2011-06-23+27 Pluto+Charon+Hydra occultation
From SwRI
Overview
The Meudon group (Sicardy, Widemann, etc), the MIT/Williams group (Person, Bosh, Pasachoff), and the PHOT SwRI/Wellesley group (Young etc.) are all chasing two bright events in June, 2011. Both are very bright in the IR, being brighter than Pluto in I, J, H, and K. The June 27 star is brighter than Pluto in B and V as well. The June 23 star is occulted by both Pluto and Charon, and the June 27 star is occulted by both Pluto and Hydra. There is a very faint star on June 23 that is also a possible Nix occutation. This is the PHOT planning page.
Contents |
Quick Tips
We have recruited new observers in Southeast Asia and Hawaii for the Hydra track. Welcome! And thank you! Here are some quick tips. If you have any questions, you can call Leslie Young at (63) 905-426-8210 ( Phillippines number, loaner cell phone,only good for calling tonight).
Timing
- This is a crowded field. You might want to get on the field by 12:30 UT and just track the field.
- If you can, observe the field before 13:20 UT to measure Pluto and the occulted star separately
- Observe the Pluto occultation for 20 minutes or more centered on 14:21 UT (Southeast Asia) or 14:14 UT (Hawaii). with 0.5-second or 1-second integrations if you have a short readout time.
- start no later than 14:11 (Southeast Asia) or 14:04 UT (Hawaii)
- Observe the Hydra occultation 20 minutes or more centered on 14:54 UT (Southeast Asia) or 14:49 UT (Hawaii) with 0.5-second integrations.
- start no later than 14:34 (Southeast Asia) or 14:39 UT (Hawaii)
- Choose a camera of readout mode (region of interest, binning) to keep readout time less than 0.25 seconds, preferably less than 0.05 seconds
Pointing and Field of View
- The occulted star is 18:25:29.0 -18:48:48 (J2000), and 18 26 09.5 -18 48 22 (Epoch of date). No need to track on Pluto. In fact tracking sidereally is preferred.
- Wider fields of view (20 arcmin) make finding the field easier, and then you can use a region of interest for the occultation runs.
- Binning? Yes, if you need to to make your readout time short. Otherwise, bin to have 2-3 pixels full-width-half-max across a star for the best photometry.
- See finder charts and stars for star-hopping further down on this page.
Filter
- Open -- no filter
Flats, biases
- Take flats and biases. Rather than separate darks and biases, it's easiest just to take a lights-off run at the same exposure times as the occultation data.
File formats
- For those using "planetary video cameras", samve files with 12 or 16 bit.
- We strongly prefer FITS files.
Timing
Accurate timing is VERY important.
- Accurate GPS times are ideal if you can do that.
- Network Timing Protocol (NTP) can help if you don't have GPS times.
- For other timing ideas, you can ask Dave Gault (+61 2 4754 4351) or Graham Blow (+64-4-479-2504) for advice up before event time.
Event Summary (times, magnitudes)
June 23 11:25 UT is the morning of June 23 in the Eastern Pacific (Hawaii, California, Mexico) and the evening of June 23 in the Western Pacific (Marshall Islands, Nauru, Philippines).
June 27 14:30 UT is the morning of June 27 in the Eastern Pacific in Hawaii and the evening of June 27 or the morning of June 28 in the Western Pacific (Marshall Islands, Nauru, Indonesia, Philippines).
| Event | UT Date | Approx Time | Vel km/s |
| Charon occultation | 2011-06-23 | 11:15:20 local times | 23.85 |
| Pluto occultation | 2011-06-23 | 11:24:49 local times | 23.81 |
| Nix occultation (faint) | 2011-06-23 | 12:39:25local times | 23.81 |
| Pluto occultation | 2011-06-27 | 14:18:41 local times | 23.92 |
| Hydra occultation | 2011-06-27 | 14:52:36 local times | 23.91 |
| Object | Approx RA | Approx Dec | B | V | R | I | J | H | K |
| 2011-06-23 PC star | 18:25:55.4750 | -18:48:07.015 | 17.4 | 15.18 | 14.4 | 12.72 | 10.957 | 10.054 | 9.743 |
| 2011-06-23 N star | 18:25:55.0631 | -18:48:08.702 | 19.8 | 18.6 | |||||
| 2011-06-27 PH star | 18:25:29.0100 | -18:48:47.570 | 14.35 | 13.71 | 13.9 | 12.97 | 12.326 | 12.091 | 11.933 |
| Pluto | 15.2 | 14.4 | 13.6 | 13.0 | 12.9 | 13.0 |
Contacts
- For overall coordination contact Leslie Young http://www.boulder.swri.edu/~layoung/
- For Hydra coordination contact Marc Buie http://www.boulder.swri.edu/~Buie/.
- For coordination in the field contact Kate Lonergan: klonerga@wellesley.edu or 781.283.2908
- Internal contact lists: [Contacts].
- Occultation telecon chat page http://data.boulder.swri.edu/~efy/occ11/
Science Goals
- Atmospheric Monitoring (how pressures and temperatures change seasonally)
- Technique - two or more chords for astrometry, one or more with moderate or high SNR (signal-to-noise ratio).
- Pluto-Charon orbit constraints
- This is a rare opportunity. This has only been observed once before, with a single chord on Charon.
- Technique - two or more chords on Pluto and two or more on Charon. These do not have to be from the same sites.
- Pluto diurnal variation
- Rare to get two events within one Pluto day (6.4 Earth days).
- Technique - two or more chords for astrometry, one or more moderate or high SNR for both events
- Hydra size and orbit constraints
- This would be the first Hydra occultation. Hydra's size is currently very uncertain (diameter between 47 and 167 km). The orbit is also uncertain, and puts some planned New Horizons imaging at risk for missing Hydra.
- Technique - Use the June 23 Pluto and Charon occultations to fine-tune a picket fence in Australia.
- See public Hydra page
- Lower atmospheric structure and oblateness
- Previous occultations have shown differences in Pluto's lower atmosphere indicative of methane heating and cooling, and evidence of a non-spherical atmosphere.
- Technique - central flash. Here we are constrained by geography. As predictions refine this spring, we can try to concentrate resources near the predicted center line. Because the Pacific offers limited mobility, we'd need to pick our locations by mid-May.
- Horizontal spatial variation in the atmosphere
- Technique - clusters of telescopes
- Vertical structure
- Technique - high SNR
- Haze constraints
- Technique - multicolor
Site Summary
What time is it? http://www.timeanddate.com/worldclock/personal.html?cities=717,91,1238,437,1440,43,132,1243,1945,778,137,103,276,929,196,240&sort=2
Site links (marked with link symbol) are for internal planning purposes. Contact Leslie Young for access.
Visa requirements: http://travel.state.gov/travel/cis_pa_tw/cis/cis_4965.html
| Mexico | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| San Pedro Martir | .84, 2.1 | nights of June 20, 21 and 22, for the 2-m and the 84-cm | PHOT/Doc (vis) CID (IR) | Dick French, Bob Howell | IWW/PHOT Cameras; Doc | ||||||
| USA | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Sedgewick | 0.4 | Confirmed | Remote | Time asked for by Bianco | |||||||
| IRTF | 3.0 | Time allocated to Gulbis | n/a | n/a | |||||||
| UH 88-inch | 2.2 | Confirmed | Optic | Tholen, remote | |||||||
| Lanihuli Observatory, WIndward Comm. College, Kaneohe HI | .4 | Contacted, interested. Maybe POETS? | ? | ? | |||||||
| Faulkes Telescope North | 2.0 | Approved | Remote | ||||||||
| Hyatt Regency, Maui | 0.36 | Approved; Bruno's group | Raptor? | HJ Bode? | |||||||
| Kauai | 0.36+0.28? | Confirmed | Watec? Raptor? | Marc Buie, Thomas Widemann, Frédéric Vachier ? | |||||||
| Waikoloa | Christopher's 0.41 | Confirmed | Craig's Photometrics FT | Craig Nance , Christopher Erickson | needs astrotimer | ||||||
| Hale A a | 0.56 (vis), 0.61 (IR) | Confirmed | PHOT/Henri (vis); NovaSensors (IR) | Eliot Young, Kevin Shoemaker,Tony, Wayne | IWW/PHOT Cameras | ||||||
| Wake | 0.36 | Contact made, official approval pending | PHOT | ? | Go/no-go May 23 | ||||||
| Guam | 0.36 | Contact made | PHOT | ? | Go/no-go May 23 | ||||||
| Howland & Baker | unfeasible | XX | XX | XX | Uninhabited | ||||||
| Line Islands (Kingman & Palmyra - US) | unfeasible | XX | XX | XX | Uninhabited | ||||||
| Nauru | |||||||||||
| Nauru | 0.36 PHOT | Contact made | PHOT/Ansel | Peter and Larry | LANL ARM. Go/no-go May 23 | ||||||
| Marshall Islands | |||||||||||
| Kwajalein | 0.61? | PRD sent to D. Marguriet | IR? | Regester | |||||||
| Majuro | 0.36 PHOT | Local contact made | PHOT | Cathy and Harold | IWW/PHOT Cameras Walker Scope and camera | ||||||
| Northern Mariana Islands (Saipan, Rota) | |||||||||||
| Micronesia | |||||||||||
| Yap | 0.36 PHOT | Contact made | ? | Go/no-go May 23 | |||||||
| Chuuk | 0.36 PHOT | Contact made | ? | Go/no-go May 23 | |||||||
| Pohnpei, | 0.36 PHOT | Contact made | ? | Go/no-go May 23 | |||||||
| Kosrae | 0.36 PHOT | Contact made | ? | Go/no-go May 23 | |||||||
| Pulau | |||||||||||
| Philippines | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Christopher Go, Cebu | .36 | Confirmed | PHOT/Eadweard | LYoung + ? | IWW/PHOT Cameras | ||||||
| Armando Lee, Astrocamp Obs, Pasay | .28 | Interested. Large enough telescope? | ? | ? | |||||||
| NISMED, Quezon City | .4 | Talked w/ Dr. Tan. Telescope is available | PHOT + local | ? | Doesn't track? | ||||||
| John Nassr, Stardust Observatory, Baguio City | .41 | For June 27 | ? | ? | |||||||
| Indonesia | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Bosscha, West Java | .6 | Confirmed | PHOT/Gjon | MBullock + JStansberry | IWW/PHOT Cameras Gjon | ||||||
| [LAPAN station, Biak Island | - | Contact made | PHOT | Go/no-go May 23 | |||||||
| LAPAN station, Tanjungsari | 0.46 | ? | |||||||||
| Avivah Yamani | ? | Emailed | |||||||||
| Papua New Guinea | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Manus Island | 0.36 | Contact made | PHOT | Difficult logistics | |||||||
| Australia | |||||||||||
| Darwin | 0.36 PHOT? | Contact made | ? | LANL ARM | |||||||
| Faulkes Telescope South | 2.0 | Confirmed | |||||||||
| Vanuatu | |||||||||||
Star info
Catalog
June 23 18:25:55.4750 -18:48:07.015
USNO B1.0 0711-0590849
June 23
Globes and Ground Tracks
- Bruno Sicardy
- Homepage http://www.lesia.obspm.fr/perso/bruno-sicardy/
- UPDATES -- look at BOTTOM of the page June 23 http://www.lesia.obspm.fr/perso/braga-ribas/list/2011/2011_06_23_CharonPluto.html, June 27 http://www.lesia.obspm.fr/perso/braga-ribas/list/2011/2011_06_27_PlutoHydra.html
- README FIRST http://www.lesia.obspm.fr/perso/bruno-sicardy/predic_occn_11/index.html
- Charon June 23 http://www.lesia.obspm.fr/perso/bruno-sicardy/predic_occn_11/Charon_2011/2011_06_23_11.238.jpg
- Pluto June 23 http://www.lesia.obspm.fr/perso/bruno-sicardy/predic_occn_11/Pluto_2011/2011_06_23_11.414.jpg
- Nix June 23 http://www.lesia.obspm.fr/perso/bruno-sicardy/predic_occn_11/Nix_2011/2011_06_23_12.657.jpg
- Pluto June 27 http://www.lesia.obspm.fr/perso/bruno-sicardy/predic_occn_11/Pluto_2011/2011_06_27_14.311.jpg
- Hydra June 27 http://www.lesia.obspm.fr/perso/bruno-sicardy/predic_occn_11/Hydra_2011/2011_06_27_14.885.jpg
- MIT Planetary Astronomy Lab
- Maps
- Ground tracks
- Larry Wasserman, Created 2010 Dec 6, using Bruno Sicardy predictions.
Finder Charts
Field Images
2011-06-23 star (Pluto and Charon occultation)
2011-06-27 star (Pluto and Hydra occultation)
Finder charts (DSS & UCAC2)
June 23
June 27
Star hopping
Bright stars near the Pluto occultation stars this June suitable for "walking" down to the field. All coordinates are J2000.
| # | Star | Mag | RA, DEC (J2000) | RA, DEC (date) | Distance |
| 1 | Sigma Sgr = Nunki = 34 Sgr = PPM 259078 = HR 7121 = SAO 187448 | 2.0 mag | 18 55 15.9 -26 17 49 | 18 55 58.6 -26 16 54 | 15 degrees away |
| 2 | Lambda Sgr = HR 6913 = SAO 186841 = PPM 268438 | 2.8 mag | 18 27 58.2 -25 25 20 | 18 28 40.7 -25 24 52 | 10 degrees away |
| 3 | Mu Sgr = HR 6812 = SAO 186497 = PPM 268080 | 3.9 mag | 18 13 45.8 -21 03 32 | 18 14 27.0 -21 03 18 | 4.5 degrees away |
| 4 | HR 6769 = SAO 161093 = PPM 234067 | 5.3 mag | 18 07 48.3 -17 09 14 | 18 08 28.3 -17 09 06 | 2 degrees away |
| 5 | HR 6933 = SAO 161540 = PPM 234623 | 5.5 mag | 18 30 11.9 -18 43 45 | 18 30 52.4 -18 43 14 | 1 degree away |
| 6 | HD 169355 = SAO 161449 = PPM 234508 | 7.3 mag | 18 24 59.9 -18 32 19 | 18 25 40.3 -18 31 54 | 0.34 deg from 23rd star; 0.30 deg from 27th star |
| 7a | HD 169602 = SAO 161423 = PPM 234526 (a double star) | 8.8 mag | 18 26 11.7 -18 32 21 | 18 26 52.1 -18 31 54 | 0.27 deg away from 23rd star |
| 7b | HD 169273 = SAO 161442 = PPM 234502 | 9.4 mag | 18 24 43.7 -18 44 10 | 18 25 24.2 -18 43 45 | 0.19 deg away from 27th star |
| x | P110623 | 15.18mag | 18:25:55.5 -18:48:07 | 18 26 35.9 -18 47 41 | 23rd star |
| x | P110627 | 13.7 mag | 18:25:29.0 -18:48:48 | 18 26 09.5 -18 48 22 | 27rd star |
Nothing brighter than 10.0 is closer to either star.
Proxies
I-band proxies
- P-6 hours 12 29 40.995 -18 44 50.17 I=12.799 Denis J122941.0-184450
- P-2 hours 16 23 32.906 -18 49 40.09 I=12.802 Denis J162332.9-184940
Schedule
Time Zones
What time is it? http://www.timeanddate.com/worldclock/personal.html?cities=717,91,1238,437,1440,43,132,1243,1945,778,137,103,276,929,196,240&sort=2
| Location | Timezone | UTC offset |
| Java (Bossca) | WIB | UTC+7 |
| Philippines (Cebu) | PHT | UTC+8 |
| Western Australia (Perth) | WST | UTC+8 |
| Cental Australia (Adalaide, Alice Springs, Darwin) | CST | UTC+9.5 |
| Eastern Australia (Cairns, Sydney, Melbourne) | EST | UTC+10 |
| Nauru | UTC+12 | |
| Marshall Islands (Majuro, Kwajaleain) | MHT | UTC+12 |
| Hawaii (Kauai, FTN, Waikoloa, MKO, Hale A'a)) | HST | UTC-10 |
| California, Baja California (Sedgewick, SPM) | PDT | UTC - 7 |
| Arizona (Flagstaff) | MST | UTC - 7 |
| Wyoming, Colorado (Laramie, Boulder) | MDT | UTC - 6 |
| Nebraska (Lincoln) | CDT | UTC - 5 |
| North Carolina, Massachusetts (Greensboro, Boston, Wellesley) | EDT | UTC - 4 |
CRITICAL DATES
| UT Time | What |
| 6/23 11:15 UT | Charon occultation - C110623 |
| 6/23 11:55 UT | Pluto occultation - P110623 |
| 6/24 01:15 UT | cutoff for first lightcurves and times |
| 6/25 00:00 UT | cutoff for final lightcurves and times |
| 6/27 14:19 | Pluto occ - P110627 |
| 6/27 14:52 | Hydra occ - H110627 |
NIGHTLY CALENDAR FOR LONG-HAUL OBSERVERS
We want to know where people are each night. For each of our observing sites, midnight is sometime midday UT, so it makes sense to ask where we are going to be during a particular UT day.
| UT Date | Java John,Mark | Cebu Melissa,Leslie | Kauai,Alice Springs Marc Buie | Nauru Larry,Peter | Majuro Cathy,Harold | Majuro,Kwaj Regester | Hale Aa Eliot, Tony | SPM Bob,Dick |
| 6/17 | home | Leslie's | home | transit | home | home | home | home |
| 6/18 | home | transit | home | Brisbane | transit | home | home | transit |
| 6/19 | home | Manila | transit | transit | transit | transit | home | Ensenada |
| 6/20 | home | Cebu | Kauai | Nauru | Majuro | Honolulu | transit | SPM |
| 6/21 | home | Cebu | Kauai | Nauru | Majuro | Majuro | Hale Aa | SPM |
| 6/22 | home | Cebu | Kauai | Nauru | Majuro | Majuro | Hale Aa | SPM |
| 6/23 | transit | Cebu | transit | Nauru | Majuro | Kwaj | Hale Aa | SPM |
| 6/24 | Bossca | Cebu | Alice Springs | Nauru | Majuro | Kwaj | Hale Aa (Tony lv) | San Diego |
| 6/25 | Bossca | Cebu | near A.S.? | Nauru | Majuro | Kwaj | Hale Aa | home |
| 6/26 | Bossca | Cebu | near A.S. | Nauru | Majuro | Kwaj | Hale Aa | home |
| 6/27 | Bossca | Cebu | near A.S. | Nauru | Majuro | Kwaj | Hale Aa | home |
| 6/28 | Bossca | Manila | near A.S. | Nauru | Majuro | Kwaj | Hale Aa | home |
| 6/29 | Yogyakarta | transit | near A.S. | Brisbane | transit | transit | transit | home |
| 6/30 | - | home | Sydney | Larry transit | home | Honolulu | home | home |
| 7/1 | John transit | home | transit | Larry home | home | Honolulu | home | home |
| 7/2 | John San Fran. | home | home | Larry home | home | transit | home | home |
| 7/3 | John Home | home | home | Larry home | home | home | home | home |
| 7/4 | John Home | home | home | Larry home | home | home | home | home |
Time Line
| UT Time | Who | Where | Local Time | What |
| 6/16 21:26 | PTamblyn | Denver | Th 6/16 15:26 = 3:26 PM | To Brisbane via SFO, AKL. |
| 6/17 03:00 | LWasserman | Phoenix | Th 6/16 20:00 = 8:00 PM | To Brisbane via LAX |
| 6/17 18:05 | MBrucker, LYoung | Denver | Fr 6/17 12:05 = 12:05 PM | MB arrive; LY pick up, get Cert. of Reg. signed. MB to stay at LY's 303-747-9161 |
| 6/17 20:00 | LWasserman | Brisbane | Sa 6/17 06:00 = 6:00 AM | arr Brisbane |
| 6/18 01:10 | PTamblyn | Brisbane | Sa 6/18 11:10 = 11:10 AM | Arr BNE |
| 6/18 13:45 | DFrench | Boston | Sa 6/18 9:45 = 09:45 AM | Dick lv Boston JetBlue 415 Boston -> San Diego 945am -> 1249pm |
| 6/18 16:36 | MBrucker, LYoung | Denver | Sa 6/18 10:36 = 10:36 AM | MB, LY fly Denver-> Cebu via Salt Lake City, Tokyo, Manila |
| 6/18 18:18 | COlkin,HReitsema | Denver | Sa 6/18 12:18 = 12:18 PM | UA-512 1218P DEN - 339P HNL & UA-1522 1030P HNL-140A Majuro |
| 6/18 19:00 | RHowell | Denver | Sa 6/18 13:00 = 01:00 PM | Southwest 2937 Denver -> San Diego 100pm -> 220pm |
| 6/18 19:49 | DFrench | San Diego | Sa 6/18 12:49 = 12:49 PM | Dick arr San Diego. Spend night in Ensenada |
| 6/18 21:20 | RHowell | San Diego | Sa 6/18 14:20 = 02:20 PM | Howell arr San Diego. Spend night in Ensenada |
| 6/19 01:39 | COlkin,HReitsema | Honolulu | Sa 6/18 15:39 = 3:39 PM | arr HNL |
| 6/19 08:30 | COlkin,HReitsema | Honolulu | Sa 6/18 22:30 = 10:30 PM | lv HNL. UA-1522 1030P HNL-140A Majuro |
| 6/19 11:00 | PTamblyn, LWasserman | Brisbane | Su 6/19 21:00 = 09:00 PM | Our 002 BNE-INU 6/19 21:00-04:45 6/20 |
| 6/19 13:40 | COlkin,HReitsema | Majuro | Mo 6/20 1:40 = 1:40 AM | Arr. Majuro. |
| 6/19 13:55 | MBrucker, LYoung | Manila | Su 6/19 21:55 = 9:55 PM | MB, LY arrive Manila. Stay HOTEL MANILA 63-2-8123456 |
| 6/19 14:18 | JRegester | Greensboro | Su 6/19 10:18 = 10:18 M | lv Greensboro. UA-4290 1018A Greensboro - 1149A Newark & UA-157 110P Newark-550P HNL |
| 6/19 16:45 | PTamblyn, LWasserman | Nauru | Mo 6/20 04:45 = 04:45 AM | arr Nauru |
| 6/19 20:18 | MBuie | Denver | Su 6/19 14:18 = 2:18 PM | UAL-786 218P DEN-355P SFO & UAL-773 454P SFO - 731P Kaui |
| 6/20 03:50 | JRegester | Honolulu | Su 6/19 17:50 = 5:50 pm | arr Hnl. |
| 6/20 04:45 | MBrucker, LYoung | Manila | Mo 6/20 12:45 = 12:45 PM | MB, LY fly Manila -> Cebu |
| 6/20 05:30 | MBuie | Kauai | Su 6/19 19:30=7:30 PM | Arrive Kauai. HOTEL LIHUE 1-808-3381625 |
| 6/20 06:06 | MBrucker, LYoung, CGo | Cebu | Mo 6/20 14:05 = 2:05 PM | MB, LY Arrive Cebu, Phil. Air flight 861. CG to pick up at airport. Stay at MARRIOTT CEBU CITY, 63-32-411-5800. Contact: Leslie cell (303-349-8638) for short calls only. |
| 6/20 12:03 | EYoung | Denver | Mo 6/20 06:03 = 6:03 AM | Lv Denver UAL 601 6:03A DEN - 7:42A SFO & UAL 6236 8:51A SFO - 11:19A KOA |
| 6/20 13:15 | TVengel | Santa Barbara | Mo 6/20 06:15 = 6:15 AM | Lv Santa Barbara UAL 5416 6:15A Santa Barbara - 7:44 SFO & UAL 601 8:51 SFO-11:19A KOA |
| 6/20 15:30 | JRegester | Honolulu | Mo 6/20 5:30=5:30 AM | Lv HNL. Continental-957 530A HNL - 839A Majuro |
| 6/20 20:39 | JRegester | Majuro | Tu 6/20 8:39=8:39 AM | arr Majuro |
| 6/20 21:19 | EYoung, TVengel | Kona | Mo 6/20 11:19 = 11:19 AM | Arr Kona, night at Hale A'a |
| 6/22 14:00 | Bullock, Stansberry | Denver | We 6/22 21:00 | depart for LAX, Taipei, Jakarta, Frontier F9-0419, EVA BR-0015, EVA BR-0237 |
| 6/22 22:35 | JRegester | Majuro | Th 6/23 10:35 = 10:35 AM | lv Majuro, continental-957 1035A MAJ - 1130A Kwajalein |
| 6/22 23:30 | JRegester | Kwajalein | Th 6/23 11:30 = 11:30 AM | arr Kwajalein |
| 6/22 23:15 | MBuie | Kauai | We 6/22 13:15=1:15 PM | depart for Alice Springs via SFO, Sydney |
| 6/23 11:15 | All | All | 6/23-24 (West) 6/22-23 (East) | Charon occultation - C110623 |
| 6/23 11:25 | All | All | Pluto occultation - P110623 | |
| 6/24 01:15 | LWasserman | Nauru | Fr 6/24 13:15 = 01:15 PM | offset - 2 hours SOFT CUTOFF FOR LIGHTCURVES & TIME |
| 6/24 03:15 | MBuie | Alice Springs | Fr 6/24 12:45 = 12:45 pm | arrive Alice Springs SOFT CUTOFF FOR OFFSET |
| 6/24 06:30 | Bullock, Stansberry | Jakarta | Fr 6/24 13:30 | arrive Jakarta, EVA Air BR-0237 |
| 6/24 06:38 | TVengel | Kona | Th 6/23 20:38 = 8:38 PM | Lv Kona UAL 299 8:38P KOA - 4:47A LAX & 6/24 UAL 6317 7:05A LAX - 7:56A Santa Barbara |
| 6/24 11:30 | Bullock, Stansberry | Bandung | Fr 6/24 18:30 | arrive Bosscha Observatory |
| 6/24 14:56 | TVengel | Santa Barbara | Fr 6/24 07:56 = 07:56 AM | arr Santa Barbara |
| 6/25 0:00 | LWasserman | Nauru | Su 6/15 12:00 = 12:00 PM | HARD CUTOFF FOR LIGHTCURVES & TIMES |
| 6/25 08:30 | MBuie | near Alice Springs? | Su 6/25 18:00 = 6:00 pm | end drive day 0 (if leave 1 day early) |
| 6/25 20:45 | DFrench | San Diego | Sa 6/25 13:45 = 01:45 pm | JetBlue 416 San Diego -> Boston 145pm -> 1005pm |
| 6/25 20:45 | BHowell | San Diego | Sa 6/25 13:45 = 01:45 pm | Southwest 3626 San Diego -> Denver 145pm -> 505pm |
| 6/25 23:05 | BHowell | Denver | Sa 6/25 17:05 = 05:05 pm | Southwest 3626 San Diego -> Denver 145pm -> 505pm |
| 6/25 21:45 | MBuie | Alice Springs | Su 6/26 7:15 = 7:15 am | sunrise |
| 6/26 00:00 | MBuie | Alice Springs | Su 6/26 9:30 = 9:30 am | start drive day 1 |
| 6/26 02:05 | DFrench | Boston | Sa 6/25 22:05 = 10:05 pm | JetBlue 416 San Diego -> Boston 145pm -> 1005pm |
| 6/26 08:30 | MBuie | near Alice Springs | Su 6/26 18:00 = 6:00 pm | end drive day 1 |
| 6/27 08:30 | MBuie | near Alice Springs | Mo 6/27 18:00 = 6:00 pm | end drive day 2 |
| 6/27 14:19 | All | All | 6/26-27 (West) 6/25-26 (East) | Pluto occ - P110627 |
| 6/27 14:52 | All | All | Hydra occ - H110627 | |
| 6/28 03:10 | MBrucker, LYoung, CGo | Cebu | Tu 6/28 11:10 = 11:10 AM | MB, LY lv Cebu, Phil. Air flight 861. |
| 6/28 04:20 | MBrucker, LYoung, CGo | Manila | Tu 6/28 12:30 = 12:20 PM | MB, LY arr Manila. Stay HOTEL MANILA 63-2-8123456 |
| 6/28 22:30 | MBrucker, LYoung | Manila | We 6/29 06:30 = 06:30 AM | MB, LY lv Manila -> Denver or Lincoln via Tokyo, Detroit |
| 6/29 00:00 | Bullock, Stansberry | Bandung | We 6/29 07:00 | depart by train for Yogyakarta |
| 6/29 02:20 | LWasserman, PTamblyn | Nauru | We 6/29 14:30 = 2:30 PM 6/29 07:00 | Our 001 INU-BNE 6/29 14:30-16:55 |
| 6/29 06:55 | LWasserman, PTamblyn | Brisbane | We 6/29 16:55 = 4:55 PM 6/29 07:00 | arr Brisbane |
| 6/29 07:00 | Bullock, Stansberry | Bandung | We 6/29 14:00 | arrive Yogyakarta |
| 6/29 06:38 | EYoung | Kona | Tu 6/28 20:38 = 8:38 PM | Lv Kona UAL 299 8:38P KOA - 4:47A LAX & 6/29 UAL 352 6:01A LAX - 9:20A DEN |
| 6/29 06:55 | JRegester | Kwajalein | We 6/29 18:55 = 6:55 PM | Lv Kwajalein. CO-956 655P Kwaj - 330A HNL via Majuro |
| 6/29 08:45 | COlkin, HReitsema | Majuro | We 6/29 20:45 = 8:45 PM | Lv Majuro,UA-4070 845P Majuro - 330A HNL |
| 6/29 13:30 | JRegester, COlkin, HReitsema | Honolulu | We 6/29 03:30 = 3:30 AM | arr Honolulu |
| 6/29 15:20 | EYoung | Denver | We 6/29 09:20 = 09:20 AM | arr Denver |
| 6/29 17:00 | COlkin, HReitsema | Honolulu | We 6/29 07:00 = 7:00 AM | lv Honolulu, HNL-DEN via SFO |
| 6/29 22:31 | LYoung | Denver | We 6/29 16:31 = 4:31 PM | LY arr Denver. Stay at house, 303-747-9161. |
| 6/29 23:05 | MBrucker | Omaha | We 6/29 17:05 = 5:05 PM | MB arr Omaha. Stay at house. |
| 6/30 00:55 | LWasserman | Brisbane | Th 6/30 10:55 = 10:55 AM | Brisbane-PHX via LAX |
| 6/30 1:05 | COlkin, HReitsema | Denver | We 6/29 19:05 = 7:05 PM | arr Denver |
| 6/30 04:00 | MBuie | Alice Springs | Th 6/30 13:30 = 1:30 PM | Quantus-731 130P Alice Springs-445P Sydney. |
| 6/30 06:45 | MBuie | Sydney | Th 6/30 16:45 = 4:45 PM | Night at HOTEL SYDNEY 61-2-9267 6511 |
| 6/30 17:09 | LWasserman | Pheonix | Th 6/30 1109 = 11:09 AM | arr PHX |
| 7/1 03:50 | MBuie | Sydney | Fr 7/1 13:50=1:50 pm | SYD-DEN via LA |
| 7/1 01:00 | Stansberry | Yogyakarta | Fr 7/1 08:00 | depart for Denpassar, Garuda Air GA-0250 |
| 7/1 09:00 | Stansberry | Denpassar | Fr 7/1 16:00 | depart for Taipei, SFO, EVA Air BR-0256, BR-0028 |
| 7/1 22:06 | MBuie | Denver | Fr 7/1 16:06 = 04:06 PM | arr Den |
| 7/2 02:00 | JRegester | Honolulu | Fr 16:00=04:00 pm | Lv HNL. HNL-Greensboro via OHARE |
| 7/2 04:30 | Stansberry | San Francisco | Fr 7/1 20:30 | arrive SFO, spend the night |
| 7/2 15:23 | JRegester | Greensboro | Sa 11:23 = 11:23 am | arr Greensboro |
| 7/2 16:30 | Stansberry | San Francisco | Sa 7/2 08:30 | depart SFO, Frontier F9-0668 |
| 7/2 19:30 | Stansberry | Denver | Sa 7/2 12:30 | arrive Denver, need to drop camera in Boulder c. 2pm. |
Tips
Observing
- Things to observe
- Occultation run
- pre and post run for really good upper baseline
- longer, high SNR exposures when Pluto and star are separated for good lower baseline
- flats - aim for high (>5,000) but not saturated (don't know for PHOT ... 30,000?)
- dark/bias. Preferable a set at each exposure time used.
- Run at your expected rate or duration before the event -- could even be daytime
- Timing
- General - start at least 5 minutes before earliest predicted ingress and continue to at least 5 minutes after latest predicted egress
- 1 sec or faster
- < 10% deadtime
- Example timeline for this event
JUNE 23 FTN TIMELINE 10:14 - 10:24 start observing, acquire field, focus 10:24 - 10:29 longer exposures 10:31 - 11:01 pre-event run 11:04 - 11:34 event run, includes Charon and Pluto 11:36 - 12:06 post-event run 12:09 - 12:14 longer exposures
JUNE 27 FTN TIMELINE 13:11 - 13:21 start observing, acquire field, focus 13:21 - 13:26 longer exposures 13:28 - 13:58 pre-event run 14:01 - 14:31 Pluto run 14:32 - 15:01 Hydra run and Pluto post-event 15:04 - 15:09 longer exposures
- Optimizing SNR
- The goal is to optimize the SNR of the normalized lightcurve averaged over a scale height (in this case, 2 s). Try different binnings, filters, exposure times and see what looks best.
- Get at least one reference star in the FOV (see #Finder_charts_.28DSS_.26_UCAC2.29, second row
- Get some good sky background (at least 50 x 50 pixels)
Reduction (June 23)
- Test data here: http://data.boulder.swri.edu/ptamblyn/pocc/dropped/.
- Kwajalein test data in Kwaj_20110427_test.tar.gz.
- Kwaj data is 16 images per file, one as main HDU followed by 15 extensios
- 1s for June 23 field is 1Hz/117044532CC000001.fits
- A (532,510)
- B (450,542)
- C (516,586) faint
- D (436,650)
- E (552,630)
- F (910,388)
- G (200,906)
- H (98,942)
- I (184,1010)
- MicroMax test data in "data of star fields and Pluto from 14-in"
- Princeton Instruments SPE format
- 1 s for June 23 field is 20110608_9.SPE, with
- A (236,286),
- B (278,320)
- C (280, 273) -- faint in I?
- D (340,297)
- E (295,240)
- F (62,123)
- Kwajalein test data in Kwaj_20110427_test.tar.gz.
- Dark subtraction and flatfielding optional
- Aperture photometry on Pluto and as many of the reference stars as are in your field.
- call this F for flux, as in F_P for Pluto, F_A for flux of star A, F_B, etc.
- During the event Pluto and star A are merged, and you measure F_P+A. Well outside of the event, you get F_P and F_A separately.
- Normalize F_P+A by some reference. If the reference is noisy you can smooth it before dividing.
- Call this R for Ratio. If we ratio to star B then during the event R_P+A = F_P+A/F_B. Well outside of the event you get R_P = F_P/F_B and R_A = F_A/F_B.
- Get the upper baseline
- R_UB = average of R_P+A away from the event
- Get the lower baseline
- The upper baseline is the Pluto flux plus the unocculted star flux (from the separated images)
- The lower baseline is just the Pluto flux.
- R_LB = R_UB - R_A
- If you get separated Pluto you could use R_LB = R_P, but Pluto has a significant lightcurve.
- Get the normalized lightcurve, LC, such that LC = 1 for unocculted star, and 0 for fully occulted star.
- LC = (R_P+A - R_LB)/(R_UB - R_LB)
- Note that LC can be greater than 1 if there are skinny high-altitude waves, and it doesn't have to go to the zero level.
- Assign times
- MicroMax (old camera): start time of 1st image = time of first pulse
- Example: time = 00:00:00. interpulse period = 1 s. Times = [0.5, 1.5, 2.5 ...]
- PhotonMax (new camera): end time of 1st image = time of first pulse + WinView exposure time (e.g., 2 ms).
- Example: time = 00:00:00. interpulse period = 1 s. Times = [-0.48, 0.52, 1.52, ...]
- MicroMax (old camera): start time of 1st image = time of first pulse
Informing Larry and Bruno
6/24 01:15 UT cutoff for first lightcurves and times 6/25 00:00 UT cutoff for final lightcurves and times
Mail the following to pocc20110623+27@boulder.swri.edu and to Bruno Sicardy <Bruno.Sicardy@obspm.fr>
1) GPS Lat & Lon & alt
2) Times of the event: immersion, emersion for 0.5 (half-light) times or 0.8 times. Even if you lightcurve goes deep, report 0.8 times to compare with shallower lightcurves.
NOTE that half-light levels refer to half-way between the star+pluto level ("one") and star alone level ("zero").
3) You can also report a table
seconds since 0 UT Pluto count error in Pluto counts counts for first reference error counts for 2nd reference error ...
4) If you're in real trouble you can drop tar or gzipped tar files of data and logs here: http://data.boulder.swri.edu/ptamblyn/pocc/. Suggested file name SITE_YYYYMMDD_tag.tar.gz or SITE_YYYYMMDD_tag.tar (e.g., Kwaj_20110427_test.tar.gz)


