From jop at astro.columbia.edu Fri Apr 6 12:30:44 2001 From: jop at astro.columbia.edu (Joe Patterson) Date: Fri, 6 Apr 2001 12:30:44 -0400 (EDT) Subject: (cba:news) RZ LMi, The Order of Battle Message-ID: <200104061630.MAA14236@tristram.phys.columbia.edu> Dear CBAers, April 6, 2001 Here's the scoop on RZ LMi so far. A note on the upcoming whole-earth campaign will follow later today, with the emphasis on southern and equatorial targets. By the way, a few days ago, did anyone notice that the Julian Date (last 4 digits) was equal to the year? If so, well... that's too bad. RZ LEO MINORIS - THE 2001 CAMPAIGN The 2001 campaign on RZ LMi has been going very well. The star flashes, and then takes away, its superhumps with great amplitude and speed, in a pattern too intricate to be resolved by any observations yet obtained. There is probably - but not certainly - an orbital signal in there too, since there are large-amplitude humps seen at quiescence. (The problem is that quiescence is very VERY short-lived, hence we must be awfully vigilant to catch the damn thing quiet for LONG ENOUGH to measure a period credibly different from the superhump period.) Here's the coverage to date. The cast of characters is ever- shifting, like a long-running Broadway play. Some obvious CBA Hall-of- Famers (Dave Harvey, Captain Bob, Lasse Jensen) are nowhere to be found. Resting, no doubt... they'll be back! And some active new people have emerged. Jeff Robertson and Tut Campbell are making a bid for Rookie of the Year honors. The campaign should be continued all the way through arrival of the next supermax, which I estimate will be April 17... then tack on 6 more days for the supermax to run its course. The larger scopes out there should especially seek coverage when the star is *faint* (17th mag), since that's when the putative orbital signal pops up. (Spectroscopy has failed to reveal Porb, and we really need to know this number.) In a few days I'll send all campaigners the densest and best portions of the 75-day light curve. But if you'd like all the (raw) data, I could send that too on request. I imagine Jeff Robertson will become the prime mover on the whole project when the time comes to fully analyze and write up for publication - but it's not settled yet. RAW DATA (delta-mag time series, before cross-calibrations to bring to a uniform scale) FILE JD/HJD PTS delta-mag and comments 29c 29.8478-.9820 544 <2.48> complex but periodic waveform 30c 30.9468-.0748 520 <0.80> possible tiny humps 31c 31.7097-.7266 47 <0.41> 32ep 32.3485-.5316 129 <0.68> 32js 32.7287-.8202 114 <0.41> 32c 32.7822-.0576 909 <0.35> 33ep 33.4375-.6523 163 <0.78> 33c 33.6934-.0322 1157 <0.43> 34ep 34.3666-.6455 199 <0.81> 34c 34.6824-.0188 1019 <0.53> 34bm 34.7231-.7670 27 <0.62> 35ep 35.3630-.6560 76 <0.90> 35e 35.5813-.9153 448 <0.525> 35c 35.6965-.0243 1302 <0.59> 35bm 35.7792-.8741 66 <0.70> 40c 40.7376-.0221 857 <2.37->2.55> 42jr 42.8819-.0201 141 <2.92> 43jr 43.8121-.9807 131 <2.39->1.50> 43mw 45mw 50tv 50.2588-.5892 225 <1.65> v noisy 52js 52.5493-.7960 541 <0.80->0.67> 53bm 53.6052-.0022 253 <0.42->0.34> 54tv 54.2754-.6256 174 <1.46> 55tv 55.2642-.7263 203 <1.57->1.63> 56tv 56.3982-.7215 279 <1.61> 57jr 57.6158-.8414 187 <0.56> 57bm 57.6020-.8506 161 <0.74->0.67> 58jh 58.5131-.6626 90 <-.70> noisy 58jr 58.6269-.9094 197 <0.62> 58bm 58.6464-.9527 152 <0.74> weak humps 59js 59.5093-.8811 856 <0.78> 60jr 60.6687-.7559 63 <0.78> 61jr 61.6612-.6869 9 <1.14> 62js 62.7128-.9158 470 <2.25->2.41> nice humps 63jr 63.5661-.6705 59 <2.63> 64js 64.7125-.9051 428 <1.65->1.30->1.18> 66jr 66.6160-.8959 200 <2.02->2.27> 67js 67.5389-.7565 435 <2.45->2.51> nice humps 67jr 67.5732-.8447 108 <2.42> 69e 69.4982-.6631 197 <2.53->2.40> 72js 72.5939-.7140 73jr 73.6585-.8806 139 <2.28->1.90> 73tk 73.7561-.8590 45 <2.0->1.9> 74jr 74.6142-.9709 174 <0.40> great humps 76jr 76.7375-.9023 99 <0.32> 78jr 78.5587-.8175 113 <0.53> 78bm 78.6134-.6872 21 <0.67> 79lc 79.6536-.8290 59 <0.67> noisy 80tk 80.7431-.8710 86 <0.59->0.62> no hump 81tk 81.7400-.8799 94 <0.64->0.66> 81jr 81.7287-.8965 113 <0.69->0.73> 82e 82.5191-.6172 135 <-0.15> humps 82jr 82.5770-.9202 241 <0.80> still humping 83js 83.6164-.7132 104 <1.42->1.54> 84tk 84.7320-.8951 57 <2.35->2.43> 85jr 85.5580-.9370 211 <2.70> giant humps 86jr 86.5880-.8912 170 <1.75->1.15->0.96> 87e 87.5158-.6629 203 <0.05> 87js 87.5653-.8492 576 <1.10->1.46> shumps returning 88e 88.5268-.6607 190 <1.08> humps 88js 88.5472-.8405 424 <2.13->2.38> great humps 88tk 88.7224-.8642 50 <2.16->2.24> 88jr 88.7701-.9365 87 <2.22->2.44> no visible humps 89jr 89.6498-.9088 152 <2.52> giant humps 91jr 91.6182-.8998 42 <2.4> useless 92e 92.5553-.6860 184 <-0.23> rising to max, no humps 93jr 93.5901-.9188 191 <1.03->1.20> 94jr 94.5799-.9179 195 <0.67->0.51> 95js 95.5190-.7676 373 <0.40> 95jr 95.6468-.9128 136 <0.29->0.42> 96e 96.5499-.6977 210 <-0.56->-0.75> 97e 97.5214-.6213 142 <-0.54> 97js 97.5239-.6919 182 <0.54> 98bm 98.7479-.8349 53 <1.78> still a good shump 99tk 99.6924-.8596 108 <0.53->0.60> still a good shump 100tk 100.6525-.8321 116 <0.65->0.69> still a good shump 102tk 102.6728-.8735 57 <0.70->0.76> not a useful time series 103tk 103.6678-.9094 81 <1.20->1.54> CONTRIBUTING STATIONS SOME PRELIMINARY CALIBS c Jonathan C-E = 0.12 BM-C = 0.10 ep Elena Pavlenko EP-C = 0.25 BM-JR = 0.13 e East (Dave Skillman) JS-JR = 0.07 JR-TK = 0.08 js John Stull and Dave Toot JR-E = 0.95 JS-E = 1.10 tv Tonny Vanmunster bm Brian Martin lc Lew Cook tk Tom and Lou Krajci jr Jeff Robertson and Tut Campbell jh Jim Hannon mw Matt Wood From jop at astro.columbia.edu Fri Apr 6 15:40:23 2001 From: jop at astro.columbia.edu (Joe Patterson) Date: Fri, 6 Apr 2001 15:40:23 -0400 (EDT) Subject: (cba:news) April's Battle Plan Message-ID: <200104061940.PAA17696@tristram.phys.columbia.edu> Dear CBAers, April 6, 2001. OK, the flowers are in bloom, the baseball season has started, so has the Masters, and the first-round leader of the Masters is (sort of) a baseball player! How wonderfully fitting is that. What could be better? The answer is, a very exciting photometry campaign on catclysmic variables with the CBA. So let's think on that subject... APRIL 2001 WHOLE-EARTH OBSERVATIONS During April 9-24 Jonathan will be at SAAO, so we'll have much improved coverage of the Earth's longitudes and latitudes. (We still have a terribly regrettable lack of representation in South America and Asia, but we press on with what we have!) This is therefore a very timely moment to work hard on CV light curves. For reasons known to no human, practically all the known helium CVs are clustered in a narrow RA range available during March-April- May. These are the binaries of shortest period, with Porb between 17 and 46 minutes, and with an impressive arsenal of machinery for producing periods. These are our prime targets, and April is the "soft underbelly" of the stars for yielding those precious periods. Here's the roster: STAR COORDINATES V MAG PERIODS V803 Cen 13 23 44.51 -41 44 30.4 13-17 1610 s and 23 hrs CR Boo 13 48 55.29 +07 57 34.8 13-17 1490 s and 20 hrs CE-315 13 12 46.93 -23 21 31.3 17.5 ~4000 s HP Lib 15 35 53.08 -14 13 12.3 13.6 1119 s GP Com 13 05 42.85 +18 01 02.6 15.5-16 2800 s, but not known to be periodic in photometry We do not plan a campaign on GP Com - last year's gave poor results - but I include it as a target for a "fishing expedition", since the star may one day awaken and flash some periodic signals at us. We have ongoing campaigns for 3 other stars, which may possibly suit your tastes in terms of sky position, magnitude, dislike for helium, etc.: AH Men 06 11 44.07 -81 49 24.1 12.5-13 complex near 3.0 hrs RZ LMi 09 51 49.02 +34 07 24.6 14.5-17.3 near 1.4 hrs DW UMa 10 33 52.95 +58 46 54.9 14.5-18 3.3 hrs and 4 days As usual, it's best to select one (or two) of these stars, and concentrate on amassing many-hour light curves of that one star. Charts and suggested comparison stars are at the CBA website. As usual, you may prefer a different comp, and that's OK as long as you identify it. _______________________________ Barring surprises, the first three objects named are the prime goals of the campaign. I want to especially talk up CR Boo and HP Lib, which in principle we can track around the Earth since they are roughly equatorial and we do have good longitude distribution. Whole-earth runs of very high quality are likely to reveal the intricate period structure, and thus the underlying orbital and precession periods. You should start observing as soon as possible, and note any surprises in terms of brightness. For example, V803 Cen or CR Boo jumping to magnitude 13.0 would indicate a "superoutburst", which we have never properly observed in any helium CV with time-series photometry. Yum, yum, that would be great. And if HP Lib sank to fainter than 14, that's never been observed either... so would merit very high priority. For the next 7-9 days, shade your choices on the bright side, and watch out for that rampaging Moon, which we really need to respect in our biz. It would be helpful if you let me know what observations you managed to get, even if the time-series is not yet analyzed. That would allow me to see the overall picture, and also communicate more precisely with the actual front-line troops... rather than send out a lot of detailed emails to people who plan to do mostly heavy-duty gardening during April. Good luck! Joe From jop at astro.columbia.edu Sat Apr 7 10:14:55 2001 From: jop at astro.columbia.edu (Joe Patterson) Date: Sat, 7 Apr 2001 10:14:55 -0400 (EDT) Subject: (cba:news) RXTE Update: 60005 Wk 271 (fwd) Message-ID: For confirmed borealites, here's the list of observation times for SU UMa this coming week. Hi Joe, This is the list of the XTE observations of SU UMa for the period 6th of April to the 12th. Apologies from being a few days later than it should be, but I have just returned from a week at the (very interesting) NAM2001 conference in Cambridge! cheers, Das ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Darren Stuart Baskill http://www.star.le.ac.uk/~dbl ----------------------------------------------------------------------------- Day 096 is APR 6 (UT). GOODTIME: 01:07:00 (229136824) to 01:40:00 (229138804) TOTAL_GT: 1.98 ksec Day 096 is APR 6 (UT). GOODTIME: 12:05:00 (229176304) to 12:38:00 (229178284) TOTAL_GT: 1.98 ksec Day 097 is APR 7 (UT). GOODTIME: 02:49:00 (229229344) to 03:10:00 (229230604) TOTAL_GT: 1.26 ksec Day 097 is APR 7 (UT). GOODTIME: 04:41:00 (229236064) to 04:52:00 (229236724) TOTAL_GT: 0.66 ksec Day 097 is APR 7 (UT). GOODTIME: 11:56:00 (229262164) to 12:32:00 (229264324) TOTAL_GT: 2.16 ksec Day 097 is APR 7 (UT). GOODTIME: 23:11:00 (229302664) to 23:44:00 (229304644) TOTAL_GT: 1.98 ksec Day 098 is APR 8 (UT). GOODTIME: 08:35:00 (229336504) to 09:05:00 (229338304) TOTAL_GT: 1.8 ksec Day 099 is APR 9 (UT). GOODTIME: 00:29:00 (229393744) to 01:12:00 (229396324) TOTAL_GT: 2.58 ksec Day 099 is APR 9 (UT). GOODTIME: 10:01:00 (229428064) to 10:34:00 (229430044) TOTAL_GT: 1.98 ksec Day 100 is APR 10 (UT). GOODTIME: 02:06:00 (229485964) to 02:45:00 (229488304) TOTAL_GT: 2.34 ksec Day 100 is APR 10 (UT). GOODTIME: 13:36:00 (229527364) to 14:09:00 (229529344) TOTAL_GT: 1.98 ksec Day 101 is APR 11 (UT). GOODTIME: 02:04:00 (229572244) to 02:36:00 (229574164) TOTAL_GT: 1.92 ksec Day 101 is APR 11 (UT). GOODTIME: 14:57:00 (229618624) to 15:30:00 (229620604) TOTAL_GT: 1.98 ksec Day 102 is APR 12 (UT). GOODTIME: 03:09:00 (229662544) to 03:44:00 (229664644) TOTAL_GT: 2.1 ksec Day 102 is APR 12 (UT). GOODTIME: 11:46:00 (229693564) to 12:19:00 (229695544) TOTAL_GT: 1.98 ksec ----------------------------------------------------------------------------- From jop at astro.columbia.edu Sat Apr 7 10:16:06 2001 From: jop at astro.columbia.edu (Joe Patterson) Date: Sat, 7 Apr 2001 10:16:06 -0400 (EDT) Subject: (cba:news) RXTE Schedule: 60005 Wk 272 (fwd) Message-ID: and here are the likely times for the following week (could possibly change) Hi Joe, Below are the XTE SU UMa observations for the period April 13th to the 19th. I will let you know if there are any later alterations by the XTE planners. Thanks again for all your help! Cheers! Das ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Day 103 is APR 13 (UT). GOODTIME: 01:39:00 (229743544) to 02:12:00 (229745524) TOTAL_GT: 1.98 ksec Day 103 is APR 13 (UT). GOODTIME: 14:09:00 (229788544) to 14:42:00 (229790524) TOTAL_GT: 1.98 ksec Day 104 is APR 14 (UT). GOODTIME: 03:24:00 (229836244) to 03:55:00 (229838104) TOTAL_GT: 1.86 ksec Day 104 is APR 14 (UT). GOODTIME: 14:59:00 (229877944) to 15:32:00 (229879924) TOTAL_GT: 1.98 ksec Day 105 is APR 15 (UT). GOODTIME: 02:37:00 (229919824) to 03:16:00 (229922164) TOTAL_GT: 2.34 ksec Day 105 is APR 15 (UT). GOODTIME: 14:01:00 (229960864) to 14:34:00 (229962844) TOTAL_GT: 1.98 ksec Day 106 is APR 16 (UT). GOODTIME: 02:28:00 (230005684) to 03:07:00 (230008024) TOTAL_GT: 2.34 ksec Day 106 is APR 16 (UT). GOODTIME: 13:45:00 (230046304) to 14:18:00 (230048284) TOTAL_GT: 1.98 ksec Day 107 is APR 17 (UT). GOODTIME: 02:19:00 (230091544) to 02:54:00 (230093644) TOTAL_GT: 2.1 ksec Day 107 is APR 17 (UT). GOODTIME: 15:08:00 (230137684) to 15:41:00 (230139664) TOTAL_GT: 1.98 ksec Day 108 is APR 18 (UT). GOODTIME: 02:10:00 (230177404) to 02:43:00 (230179384) TOTAL_GT: 1.98 ksec Day 108 is APR 18 (UT). GOODTIME: 14:17:00 (230221024) to 14:50:00 (230223004) TOTAL_GT: 1.98 ksec Day 109 is APR 19 (UT). GOODTIME: 02:38:00 (230265484) to 03:13:00 (230267584) TOTAL_GT: 2.1 ksec Day 109 is APR 19 (UT). GOODTIME: 15:55:00 (230313304) to 16:20:00 (230314804) TOTAL_GT: 1.5 ksec ----------------------------------------------------------------------------- From jop at astro.columbia.edu Thu Apr 12 12:21:52 2001 From: jop at astro.columbia.edu (Joe Patterson) Date: Thu, 12 Apr 2001 12:21:52 -0400 (EDT) Subject: (cba:news) April campaign underway Message-ID: Dear CBAers, Although we are more or less *always* campaigning - like guerilla soldiers - these two weeks have given us extra leverage over the range of world longitudes and latitudes. Jonathan is observing at the 1 m in South Africa, and Doug Welch is providing quite a bit of data at the 1.9 m in Australia. So let's see how things are going... RES AUSTRALIS AH Men... I think we'll go only ONE more day. We have forty days now, and the data are sufficient to reveal the pertinent periods. Definitely a quantum improvement on previous results... including a long-baseline ephemeris for Porb (0.127198 d) and a clarification of the superhumps - it's primarily a *negative* superhumper, with the nodal frequency present also (always) and a positive superhumper during one observing season. After Friday the 13th, we'll quit on this one. V803 Centauri. Perfect for all-night coverage now. Dancing to its little 23-hour tune, with accompanying small superhumps (27 minutes). Very, very fine object. CR Bootis. Also very well-positioned, decently bright (13.5-14.5) and at +8 degrees it's available to everybody. I really hope for contributions from USA, Europe, and NZ/AU, but so far we've had just a few nibbles. We last visited CR Boo in 1996, and did OK, but by far the bulk of these observations came from USA/Chile - not much longitude leverage there! Kiwis, Yanks, Euros, let the good times (and accompanying delta-magnitudes) roll! RES BOREALIS RZ LMI. Time to bring down the curtain. It's been a 90-day campaign, long enough to get whatever we're going to get. Time to ship off to Jeff Robertson and Matt Wood, and let them mine for the science. Leaving just two prime northern objects, DW UMa and CR Boo. DW UMa. We're doing well on this star and should keep going another few weeks. Nice eclipses and humps to show the neighbors. CR Boo. See above. These next 12 days are perhaps the critical time for this star! We have other stars on our program (from the last cba note), but I just wanted to send a simple list to keep the focus sharp. Buena suerte! joe From jop at astro.columbia.edu Fri Apr 20 13:07:10 2001 From: jop at astro.columbia.edu (Joe Patterson) Date: Fri, 20 Apr 2001 13:07:10 -0400 (EDT) Subject: (cba:news) V803 Cen erupts Message-ID: Dear CBAers, Andrew Pearce reported from Australia last night that V803 Cen had just jumped into a high state, at 12.7. A few hours later, Stefano observed it from South Africa and it continued bright. Certainly looks like the superoutburst (or at least this helium dwarf nova's version of a superoutburst) we've been waiting for the last 28 nights of coverage. So now's the time to spring to action! Stan caught one last year, but too late in the observing season. It's the first we've ever caught properly (and with coverage for the preceding 28 nights - I'd say that qualifies as "properly"!). Now we have to get the time-series coverage needed to study the developing and then decaying superhump. In our recent paper (May 2000 PASP) we gave a somewhat speculative account of how this proceeds, or might proceed, based on the fragmentary data available then. Now we get to find out if we were right. The superoutburst is probably very short, I think less than 5 days. Go for the gusto. Updates on CR Boo and DW UMa, the northern targets, coming over the weekend... and some data on V803 Cen. Joe From jop at astro.columbia.edu Sat Apr 28 07:50:21 2001 From: jop at astro.columbia.edu (Joe Patterson) Date: Sat, 28 Apr 2001 07:50:21 -0400 (EDT) Subject: (cba:news) Victories of April Message-ID: <200104281150.HAA24074@tristram.phys.columbia.edu> Dear CBAers, Time to report on our April campaigns... V803 CEN has been covered thoroughly now for 37 nights, with usually quite long coverage (often >10 hours). Superhumps were seen on every night, and we were able to count cycles reliably from night to night, which we could not quite do in the 1997 campaign. The most critical observations came from New Zealand (Fred and Jennie, Bob Rea, Bill Allen), with South Africa and Australia (Jonathan, Doug Welch) chipping in too. The usual 22-23 hour periodicity (dwarf-nova eruption?) was present throughout. But the most interesting result was the value of the superhump period, just 0.45% longer than Porb... This roughly determines the mass of the secondary star (the donor) to be 0.015+-0.005 Mo. Our puniest secondary yet (most are in the range 0.08-0.20 Mo)! We can quit on V803 Cen now. We'll never - not for a few years anyway - get coverage quite this good, and the star was even gracious enough to stage a supermax during the campaign. Time to move on. CR BOO has been a steady target of John Stull, with contributions also from Tonny and Dave East. Nothing recent from the Kiwis, who are rewriting the book on V803 Cen. The star is vigorously superhumping, but we really need much more extensive coverage, and from a range of longitudes. With its equatorial position the star should be a prime target - the prime target - for everyone. The other two stars needing mention now are DW UMA and HP LIB. The former is particularly good for some of you because of its far-northern position, and we'll keep after it. We'll start a proper campaign on HP Lib within a few weeks, but this is a pretty good time to get started... so if anyone wants to get us started, we'll take it from there! By the way, I plan to attend the IAPPP conference in Big Bear, CA on May 23, and then the Riverside ATM conference after that. Any other CBAers going? Definitely good territory for recruitment, and for CBA networking too. So: in the north, CR Boo, DW UMa, HP Lib in the south, CR Boo, HP Lib joe For light curve lovers, here's a nice run on V803 Cen from Fred and Jennie. Suitable for framing. JD V-C 24.85531 1.167 24.8557 1.161 24.85611 1.143 24.85651 1.15 24.85691 1.16 24.85732 1.184 24.85771 1.2 24.85811 1.18 24.85852 1.173 24.85891 1.177 24.85932 1.21 24.85971 1.226 24.86012 1.199 24.86052 1.182 24.86092 1.231 24.86132 1.178 24.86173 1.243 24.86212 1.197 24.8635 1.141 24.8639 1.234 24.86431 1.191 24.8647 1.183 24.8651 1.227 24.86551 1.235 24.8659 1.226 24.86631 1.208 24.8667 1.189 24.86711 1.176 24.86751 1.177 24.86791 1.219 24.86831 1.113 24.86871 1.17 24.86911 1.158 24.86951 1.158 24.86992 1.171 24.87031 1.149 24.87072 1.195 24.87112 1.196 24.87152 1.223 24.87192 1.187 24.87233 1.198 24.87272 1.193 24.87312 1.209 24.87352 1.162 24.87432 1.17 24.87472 1.183 24.87513 1.174 24.87552 1.201 24.87593 1.188 24.87633 1.169 24.87672 1.181 24.87713 1.163 24.87753 1.185 24.87794 1.155 24.87833 1.173 24.87874 1.179 24.87914 1.196 24.87954 1.233 24.87994 1.261 24.88074 1.166 24.88114 1.182 24.88155 1.21 24.88195 1.203 24.88236 1.211 24.88277 1.207 24.88316 1.187 24.88356 1.207 24.88396 1.224 24.88436 1.201 24.88476 1.218 24.88516 1.212 24.88557 1.2 24.88595 1.195 24.88635 1.17 24.88675 1.193 24.88715 1.215 24.88756 1.158 24.88795 1.203 24.88835 1.176 24.88876 1.162 24.88918 1.161 24.88956 1.218 24.88997 1.255 24.89036 1.218 24.89076 1.152 24.89117 1.186 24.89156 1.2 24.89197 1.201 24.89237 1.188 24.89276 1.145 24.89317 1.167 24.89358 1.168 24.89397 1.189 24.89438 1.143 24.89478 1.184 24.89517 1.172 24.89558 1.196 24.89598 1.208 24.89639 1.164 24.89679 1.22 24.89719 1.164 24.89759 1.182 24.898 1.238 24.89839 1.19 24.8988 1.199 24.8992 1.236 24.89959 1.212 24.9 1.223 24.90041 1.219 24.9008 1.199 24.9012 1.196 24.90161 1.191 24.90202 1.188 24.90241 1.233 24.9028 1.188 24.90321 1.194 24.9036 1.194 24.90399 1.229 24.90439 1.262 24.90479 1.214 24.90519 1.173 24.90558 1.161 24.90597 1.137 24.90638 1.148 24.90677 1.153 24.90717 1.156 24.90757 1.167 24.90796 1.174 24.90836 1.201 24.90876 1.174 24.90916 1.172 24.90955 1.169 24.90994 1.167 24.91035 1.141 24.91074 1.146 24.91113 1.143 24.91153 1.127 24.91193 1.173 24.91233 1.167 24.91273 1.127 24.91312 1.098 24.91353 1.149 24.91394 1.165 24.91433 1.185 24.91473 1.152 24.91514 1.139 24.91553 1.128 24.91594 1.17 24.91634 1.168 24.91674 1.179 24.91714 1.208 24.91755 1.183 24.91794 1.194 24.91835 1.198 24.91875 1.221 24.91914 1.186 24.91955 1.159 24.91995 1.19 24.92035 1.206 24.92075 1.214 24.92115 1.156 24.92155 1.205 24.92196 1.194 24.92235 1.186 24.92275 1.202 24.92315 1.155 24.92354 1.149 24.92393 1.21 24.92433 1.175 24.92472 1.191 24.92513 1.141 24.92552 1.138 24.92592 1.12 24.92631 1.184 24.9267 1.167 24.92709 1.171 24.9275 1.184 24.9279 1.184 24.92829 1.16 24.92868 1.196 24.92907 1.141 24.92947 1.118 24.92987 1.129 24.93027 1.165 24.93066 1.156 24.93105 1.125 24.93145 1.098 24.93185 1.151 24.93225 1.164 24.93264 1.182 24.93303 1.144 24.93343 1.116 24.93383 1.11 24.93422 1.148 24.93462 1.139 24.93501 1.155 24.93541 1.192 24.9358 1.189 24.9362 1.182 24.9366 1.209 24.93699 1.179 24.93739 1.144 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