara, Hideo, Moffat, Anthony F. J., Morris, Mark R., Morris, Patrick W., Onaka, Takashi, Ressler, Michael E., Richardson, Noel D., Russell, Christopher M. P., Sanchez-Bermudez, Joel, Smith, Nathan, Soulain, Anthony, Stevens, Ian R., Tuthill, Peter, Weigelt, Gerd, Williams, Peredur M., Yamaguchi, Ryodai
Publikováno v:
Lau, R.M., Hankins, M.J., Han, Y. et al. Nested dust shells around the Wolf-Rayet binary WR 140 observed with JWST. Nat Astron (2022)
Massive colliding-wind binaries that host a Wolf-Rayet (WR) star present a potentially important source of dust and chemical enrichment in the interstellar medium (ISM). However, the chemical composition and survival of dust formed from such systems
Externí odkaz:
http://arxiv.org/abs/2210.06452