Browse our catalogue of tasks and access state-of-the-art solutions. 2013, ApJ phase coverage:-14.6 to 17.3 d past B maximum wavelength coverage: 0.83 to 2.50 micron media: Gemini web feature Get the latest machine learning methods with code. Hsiao, E. Y. ORCID iD: 0000-0003-1039-2928. Along with the accompanying paper, Phillips et al. The La Silla/QUEST Variability Survey (LSQ) and the Carnegie Supernova Project (CSP II) are collaborating to discover and obtain photometric light curves for a large sample of low-redshift (z < 0.1) Type Ia supernovae (SNe Ia). Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program. The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supernovae (SNe Ia) as a function of redshift, and to set observational constraints on the dark energy contribution to the total energy content of the universe. Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events 2020 Author(s): Hsiao, EY We analyse four colours (B - V, u - g, g - r, and g - Y) and find that SN II colour curves can be described by two linear regimes during the photospheric phase. (2018), we introduce the Carnegie Supernova Project-II (CSP-II), to follow up nearby SNe Ia in both the optical and the NIR. Along with the accompanying paper, Phillips et al. 2015, A&A phase coverage:-12.8 to 35.1 d past B maximum wavelength coverage: 0.83 to 2.50 micron NIR spectra of SN 2011fe download: SpeX + GNIRS spectra paper: Hsiao et al. In particular, this paper focuses on the CSP-II NIR spectroscopy program, describing the survey strategy, instrumental setups, data reduction, sample characteristics, and future analyses on the data set. The SN reached a peak r-band absolute magnitude of ˇ19 mag and an even brighter UV peak, and its light curve evolution resembles that of SN 1988Z. We present a study of observed Type II supernova (SN II) colours using optical/near-infrared photometric data from the Carnegie Supernovae Project-I. This work was part of the Carnegie Supernova Project II, a National Science Foundation-funded program to observe supernovae. An analysis of the first set of low-redshift (z < 0.08) Type Ia supernovae (SNe Ia) monitored by the Carnegie Supernova Project between 2004 and 2006 is presented. 2019). the Carnegie Supernova Project II (CSP-II) beginning two days after discovery and extending until +887 days (d). (2020) "The Carnegie Supernova Project II. Taddia et al. Ashall, C. ORCID iD: 0000-0002-5221-7557. Along with the accompanying paper, Phillips et al., we introduce the Carnegie Supernova Project-II (CSP-II), to follow-up nearby SNe Ia in both the optical and the NIR. We analyse four colours (B - V, u - g, g - r, and g - Y) and find that SN II colour curves can be described by two linear regimes during the photospheric phase. We present a study of observed Type II supernova (SN II) colours using optical/near-infrared photometric data from the Carnegie Supernovae Project-I.We analyse four colours (B−V, u−g, g−r, and g−Y) and find that SN II colour curves can be described by two linear regimes during the photospheric phase. We present a study of observed Type II supernova (SN II) colours using optical/near-infrared photometric data from the Carnegie Supernovae Project-I. Although this object spectroscopically resembles the well-observed SN 2010jl, it does exhibit different LC evolution and dust signatures. We present optical and near-infrared (NIR) (ugriYJH) photometry of host galaxies of Type Ia supernovae (SN Ia) observed by the Carnegie Supernova Project-I. Along with the accompanying paper, Phillips et al., we introduce the Carnegie Supernova Project-II (CSP-II), to follow-up nearby SNe Ia in both the optical and the NIR. In particular, this paper focuses on the CSP-II NIR spectroscopy program, describing the survey strategy, instrumental setups, data reduction, sample characteristics, and future analyses on the data set. The Carnegie Supernova Project II (CSP2) is one such survey that aims at achieving very high precision photometry. NIR spectra of iPTF13ebh download: FIRE + SpeX + GNIRS spectra paper: Hsiao et al. CiteSeerX - Document Details (Isaac Councill, Lee Giles, Pradeep Teregowda): Abstract. (2018), we introduce the Carnegie Supernova Project-II (CSP-II), to follow up nearby SNe Ia in both the optical and the NIR. The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young, low-redshift supernovae between 2004 and 2009. Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events. Type Ia supernovae also provide the most powerful observational tool currently available for studying the expansion history of the universe and the nature of dark energy. lasting (1988Z-like) Type IIn SN 2014ab initiated by Carnegie Supernova Project-II (CSP-II; Phillips et al. 2015 as a part of the Carnegie Supernova Project-II (CSP-II; e.g., Phillips et al. Get the latest machine learning methods with code. Tip: you can also follow us on Twitter In particular, this paper focuses on the CSP-II NIR spectroscopy program, describing the survey strategy, instrumental setups, data reduction, sample characteristics, and future analyses on the data set. Observational signatures of AT 2014ej reveal that it is … Posted in: Science & Technology | Tagged: College of Arts and Sciences, Department of Physics, Eric Hsiao Post navigation. The Supernova Survey was a time-domain survey, involving repeat imaging of the same region of sky every other night, weather permitting. Browse our catalogue of tasks and access state-of-the-art solutions. (2020), “Carnegie Supernova Project-II: A New Method to Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program* E. Y. Hsiao ... 7 Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA 8 Department of Physics and Astronomy, Aarhus University, Ny Munkegade, DK-8000 Aarhus C, Denmark Hoeflich, P. Stritzinger, M. Show others and affiliations. Publications of the Astronomical Society of the Pacific, 131, 14002. The primary scientific motivation was to detect and measure light curves for several hundred supernovae through repeat scans of the SDSS Southern equatorial stripe 82 (about 2.5° wide by ~120° long). We therefore propose to embark on a long-term program, the Carnegie Supernova Project (CSP), with the goal of obtaining exceedingly-well calibrated optical/near-infrared light curves and optical spectroscopy of over 200 Type~Ia and Type~II supernovae. It is a five-year program that will obtain optical and near-infrared observations of 100-150 Type Ia supernovae located in the smooth Hubble flow. • Hsiao, Hoeflich, Ashall et al. 2006) by observing objects from untargeted searches detected in the Hubble flow. (2020) "The Carnegie Supernova Project II. Eric Y. Hsiao SN Workshop at IPMU, December 13, 2012 CSP2 ‣ We propose to carry out a second stage of the CSP with the goal of producing optical and NIR light curves of 100-200 SNe Ia in the redshift 2019; Hsiao et al. 2019); CSP-II was a National Science Foundation-supported program to study Type Ia SNe as distance indicators, which aimed to improve upon CSP-I (Hamuy et al. The Astrophysical Journal Letters, 875, 14. Presented in this paper is the CSP-I photometric data release of low-redshift stripped-envelope core-collapse supernovae. These observations are complemented with data from the CHilean Automatic Supernova sEarch, the Public ESO Spectroscopic Survey of Transient Objects, and from the Backyard Observatory Supernova Search. The Carnegie Supernova Project Supernovae are essential to understanding the chemical evolution of the universe. • Ashall, Lu, Burns, Hsiao et al. Carnegie Supernova Project-II: Using Near-infrared Spectroscopy to Determine the Location of the Outer Ni-56 in Type Ia Supernovae. Abstract. Carnegie Supernova Project-II: Using Near-infrared Spectroscopy to Determine the Location of the Outer 56Ni in Type Ia Supernovae. SN 2014ab serves as a new and important (2020), “Carnegie Supernova Project II: The slowest rising Type Ia supernova LSQ14fmg and clues to the origin of super-Chandrasekhar/03fg-like events”, ApJ, 900, 140. • Hsiao, E. Y. et al., 2019. CSP-II also worked to Carnegie Supernova Project II Eric Y. Hsiao. The data consist of well-sampled, high-precision optical (ugriBV) and near-infrared (NIR; YJHK{sub s} ) light curves in a well-understood photometric system. Tip: you can also follow us on Twitter We determine host galaxy stellar masses and, for the first time, study their correlation with SN Ia standardized luminosity across optical and NIR (uBgVriYJH) bands. 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