J/ApJ/741/97         Light curves of Ibc supernovae              (Drout+, 2011)

The first systematic study of type Ibc supernova multi-band light curves. Drout M.R., Soderberg A.M., Gal-Yam A., Cenko S.B., Fox D.B., Leonard D.C., Sand D.J., Moon D.-S., Arcavi I., Green Y. <Astrophys. J., 741, 97 (2011)> =2011ApJ...741...97D 2011ApJ...741...97D
ADC_Keywords: Supernovae ; Photometry, VRI Keywords: supernovae: general - gamma-ray burst: general Abstract: We present detailed optical photometry for 25 Type Ibc supernovae (SNe Ibc) within d∼150Mpc obtained with the robotic Palomar 60 inch telescope in 2004-2007. This study represents the first uniform, systematic, and statistical sample of multi-band SNe Ibc light curves available to date. We correct the light curves for host galaxy extinction using a new technique based on the photometric color evolution, namely, we show that the (V-R) color of extinction-corrected SNe Ibc at Δt∼10days after V-band maximum is tightly distributed, <(V-R)V10≥0.26±0.06mag. Using this technique, we find that SNe Ibc typically suffer from significant host galaxy extinction, <E(B-V)≳0.4mag. A comparison of the extinction-corrected light curves for helium-rich (Type Ib) and helium-poor (Type Ic) SNe reveals that they are statistically indistinguishable, both in luminosity and decline rate. We report peak absolute magnitudes of <MR≥-17.9±0.9 mag and <MR≥-18.3±0.6mag for SNe Ib and Ic, respectively. Description: We used the robotic Palomar 60 inch telescope, in 2004-2007, to obtain multi-epoch, multi-band optical observations (R-, V-bands) for our 25 SNe follow-up campaign. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 72 25 Sample of type Ibc supernovae table2.dat 37 842 P60 Photometry (from erratum 2012,ApJ,753,180) refs.dat 84 38 References -------------------------------------------------------------------------------- See also: B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- SN Supernova name (YYYYaa) 8- 10 A3 --- n_SN [c-i, ] Individual notes on SN (1) 12- 24 A13 --- Gal Host galaxy designation 26- 28 I3 Mpc Dist [17/115] Distance 30- 31 I2 Mpc e_Dist Distance uncertainty 32- 34 A3 --- n_Dist [dhe, ] Origin of Dist (1) 36 A1 --- u_Inc [~] Uncertainty flag on Inc 37- 38 I2 deg Inc [28/90]? Inclination 40- 43 F4.1 deg E_Inc ? Positive error on Inc 45- 48 F4.1 deg e_Inc ? Negative error on Inc 50- 54 F5.3 mag E(B-V) Estimated Milky Way extinction from Schlegel et al. (1998ApJ...500..525S 1998ApJ...500..525S) 56- 60 A5 --- Dref Discovery circular number (2) 62- 66 A5 --- SpT SN spectral type (IIb, Ib, Ibn, Ic or Ic-BL) 68- 72 A5 --- Cref Classification circular number (2) -------------------------------------------------------------------------------- Note (1): Flag as follows: c = P60 observations conducted under the Caltech Core-Collapse Supernova Program. d = Redshift-independent distance. e = Host galaxy is a member of the Virgo cluster. Distance is adopted from Mould et al. (2000ApJ...529..786M 2000ApJ...529..786M). f = Previous photometry has been published by Gal-Yam et al. (2005ApJ...630L..29G 2005ApJ...630L..29G). g = Previous photometry has been published by Pastorello et al. (2008MNRAS.389..131P 2008MNRAS.389..131P). h = Distance is derived from the host galaxy redshift reported in (Antilogus et al. 2006ATel..854....1A 2006ATel..854....1A). i = Previous photometry has been published by Foley et al. (2007ApJ...657L.105F 2007ApJ...657L.105F) and Pastorello et al. (2007Natur.447..829P 2007Natur.447..829P). Note (2): Entries refer to electronic circular numbers prefaced by "I" (IAUC), "C" (CBET), or "A" (ATEL), and the full references are listed in refs.dat file. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- SN Supernova name 10 A1 --- Filt [RV] Filter used in the observation (R or V) 12- 13 I2 --- Ref [1/22]? Origin of data (1) 15- 23 F9.1 d JD [2453219/2454160] Observation Julian Date 25- 26 A2 --- l_mag [≤] Limiting flag on mag 28- 32 F5.2 mag mag [13.62/20.68] Observed magnitude in Filt 34- 37 F4.2 mag e_mag [0/0.24]? Uncertainty in mag -------------------------------------------------------------------------------- Note (1): Flag as follows: 1 = Plotted data are supplemented by photometry in IAUC8377. 2 = Plotted data are supplemented by photometry in IAUC8381. 3 = Plotted data are supplemented by photometry in IAUC8425. 4 = Plotted data are supplemented by photometry in IAUC8425. 5 = Plotted data are supplemented by photometry in IAUC8443. 6 = Plotted data are supplemented by photometry in IAUC8446, CBET99. 7 = Plotted data are supplemented by photometry in IAUC8452. 8 = Plotted data are supplemented by photometry in IAUC8454. 9 = Plotted data are supplemented by photometry in IAUC8454. 10 = Plotted data are supplemented by photometry in IAUC8503, CBET130. 11 = Plotted data are supplemented by photometry in IAUC8605. 12 = Plotted data are supplemented by photometry in IAUC8623. 13 = Plotted data are supplemented by photometry in IAUC8639. 14 = Plotted data are supplemented by photometry in Pastorello et al. (2008MNRAS.389..131P 2008MNRAS.389..131P). 15 = Plotted data are supplemented by photometry in IAUC8639. 16 = Plotted data are supplemented by photometry in IAUC8658. 17 = Plotted data are supplemented by photometry in IAUC8669. 18 = Plotted data are supplemented by photometry in IAUC8713. 19 = Plotted data are supplemented by photometry in IAUC8728. 20 = Plotted data are supplemented by photometry in Foley et al. (2007ApJ...657L.105F 2007ApJ...657L.105F) and Pastorello et al. (2007Natur.447..829P 2007Natur.447..829P). 21 = Plotted data are supplemented by photometry in IAUC8792. 22 = Plotted data are supplemented by photometry in IAUC8794. -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Ref Reference code 7- 25 A19 --- BibCode Bibcode 27- 46 A20 --- Aut Author's name 48- 84 A37 --- Other Other reference -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 25-Feb-2013
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