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I point out that Paul's VS and nova discoveries are summarized in IBVS 3923 (13 August 1993). Finder charts are provided for PC1 to PC10. Regards, Mati morel@ozemail.com.au ----- Original Message ----- From: "Taichi Kato" <tkato@kusastro.kyoto-u.ac.jp> To: <vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp>; <vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp> Sent: Monday, April 21, 2003 8:27 PM Subject: [vsnet-chat 6246] History: VS discoveries Paul Camilleri > History: VS discoveries Paul Camilleri > > I noticed (by chance) the following e-mails, which I received from > Paul Camilleri on 1992 December 29. I hope this historical document is > still of interest. > > Regards, > Taichi Kato > === > > VARIABLE STAR DISCOVERIES BY PAUL J. CAMILLERI > NAME > PC1 > 17H 21M 56.2S -51D 25' 26" (2000) > RANGE: 11.0 - (13P > TYPE: MIRA > DATE DISCOVERED 1991 MARCH 15TH > ID. GSC 8353-973 > > PC2 > 16H 35M 38.7S -52D 14' 14" (2000) > RANGE: 10 - 13P > TYPE: MIRA OR SR > DATE DISCOVERED 1991 JULY 15TH > ID. GSC 8337-164 > > PC3 > 16H 39M 18S -54D 04' 36" (2000) > RANGE: 11 - 17P > TYPE: MIRA > DATE DISCOVERED 1991 OCTOBER 9TH > ID. DISCOVERED BY MCNAUGHT IN 1987 > > PC4 > 8H 36M 48.9S -36D 27' 37.9" (2000) > RANGE: 8.5 - 11.0P > TYPE: MIRA > DATE DISCOVERED 1992 MAY 31ST > ID. NSV 4154 > > PC5 > 10H 01M 32S -46D 34'.8 (1950) > RANGE: 9.0 - (13P > TYPE: MIRA > DATE DISCOVERED 1992 JUNE 6TH > ID. NSV 4721, BV141 > > PC6 > 9H 59M 06S -46D 58' (1950) > RANGE: 10 - (12PV > TYPE: MIRA > DATE DISCOVERED 1992 JUNE 6TH. > ID. ? > > PC7 > 14H 47M 42S -54D 34' (1950) > RANGE: 11 - (12PV > TYPE:MIRA > DATE DISCOVERED 1992 JULY 26 > ID. NSV 6825 > DISCOVERED BY ROB MCNAUGHT IN 1987 > PC8 > 12h 37m 24s -57d 09' (1950) > RANGE: 10.5 - 12.0PV > TYPE: ?? > DATE DISCOVERED 1992 DECEMBER 01ST > ID. POSSIBLE STAR 2023 IN CARBON STAR CATALOGUE > > PC09 > 11h 38m 48s -76d 44' (1950) > RANGE: 11 - (12PV > TYPE: MIRA?? > DATE DISCOVERED 1992 DECEMBER 02ND > ID. ?? > > === > > (PC4)NEW VARIABLE IN PYXIS > POSITION: 08h 36m 48.9s > -36d 27' 37.9" (2000) > > Discovered 1992 May 31 > > Observations:(All observations Photo-Visual) > 1991 Dec. 11 (12pv > 1992 Jan. 05 (12pv > 1992 Feb. 25 ~11pv > 1992 Mar. 06 ~11pv > 1992 Apr. 25 ~9.5pv > 1992 May. 28 ~9.0pv > 1992 May. 30 ~9.0pv > 1992 Jun. 02 9.0v > 1992 Jun. 19 9.5v > 1992 Jun. 23 9.5v > 1992 Oct. 01 (12pv > 1992 Nov. 28 (12pv > 1992 Dec. 13 (13.5v > 1992 Dec. 26 (13.5v > Note: The (PV)Magnitudes were very diffucult to estimate as NSV 4154 > lies a few seconds North of a bright magnitude 9 star, that was > very diffucult to resove on the small scale of the 85mm lens. > > RANGE: 9.0 - (12PV > TYPE: MIRA > > Identifition: > NSV 4154 > Not Listed in the following catalogues: > GCVS 4th ed > 67 - 70th Name list > Symbiotic Star Catalogue > Red Star Catalogue > > > === > > Sorry I forgot to send the Offsets, and the Magnitudes from Alan. > > Comparsion star OffSets for NSV 4154 > Star (+/-0.05 arc minute) > A 13.33E 00.50N > B 01.33W 11.83S > C 02.16W 03.83S > D 00.83W 05.66S > E 04.50E 01.16N > F 01.33E 06.33S > G 06.83W 00.50S > H 02.16W 00.16S > K 03.66E 02.50N > L 01.16E 01.83S > M 01.16W 03.00N > N 00.16W 02.33S > O 03.00E 00.66N > P 01.66E 01.16N > Q 00.33E 01.50N > 94 06.00W 27.33S > 106 07.60W 25.60S > 82 32.00W 14.30S > > Photometry of Comparison for NSV 4154 > > Star V U-B B-V V-R sV s(U-B) s(B-V) s(V-R) > 82 8.25 -0.39 -0.10 - 0.01 0.01 0.01 - > a 8.70 - (+0.37) +0.21 0.01 - - 0.04 > b 9.43 - +0.08 -0.02 0.01 - 0.00 0.01 > 94 9.47 +0.03 +0.20 - 0.04 0.01 0.01 - > c 10.02 - +0.12 +0.02 0.01 - 0.01 0.02 > 106 10.63 +0.17 +0.41 - 0.01 0.02 0.02 - > d 10.84 - +1.76 +1.16 0.03 - 0.06 0.01 > e 11.09 - +0.26 +0.14 0.02 - 0.01 0.02 > f 11.25 - +1.00 +0.57 0.01 - 0.02 0.02 > g 12.30 - +0.82 +0.44 0.03 - 0.02 0.02 > k 12.50 - +0.51 +0.29 0.03 - 0.02 0.03 > h 12.54 - +1.71 +0.94 0.06 - 0.04 0.00 > l 13.13 - +1.27 +0.63 0.02 - 0.01 0.09 > > The B measures of star 'a' were discordant; the second measure, > believed to be correct, is tabulated. > > Cheers,Paul > > === > (Reply on 1992 December 30) > > Dear Paul, > > Many of PC variables have been identified with IRAS-PSC objects, > supporting the Mira classification. > For full description, please see the Catalog. > Will it be possible to distribute your list to our observers for > future monitoring? (although many are located too south in Japan) > > PC1 > IRAS17179-5122 171759.4 -512233 (1950.0) > F12=19.05 F25=8.31 F60=1.44 F100=10.00L > VAR= 1 LRS=31 > > PC2 > IRAS16317-5208 163143.7 -520808 (1950.0) > F12=5.25 F25=1.90 F60=1.90 F100=13.18 > VAR=82 LRS=-1 > > PC3 > IRAS16353-5358 163521.9 -535845 (1950.0) > F12=1.32 F25=0.58 F60=1.32 F100=7.58 > VAR=23 LRS=-1 > > PC5 > 100132 -4634.8 NSV04721 ? 10.5 <13.0 P > IRAS10015-4634 100131.4 -463442 (1950.0) > F12=5.75 F25=1.90 F60=0.76 F100=1.90L > VAR=26 LRS=-1 > 100329.9 -464918 (2000.0) GCSS652 11.4 9.6 - - > > PC6 > IRAS09590-4656 095904.2 -465602 (1950.0) > F12=3.98 F25=1.58 F60=0.69L F100=1.74L > VAR= 0 LRS=-1 > > PC7 > 144742 -5434 NSV06825 ? 11.8 15.2 P > IRAS14474-5433 144729.9 -543358 (1950.0) > F12=19.05 F25=10.96 F60=1.90 F100=25.11L > VAR=12 LRS=24 > > PC8 > IRAS12374-5706 123724.3 -570619 (1950.0) > F12=12.02 F25=3.98 F60=0.69L F100=12.02L > VAR=43 LRS=13 > > Regards, > Taichi Kato >
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