Zobrazeno 1 - 10
of 122
pro vyhledávání: '"Stritzinger, Maximilian D"'
Autor:
Gutiérrez, Claudia P., Mattila, Seppo, Lundqvist, Peter, Dessart, Luc, González-Gaitán, Santiago, Jonker, Peter G., Dong, Subo, Coppejans, Deanne, Chen, Ping, Charalampopoulos, Panos, Elias-Rosa, Nancy, Reynolds, Thomas, Kochanek, Christopher, Fraser, Morgan, Pastorello, Andrea, Gromadzki, Mariusz, Neustadt, Jack, Benetti, Stefano, Kankare, Erkki, Kangas, Tuomas, Kotak, Rubina, Stritzinger, Maximilian D., Wevers, Thomas, Zhang, Bing, Bersier, David, Bose, Subhash, Buckley, David A. H., Dastidar, Raya, Gangopadhyay, Anjasha, Hamanowicz, Aleksandra, Kollmeier, Juna, Mao, Jirong, Potter, Stephen B., Romero-Colmenero, Encarni, Singh, Mridweeka, Somero, Auni, Terreran, Giacomo, Vaisanen, Petri, Wyrzykowski, Lukasz
We present ultraviolet, optical and near-infrared photometric and optical spectroscopic observations of the luminous, fast blue optical transient (LFBOT), CSS161010:045834-081803 (CSS161010). The transient was found in a low-redshift (z=0.033) dwarf
Externí odkaz:
http://arxiv.org/abs/2408.04698
Autor:
Burrow, Anthony, Baron, E., Burns, Christopher R., Hsiao, Eric Y., Lu, Jing, Ashall, Chris, Brown, Peter J., DerKacy, James M., Folatelli, G., Galbany, Lluís, Hoeflich, P., Krisciunas, Kevin, Morrell, N., Phillips, M. M., Shappee, Benjamin J., Stritzinger, Maximilian D., Suntzeff, Nicholas B.
We present a method of extrapolating the spectroscopic behavior of Type Ia supernovae (SNe Ia) in the near-infrared (NIR) wavelength regime up to 2.30 $\mu$m using optical spectroscopy. Such a process is useful for accurately estimating K-corrections
Externí odkaz:
http://arxiv.org/abs/2404.04724
Autor:
Dong, Yize, Valenti, Stefano, Ashall, Chris, Williamson, Marc, Sand, David J., Van Dyk, Schuyler D., Jha, Saurabh W., Lundquist, Michael, Modjaz, Maryam, Andrews, Jennifer E., Jencson, Jacob E., Hosseinzadeh, Griffin, Pearson, Jeniveve, Kwok, Lindsey A., Boland, Teresa, Hsiao, Eric Y., Smith, Nathan, Elias-Rosa, Nancy, Srivastav, Shubham, Smartt, Stephen, Fulton, Michael, Zheng, WeiKang, Brink, Thomas G., Filippenko, Alexei V., Shahbandeh, Melissa, Bostroem, K. Azalee, Hoang, Emily, Janzen, Daryl, Mehta, Darshana, Meza, Nicolas, Shrestha, Manisha, Wyatt, Samuel, Auchettl, Katie, Burns, Christopher R., Farah, Joseph, Galbany, L., Gonzalez, Estefania Padilla, Haislip, Joshua, Hinkle, Jason T., Howell, D. Andrew, De Jaeger, Thomas, Kouprianov, Vladimir, Kumar, Sahana, Lu, Jing, McCully, Curtis, Moran, Shane, Morrell, Nidia, Newsome, Megan, Pellegrino, Craig, Polin, Abigail, Reichart, Daniel E., Shappee, B. J., Stritzinger, Maximilian D., Terreran, Giacomo, Tucker, M. A.
We present optical and near-infrared observations of SN~2022crv, a stripped envelope supernova in NGC~3054, discovered within 12 hrs of explosion by the Distance Less Than 40 Mpc Survey. We suggest SN~2022crv is a transitional object on the continuum
Externí odkaz:
http://arxiv.org/abs/2309.09433
Autor:
Stritzinger, Maximilian D., Baron, Eddie, Taddia, Francesco, Burns, Chris R., Galbany, Morgan Fraserm Lluis, Holmbo, Simon, Hoeflich, Peter, Morrell, Nidia, Hsiao, E. Y., Johansson, Joel P., Karamehmetoglu, Emir, Kuncarayakti, Hanindyo, Lyman, Joe, Moriya, Takashi J., Phan, Kim, Phillips, Mark M., Anderson, Joseph P., Ashall, Chris, Brown, Peter J., Castellon, Sergio, Della Valle, Massimo, Gonzalez-Gaitan, Santiago, Gromadzki, Mariusz, Handberg, Rasmus, Lu, Jing, Nicholl, Matt, Shahbandeh, Melissa
Publikováno v:
A&A 686, A79 (2024)
We present a comprehensive data set of supernova (SN) 2016adj located within the central dust lane of Centaurus A. SN 2016adj is significantly reddened and after correcting the peak apparent $B$-band magnitude ($m_B = 17.48\pm0.05$) for Milky Way red
Externí odkaz:
http://arxiv.org/abs/2309.05031
Autor:
Ergon, Mattias, Lundqvist, Peter, Fransson, Claes, Kuncarayakti, Hanindyo, Das, Kaustav K., De, Kishalay, Ferrari, Lucia, Fremling, Christoffer, Medler, Kyle, Maeda, Keiichi, Pastorello, Andrea, Sollerman, Jesper, Stritzinger, Maximilian D.
We use the light curve and spectral synthesis code JEKYLL to calculate a set of macroscopically mixed Type IIb supernova (SN) models, which are compared to both previously published and new late-phase observations of SN 2020acat. The models differ in
Externí odkaz:
http://arxiv.org/abs/2308.07158
The intrinsic colors of Type Ia supernovae (SNe Ia) are important to understanding their use as cosmological standard candles. Understanding the effects of reddening and redshift on the observed colors are complicated and dependent on the intrinsic s
Externí odkaz:
http://hdl.handle.net/10150/623230
http://arizona.openrepository.com/arizona/handle/10150/623230
http://arizona.openrepository.com/arizona/handle/10150/623230
Autor:
Desai, Dhvanil D., Ashall, Chris, Shappee, Benjamin J., Morrell, Nidia, Galbany, Lluís, Burns, Christopher R., DerKacy, James M., Hinkle, Jason T., Hsiao, Eric, Kumar, Sahana, Lu, Jing, Phillips, Mark M., Shahbandeh, Melissa, Stritzinger, Maximilian D., Baron, Eddie, Bersten, Melina C., Brown, Peter J., de Jaeger, Thomas, Elias-Rosa, Nancy, Folatelli, Gastón, Huber, Mark E., Mazzali, Paolo, Müller-Bravo, Tomás E., Piro, Anthony L., Polin, Abigail, Suntzeff, Nicholas B., Anderson, Joseph P., Chambers, Kenneth C., Chen, Ting-Wan, de Boer, Thomas, Fulton, Michael D., Gao, Hua, Gromadzki, Mariusz, Inserra, Cosimo, Magnier, Eugene A., Nicholl, Matt, Ragosta, Fabio, Wainscoat, Richard, Young, David R.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 524, Issue 1, September 2023, Pages 767-785
We present photometric and spectroscopic observations and analysis of SN 2021bxu (ATLAS21dov), a low-luminosity, fast-evolving Type IIb supernova (SN). SN 2021bxu is unique, showing a large initial decline in brightness followed by a short plateau ph
Externí odkaz:
http://arxiv.org/abs/2303.13581
Autor:
Lu, Jing, Hsiao, Eric Y., Phillips, Mark M., Burns, Christopher R., Ashall, Chris, Morrell, Nidia, Ng, Lawrence, Kumar, Sahana, Shahbandeh, Melissa, Hoeflich, Peter, Baron, E., Uddin, Syed, Stritzinger, Maximilian D., Suntzeff, Nicholas B., Baltay, Charles, Davis, Scott, Diamond, Tiara R., Folatelli, Gaston, Förster, Francisco, Gagné, Jonathan, Galbany, Lluís, Gall, Christa, González-Gaitán, Santiago, Holmbo, Simon, Kirshner, Robert P., Krisciunas, Kevin, Marion, G. H., Perlmutter, Saul, Pessi, Priscila J., Piro, Anthony L., Rabinowitz, David, Ryder, Stuart D., Sand, David J.
We present the largest and most homogeneous collection of near-infrared (NIR) spectra of Type Ia supernovae (SNe Ia): 339 spectra of 98 individual SNe obtained as part of the Carnegie Supernova Project-II. These spectra, obtained with the FIRE spectr
Externí odkaz:
http://arxiv.org/abs/2211.05998
Autor:
Sai, Hanna, Wang, Xiaofeng, Elias-Rosa, Nancy, Yang, Yi, Zhang, Jujia, Lin, Weili, Mo, Jun, Piro, Anthony L., Zeng, Xiangyun, Andrea, Reguitti, Brown, Peter, Burns, Christopher R., Cai, Yongzhi, Fiore, Achille, Hsiao, Eric Y., Isern, Jordi, Itagaki, K., Li, Wenxiong, Li, Zhitong, Pessi, Priscila J., Phillips, M. M., Schuldt, Stefan, Shahbandeh, Melissa, Stritzinger, Maximilian D., Tomasella, Lina, Vogl, Christian, Wang, Bo, Wang, Lingzhi, Wu, Chengyuan, Yang, Sheng, Zhang, Jicheng, Zhang, Tianmeng, Zhang, Xinghan
Early-time radiative signals from type Ia supernovae (SNe Ia) can provide important constraints on the explosion mechanism and the progenitor system. We present observations and analysis of SN 2019np, a nearby SN Ia discovered within 1-2 days after t
Externí odkaz:
http://arxiv.org/abs/2205.15596
Autor:
Wang, Qinan, Rest, Armin, Zenati, Yossef, Ridden-Harper, Ryan, Dimitriadis, Georgios, Narayan, Gautham, Villar, V. Ashley, Magee, Mark R., Foley, Ryan J., Shaya, Edward J., Garnavich, Peter, Wang, Lifan, Hu, Lei, Bodi, Attila, Armstrong, Patrick, Auchettl, Katie, Barclay, Thomas, Barentsen, Geert, Bognár, Zsófia, Brimacombe, Joseph, Bulger, Joanna, Burke, Jamison, Challis, Peter, Chambers, Kenneth, Coulter, David A., Csörnyei, Géza, Cseh, Borbála, Deckers, Maxime, Dotson, Jessie L., Galbany, Lluís, González-Gaitán, Santiago, Gromadzki, Mariusz, Gully-Santiago, Michael, Hanyecz, Ottó, Hedges, Christina, Hiramatsu, Daichi, Hosseinzadeh, Griffin, Howell, D. Andrew, Howell, Steve B., Huber, Mark E., Jha, Saurabh W., Jones, David O., Könyves-Tóth, Réka, Kalup, Csilla, Kilpatrick, Charlie, Kriskovics, Levente, Li, Wenxiong, Lowe, Thomas B, Margheim, Steven, McCully, Curtis, Mitra, Ayan, Muñoz, Jose A., Nicholl, Matt, Nordin, Jakob, Pál, András, Pan, Yen-Chen, Piro, Anthony L, Rest, Sofia, Rino-Silvestre, João, Rojas-Bravo, César, Sárneczky, Krisztián, Siebert, Matthew R., Smartt, Stephen J., Smith, Ken, Sódor, Ádám, Stritzinger, Maximilian D., Szabó, Róbert, Szakáts, Róbert, Tucker, Brad E., Vinkó, József, Wang, Xiaofeng, Wheeler, J. Craig, Young, David R., Zenteno, Alfredo, Zhang, Kaicheng, Zsidi, Gabriella
Publikováno v:
The Astrophysical Journal, 2021, Volume 923, Number 2
We present the 30-min cadence Kepler/K2 light curve of the Type Ia supernova (SN Ia) SN 2018agk, covering approximately one week before explosion, the full rise phase and the decline until 40 days after peak. We additionally present ground-based obse
Externí odkaz:
http://arxiv.org/abs/2108.13607