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Astronomy & Astrophysics
C. Baltay, L. Grossman, R. Howard, D. Rabinowitz, I. Arcavi, N. Barbour, J. Burke, C. Contreras, B. Dilday, M. Graham, D. Hiramatsu, G. Hossenzadeh, D. A. Howell, C. McCully, R. McKinnon, K. Ment, R. Montesi, C. Pellegrino, S. Valenti
Summary: This paper presents the data release of a new sample of 140 type Ia supernovae from the LaSilla-QUEST/Las Cumbres Observatory (LCO) collaboration. The supernovae were discovered through various surveys and spectroscopically identified as SNe Ia, with light-curves obtained from rapid cadence photometric follow-up. Detailed analysis included precise galaxy background subtraction from the supernova magnitudes.
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
(2021)
Article
Astronomy & Astrophysics
D. O. Jones, W. D. Kenworthy, M. Dai, R. J. Foley, R. Kessler, J. D. R. Pierel, M. R. Siebert
Summary: We developed a SALT3 light-curve model that uses the host-galaxy masses of 296 low-redshift SNe Ia to derive a spectral energy distribution-host-galaxy mass relationship. The model showed that SNe in low-mass host galaxies have larger Ca ii H and K, Ca ii near-infrared triplet, and Si ii equivalent widths, indicating higher explosion energies per unit mass. However, the model did not substantially reduce data-model residuals for a typical light curve in our sample nor significantly reduce Hubble residual dispersion.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Alice G. Stone, Heather T. Johnson, John M. Blondin, Richard A. Watson, Kazimierz J. Borkowski, Carla Frohlich, Ivo R. Seitenzahl, Stephen P. Reynolds
Summary: The youngest Galactic supernova remnant, G1.9+0.3, exhibits highly asymmetric features, suggesting an asymmetric explosion. Simulation studies show that in the 2D model at the age of G1.9+0.3, almost no iron is observed, while in the 3D model some characteristics resemble those of G1.9+0.3.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
James D. Keegans, Marco Pignatari, Richard J. Stancliffe, Claudia Travaglio, Samuel Jones, Brad K. Gibson, Dean M. Townsley, Broxton J. Miles, Ken J. Shen, Gareth Few
Summary: In this study, complete abundance yields for 39 models of Type Ia supernova explosions were calculated based on three progenitors and 13 metallicities. The results show that the understanding of nucleosynthesis in Type Ia supernovae is influenced by different progenitor masses and compositions. The reliability of the results is further confirmed by comparing them with relevant models from previous literature.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2023)
Article
Astronomy & Astrophysics
J. M. Diego, G. Bernstein, W. Chen, A. Goobar, J. P. Johansson, P. L. Kelly, E. Mortsell, J. W. Nightingale
Summary: The observed magnifications and light curves of the quadruply imaged iPTF16geu supernova provide valuable insights into the lens system and suggest the need for contributions from microlensing structures. By combining macro and micro lens models, we find that higher stellar surface mass densities are preferred and conclude that microlensing from the baryonic component is sufficient to explain the observed flux ratios and light curves.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
S. Dhawan, A. Goobar, M. Smith, J. Johansson, M. Rigault, J. Nordin, R. Biswas, D. Goldstein, P. Nugent, Y-L Kim, A. A. Miller, M. J. Graham, M. Medford, M. M. Kasliwal, S. R. Kulkarni, Dmitry A. Duev, E. Bellm, P. Rosnet, R. Riddle, J. Sollerman
Summary: A sample of 761 spectroscopically classified SNe Ia from the first year of operations (DR1) of the Zwicky Transient Facility (ZTF) is reported. The sample has a median redshift (z) over bar = 0.057 and is already comparable in size to the entire combined literature low-z anchor sample. The median first detection is about 10 days earlier than the median in the literature.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Anirban Dutta, Avinash Singh, G. C. Anupama, D. K. Sahu, Brajesh Kumar
Summary: The study examines the optical and ultraviolet properties of Type Ia supernova SN 2017hpa, finding that it falls within the normal range for this type of supernova. Spectroscopic analysis reveals unique features in the evolution of SIII and CII absorption lines, providing insights into the composition and velocity gradients in the supernova ejecta.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Multidisciplinary Sciences
Erik C. Kool, Joel Johansson, Jesper Sollerman, Javier Moldon, Takashi J. Moriya, Seppo Mattila, Steve Schulze, Laura Chomiuk, Miguel Perez-Torres, Chelsea Harris, Peter Lundqvist, Matthew Graham, Sheng Yang, Daniel A. Perley, Nora Linn Strotjohann, Christoffer Fremling, Avishay Gal-Yam, Jeremy Lezmy, Kate Maguire, Conor Omand, Mathew Smith, Igor Andreoni, Eric C. Bellm, Joshua S. Bloom, Kishalay De, Steven L. Groom, Mansi M. Kasliwal, Frank J. Masci, Michael S. Medford, Sungmin Park, Josiah Purdum, Thomas M. Reynolds, Reed Riddle, Estelle Robert, Stuart D. Ryder, Yashvi Sharma, Daniel Stern
Summary: Through the study of SN 2020eyj, we discovered a type Ia supernova with helium-rich circumstellar material. Based on our modeling, we conclude that this circumstellar material likely originates from a single-degenerate binary system, which is a frequently proposed formation channel.
Article
Astronomy & Astrophysics
Yan-Hong Yao, Xin-He Meng
Summary: This paper investigates the impact of backreaction effects in the spatially averaged inhomogeneous Universe and proposes new effective sources for backreaction effects, namely the effective perfect fluid energy density and pressure. The backreaction models are fitted using two metrics, the Friedmann-Lemaitre-Robertson-Walker metric and a template metric with an evolving curvature parameter. The results show that there are significant parameter tensions between different data sets, indicating a need for modifications in the treatment of the geometrical instantaneous spatially-constant curvature.
PHYSICS OF THE DARK UNIVERSE
(2022)
Article
Astronomy & Astrophysics
N. Elias-Rosa, P. Chen, S. Benetti, S. Dong, J. L. Prieto, E. Cappellaro, J. A. Kollmeier, N. Morrell, A. L. Piro, M. M. Phillips
Summary: The study presented the spectrum and light curve characteristics of a Type Ia supernova SN 2016jae, identifying a narrow Hα emission line in its nebular-phase spectra, possibly originating from an expanding hydrogen-rich shell. This new observation provides insights into the evolution of such supernovae.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
John T. O'Brien, Wolfgang E. Kerzendorf, Andrew Fullard, Marc Williamson, Rudiger Pakmor, Johannes Buchner, Stephan Hachinger, Christian Vogl, James H. Gillanders, Andreas Flors, Patrick van der Smagt
Summary: A new probabilistic method for reconstructing the outer ejecta of Type Ia supernovae was proposed, utilizing machine learning to accelerate radiative transfer code for model evaluation. Analysis of the posterior distribution revealed a complex parameter space and degenerate models, with results favoring detonation scenarios and offering a novel way to compare simulations to observations.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Astronomy & Astrophysics
S. Dhawan, E. Morstell
Summary: The nature of dark matter and the possibility of it being comprised of primordial black holes are investigated using Type Ia supernovae. The fraction of dark matter in compact objects is constrained to be below 0.50 at 95% confidence level, demonstrating robustness to different cosmological models. With a prior assumption on the homogeneity parameter, it is found that the fraction of dark matter in primordial black holes is less than 0.32 at 95% confidence level. The study concludes that stellar mass primordial black holes cannot account for all of the observed dark matter.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
C. McCutcheon, Y. Zeng, Z-W Liu, R. G. Izzard, K-C Pan, H-L Chen, Z. Han
Summary: This study simulates the interaction between supernova ejecta and donor stars, finding that the choice of explosion model does not significantly affect the mass stripped and modal velocity of the ejected material.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
J. Johansson, S. B. Cenko, O. D. Fox, S. Dhawan, A. Goobar, V Stanishev, N. Butler, W. H. Lee, A. M. Watson, U. C. Fremling, M. M. Kasliwal, P. E. Nugent, T. Petrushevska, J. Sollerman, L. Yan, J. Burke, G. Hosseinzadeh, D. A. Howell, C. McCully, S. Valenti
Summary: The study presented optical and NIR observations of 42 Type Ia supernovae, and found no evidence for a mass step between color- and stretch-corrected peak J and H magnitudes for galaxies of different host stellar masses. The mass step remained significant at optical wavelengths when using a global R-V, but vanished when each SN was corrected using their individual best-fit R-V.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Benjamin E. Stahl, Thomas de Jaeger, WeiKang Zheng, Alexei Filippenko
Summary: The snapshot distance method is a modern technique for estimating the distance to SN Ia, allowing estimation from minimal observations through deep learning applied to spectra. By comparing with traditional methods, it demonstrates robustness relative to the temporal sampling of provided spectroscopic and photometric information, as well as standard light-curve shapes.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Shuang Wang, Sixiang Wen, Miao Li
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2017)
Article
Astronomy & Astrophysics
Shuang Wang, Sixiang Wen, Lanjun Zhou, Miao Li
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2017)
Article
Astronomy & Astrophysics
Xue Zhang, Qing-Guo Huang, Xiao-Dong Li
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2019)
Article
Astronomy & Astrophysics
Feng Fang, Jaime Forero-Romero, Graziano Rossi, Xiao-Dong Li, Long-Long Feng
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2019)
Article
Astronomy & Astrophysics
Jianming Zhang, Qiyue Qian, Yiqing Guo, Xin Wang, Xiao-Dong Li
Summary: The study investigates the role of gravitational waves in the heat death of the Universe, finding that they lead to energy dissipation in dynamical systems, transitioning to a state of rest and death. Energy loss due to gravitational wave emission in dark matter systems is estimated through N-body simulations, though the analysis may be invalidated by multiple unknown factors.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Ziyong Wu, Zhenyu Zhang, Shuyang Pan, Haitao Miao, Xiaolin Luo, Xin Wang, Cristiano G. Sabiu, Jaime Forero-Romero, Yang Wang, Xiao-Dong Li
Summary: Researchers have developed a deep learning technique to infer the nonlinear velocity field from the dark matter density field. Their analysis shows that neural networks may have an overwhelming advantage over perturbation theory in reconstructing velocity or momentum fields.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Shuren Zhou, Zhenjie Liu, Qinglin Ma, Yu Liu, Le Zhang, Xiao-Dong Li, Yang Wang, Xin Wang, Yu Yu, Hao-Ran Yu, Yi Zheng
Summary: This study investigates the impacts of massive neutrinos on the cosmic velocity fields and finds that the vorticity power spectra are highly sensitive to the mass sum of neutrinos, offering potential signatures for detecting massive neutrinos. The study also quantitatively tests the sensitivity of the density and velocity power spectra to the neutrino mass sum, with the vorticity spectrum showing the highest sensitivity. The results highlight the importance of peculiar velocity field measurements, particularly of vorticity and divergence components, in determining neutrino mass and mass hierarchy.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Yang Wang, Nicola R. Napolitano, Weiguang Cui, Xiao-Dong Li, Alexander Knebe, Chris Power, Frazer Pearce, Lin Tang, Gustavo Yepes, Xi Kang
Summary: This work presents a model to describe the star formation histories (SFHs) of individual galaxies from three simulations. The model divides SFHs into two components: the 'main sequence' and the 'variation', which are generated by tracing the history of the SFR-M-* main sequence and reproducing scatter around it using fractional Brownian motions. The study finds that the evolution of the main sequence varies between simulations, fractional Brownian motions can reproduce many features of SFHs but discrepancies still exist, and variations and mass-loss rate are crucial for reconstructing the SFHs of the simulations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Haitao Miao, Yan Gong, Xuelei Chen, Zhiqi Huang, Xiao-Dong Li, Hu Zhan
Summary: As a Stage IV space-based telescope, the China Space Station Telescope (CSST) efficiently explores the Universe through simultaneous photometric and spectroscopic surveys. This study investigates several powerful CSST cosmological probes and demonstrates their capability to significantly improve the precision of current observations. By including various surveys, CSST can achieve 1% accuracy in omega(m) and sigma(8), and 5% and 20% accuracy in w(0) and w(a) respectively. CSST's multi-probe surveys provide powerful tools for exploring the Universe and advancing cosmological research.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Liang Xiao, Zhiqi Huang, Yi Zheng, Xin Wang, Xiao-Dong Li
Summary: The tomographic Alcock-Paczynski (AP) method is a powerful tool for calibrating cosmology using the redshift evolution of anisotropic clustering. However, redshift errors can affect the resolution of nonlinear structure and contaminate the results. This study investigates how redshift errors propagate to cosmological parameters in tomographic AP analysis and finds that the method remains useful for future spectroscopic surveys.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Jiacheng Ding, Yunlei Huang, Xiao-Dong Li, Xin Wang, Yang Wang, Lili Yang
Summary: Since the discovery of neutrinos, their origin has remained a mystery until their association with TXS 0506+056. The recent publication of the fourth catalogue of active galactic nuclei (4LAC) has provided useful data to study these phenomena, particularly the blazars, which constitute the majority of the objects in the catalogue. By utilizing machine learning algorithms and deep learning techniques, researchers have achieved impressive success in classifying blazars, including the challenging task of classifying blazars of uncertain type (BCUs). The study also reveals a potential association between blazars and neutrinos, suggesting the possibility of using neutrinos as a feature for object classification in the future.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Cristiano G. Sabiu, Ben Hoyle, Juhan Kim, Xiao-Dong Li
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2019)
Article
Astronomy & Astrophysics
Xiaolin Luo, Shuang Wang, Sixiang Wen
ASTROPHYSICAL JOURNAL
(2019)
Article
Astronomy & Astrophysics
Xiao-Dong Li, Changbom Park, Cristiano G. Sabiu, Hyunbae Park, Cheng Cheng, Juhan Kim, Sungwook E. Hong
ASTROPHYSICAL JOURNAL
(2017)
Article
Astronomy & Astrophysics
Xiao-Dong Li, Cristiano G. Sabiu, Changbom Park, Yuting Wang, Gong-bo Zhao, Hyunbae Park, Arman Shafieloo, Juhan Kim, Sungwook E. Hong
ASTROPHYSICAL JOURNAL
(2018)