Zobrazeno 1 - 10
of 118
pro vyhledávání: '"Hsiao, Eric Y."'
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:
Wang, Lingzhi, Hu, Maokai, Wang, Lifan, Yang, Yi, Yang, Jiawen, Gomez, Haley, Chen, Sijie, Hu, Lei, Chen, Ting-Wan, Mo, Jun, Wang, Xiaofeng, Baade, Dietrich, Hoeflich, Peter, Wheeler, J. Craig, Pignata, Giuliano, Burke, Jamison, Hiramatsu, Daichi, Howell, D. Andrew, McCully, Curtis, Pellegrino, Craig, Galbany, Lluís, Hsiao, Eric Y., Sand, David J., Zhang, Jujia, Uddin, Syed A, Anderson, J. P., Ashall, Chris, Cheng, Cheng, Gromadzki, Mariusz, Inserra, Cosimo, Lin, Han, Morrell, N., Morales-Garoffolo, Antonia, üller-Bravo, T. E. M, Nicholl, Matt, Gonzalez, Estefania Padilla, Phillips, M. M., Pineda-García, J., Sai, Hanna, Smith, Mathew, Shahbandeh, M., Srivastav, Shubham, Stritzinger, M. D., Yang, Sheng, Young, D. R., Yu, Lixin, Zhang, Xinghan
Dust associated with various stellar sources in galaxies at all cosmic epochs remains a controversial topic, particularly whether supernovae (SNe) play an important role in dust production. We report evidence of dust formation in the cold, dense shel
Externí odkaz:
http://arxiv.org/abs/2310.14874
Autor:
Dong, Yize, Valenti, Stefano, Ashall, Chris, Williamson, Marc, Sand, David J., Van Dyk, Schuyler D., Filippenko, Alexei V., 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., 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.
Publikováno v:
ApJ 974 316 (2024)
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:
Uddin, Syed A., Burns, Christopher R., Phillips, Mark M., Suntzeff, Nicholas B., Freedman, Wendy L., Brown, Peter J., Morrell, Nidia, Hamuy, Mario, Krisciunas, Kevin, Wang, Lifan, Hsiao, Eric Y., Goobar, Ariel, Perlmutter, Saul, Lu, Jing, Stritzinger, Maximilian, Anderson, Joseph P., Ashall, Chris, Hoeflich, Peter, Shappee, Benjamin J., Persson, S. E., Piro, Anthony L., Baron, Eddie, Contreras, Carlos, Galbany, Lluís, Kumar, Sahana, Shahbandeh, Melissa, Davis, Scott, Anais, Jorge, Busta, Luis, Campillay, Abdo, Castellón, Sergio, Corco, Carlos, Diamond, Tiara, Gall, Christa, Gonzalez, Consuelo, Holmbo, Simon, Roth, Miguel, Serón, Jacqueline, Taddia, Francesco, Torres, Simón, Baltay, Charles, Folatelli, Gastón, Hadjiyska, Ellie, Kasliwal, Mansi, Nugent, Peter E., Rabinowitz, David, Ryder, Stuart D.
We present an analysis of Type Ia Supernovae (SNe~Ia) from both the Carnegie Supernova Project~I (CSP-I) and II (CSP-II), and extend the Hubble diagram from the optical to the near-infrared wavelengths ($uBgVriYJH$). We calculate the Hubble constant,
Externí odkaz:
http://arxiv.org/abs/2308.01875
Autor:
Wang, Qinan, Rest, Armin, Dimitriadis, Georgios, Ridden-harper, Ryan, Siebert, Matthew R., Magee, Mark, Angus, Charlotte R., Auchettl, Katie, Davis, Kyle W., Foley, Ryan J., Fox, Ori D., Gomez, Sebastian, Jencson, Jacob E., Jones, David O., Kilpatrick, Charles D., Pierel, Justin D. R., Piro, Anthony L., Polin, Abigail, Politsch, Collin A., Rojas-bravo, César, Shahbandeh, Melissa, Villar, V. Ashley, Zenati, Yossef, Ashall, C., Chambers, Kenneth C., Coulter, David A., De Boer, Thomas, Dilullo, Nico, Gall, Christa, Gao, Hua, Hsiao, Eric Y., Huber, Mark E., Izzo, Luca, Khetan, Nandita, Lebaron, Natalie, Magnier, Eugene A., Mandel, Kaisey S., Mcgill, Peter, Miao, Hao-yu, Pan, Yen-chen, Stevens, Catherine P., Swift, Jonathan J., Taggart, Kirsty, Yang, Grace
We present high-cadence ultraviolet through near-infrared observations of the Type Ia supernova (SN Ia) 2023bee in NGC~2708 ($D = 32 \pm 3$ Mpc), finding excess flux in the first days after explosion relative to the expected power-law rise from an ex
Externí odkaz:
http://arxiv.org/abs/2305.03779
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:
Yang, Yi, Baade, Dietrich, Hoeflich, Peter, Wang, Lifan, Cikota, Aleksandar, Chen, Ting-Wan, Burke, Jamison, Hiramatsu, Daichi, Pellegrino, Craig, Howell, D. Andrew, McCully, Curtis, Valenti, Stefano, Schulze, Steve, Gal-Yam, Avishay, Wang, Lingzhi, Filippenko, Alexei V., Maeda, Keiichi, Bulla, Mattia, Yao, Yuhan, Maund, Justyn R., Patat, Ferdinando, Spyromilio, Jason, Wheeler, J. Craig, Rau, Arne, Hu, Lei, Li, Wenxiong, Andrews, Jennifer. E., Galbany, Lluis, Sand, David. J., Shahbandeh, Melissa, Hsiao, Eric Y., Wang, Xiaofeng
A rare class of supernovae (SNe) is characterized by strong interaction between the ejecta and several solar masses of circumstellar matter (CSM) as evidenced by strong Balmer-line emission. Within the first few weeks after the explosion, they may di
Externí odkaz:
http://arxiv.org/abs/2211.04423
Autor:
Kumar, Sahana, Hsiao, Eric Y., Ashall, Chris, Phillips, Mark M., Morrell, Nidia, Hoeflich, Peter, Burns, Chris R., Galbany, Lluis, Baron, Eddie, Contreras, Carlos, Davis, Scott, Diamond, Tiara, Forster, Francisco, Graham, Melissa L., Karamehmetoglu, Emir, Kirshner, Robert P., Koribalski, Baerbel, Krisciunas, Kevin, Lu, Jing, Marion, G. H., Pessi, Priscila J., Piro, Anthony L., Shahbandeh, Melissa, Stritzinger, Maximillian D, Suntzeff, Nicholas B., Uddin, Syed A.
We present multi-wavelength time-series spectroscopy of SN 2013aa and SN 2017cbv, two Type Ia supernovae (SNe Ia) on the outskirts of the same host galaxy, NGC 5643. This work utilizes new nebular-phase near-infrared (NIR) spectra obtained by the Car
Externí odkaz:
http://arxiv.org/abs/2210.06993
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:
Hosseinzadeh, Griffin, Kilpatrick, Charles D., Dong, Yize, Sand, David J., Andrews, Jennifer E., Bostroem, K. Azalee, Janzen, Daryl, Jencson, Jacob E., Lundquist, Michael, Retamal, Nicolas E. Meza, Pearson, Jeniveve, Valenti, Stefano, Wyatt, Samuel, Burke, Jamison, Hiramatsu, Daichi, Howell, D. Andrew, McCully, Curtis, Newsome, Megan, Gonzalez, Estefania Padilla, Pellegrino, Craig, Terreran, Giacomo, Auchettl, Katie, Davis, Kyle W., Foley, Ryan J., Miao, Hao-Yu, Pan, Yen-Chen, Rest, Armin, Siebert, Matthew R., Taggart, Kirsty, Tucker, Brad E., Leung, Feng Lin Cyrus, Swift, Jonathan J., Yang, Grace, Anderson, Joseph P., Ashall, Chris, Benetti, Stefano, Brown, Peter J., Cartier, Régis, Chen, Ting-Wan, Della Valle, Massimo, Galbany, Lluís, Gomez, Sebastian, Gromadzki, Mariusz, Haislip, Joshua, Hsiao, Eric Y., Inserra, Cosimo, Jha, Saurabh W., Killestein, Thomas L., Kouprianov, Vladimir, Kozyreva, Alexandra, Müller-Bravo, Tomás E., Nicholl, Matt, Paraskeva, Emmy, Reichart, Daniel E., Ryder, Stuart, Shahbandeh, Melissa, Shappee, Ben, Smith, Nathan, Young, David R.
Publikováno v:
The Astrophysical Journal, 935:31 (23pp), 2022 August 10
We present high-cadence optical, ultraviolet (UV), and near-infrared data of the nearby ($D\approx23$ Mpc) Type II supernova (SN) 2021yja. Many Type II SNe show signs of interaction with circumstellar material (CSM) during the first few days after ex
Externí odkaz:
http://arxiv.org/abs/2203.08155