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Remote Observing at the Dark Ridge Observatory And Beyond… Thomas C. Smith, Director, Dark Ridge Observatory STAR 2008, San Luis Obispo, California A Statement of Fact Students that utilize remote observatories to conduct their scientific research are often at the mercy and whims of the observatory owner/operator What is the Problem In today’s growing arsenal of remote observatories, many have provided the use of their equipment for both research and astrophotography but for most remote sites the support ends there So What’s Different At the Dark Ridge Observatory students are made a part of the entire observatory and observing process including data reduction, analysis and incorporation into scientific papers in both refereed and non-refereed scientific journals A Bit More Detail At the Dark Ridge Observatory the student is guided through the nuances of the host equipment to achieve scientific accuracy for their measurements This process provides mentoring for the student in areas of data collection, reduction and understanding of the use of astronomical images in science Introduction Three fall semesters in 2005/6/7 (Cuesta Community College and the California Polytechnic University in San Luis Obispo, California) Hands-on observations made at the Dark Ridge Observatory in Atascadero, CA. Remote observations made at the Dark Ridge Observatory in Weed, New Mexico Having “the” expert on the equipment a major part of the science project Dark Ridge Observatory The Dark Ridge Observatory (DRO) is now located in the Sacramento Mountains of southeastern New Mexico Elevation 7100 feet (2164 meters) Winter/Spring best with monsoon-like conditions in the summer and early fall Clear night seeing (0.7 – 2.0 arc-seconds typical, early measurements of a prototype DIMM seeing monitor) 501(c)(3) non-profit observatory utilizing the equipment and facilities of the Dark Ridge Ranch DRO (continued) Early vision of the observatory phase one. The proposed rendition looking at phase 1 of the DRO construction effort. DRO (continued) Current construction progress. View out the control room window to the first of three roll-off observatories in phase 1 of the construction work. Equipment available at DRO One 8” LX200R telescope w/DIMM (seeing) capabilities Two 14” LX200/GPS(R) telescopes w/ parallel-mounted 5” f/5 refractors The Dark Ridge 20” Alt-Az Ritchie-Chrétien (being rebuilt) The Morgan 24” Cassegrain hosted for the AAVSO (soon) One SBIG ST-7XE CCD camera w/ UBVRcIc filters One SBIG ST-8XME CCD camera w/ UBVRcIc filters and external guide head One Apogee AP-8 CCD camera w/ UBVRcIc and Hα, Hβ and OIII narrowband filters (for the 20” RC) One Meade DSI (color) CCD camera One Meade DSI Pro II (monochromatic) CCD camera One SBIG ST-402 CCD camera (clear filter only) One SBIG DSS-7 Spectrograph One SBIG SGS Spectrograph (1800rules/mm in Hi-Res and 600rules/mm in Low-Res) Focal reducer/field-flatteners for the LX200 systems Davis site weather station Science Collaborations Students have been involved in the following areas: Double star astrometry using CCD cameras Exo-planet follow-up using time-series photometry Newly discovered variable star time-series photometry in conjunction with the Global Network of Astronomical Telescopes (GNAT) directed by Dr. Eric Craine New hardware investigations (dual-channel photometer SAS2006) Discovering instrument limitations (Purposeful Defocus paper AAS 2005) And more… So What Makes the Difference Deciding the science to be performed Having the equipment expert or “SME” mentoring the students Choosing the observing parameters and iterative testing to obtain the proper setup Near real-time data image collection and reduction Sending the finalized data analysis to the student for inclusion in their publication Hi Tom, A Typical Collaboration I have done a little bit of 'data mining' in the WDS Catalog and have found a few interesting M type double stars. Only one is a confirmed binary (GRB Hi Jo, 34AB). HJ 5453AB hasn't changed theta in almost 200 years and it's rho has only changed 0.1'. just judging by numbers alone (although I still have a lot to learn about it), stars STF 72 126AB seem to have similar proper The declinations of all the areand wellSTF placed for decent observations. motion, their rho andbut theta changing somewhat rapidly to compared to HJ Most are quiteand bright however thisare should not make it too difficult image5453AB. them. During the start of a student collaboration there are many all are brighter than mag 11.1 and have separations greater than 23'. Right now I am in the middle of a horrific wind storm with gusts over 80 miles an hours. It has also beenthings raining here and cloudy need when not raining so that attending to Jo I have done no imaging beyond what I did a week ago. If the weather patter Hi Tom, holds to the predictions it should be really nice for the next three the are days/nights so maybe I can getbefore a chance to image theseactual systems. Haveimages you attached are what I think are the components. for whatever reason, looked at them on Aladin to see if you can identify the components? GRB 34AB is not centered. STF 72 has an incredibly sparse field taken very similar to 3 Peg. STF 126AB has several possible secondary I'll let you know what I find. stars. however, I believe the brightest one is the secondary because it Jo, is comparable to other tenth magnitude stars on Aladin. email Here is one such example Thomas C. Smith I managed to get the computer for the 14” fixed and imaged all four of the M Dark Ridge Observatory stars tonight. I’ll put it together in an Excel spreadsheet like the previous ones Jo conversation that took but only after I get the paper parts that I owe you togetherplace: first. Here is a teaser “RAW” image for you of STF 126AB. Thomas C. Smith Dark Ridge Observatory Collaboration (continued) Although this data is from a different star than that of the previous conversation it shows the way that the student receives the data when fully processed at DRO, however it is encouraged that the student perform their own analysis, guided by DRO. Student Papers Here is a non-comprehensive list of papers, authored by the students, that have been reviewed by, produced at or in cooperation with the Dark Ridge Observatory “Light Curves of Two GNAT MG1 Survey Stars: A OneSemester Community College Pilot Research Project”: JAAVSO 12/18/2006 “A Compact, Off-the-Shelf Low-Cost Dual Channel Photometer”. Presented at 2006 SAS “An Experiment in Relating CCD Differential Photometric Precision to Varying Degrees of Image Focus”: AAS 2005 “Measurements of a Visual Double Star STF-2079”: JDSO “High School Observations of the Visual Double Star 3Pegasi”: JDSO … The “Real” Magic Students actually performing hands-on data collection that was used for a publication sited on the preceding slide. A three-student team working at the Orion Observatory being advised and mentored by the Dark Ridge Observatory Conclusion Dark Ridge Observatory and the interactive work that is conducted between the students and the on-site SME really make a significant difference in the way the students both learn about science through astronomy as well as the way they get ENERGIZED for all their future endeavors. It takes a lot of work and patience to accomplish first-rate astronomical science and in the production, presentation of their work into journals, speaking at recognized conferences and this is where Dark Ridge Observatory and student collaboration is really making a profound difference. Recent News at DRO The Dark Ridge 20” RC Alt-Az telescope is in the shop for rebuild and placement in it’s new permanent roll-off observatory building. The AAVSO has acquired the Lowell “Morgan” 24” Cassegrain telescope and has choose the Dark Ridge Observatory to upgrade and host it on the ridge top in Weed, New Mexico! This will be the AAVSO’s northern hemisphere research telescope. What an honor! The Dark Ridge Observatory Thanks You! Any questions? Thomas C. Smith Director, Dark Ridge Observatory 701 NM Hwy 24, Weed, New Mexico 88354 (575) 687-2168 http://www.DarkRidgeObservatory.org a 501(c)(3) tax-exempt, non-profit, scientific research and educational charitable organization. “High on the ridge and high on astronomical research and education”