J/MNRAS/394/2266 SN 2005cs one-year photometry (Pastorello+, 2009)
SN 2005cs in M51.
II. Complete evolution in the optical and the near-infrared.
Pastorello A., Valenti S., Zampieri L., Navasardyan H., Taubenberger S.,
Smartt S.J., Arkharov A.A., Barnbantner O., Barwig H., Benetti S.,
Birtwhistle P., Botticella M.T., Cappellaro E., Del Principe M.,
Di Mille F., Di Rico G., Dolci M., Elias-Rosa N., Efimova N.V., Fiedler M.,
Harutyunyan A., Hoflich P.A., Kloehr W., Larionov V.M., Lorenzi V.,
Maund J.R., Napoleone N., Ragni M., Richmond M., Ries C., Spiro S.,
Temporin S., Turatto M., Wheeler J.C.
<Mon. Not. R. Astron. Soc., 394, 2266-2282 (2009)>
=2009MNRAS.394.2266P 2009MNRAS.394.2266P
ADC_Keywords: Supernovae ; Photometry, UBVRI ; Photometry, infrared
Keywords: supernovae: general - supernovae: individual: SN 2005cs -
supernovae: individual: SN 1997D - supernovae: individual: SN 1999br -
supernovae: individual: SN 2003Z - galaxies: individual: M51
Abstract:
We present the results of the one-year long observational campaign of
the type II plateau SN 2005cs, which exploded in the nearby spiral
galaxy M51 (the Whirlpool galaxy). This extensive data set makes SN
2005cs the best observed low-luminosity, 56Ni-poor type II plateau
event so far and one of the best core-collapse supernovae ever.
Description:
The systematic photometric monitoring of SN 2005cs began on 2005 June
30, 3d after the SN discovery. However, earlier unfiltered images
obtained by amateur astronomers were also collected. These data are
particularly important because they show the light-curve evolution
soon after the shock breakout. There is no evidence of the SN presence
in images obtained on 2005 June 26, but the SN was clearly visible the
subsequent day. The SN was then followed for one year (until 2006
July) in the optical bands, and until 2006 December in the NIR. A few
optical observations obtained in 2007 show no trace of the SN.
Objects:
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RA (2000) DE Designation(s)
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13 29 53.4 +47 10 28 SN 2005cs = SN 2005cs
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2.dat 106 89 *UBVRIz magnitudes of SN 2005cs
table3.dat 66 38 *Early time BVR magnitudes of SN 2005cs from
amateur observations
table4.dat 62 24 *JHK magnitudes of SN 2005cs
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Note on table2.dat: The errors take into account both measurement errors and
uncertainties in the photometric calibration. The observations presented in
Paper I (2006MNRAS.370.1752P 2006MNRAS.370.1752P) are also reported, recalibrated with the new
sequence of stars identified in Fig. 1.
Note on table3.dat: The errors take into account both measurement errors and
uncertainties in the photometric calibration. The B-band magnitudes are
derived from filtered images. All other images were unfiltered, but rescaled
to the V- or R-band photometry depending on the peak of the quantum-efficiency
curve of the detectors used by the amateurs (see also the discussion in
Pastorello et al., 2008, Cat. J/MNRAS/389/955).
Note on table4.dat: The errors take into account both measurement errors and
uncertainties in the photometric calibration.
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See also:
B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)
Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 10 A10 "DD/MM/YYYY" Date Observation date
12- 21 F10.2 d JD Julian date
23 A1 --- l_Umag Limit flag on Umag
24- 29 F6.3 mag Umag ? U magnitude
31- 35 F5.3 mag e_Umag ? rms uncertainty on Umag
37 A1 --- l_Bmag Limit flag on Bmag
38- 43 F6.3 mag Bmag ? B magnitude
45- 49 F5.3 mag e_Bmag ? rms uncertainty on Bmag
51 A1 --- l_Vmag Limit flag on Vmag
52- 57 F6.3 mag Vmag ? V magnitude
59- 63 F5.3 mag e_Vmag ? rms uncertainty on Vmag
65 A1 --- l_Rmag Limit flag on Rmag
66- 71 F6.3 mag Rmag ? R magnitude
73- 77 F5.3 mag e_Rmag ? rms uncertainty on Rmag
79 A1 --- l_Imag Limit flag on Imag
80- 85 F6.3 mag Imag ? I magnitude
87- 91 F5.3 mag e_Imag ? rms uncertainty on Imag
93- 98 F6.3 mag zmag ? z magnitude
100-104 F5.3 mag e_zmag ? rms uncertainty on zmag
106 I1 --- Inst [1/8] Instrument code (1)
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Note (1): Instrument code as follows:
1 = 0.8-m Wendelstein Telescope + MONICA (University Observatory
Munich, Mt Wendelstein, Germany)
2 = 2.2-m Calar Alto Telescope + CAFOS (German-Spanish Astronomical
Center, Sierra de Los Filabres, Andalucia Spain)
3 = 1.82-m Copernico Telescope + AFOSC (INAF - Osservatorio
Astronomico di Asiago, Mt Ekar, Asiago, Italy)
4 = 8.2-m Subaru Telescope + FOCAS (National Astronomical Observatory
of Japan, Mauna Kea, Hawaii, US)
5 = 0.72-m Teramo-Normale Telescope + CCD camera (INAF -
Osservatorio Astronomico di Collurania, Teramo, Italy)
6 = 2.0-m Liverpool Telescope + RatCAM (La Palma, Spain)
7 = 3.58-m Telescopio Nazionale Galileo + Dolores (Fundacion Galileo
Galilei - INAF, La Palma, Spain)
8 = 1.52-m Cassini Telescope + BFOSC (INAF - Osservatorio Astronomico
di Bologna, Loiano, Italy)
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 10 A10 "DD/MM/YYYY" Date Observation date
12- 21 F10.2 d JD Julian date
23 A1 --- l_Bmag Limit flag on Bmag
24- 29 F6.3 mag Bmag ? B magnitude
31- 35 F5.3 mag e_Bmag ? rms uncertainty on Bmag
37 A1 --- l_Vmag Limit flag on Vmag
38- 43 F6.3 mag Vmag ? V magnitude
45- 49 F5.3 mag e_Vmag ? rms uncertainty on Vmag
51 A1 --- l_Rmag Limit flag on Rmag
52- 57 F6.3 mag Rmag ? R magnitude
59- 63 F5.3 mag e_Rmag ? rms uncertainty on Rmag
65 A1 --- Inst [A-J] Instrument code (1)
66 A1 --- n_Inst [+] +: Photometry obtained from images with
filters
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Note (1): Instrument code as follows:
A = 80-mm Skywatcher ED80 Refractor Telescope + SBIG ST-7 Dual CCD
Camera with KAF-0400 (I. Uhl, Rheinzabern, Germany)
B = 0.2-m Orion SVP Reflector Telescope + Starlight Xpress MX5C CCD
Camera (C. McDonnell, Holliston, Massachusetts, US)
C = 0.4-m Newton Telescope + ERG110 CCD (Osservatorio Astronomico
Geminiano Montanari, Cavezzo, Modena, Italy)
D = 0.35-m Maksutov Newtonian Reflector Telescope + SBIG ST10XME CCD
Camera with KAF-3200ME (M. Fiedler, Astroclub Radebeul, Germany)
E = 0.356-m Celestron 14 CGE Telescope + SBIG ST-2000 CCD (P. Marek,
Skymaster Observatory, Variable Star Section of Czech
Astronomical Society, Borovinka, Czech Republic)
F = 0.4-m Meade Schmidt-Cassegrain Telescope + Marconi (E2V) CCD
47-10 (P. Birtwhistle, Great Shefford Observatory, West
Berkshire, England)
G = 0.203-m f/4.0 Meade Newtonian Reflector Telescope + DSI-Pro II
CCD Camera (W. Kloehr, Schweinfurt, Germany)
H = 0.28-m Celestron 11 + MX7-C CCD (U. Bietola, Gruppo Imperiese
Astrofili, Imperia, Italy)
I = 0.20-m Celestron 8 SCT + Starlight Xpress MX916 CCD (P. Corelli,
Mandi Observatory, Pagnacco, Udine, Italy)
J = 0.25-m Newton f/4.8 Telescope + StarLight Xpress SXL8 CCD (T.
Scarmato, Toni Scarmato's Observatory, San Costantino di
Briatico, Vibo Valentia, Italy)
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Byte-by-byte Description of file: table4.dat
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Bytes Format Units Label Explanations
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1- 10 A10 "DD/MM/YYYY" Date Observation date
12- 21 F10.2 d JD Julian date
23- 28 F6.3 mag Jmag ? J magnitude
30- 34 F5.3 mag e_Jmag ? rms uncertainty on Jmag
36- 41 F6.3 mag Hmag ? H magnitude
43- 47 F5.3 mag e_Hmag ? rms uncertainty on Hmag
49- 54 F6.3 mag Kmag ? K magnitude
56- 60 F5.3 mag e_Kmag ? rms uncertainty on Kmag
62 A1 --- Inst [1/2] Instrument code (1)
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Note (1): Instrument code as follows:
1 = 1.08-m AZT24 Telescope + SWIRCAM (Pulkovo Observatory, St
Petersburg, Russia + INAF-Osservatori Astronomici di Roma and
Teramo, Stazione di Campo Imperatore, Italy);
2 = 3.58-m Telescopio Nazionale Galileo + NICS (Fundacion Galileo
Galilei - INAF, La Palma, Spain).
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History:
From electronic version of the journal
References:
Pastorello et al., Paper I 2006MNRAS.370.1752P 2006MNRAS.370.1752P
(End) Patricia Vannier [CDS] 17-Nov-2010