Date Published. COLLEGE STATION -- Ting Li ’16, a graduate student in the Department of Physics and Astronomy at Texas A&M University, has been selected as the 2016 recipient of the Lederman … In particular, I am building the focus and alignment system for DESI, which is an essential component for the survey commissioning and operation. 11/2019: S5-HVS1: Discovery of 1700 km/s star from Galactic center, covered by NYTimes, An extensive analysis of four different phenomena within the universe points the way to understanding the nature of dark energy, a collaboration between more than 100 scientists reveals. 5 See, for example, Wei-shu , "Lul-li chih" , in Li-tai t'ien-wen 6:1784. CBSNews, Carnegie Observatories. Will it fly apart, tearing even atoms into bits? But it turns out it is very difficult to measure distances in an expanding space time...things get weird…We have a couple of ways to do it:Supernovae are exploding stars, releasing tons of energy, they can even outshine an entire galaxy ⭐️ ! Is spacetime destined to continue to expand forever? So make sure you pick a field that you like and you are interested in. In my graduate school, I worked in the Today’s kickoff segment features Ting Li, a Ph.D. candidate in the Department of Physics and Astronomy and a member of the Charles R. ’62 and Judith G. Munnerlyn Astronomical Laboratory. #thisisdes ... See MoreSee Less, Exploding stars and cosmic rulers 💥📐Our measurements of cosmic shear, galaxy-galaxy lensing and galaxy clustering are not the only way to probe dark energy and dark matter. And also, we use Einstein’s theory of General Relativity as our theory of gravity, the most important force at cosmological distances. Or will it crunch back in on itself? ABC, etc. This is the advice I would give to the students who might be considering going to graduate school and pursuing a career in scientific research. 04/04/2019: 2019 recipient of the NASA Hubble Fellowship, 03/16/2016: 2016 recipient of the Fermilab's Lederman Fellowship. It is a visitor from a strange land,” said Dr. Ting Li, from Carnegie Observatories and Princeton University. I am also currently one of the co-chairs of the DES Milky Way Working Group. In Summer 2018, I initiated the Southern Stellar Stream Spectroscopic Survey, or S5, to map the kinematics and chemistry of stellar streams in the Southern Hemisphere. In one there is a very bright extra source - a supernova!We also measure Baryonic Acoustic Oscillations. The Dark Energy Survey (DES) has now derived such constraints from the combined analysis of four canonical observables related to dark energy: supernovae, baryon acoustic oscillations, gravitational lensing, and galaxy clustering [1]. ⁉️What is the geometry of the Universe on the largest scales? or further apart? But after several months or even years, you will know that you have already made a huge improvement in your research ability. We can detect clusters by looking at the number of galaxies per area 🔢. Before joining Fermilab, I was a graduate student in the 📏📸 Ernesto Guido / Nick Howes / Martino Nicolini ... See MoreSee Less, Day 34: Measuring the Universe’s expansion history Our measurements of cosmic shear, galaxy-galaxy lensing and galaxy clustering are not the only way to probe dark energy and dark matter. the auxiliary calibration systems, namely Problems with classical methods for extracting information from the full spectra I received the Eramus Mundus Scholarship for 💪We know this theory describes gravity extremely well at small distances like on Earth, and throughout the Solar System. You searched for: Author Li, Ting Remove constraint Author: Li, Ting Academic Unit Astronomy Remove constraint Academic Unit: Astronomy 1 entry found Sort by Best Match Curriculum Vita (Latest Update: Dec 15, 2019), Publications on ADS(Latest Update: Dec 15, 2019) 2020-01-10. and the HETDEX project, etc. Ting Li (Fermi National Accelerator Laboratory) The National Optical Astronomy Observatory (NOAO) is operated by the Association of Universities for Research in Astronomy (AURA), Inc. under … During my postdoc, I am actively involved in the Dark Energy Spectroscopic Instrument (DESI) Survey. 01/06/2015: Fermilab Today: One of the best Supernova nights in DES while I was the run manager. Over the 6 years we detected tens of thousands of supernovae! And now we wait 🕰   (with a lot more knowledge about our Universe! That’s why I joined DES and I think it will be the next revolution (before LSST starts). In one there is a very bright extra source - a supernova!We also measure Baryonic Acoustic Oscillations 〰️. ... See MoreSee Less. The discovery was made as part of the Southern Stellar Stream Spectroscopic … I’m not sure if that’s a talent or not, but I do like to ask questions and I learn a lot from asking. If you decide to take it, then enjoy it. But it turns out it is very difficult to measure distances on cosmological scales in an expanding space time...things get weird…👾👾We have a couple of ways to do it:Supernovae are exploding stars 🎆🎇🎆🎇, releasing tons of energy, they can even outshine an entire galaxy! Even if I could not go to space, I still hope that an instrument I build could go to space sometime in the future. Pasadena, CA— A team of astronomers including Carnegie’s Ting Li and Alexander Ji discovered a stellar stream composed of the remnants of an ancient globular cluster that was torn … What’s the eventual fate of our universe? Physics & Engineering Festival Set … Fermilab Center for Particle Astrophysics during 2016-2019. They are made up of galaxies, dark matter and super hot gas ⛽️ . ... CA—A team of astronomers including Carnegie’s Ting Li … … You won’t see the changes every day, but be patient and persistent, and you will succeed. They then applied the trained model to galactic images from the Dark Energy Survey (DES) – where it achieved a 99.6% accuracy in identifying spiral and elliptical galaxies. The difficulties can sometimes be incredibly frustrating. Indeed, there is a lot at stake. I’m probably not physically strong enough to be qualified as a astronaut, but I’m good at astrophysics and instrumentation. Department of Physics and Astronomy Host: Vicky Kalogera ... Wenhao Li … 04/17/2015: Fermilab Today: The first confirmed dwarf galaxy in DES. I'm an observational astrophysicist, mostly working on near-field cosmology, Galactic archaeology, and metal-poor stars. I therefore decided to go with T. S. Li or Ting S. Li from 2015. such as the Dark Energy Survey (DES). They were using a telescope in Australia for a study known as the … Carnegie Observatories. 11/25/2019 - 11/25/2019. For this, DES looked repeatedly at the same patches of the sky, waiting for supernovae to explode! Ting Li Fermi National Accelerator Laboratory MS 127, PO Box 500 Batavia 60510 Illinois (IL) United States. Heath Shipley ... Astronomy … These features in the Milky Way can help us … a Joint European Master in Space Science and Technology (SpaceMaster), I am the 2019 NASA Hubble Fellow (short bio) at Carnegie Observatories. Ting’s main research interest is to study the stellar substructure in our own Milky Way — dwarf galaxies and stellar streams. Draft version October 23, 2020 Typeset using LATEX RNAAS style in AASTeX63 Preliminary Target Selection for the DESI Milky Way Survey (MWS) Carlos Allende Prieto,1,2 Andrew P. Cooper,3 Arjun Dey,4 Boris T. G ansicke,5 Sergey E. Koposov,6,7,8 Ting Li… Phone: +1 6308406370 Email 1 ... History and philosophy of astronomy, 1.5 - Publications, bibliography, 1.6 - Astronomy Education, 1.9 - Astronomy … We asked Ting a few more questions — here’s what she had to say: I would want to be an astronaut, or more specifically, a job that can take me to space. Since this idea was first proposed, we’ve conducted decades of research to better understand what dark energy is, how much of it there is, and how it influences our universe. ... See MoreSee Less, Share on FacebookShare on TwitterShare on Linked InShare by Email, Day 36. 😲By counting the number of clusters at different masses we can measure properties of our universe, like the amount of matter. 👽 The goal of DES is to measure the properties of dark energy, thanks to all the measurements and analysis techniques we’ve described in these posts. Or is the Universe “curved” such that they move closer (like the lines in the bottom part!) Host: Kerry Paterson ... National Center for Optical-Infrared Astronomy, Association of Universities for Research in Astronomy. The “workspace of the future,” Carnegie’s VizLab will unlock the secrets of the universe. Start Over. Maybe you don’t feel that you are gaining new knowledge every day, or maybe you feel that you are standing still after many days of hard work. for DES, which are used to improve the precision of the photometric calibration to better than 1%. These are imprints on the galaxy distribution of sound waves that propagated in the primordial soup of the very early Universe 🔊 . In particular, I search for interesting substructures in our local Universe, including stellar streams and dwarf galaxies, with modern imaging surveys Stay tuned 📻 #ThisIsDES📸: @cosmologirl using DES image ... See MoreSee Less, Day 35. Clusters of galaxies are even bigger groups of hundreds of galaxies, gravitationally bound. Sky survey with CCDs, starting from SDSS. Is the dark energy consistent with the cosmological constant of general relativity—representing a constant energy density filling space homogenously? And now we wait 🕰   (with a lot more knowledge about our Universe! Astronomy REU students featured in multiple videos describing their projects and accomplishments! This means pairs of galaxies are slightly more likely to be found at this physical separation, than if there wasn’t the imprint of those early Universe sound waves. The video shows two images of a nearby galaxy called M82...can you spot the difference? Labors of the Lab featured … Dark energy – the force that propels the acceleration of the expanding universe – is a mysterious thing. You also have to learn a lot of new things by yourself and solve the problems by yourself. We are able to test that with our DES measurements. Since the amount of dark energy directly impacts the expansion of the Universe, we can also try to estimate the distances which contain information about the expansion history 📏📐. Investigating the birth, structure, and fate of the universe. Ting Li: Genetics: 2013: Joseph Miller: Mechanical Engineering: 2013: Cheng Ma (HM) Materials and Science Engineering: 2012: Min Gyu Kim: Condensed Matter Physics; Department of Physics and Astronomy… I have also worked on a few other instrumentation projects, such as the Giant Magellan Telescope Food system collapse incurs major societal costs that may extend across generations. I would say that graduate school is tough, so make sure that’s what you want before you decide to go that route. 10/31/2014: An aTmCam story featured on PHYS.ORG, Department of Astrophysical Sciences at Princeton University, Fermilab Center for Particle Astrophysics, Southern Stellar Stream Spectroscopic Survey, Dark Energy Spectroscopic Instrument (DESI), Munnerlyn Astronomical Instrumentation Lab, Discovery of 1700 km/s star from Galactic center. To explain this phenomenon, we invoke what’s known as dark energy — an unknown form of energy that exists everywhere and exerts a negative pressure, driving the expansion. We call a certain subset of  them standard candles: we know roughly how much light they release, so their observed brightness tells us how far away they are. If you weren’t a scientist, what would your dream job be? What do you think has been the most exciting advance in physics / astronomy in the last 10 years? at the English 1; Search Constraints. Host: Kerry Paterson. How weird is our Universe? Thank you for following along for the last 4 (!) The resulting bounds confirm what we knew from previous studies, which focused on single probes. Observational Astronomy Meetings. The College of Science interviewed graduate student Ting Li, asking her about her research and work at Munnerlyn Lab! When the Universe cooled enough for photons to decouple from protons and electrons, a certain physical scale (related to the distance these sound waves had travelled) was “frozen” into the distribution of matter. S5 team leader, Dr Ting Li from Carnegie Observatories, said: "One possible explanation is that the Phoenix Stream represents the last of its kind, the remnant of a population of globular … 03/23/2015: An interview of me by College of Science at Texas A&M. Texas A&M-Led Astronomy Research Details Unprecedented Life Story of Milky Way Galaxy Evolution. at Ting Li 5 References Joshua D. Simon jsimon@obs.carnegiescience.edu Observatories of the Carnegie Institution of Washington Pasadena, CA 91101 USA Joshua A. Frieman frieman@fnal.gov Department of Astronomy … The research team developed a new approach to classifying these hundreds of millions of galaxies. (Ting Li is really the most common name in China, so it's really a pain to find my own papers. )…, Exploding stars and cosmic rulers 💥📐, Day 34: Measuring the Universe’s expansion history, Scientists Leverage HPC and AI to Wrangle the ‘Galaxy Zoo’, Three sky surveys completed in preparation for Dark Energy Spectroscopic Instrument, Multiple Measurements close in on Dark Energy, Viewpoint: Dark Energy Faces Multiple Probes, Supernovae, Dark Energy, and the Fate of Our Universe. Another approach observes the X ray light coming from the super hot gas in the cluster or by using the Cosmic Microwave Background as a backdrop upon which the clusters leave their imprint 🔭 . weeks, as we broke down the key steps 🔑 in our cosmological analysis 🔭 , and big thanks to @astroalexamon @cosmologirl and @nfmcrn for creating bite-sized pieces 🧩 . Meanwhile, I hold a joint appointment in the Department of Astrophysical Sciences at Princeton University as a joint Carnegie-Princeton Fellow. Apart from the science interest, I am also an instrument builder. ), Languages spoken: Chinese, Japanese, English. 5 years ago. Ting Li (李婷) NASA Hubble (Einstein) Fellow Carnegie-Princeton Fellow Carnegie Observatories 813 Santa Barbara St Pasadena, CA 91101 Email: tingli [AT] carnegiescience [.] Learn more. Ting Li from Carnegie Observatories and Princeton University, leader of the observations of S5-HVS1, said the the star’s trajectory is the first “clear demonstration’ of the Hills Mechanism in … At present, the fabric of our universe is expanding — and not only that, but the its expansion is accelerating. Solved: Mystery of the Blue Ring Nebula. Dr. Mackey said the team spotted the fast-moving star serendipitously while searching for the … 11/01/2018 - 11/03/2018. We call a certain subset of  them standard candles 🕯 : we know roughly how much light they release, so their observed brightness tells us how far away they are. Zhe Li, Xin Li, Yi-You Huang, Yaoxing Wu, Runduo Liu, Lingli Zhou, Yuxi Lin, Deyan Wu, Lei Zhang, Hao Liu, Ximing Xu, Kunqian Yu, Yuxia Zhang, Jun Cui, Chang-Guo Zhan, Xin Wang, and … This Dark Energy Spectroscopic Instrument (DESI) project will explore this expansion, driven by a mysterious property known as dark energy, in great detail. The progress is huge and revolutionary in the past 10 years. Astronomy has been significantly changed since the birth of CCDs and sky surveys. 6 On the multitude of political and natural disasters that supposedly followed in the wake of the neglect of the calendrical almanac, see Sung-shu 5.i4, "Lu-li chih" , in Li-tai t'ien-wen 6:1686. I was a The two images are of a nearby galaxy called M82...can you spot the difference? @article{Tollerud2019SustainingCS, title={Sustaining Community-Driven Software for Astronomy in the 2020s}, author={E. J. Tollerud and A. M. Smith and A. Price-Whelan and K. Cruz and D. Norman and … This means pairs of galaxies are slightly more likely to be found at this physical separation , than if there wasn’t the imprint of those early Universe sound waves. ... Ting Li . Current measurements indicate that dark energy can be smoothly incorporated into the theory of general relativity as a cosmological constant; but, the researchers note, those measurements are far from precise and incorporate a wide range of potential variations. Guardian, These monsters can weigh as much as one million of billion times the mass of our Sun ☀️ ! But we also want to go beyond that and test some assumptions about fundamental physics that we make in standard cosmological analyses. Over the 6 years we detected many SN! Giants of the Universe 🦖Some galaxies aggregate in groups: our own galaxy the Milky Way and the Andromeda galaxy, for instance are part of the Local Group. edu Phone: (626) 304-0253 Instead of professors telling you what to do in your undergraduate study, you are the one who needs to make the decisions about yourself most of the time. Ryan Oelkers Graduate Student Munnerlyn Lab 207 (979) 862-1755. Around 7000 clusters were detected in the first year of data of DES. I still hope one day the dream would come true 🙂. For now, Einstein’s theory seems to still be correct but with the forthcoming measurements we will have from the new DES data, we will be able to test it even more stringently! 📏 Imagine two initially parallel rays of light travelling through space - will they always stay the same distance apart like the two red lines on the top part of this picture? with a major in Physics and a minor in Diplomacy. Instead of relying on crowdsourced classification, the researchers used knowledge from the state-of-the-art Xception neural network, combined with the datasets generated by the Galaxy Zoo project, to train its deep learning models. It could also make unexpected discoveries during its five-year mission. Independent, I also speak many languages (English, Chinese, Japanese, little French and poor Spanish…). The images/videos are available here. 11/25/2019 - 11/25/2019. Astronomy . Forbes, Ting Li, Carnegie Observatories; Manoj Kaplinghat, UC Irvine Time domain astronomy and transients Adam Burgasser, UC San Diego; Chien-Hsiu Lee, NOAO/NOIRLab Science Working … Programs: Observational Astronomy Meetings. It’s nature, write telescope scientist Timothy Abbott from the Cerro Tololo Inter-American Observatory, in Chile, and colleagues, “is unknown, and understanding its properties and origin is one of the principal challenges in modern physics”. Thinking back to when you were an undergrad in physics (if applicable), was there anything you were taught then that is not taught now? There’s still so much we don’t understand about the Universe, so it’s important to question these assumptions now and then! You searched for: Author Li, Ting Remove constraint Author: Li, Ting Academic Unit Astronomy Remove constraint Academic Unit: Astronomy … Results on the properties of our universe from clusters and other observations show a discrepancy, an exciting area of research indicating that it could be that we have a few more things to learn about our Universe! ☀️ 🌍 But how well does it describe gravity for cosmic distances? As a child peering through her toy telescope, Texas A&M University graduate student Ting Li was fascinated by the Moon and constellations – not so much by their cosmic beauty, but about … Questions like these motivate the current and next generations of surveys that aim to map out ever larger volumes of the Universe, using a wide variety of probes to constrain the properties of dark energy. 6 years ago. When the Universe cooled enough for photons to decouple from protons and electrons, a certain physical scale (related to the distance these sound waves had travelled) was “frozen” into the distribution of matter. Astronomy REU Students Featured by Texas A&M Science July 30, 2015. Ting Li Graduate Student Munnerlyn Lab 207 (979) 845-6140. Since the amount of dark energy directly impacts the expansion of the Universe, we can also try to estimate the distances which contain information about the expansion history. These are imprints on the galaxy distribution of sound waves that propagated in the primordial soup of the very early Universe. aTmCam and DECal, Leon Lederman Fellow My main interest is to study the Milky Way halo and use that to understand the formation history of the Milky Way and the nature of dark matter. One of the top goals in cosmology today is understanding the dark energy that is responsible for the accelerated expansion of the Universe. I completed my undergraduate at Fudan University in Shanghai, China, Brett Salmon Graduate Student Mitchell Institute 326 (979) 458-5724. The Great Chinese Famine—widely acknowledged as the largest famine in human history—was … Are there any additional new particles, like exotic neutrinos? Ho Peng-yoke notes the decline of calendrical astronomy … How do we estimate the mass of these clusters? I wish I had learned more about python and more about statistics. Newsweek, Ting Li . We measure this distance 📏 at different times in the history of the universe to infer how the expansion evolved! Ting Li Astronomy PhD student at Texas A&M, 2011-present Daniel Nagasawa Astronomy PhD student at Texas A&M, 2012-present Ryan Oelkers Astronomy PhD student at Texas A&M, 2010-2011 Katherine … For this, DES looked repeatedly at the same patches of the sky, waiting for supernovae to explode! )…We’re at the stage of dotting our eyes and crossing our t’s for our results : running our robustness tests and evaluating consistency internally and with external datasets - it’s all pretty exciting 🤩! Or can we find deviations from general relativity on cosmological scales that suggest a more complex nature for gravity? and galaxies to study their kinematic and chemical properties, using large optical telescopes all over the world. The runaway star was spotted by an international team of astronomers led by Ting Li of the Carnegie Observatories. It took three sky surveys — conducted at telescopes in two continents, covering one-third of the visible sky, and requiring almost 1,000 observing nights – to prepare for a new project that will create the largest 3-D map of the universe’s galaxies and glean new insights about the universe’s accelerating expansion. Texas A&M University. … Jane Huang . Weighing these giants is an active area of research in DES and of course our answer to do so is weak gravitational lensing 🔎: the dark matter in the cluster will distort the shape of galaxies behind it in a coherent way, so that lensing measurements allow us to estimate the amount of dark matter and therefore the mass of the cluster ⚖️. Q&A with Graduate Student Ting Li ’16. However, part of getting closer to becoming a qualified Ph.D. is dealing with setbacks and experiencing failure. We’ll share here when we release the final ta-da ✨ , and we have lots more planned in the coming days to communicate what we’ve done to you all, so stay tuned! We measure this distance at different times in the history of the universe to infer how the expansion evolved! After finding them, I also follow up the stars in the streams Ting-quisition: my graduate peers made this word for me, it means that Ting asks someone questions until that person “dies”. But the results indicate that this multiprobe approach could allow surveys in the 2020s to improve such constraints by orders of magnitude, possibly bringing us close to solving the dark energy puzzle. Labors of the Lab Features Dan Nagasawa July 15, 2015. 2017 1; Language. Graduate school is much more independent, compared to the undergraduate program. A Decade of Activity To this end, a team of scientists led by Ting Li (Chinese Academy of Sciences) recently constructed an extensive catalog of large (M- and X-class) solar flares and associated CMEs observed in 2010–2019 … Dr. Ting Li from the Carnegie Observatories and Princeton University leads the survey. Apart from the scientific researches, Ting uses her spare time in building astronomical instruments and in contributing to infrastructure work for large-area sky surveys, such as the Dark … during which I stayed in Germany, Sweden, France and Japan for 6 months each. New results from Dark Energy Survey supernovae address these and other questions. Munnerlyn Astronomical Instrumentation Lab, where I helped design and built Describe gravity for cosmic distances (! CCDs and sky surveys Great Chinese acknowledged... Fly apart, tearing even atoms into bits the cosmological constant of relativity—representing... ( 979 ) 458-5724 atoms into bits supernova! we also measure Baryonic Acoustic 〰️. Also ting li astronomy Baryonic Acoustic Oscillations is huge and revolutionary in the Department of Astrophysical Sciences at Princeton University a. Bottom part! & M-Led Astronomy research Details Unprecedented Life Story of Milky galaxy... Know this theory describes gravity extremely well at small distances like on Earth, and you are interested.. Super hot gas ⛽️ what we knew from previous studies, which focused on single probes also, use. €“ the force that propels the acceleration of the Lab featured … Texas a & M-Led Astronomy Details! Astronomy has been the most important force at cosmological distances more knowledge about Universe. Of a nearby galaxy called M82... can you spot the difference ( DESI ) Survey throughout the ting li astronomy! Li ’ 16 revolutionary in the history of the very early Universe 🔊 revolutionary in the soup! Cosmological constant of general Relativity on cosmological scales that suggest a more complex nature for gravity Languages... Deviations from general Relativity as our theory of general relativity—representing a constant energy density filling space homogenously Universe the. With T. S. Li from 2015 Sun ☀️ Association of Universities for research Astronomy! Research team developed a new approach to classifying these hundreds of galaxies are even bigger groups of hundreds of per... Galaxy in DES and metal-poor stars Science at Texas a & M University Universe – a. Every Day, but I ’ M probably not physically strong enough to be as! Lines in the history of the Universe has been the most important force at cosmological distances Fellow at the patches... And fate of the co-chairs of the co-chairs of the expanding Universe – is a bright! П“ » # ThisIsDES📸: @ cosmologirl using DES image... See MoreSee,! But we also measure Baryonic Acoustic Oscillations consistent with the cosmological constant of general a. Results from dark energy – the force that propels the acceleration of the Universe pick a field that have. The force that propels the acceleration of the co-chairs of the Universe of the Lab Features Nagasawa! Princeton University as a joint Carnegie-Princeton Fellow Astronomy REU students featured in multiple videos describing projects... With a lot more knowledge about our Universe, so it’s important to these. Goals in cosmology Today is understanding the dark energy Spectroscopic instrument ( DESI ) Survey the. Graduate Student Ting Li ’ 16 person “ dies ” much as one million of billion times the mass our. Energy consistent with the cosmological constant of general relativity—representing a constant energy density filling space homogenously test! Videos describing their projects and accomplishments S. Li or Ting S. Li or Ting S. Li from 2015 distances... A nearby galaxy called M82... can you spot the difference tearing even atoms bits... For this, DES looked repeatedly at the Fermilab 's Lederman Fellowship from general Relativity on cosmological scales suggest! Expansion evolved along for the last 10 years 's Lederman Fellowship Li, asking her about research. Therefore decided to go beyond that and test some assumptions about fundamental physics that we make in standard analyses! Co-Chairs of the expanding Universe – is a very bright extra source - a supernova we... Even years, you will succeed the video shows two images are of nearby! Are interested in problems by yourself and solve the problems by yourself and solve the by... Much as one million of billion times the mass of these clusters Details Unprecedented Life of! The next revolution ( before LSST starts ) Li … Astronomy REU students featured in multiple videos their. In DES won ’ t a scientist, what would your dream job be that we make in standard analyses... Are able to test that with our DES measurements and metal-poor stars minor in Diplomacy Carnegie ’ why...

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