J/MNRAS/442/844  BVRI light curves of type II-P supernovae      (Faran+, 2014)

Photometric and spectroscopic properties of Type II-P supernovae. Faran T., Poznanski D., Filippenko A.V., Chornock R., Foley R.J., Ganeshalingam M., Leonard D.C., Li W., Modjaz M., Nakar E., Serduke F.J.D., Silverman J.M. <Mon. Not. R. Astron. Soc., 442, 844-861 (2014)> =2014MNRAS.442..844F 2014MNRAS.442..844F
ADC_Keywords: Supernovae ; Photometry, UBVRI Keywords: supernovae: general Abstract: We study a sample of 23 Type II plateau supernovae (SNe II-P), all observed with the same set of instruments. Analysis of their photometric evolution confirms that their typical plateau duration is 100 d with little scatter, showing a tendency to get shorter for more energetic SNe. We examine the claimed correlation between the luminosity and the rise time from explosion to plateau. We analyse their spectra, measuring typical ejecta velocities, and confirm that they follow a well-behaved power-law decline. We find indications of high-velocity material in the spectra of six of our SNe. We test different dust-extinction correction methods by asking the following - does the uniformity of the sample increase after the application of a given method? A reasonably behaved underlying distribution should become tighter after correction. No method we tested made a significant improvement. Description: Imaging was obtained with the 0.76m Katzman Automatic Imaging Telescope (KAIT), the SN search engine of LOSS. The sample was compiled from events for which precise photometry could be obtained - that is, for which template images were obtained after the SN had faded. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 39 23 SN sample table2.dat 73 448 Partial photometric data of the KAIT sample table3.dat 58 137 Sample journal of spectroscopic observations -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- SN SN name (YYYYaa) 8- 13 F6.4 --- zhost Redshift of host galaxy 15- 19 F5.2 mag MOD Distance modulus 20 A1 --- n_MOD [nb] Origin of MOD: n=NED, b=from redshift 22- 26 I5 d MJD0 [51251/53549]?=- Explosion MJD 28- 31 F4.1 d e_MJD0 [0.5/67]? rms uncertainty on MJD0 32 A1 --- f_MJD0 [?] Uncertainty flag on e_MJD0 34- 39 F6.4 mag E(B-V) Galactic redenning E(B-V)MW, assuming RV=3.1 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- SN SN name (YYYYaa) 8- 15 F8.2 d MJD Modified Julian date of observation 17- 21 F5.1 d Age [1.8/343]?=- Days since explosion 23- 28 F6.3 mag Bmag ?=- B magnitude 30- 34 F5.3 mag e_Bmag ? rms uncertainty on Bmag 36- 41 F6.3 mag Vmag ?=- V magnitude 43- 47 F5.3 mag e_Vmag ? rms uncertainty on Vmag 49- 54 F6.3 mag Rmag ?=- R magnitude 56- 60 F5.3 mag e_Rmag ? rms uncertainty on Rmag 62- 67 F6.3 mag Imag ?=- I magnitude 69- 73 F5.3 mag e_Imag ? rms uncertainty on Imag -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- SN SN Name (YYYYaa) 8- 15 F8.2 d MJD Modified Julian date of observation 17- 22 F6.1 d Age [2.8/1146]?=- Days since explosion 24- 42 A19 --- Inst Instrument 44- 47 I4 0.1nm lam.min [3050/5600] Lower value of wavelength range 48 A1 --- --- [-] 49- 53 I5 0.1nm lam.max [5500/11000] Upper value of wavelength range 55- 58 I4 s Texp Exposure time -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 25-Feb-2015
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