NASA/IPAC Teacher Archive Research Program
(NITARP)



PROGRAM INFORMATION

+ Home Page
+ Program News

+ Round 1
+ Round 2
+ Round 3
+ Round 4
+ Round 5
+ Round 6
+ (All programs)

+ Accomplishments
+ Educational Products
+ AAS Posters & Photos
+ Press Coverage

+ Visiting the SSC
+ Policies and Procedures


CURRENT TEAMS

+ Round 6


Other EPO programs using real data

Round 1 - Arp 102B Program News

Click on any teacher's name to see activities associated with NITARP.

Highlights of team activities

January 2006

The group presented their research results at the January 2006 AAS meeting. poster (pdf), and ADS abstract.

November 2005

On Nov 11, 2005, Harlan Devore gave a power point presentation called "Seeing the Universe in Another Light" at the North Carolina Science Teachers Association fall convention. About 30 teachers were present. He had participants work through the first activity in the NASA Multiwavelength Educational Outreach Activities. Mr. Devore then outlined and demonstrated the other four activites. In addition, he outlined the mission and capabilities of Spitzer, provided information on how to access and view Spitzer images, and described the Spitzer Teacher Program. Each participant was provided a CD-ROM with a copy of his power point and the instructions needed for the five NASA activities.

October 2005

Harlan Devore's school newspaper, The Hoofbeat, ran a front page article on the ARP102B project in its October 2005 issue. The newspaper reaches about 1500 students and 120 teachers.

Howard Chun ran two in-service workshops on the last two Wednesdays of October for science teachers in his school district: one on classroom infrared activities, and the other on multi-wavelength (including infrared) astronomy research in the science classroom. The teachers really enjoyed Michelle's IR video. The teachers went away with new ideas for activities and science fair projects in their physical science, biology, and chemistry classes. Mr. Chun had ten teachers attending each workshop.

Mr. Chun gave a one hour lecture on the Spitzer Space telescope, the teacher researcher program, and our group's research to a group of approximately 50 amateur astronomers at the Seagrave Memorial Observatory in Scituate, RI. It was a different experience talking to a knowledgeable and informed audience. He was peppered with questions throughout the lecture. The Spitzer DVD was very useful. He showed the IR video, the simulated launch, and the pretty visible to IR pictures. They were also quite interested in how he used IR in the classroom and with his students.

September 2005

Lauren Chapple has set up a secondary science staff meeting for second semester. It will include a presentation on Spitzer and how it is to be used in the classroom. He is also introducing his Spitzer project and Harlan Devore's as an option for the spring research project. Students must do a stellar spectroscopy project to qualify for either Spitzer or AGN projects.

August 2005

Harlan Devore from the "The Supermassive Black Hole in Arp102B " team, was featured in a Fayetteville Observer Article in the August 4, 2005 issue. The article was titled: "Teachers, students study final frontier" The newspaper has a circulation of about 70,000.

At the Hands-On Universe Conference at Yerkes Observatory in mid-August, Mr. Devore presented an overview of the Spitzer Telescope, its instruments and capabilities, and how to use Leopard to retrieve images. He used DS9 software to show samples of MIPS and IRAC images. In addition, he described the Spitzer Teachers Program and gave an overview the ARP102B project. The audience of about 30 people included scientists, astronomy professors, and high school teachers. Most were Teacher Resource Agents (TRAs) -- teacher trainers for HOU. Three of the teachers present were also graduates of the TLRBSE or RBSE programs. The presentation is in power point and is available for other teachers who want to clone it.

Lauren Chapple used Spot to create a list of background flux (in MJY/sr) vs wavelength for our target area. Mr. Devore coordinated with Dr. Chary and got the pixel width of the spectral extraction area from each of our .fits images. He set up a spreadsheet, using platescale to convert the pixel area of each extraction into solid angles (in sr). He then multiplied it by the integration time (in s) and used that to factor the background flux. Unfortunately, the background flux numbers he is getting are still too large - larger than the signal flux. In the next few days, Mr. Devore plans to go over his work again to see if he can figure out what he did wrong. If he can't, he will ask Dr. Chary to review his calculations.

Mr. Devore's student Katie has recently finished identification of lines in a second set of spectra. They are finding quite a few lines that just don't match any of the common spectral lines found in AGNs. They suspect that the lines may be significantly Doppler shifted. If so, the torus region does not seem to be homogeneous because there is not a matching line that is shifted in the other direction for most of these lines.

Mr. Devore's student Brian elected to take his Astronomy class rather than the Research in Science class. As a result, he will be playing a much smaller role in the analysis because he will not have much class time to work on it.

Lauren Chapple has put in for time at his next science department meeting / inservice to present the Spitzer project.

June 2005

The data for the "Supermassive Blackhole in APR102B" project has been archived and released. Teachers and four students visited the Spitzer Science Center to work on data analysis with contact scientist Dr. Ranga Chary. The visit was a great success for all.

May 2005

The data for the "Supermassive Blackhole in APR102B" project has been archived and released. Data analysis is proceding and the teachers are scheduled to visit the Spitzer Science Center on June 27th, 2005.

April 2005

Project status is as follows: SST imaged our project on Mar 18th. The Spitzer Help Desk notified me that preprocessing was completed and data released on April 20th. Dr Ram-Chary looked at the spectral data and said that it looked good. I am able to go to Pasadena at anytime during the months of Jun and July to do the analysis, although I prefer an earlier date because I want to finish most of the analysis and writing before school starts again. I have coordinated with Dr Ram-Chary, and he is available to assist us with the analysis during the week of Jun 27th.

From Lauren: I have applied for Spitzer / IR "in-service" time for next fall within our school district.

March 2005

longer work summary (pdf)

Funding for NITARP comes from the NASA ADP program and NASA/Archive EPO program.

Questions? E-mail nitarp -- at -- ipac DOT caltech DOT edu