Pulsar Search Collaboratory

Slides:



Advertisements
Similar presentations
During the past few decades, scientists have discovered smaller sub- atomic particles that create the electrons, protons, and neutrons of an atom. As they.
Advertisements

Team Taylor Observations with the GBT Candidates When a plot or dataset looks like it has a unknown Pulsar, students submit it to one of the astronomers.
White Dwarf Stars Low mass stars are unable to reach high enough temperatures to ignite elements heavier than carbon in their core become white dwarfs.
Neutron Stars. Gradual compression of a stellar iron core  trans. [g cm -3 ] CompositionDegen. pressure Remarks Iron nuclei; nonrel. free e - nonrel.
1 Stellar Remnants White Dwarfs, Neutron Stars & Black Holes These objects normally emit light only due to their very high temperatures. Normally nuclear.
Team Presentation July 22, Jodrell Bank is the original arboretum for Manchester University. Immediately after World War II, first radio telescope.
How Do Astronomers Learn About the Universe?
Measuring Dispersion in Signals from the Crab Pulsar Jared Crossley National Radio Astronomy Observatory Tim Hankins & Jean Eilek New Mexico Tech Jared.
Neutron Stars and Black Holes
Neutron Stars and Pulsars Marcus Shinbo Melissa Onishi Astronomy Pd. 3 18, April, 2011.
Compact Objects Astronomy 315 Professor Lee Carkner Lecture 15.
Microwave: The Cosmic Microwave Background (CMB). Shortly after the Big Bang, the Universe cooled enough to allow atoms to form. After this point in time,
Compact Objects Astronomy 315 Professor Lee Carkner Lecture 15.
Compact Objects Astronomy 315 Professor Lee Carkner Lecture 15 “How will we see when the sun goes dark?” “We will be forced to grope and feel our way.”
Dakota Johnson, Tildon Johnson, Kyle Barker Rowan County Senior High School Mentor: Mrs. Jennifer Carter Abstract Data Analysis Acknowledgements Radio.
Announcements. Radio Astronomy of Pulsars Tiffany Pewett
Abstract Pulsars are highly magnetized, rotating neutron stars that emit a beam of electromagnetic radiation. The radiation can only be observed when the.
Intro Over this week, we observed using three telescopes (the 40ft, the 20m, and the GBT). We also analyzed pointings for candidates which we observed.
PSR J1400 – 1410 Jessica Pal Rowan County Senior High School Introduction Data Analysis Summary Acknowledgements Results A pulsar is a rapidly rotating.
Welcome to the Pulsar Search Collaboratory (PSC) – West! NRAO University Wisconsin – Milwaukee West Virginia University Yerkes Observatory University of.
1 Stellar Remnants White Dwarfs, Neutron Stars & Black Holes These objects normally emit light only due to their very high temperatures. Normally nuclear.
Hulse Team Pulsar Research Adam Kelsey, Consuela Hancock, Magaly Rosales, Cameron Deem, What Exactly Is A Pulsar? A pulsar is a rapidly spinning neutron.
Your Discovery is Here. The Pulsar Search Collaboratory.
Introduction “Tick, tock, tick, tock.” Clocks help keep us on schedule everyday, but how does our own galaxy keep in time? Pulsar’s are natures very own,
Looking at What We Can’t See: Pulsar Radio Observations ST 562 Radio Astronomy For Teachers By: Cecilia Huang and Joleen Welborn.
Team Lyne Conclusive Presentation Pulsar Search Collaboratory Heather Frank, Tyler Farrell, Annie B. Agee, Emily Dick, Trent McDaniel Caitlin Ahrens &
Who discovered the first pulsar? Jocelyn Bell Pulsars spin fast due to what physics concept?
Radio Waves Interaction With Interstellar Matter
JABAK Pulsar Data Analysis Introduction/Purpose When we arrived in Green bank, we did not know what a pulsar was. Now we know their identifying qualities.
Death of Stars II Physics 113 Goderya Chapter(s): 14
Team Hulse James J. Joshua M. Daniel P. Adam P. James M. Shane J.
Observational Properties Of Pulsars N'Diaye Maxime L3-PS.
Team Lyne Delaney Jeanine Pigott Elizabeth Leigh Schmitz Mariah Francine Gnegy Zachary Filmore Ramey Dana Marie Dawley Thomas Eugene Hillenbrand Team Mentor:
Pulsar Search Collaboratory Team Bell Cameron Meador Joey Martinez Erin Fankhanel Evan Graber April Liska Kriston Smith Teachers Mr.Weaver Mrs. Larew.
Light Introduction: Slide 1 Light Introduction. Light Introduction: Slide 2 Light -- an Electromagnetic Wave.
Gamma-Ray Emission from Pulsars
A pulsar is a supernova remnant which is a super dense, rapidly spinning neutron star which emits dipole electromagnetic radiation and features a strong.
Neutron Stars & Black Holes (Chapter 11) APOD. Student Learning Objective Indentify properties of Neutron Stars & Black Holes NASA.
Announcements Quiz 7 due tonight, practice problems in Problem Sets 7A, 7B Approximate schedule for this week: Today: Finish Chapter 12, Chapter 13 Remainder.
Units to read 67,68, 69, 70, 54.
Long-Term Timing of Globular Cluster Pulsars
The Legacy of Supernovae
Radio astronomy at Green Bank
Andy Marx Jason Granstedt Jeremy Thorley Robbie Culbertson
Pulsar Data Search Evaluation
Erin W Gunner H Anna D Shane C Carly L Shane S. Mentor: Sean
Team Taylor: John, Lori, Casey, Tonia, Joey, Elizabeth, and Lazar
An In-depth Analysis of Radio Astronomy
Earth Science 25.2B : Stellar Evolution
Energy Nuclear Fission Nuclear Fusion
Spiral Arms.
Parkes’ Potential Pulsars
Understand the electromagnetic spectrum and how it is organized.
White Dwarf Stars Low mass stars are unable to reach high enough temperatures to ignite elements heavier than carbon in their core become white dwarfs.
White Dwarf Stars Low mass stars are unable to reach high enough temperatures to ignite elements heavier than carbon in their core become white dwarfs.
Team Bell Pulsar Analysis
The Hunt for Pulsars Rowan County Pulsar Astronomers Abstract
Pulsar 3: Significant peaks, well above the noise
A beginning, middle and end
Pulsar Data II Single-Pulse Plots
Pulsar Data I 1.
The Death of a Star.
Team hulse pulsar collaboration
Disney Reaches for the Stars Pulsar Search Collaboratory
Understand the electromagnetic spectrum and how it is organized.
Pulsar Data II Single-Pulse Plots
Team Parkes PSC 2011.
The Death of a Star.
Tools and Technology of Space
Understand the electromagnetic spectrum and how it is organized.
Presentation transcript:

Pulsar Search Collaboratory Team Lyne ROCKS!

Introduction Pulsars are neutron stars They spin rapidly Strong magnetic fields Made from the implosion of a massive star Emit radio signals across the spectrum

Why Pulsars are Important! They are EXTREMELY accurate time keepers Can be used to study and understand space time Can help locate planets and other interstellar objects Help us understand relativity Allow us to study the physics of sub-atomic particles

Pulsar Search Collaboratory Last summer, GBT Drift Scan 130 Terabytes of data collected 30 Terabytes for students to analyze Goal: to locate unknown pulsars in the scan

Our Methodology Check Pulse Profile for regular peaks Check Phase for vertical bands Check Sub-Band for broad frequency Check DM for greater than zero and one peak Check Reduced X2 for signal

Other Phenomena RFI – Radio waves that are emitted on Earth that interfere with the radio telescope readings. Interstellar Noise – Caused by free electrons in the interstellar medium Solar Emissions traveling through space Remnants of Supernovas

What we have found/concluded! BJ

Shane

Katie

Laura

Drew

Questions?