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. info ('Using existing %s egg: %s' % (project_name, setup_fn)) cmd. If the universe were gravity-dominated then it should be decelerating. DEBUG): cmd. What does CSP stand for? Sixteen years ago, NASA’s Galaxy Evolution Explorer (GALEX) spacecraft discovered a large, faint blob of gas with a star at its center—an object unlike anything previously seen in our Milky Way galaxy. Download PDF Package. Pasadena, CA— In a refurbished Southern California garage, Carnegie astrophysicists are creating the virtual reality-enabled scientific workspace of the future where they will unlock the mysteries of the cosmos. From 2014 to 2017 she was the Carnegie Origins Postdoctoral Fellow—a joint position between Carnegie’s Department of Terrestrial Magnetism (now part of EPL) and the Carnegie Observatories. 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. 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. A short summary of this paper. append ('-v') old_chdir = os. Using the tools developed in her Ph.D., Belin discovered a new role for actin in aiding the repair of DNA breaks in human cells caused by carcinogens, UV light, and other mutagens. where A, μ 1, μ 2, σ 1, and σ 2 are fixed at the following values derived from a training set of 74 SNe Ia observed in the optical (ugriBV) by the Carnegie Supernova Project (CSP), 54 of which also had NIR (YJH) coverage (see C. Burns et al. At the moment, the reality of the accelerating universe remains controversial because of possible errors in measuring these objects. Free PDF. The Carnegie Supernova Project has developed an analysis package, written in python, called SNooPy. 2013, in preparation, for further details): Phillip Cleves’ Ph.D. research was on determining the genetic changes that drive morphological evolution. Computing resources for this work were made possible by the Ahmanson Foundation. Johanna Teske became the first new staff member to join Carnegie’s newly named Earth and Planets Laboratory (EPL) in Washington, D.C., on September 1, 2020. The low-redshift portion of the Carnegie Supernova Project (CSP) seeks to remedy this situation by providing photometry and spectrophotometry of a large sample of supernovae taken on telescope/filter/detector systems that are well understood and well characterized. This material is based upon work supported by the National Science Foundation under Grants AST-0306969, AST-0607438, AST-1008343,  AST-1613426, AST-1613455, and AST-161347. We present an analysis of the final data release of the Carnegie Supernova Project I, focusing on the absolute calibration of the luminosity-decline rate relation for Type Ia supernovae (SNe Ia) using new intrinsic color relations with respect to the color-stretch parameter, s BV, enabling improved dust extinction corrections. Six years after its initial discovery—reported in The Astronomer’s Telegram by Carnegie’s Thomas Holoien—the researchers, led by Anna Payne of University of Hawai’i at Mānoa, can now say that the phenomenon they observed, called ASASSN-14ko, is a periodically recurring flare from the center of a galaxy more than 570 million light-years away in the. The Carnegie Supernova Project The recent discovery that the universe is expanding at an accelerating rate has profoundly affected physics. Download Full PDF Package. However, the presently available data sets of optical and near-infrared light curves of supernovae are relatively small and/or heterogeneous, and employ photometric systems that are poorly characterized. The CAPSCam planet search effort is on the verge of yielding a harvest of astrometrically discovered planets, as well as accurate parallactic distances to many young stars and M dwarfs. It will be constructed in the Las Campanas Observatory in Chile. The goal is to obtain highly calibrated optical/near-infrared light curves—measurements of the light intensity of these objects over time—and  their chemical signatures for over 200 Type~Ia and Type~II supernovae. Cleves returned to his passion for coral research in his postdoctoral work in John Pringles’ lab at Stanford. Highlights of this program include the detection of five of the first six exoplanets, the first eccentric planet, the first multiple planet system, the first sub-Saturn mass planet, the first sub-Neptune mass planet, the first terrestrial mass planet, and the first transit planet.Over the course of 30 years we have. SNooPy can therefore determine distances to … What is the abbreviation for Carnegie Supernova Project? append (setup_fn) if os. Similarly, there are relatively few supernovae whose spectral evolution has been well sampled, both in wavelength and phase, with precise spectrophotometric observations. 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. Supernovae are essential to understanding the chemical evolution of the universe. With over eight years of CAPSCam data, they are beginning to see likely true astrometric wobbles beginning to appear. Methods: Carnegie Supernova Project (CSP) optical and near-infrared light curves and visual-wavelength spectroscopy of the Type IIn SNe 2005kj, 2006aa, 2006bo, 2006qq, and 2008fq are presented. Using new genetic mapping and reverse genetic tools developed during his Ph.D., Cleves identified regulatory changes in a protein called bone morphogenetic protein 6 that were responsible for an evolved increase in tooth number in stickleback. get ('PYTHONPATH'): env ['PYTHONPATH'] = setup_fn + os. 37 Full PDFs related to this paper. For more see http://csp.obs.carnegiescience.edu/. We use the spectroscopy and homogeneous photometry of 97 Type Ia supernovae (SNe Ia) obtained by the Carnegie Supernova Project as well as a subset of 36 SNe Ia presented by Zheng et al. With a larger number of objects, an updated ﬁt to the Lira relation is presented along with path. Along with the accompanying paper, Phillips et al. exists (setup_fn): logger. The blob is represented as blue in the ultraviolet images of GALEX—although it doesn't actually emit. The supernova project is observationally intensive, not just requiring many nights of telescope time, but extensive data reduction, analysis, and interpretation as well. Our multi-national team has been collecting data for 30 years, using the Precision Doppler technique. of the Carnegie Supernova Project. Problems with Small Area Surveys: Lensing Covariance of Supernova Distance Measurements Asantha Cooray,1 Dragan Huterer,2 and Daniel E. Holz2,3 1Center for Cosmology, Department of Physics and Astronomy, University of California, Irvine, California 92697, USA 2Kavli Institute for Cosmological Physics and Department of Astronomy and Astrophysics, University of Chicago, CSP abbreviation stands for Carnegie Supernova Project. SNooPy2 has seen a number of changes that were motivated by making the installing process less painful (for you and me!). Astronomical Journal, 2009. READ PAPER. To ensure that an army of researchers are available there is a mentoring program for undergraduate and graduate-level students from within a broad and diverse pool of young people within California, and at universities in Arizona, Toronto, and Chile. A short summary of this paper. (2018), we introduce the Carnegie Supernova Project-II (CSP-II), to follow up nearby SNe Ia in both the optical and the NIR. Premium PDF Package. Campanas Observatory During the next 5 years the Low-Z Carnegie Supernova Project aims to obtain high-quality gap-free optical/NIR light-curves and spectro-photometry of ~220 nearby Type Ia, II, and Ibc supernovae, with the purpose to The Carnegie Supernova Project II is an NSF-funded, five-year program to obtain optical and near-infrared observations of 100-150 Type Ia supernovae located in the smooth Hubble flow. These concerns are being addressed with a comprehensive study of both Type Ia and II supernovae in the nearby universe with a long-term program called the Carnegie Supernova Project (CSP). It is a segmented mirror telescope that employs seven of today’s largest stiff monolith mirrors as segments. Her Ph.D. research involved developing new tools for in vivo imaging of actin in cell nuclei. It's fundamental use is for fitting TypeIa supernova light-curves using template derived from the CSP uBVgriYJH photometry. This paper. New work published in Nature by a Caltech-led team including Carnegie astrophysicists Mark Seibert and Andrew McWilliam revealed that the phenomenon is the extremely difficult-to-spot result of a stellar collision in which two stars merged into one. Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events Hsiao, EY Hoeflich, P We introduce a new light-curve parameter very similar to stretch that is better suited for fast-declining events, and ﬁnd that these peculiar types can be seen as extensions to the population of “normal” SNe Ia. PDF. SN(oo)py is a python package that contains many tools for the analysis of TypeIa supernovae. Pasadena, CA—New work from the Carnegie Supernova Project provides the best-yet calibrations for using type Ia supernovae to measure cosmic distances, which has implications for our understanding of how fast the universe is expanding and the role dark energy may play in driving this process.Led by Carnegie astronomer Chris Burns, the team’s findings are published in The Astrophysical Journal. I'm a research associate at the Carnegie Observatories and primarily work on the Carnegie Supernova Project.My research interests involve cosmology, the distance scale, inter-stellar dust, and applying numerical techniques to solve scientific problems. to examine maximum-light correlations in a four-dimensional (4D) parameter space: B-band absolute magnitude, M B, Si ii λ6355 velocity, ${v}_ {\mathrm {Si} {\rm\small {II}}}$, and Si ii pseudo-equivalent … 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. We present final natural-system optical (ugriBV) and near-infrared (YJH) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). environ. 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 The campus has just undertaken its new experiential. He also develops computational methods to derive fundamental principles of evolution, such as how fast natural populations acquire new mutations and how past climates shaped continental-scale biodiversity patterns. Formed 400 million years after the Big Bang, GN-z11 was previously determined by space telescope data to be the most-distant object yet discovered. getcwd if setup_fn is not None and os. The Carnegie Supernova Project (CSP) is aimed at providing an independent measure of change in the the Hubble expansion as a function of redshift, and setting constraints dark energy contribution to the total energy content of the universe. path. * The zero points (zp) are in the sense that m = -2.5log(F) + zp, where F is the photon flux through filter S X: ** The color terms are used to convert standard to natural photometry: Belin changed course for her postdoctoral work, in, Evolutionary geneticist Moises Exposito-Alonso joined the Department of Plant Biology as a staff associate in September 2019. Download Free PDF. The Carnegie Supernova Project (CSP) was a five-year observational survey conducted at Las Campanas Observatory that obtained, among other things, high-quality light curves of ~100 low-redshift Type Ia supernovae (SNe Ia). Download PDF. L. Contreras. The Astronomical Journal, 2010. The high-redshift CSP is aimed at providing an independent estimate of the dark energy contribution to the total energy content of the universe. Commissioning of the telescope is scheduled to begin in 2021. These contrary results suggest a new form of “dark energy”—some kind of repulsive force—is driving the universe. These students, with the postdoctoral fellows involved in this endeavor, will be involved in front-line research using first-class facilities. In doing so, a more coherent picture ascribing the variety of observed SNe IIn types to particular progenitor scenarios is sought. Pasadena, CA— The mysterious Blue Ring Nebula has puzzled astronomers since it was discovered in 2004. She uses observations to estimate exoplanet interior and atmospheric compositions, and the chemical environments of their formation. The Carnegie Supernova Project is supported by the U.S. National Science Foundation. Wendy Freedman. 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. The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae. Six off-axis 8.4 meter or 27-foot segments surround a central on-axis segment, forming a single optical surface 24.5 meters, or 80 feet, in diameter with a total collecting area of 368 square meters. Presented in this paper is the CSP-I photometric data release of low-redshift stripped-envelope core-collapse supernovae. Pasadena, CA—In a case of cosmic mistaken identity, an international team of astronomers revealed that what they once thought was a supernova is actually periodic flaring from a galaxy where a supermassive black hole gives off bursts of energy every 114 days as it tears off chunks of an orbiting star. Presented here is the second data release of nearby SN Ia photometry consisting of 50 objects, with a subset of 45 having near-infrared follow-up observations. The fund supports a postdoctoral fellowship in astronomy that rotates between the Carnegie Science departments of Terrestrial Magnetism in Washington, D.C., and the Observatories in Pasadena California. He used the emerging model organism, the stickleback fish, to map genetic changes that control skeletal evolution. For more see  http://instrumentation.obs.carnegiescience.edu/. He investigates whether and how plants will evolve to keep pace with climate change by conducting large-scale ecological and genome sequencing experiments. Our basic knowledge of supernovae comes from the study of their photometric and spectroscopic properties. She has been a NASA Hubble Fellow at the Carnegie Observatories in Pasadena, CA, since 2018. The Carnegie Supernova Project Supernovae are essential to understanding the chemical evolution of the universe. The work was undertaken as part of the Carnegie Supernova Project, a National Science Foundation-funded effort to study Type Ia supernovae, which are essential for understanding the chemical history of the universe, as well as fundamental to calculating the rate of its expansion. THE CARNEGIE SUPERNOVA PROJECT: FIRST PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE. A portal to fake universes may sound like science fiction, but it is now a reality at the Carnegie Observatories. It is not a fixed altorithm for fitting lightcurves, but rather a collection of tools that are useful for building your own fitter (or fitting interactively). These are specific types of exploring stars with exceptional luminosity that allow astronomers to determine distances and the acceleration rate at different distances. The Earthbound Planet Search Program has discovered hundreds of planets orbiting nearby stars using telescopes at Lick Observatory, Keck Observatory, the Anglo-Australian Observatory, Carnegie's Las Campanas Observatory, and the ESO Paranal Observatory. The recent discovery that the universe is expanding at an accelerating rate has profoundly affected physics. 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 (CSP) is one of several ongoing efforts to improve the quality of the low-redshift data. This work illustrated how molecular changes can generate morphological novelty in vertebrates. The Giant Magellan Telescope will be one member of the next class of super giant earth-based telescopes that promises to revolutionize our view and understanding of the universe. Actin is a major structural element in eukaryotic cells—cells with a nucleus and organelles —forming contractile polymers that drive muscle contraction, the migration of immune cells to  infection sites, and the movement of signals from one part of a cell to another. These contrary results suggest a new form of “dark energy”—some kind of repulsive force—is driving the universe. I have tried to update to the latest and most stable python modules and remove the cruft that was simply too difficult to run on modern … PDF. In two newly published Nature Astronomy papers, a team led by Linhua Jiang at the Kavli Institute for Astronomy and Astrophysics at Peking University took near-infrared spectra using ground-based telescopes that confirmed the galaxy’s distance. 9 Over the five-year period ending in 2009 May, the CSP has obtained densely sampled optical and near-infrared (NIR) light curves of ~100 SNe Ia in a well-understood, homogeneous photometric system (Hamuy et al. Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events - IOPscience The American Astronomical Society (AAS), established in 1899 and based in Washington, DC, is the major organization of professional astronomers in North America. Any opinions, findings and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation (NSF). Download Full PDF Package. His goal is to use these first principles and computational approaches to forecast evolutionary outcomes of populations under climate change to anticipate potential future, Mistaken identity: A presumed supernova is actually something much rarer, Most-distant galaxy helps elucidate the early universe, The “workspace of the future,” Carnegie’s VizLab will unlock the secrets of the universe, Carnegie Institution for Science, 1530 P Street NW, Washington DC 20005 P: (202)-387-6400 F: (202)-387-8092. If the universe were gravity-dominated then it should be decelerating. Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events Hsiao, EY Hoeflich, P Title: The Carnegie Supernova Project-I: Correlation Between Type Ia Supernovae and Their Host Galaxies from Optical to Near-Infrared Bands. Teske is interested in the diversity in exoplanet compositions and the origins of that diversity. The Cynthia and George Mitchell Foundation and Sheridan Lorenz supported several CSP workshops. PDF. 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. 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. The GMT, Along with Alycia Weinberger and Ian Thompson, Alan Boss has been running the Carnegie Astrometric Planet Search (CAPS) program, which searches for extrasolar planets by the astrometric method, where the planet's presence is detected indirectly through the wobble of the host star around the center of mass of the system. The GMT has a unique design that offers several advantages. 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