Deep Space Exploration Society

Slides:



Advertisements
Similar presentations
PAPER’s Sweet Sixteen: Imaging the Low Frequency Sky with a Sixteen Element Array Nicole Gugliucci for the PAPER Team* USNC/URSI National Radio Science.
Advertisements

This absorption line was found on November 19 th at right ascension 18:23:00 and declination 13:09:00. In this example, the data taken by the BON database.
Team Presentation July 22, Jodrell Bank is the original arboretum for Manchester University. Immediately after World War II, first radio telescope.
Pulsating Pulsars: Adventures Outside the Gridding Iron Susan Booth (VAST), Nick Borowicz (Argo Community HS, Summit, IL), Rob Culbertson (Langley HS,
Photo by Serge Bruneil
Submillimeter Data for SINGS George J. Bendo & Robert D. Joseph (A ''George's Adventures in Learning OpenOffice'' Presentation)
B RA:16:45 DEC: -03:17 DM: We used a known pulsar to practice on. You have to do a practice pulsar to make sure that the computers and equipment.
What does do? Mini-project for CSE 260 Qian Peng 15 November 2001 Ref.
Problem 3.1. Plot of raw data R-chart What about subgroup 8? Raw data indicates a possible outlier. May also be isolated special cause. Check measurement.
PHY134 Introductory Astronomy
Various Techniques for Measuring Astronomical Distances Alex Blanton 1.
Part 5: The Galaxy and the Universe In this final part of the course, we will: 1. Look at the big spatial picture: Are there organizations of stars? What.
Andromeda and the Dish by Angelica Vialpando Jennifer Miyashiro Zenaida Ahumada.
Pulsing Prizes By: Kyle Wenger and Megan Weaver, (Broadway High School, Broadway, VA) How old might they be? Using the ATNF catalog we have approximated.
Constellation Notes. Constellations Day 1 Objective: You will use critical thinking skills in order to differentiate between astronomy and astrology.
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.
Astronomy II - SeeS Galaxies and Distant Objects.
Astronomy 1001 Lecture 1 5/30/07. The Moon Project Goal: understand how the moon “works” –Measure Lunar month, explain phases, connect actual observations.
THE MILKY WAY Intro Info.
Stars, Suns, and Moons. A spherical object in space made up of Hydrogen, Helium (or other gases), and that gives off its own light is called a A: moon.
(there’s no place like home) The Milky Way Galaxy.
Unit I - Lesson I “Foundations of Astronomy” Astronomy.
Mapping the Stars Section 1-3 Summary. Patterns in the sky Constellations: sections of the sky that contain recognizable star patterns – Today scientists.
Planet A large, round celestial object that travels around a star – example: Earth.
© 2011 Pearson Education, Inc. Chapter 1 Charting the Heavens.
How big is big?.
Preliminary Baseline 420 MHZ Celestial Drift Scan Survey
SARA Conference Meter Dish Demo
Finding the next Galactic extragalactic FRB
Lecture 30- The Structure of the Milky Way Galaxy
EDGES: The ‘Global’ Perspective
Part 5: The Galaxy and the Universe
Do Now On the back of the notes, write down three things that you know about the universe.
The basic structural unit of the universe appears to be the galaxy.
Charting the Heavens.
The Structure of the Milky Way
Completed Star Chart – Virgo Galaxy Cluster
Probing Magnetized Turbulence in the Fermi Bubbles
Andy Marx Jason Granstedt Jeremy Thorley Robbie Culbertson
What do the pictures represent?
Erin W Gunner H Anna D Shane C Carly L Shane S. Mentor: Sean
The Universe Chapter 25.3.
ASTRONOMY 181. ASTRONOMY 181 The SPECIAL Theory of RELATIVITY.
Natural Sciences Grade 7
Natural Sciences Grade 7
An In-depth Analysis of Radio Astronomy
Pulsar Search Collaboratory
Astronomy Picture of the Day – 16 Jul 06
Annual Members Meeting
Learning Goals: I will:
Parkes’ Potential Pulsars
Gyrochronology: Aging Nearby, Debris Disk Candidate Stars
What is Astronomy? An overview..
The Hunt for Pulsars Rowan County Pulsar Astronomers Abstract
Deep Space Exploration Society
Homework: Due at Midnight
20.2 The Milky Way and Other Galaxies
Study Guide 3-2 Milky Way Universe Exploration
Pulsar Data II Single-Pulse Plots
Lecture 33- What’s the Milky Way made of?
GALAXIES Pages
Describe the overall scale and structure of the universe.
Pulsar Data II Single-Pulse Plots
IN A WORLD FAR, FAR, AWAY…….
Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic.
Star Notes.
What is Astronomy? An overview..
After Bellwork, Read the FYI on the “Cosmological Distance Ladder” then answer the two questions in your science journal.
Describe the overall scale and structure of the universe.
Introduction You are an astronomer who has just made this image. As you study this image, what questions do you ask? Elicit answers from your audience.
Presentation transcript:

Deep Space Exploration Society Science Meeting 9-24-2018

Agenda Overview of 2018 Radio Astronomy Guide Overview of this weekends observations

Deep Space Exploration Society 2018 Radio Astronomy Guide Revision 2 Overview

September 22, 2018 Observation Trip

Observation Trip 9-22-18 Observers: Gary Agranat, Jay Wilson, Richard Russel Receiver: SpectraCyber with 1420 Mhz. Cavity Filter on 60-foot dish Pointing System: System 1 Special Thanks to DSES President Steve Plock for setting up for the observation team!

Dish Photos

SpectraCyber Data

Lots of Notes

Results

Target: 3C274 (Calibration Source: 203 JY) RA: 12h28m DEC: 12 39m File: 18 47 14 UTC 3

Target: NGC 5457 Galaxy RA: 14h03m DEC: 54° 39m File: 19 38 28 UTC 1

Target: Unknown RA: 14h51m23s DEC: 44° 40m File: 19 58 41 UTC 3

Target: Unknown RA: 14h57m DEC: 42°35m File: 20 03 19 UTC 2

Target: 3C286 (Calibration Source: 14 Target: 3C286 (Calibration Source: 14.68 JY) RA: 13h29m12s DEC: 31° 12m File: 20 24 46 UTC 6

Target: Centaurus A RA: 13h23m DEC: -41° 10m File: 20 40 50 UTC 1

Target: Virgo A RA: 12h29m DEC: 12° 28m File: 21 10 16 UTC 10

Target: Unknown RA: 14h51m DEC: -6° 21m File: 21 37 10 UTC 1

Target: Unknown RA: 14h59m DEC: -46° 20m File: 21 45 46 UTC 9

Scan Across Declination -28°45m (approximate) This crosses Milky Way and SAG A* RA: 15h15m RA: 15h30m RA: 15h45m RA: 16h00m RA: 16h15m RA: 16h30m RA: 16h45m RA: 17h00m

Scan Across Declination -28°45m (approximate) This crosses Milky Way and SAG A* RA: 17h15m RA: 17h30m RA: 17h45m RA: 18h00m RA: 18h15m RA: 18h30m RA: 18h45m RA: 19h00m

Scan Across Declination -28°45m (approximate) This crosses Milky Way and SAG A* RA: 19h15m RA: 19h30m RA: 19h45m RA: 20h00m

Source: Seasonal Star Chart : Hubbard Scientific 2007 7.5 7.5 8.0 6.0 7.0 6.0 5.7 6.6 9.5 10.0+ 10.0+ 10.0 9.6 8.5 8.6 7.5 8.5 6.0 6.0 5.5 Source: Seasonal Star Chart : Hubbard Scientific 2007

Galactic Rotation Rate Data Gal Lat Gal Long RA DEC AZ EL File: UTC 17h45m37s -28d56m10s 162 205 23 10 39: UTC 2 10 18h07m46s -20d17m24s 154 27 23 10 39: UTC 14 20 18h27m32s -11d29m19s 146 33 23 10 39: UTC 25 30 18h46m05s -02d36m33s 138.6 40.25 23 10 39: UTC 37 40 19h04m23s 06d17m14s 125.6 44.3 23 10 39: UTC 50

Galactic Rotation Rate Data GLAT: 0 GLONG: 0 GLAT: 0 GLONG: 10

Galactic Rotation Rate Data GLAT: 0 GLONG: 20 GLAT: 0 GLONG: 30

Galactic Rotation Rate Data GLAT: 0 GLONG: 40

Summary The raw data collected during the observation trip will be analyzed The calibration sources did not show any signal above the noise. This may indicate that the noise level is at least 203 JY which was the highest signal calibration source attempted. (3C274) The one galaxy (NGC5457) observation did not appear per the observation guide. A number of unknown signals were present that were not in the guide – these will be added and researched to determine their identification

Summary A drift scan across Milky Way through SAG A* appeared to be show the edges of the Milky Way and the approximate location of SAG A* Measurements were taken at different Galactic Longitudes to calculate the Galactic rotation rate. The Doppler shift of each point will be determined. The rotation rate is based on Doppler (km/second) and source location. The results will be calculated and briefed at next science meeting. This was an excellent observation trip!