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J/PAZh/35/451       Light Curves of RS Pup                  (Berdnikov+, 2009)

Search for Evolutionary Changes in Cepheid Periods Using the Harvard Plate Collection: RS Puppis. Berdnikov L.N., Henden A.A., Turner D.G., Pastukhova E.N. <Pis'ma Astron. Zh. 35, 451 (2009)> =2009PAZh...35..451B =2009AstL...35..406B
ADC_Keywords: Stars, variable ; Photometry Keywords: Cepheids - period variability - stellar evolution Abstract: Based on photographic plates from the Harvard College Observatory, we have made 1492 magnitude estimates for the long-period classical Cepheid RS Pup (P=41.4d). Together with the observations taken from the literature, our data have allowed us to construct an O-C diagram spanning a time interval of 135-years. Objects: --------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------- 08 13 04.2 -34 34 43 RS Pup = V* RS Pup --------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 80 48 Times of maximum light for RS Pup table3.dat 17 200 Standard B and V light curves for RS Pup
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 10 F10.2 d JD Julian date of maximum light 12- 15 F4.2 d e_JD Error on JD 17- 19 A3 --- Filt [PG VIS] Filter 21- 24 I4 --- E Epoch number 26- 30 F5.2 d O-C O-C residuals 32- 34 I3 --- N Number of observations 36- 80 A45 --- Ref Data source
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 5 F5.3 --- Phase [0/1] Phase 7- 11 F5.3 mag Bmag B magnitude 13- 17 F5.3 mag Vmag V magnitude
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 26-Jun-2009
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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