J/ApJS/241/38   A comprehensive analysis of Spitzer supernovae   (Szalai+, 2019)

A comprehensive analysis of Spitzer supernovae. Szalai T., Zsiros S., Fox O.D., Pejcha O., Muller T. <Astrophys. J. Suppl. Ser., 241, 38 (2019)> =2019ApJS..241...38S 2019ApJS..241...38S
ADC_Keywords: Supernovae; Photometry, infrared; Stars, distances Keywords: circumstellar matter ; infrared: stars ; supernovae: general Abstract: The mid-infrared (mid-IR) wavelength regime offers several advantages for following the late-time evolution of supernovae (SNe). First, the peaks of the SN spectral energy distributions shift toward longer wavelengths, following the photospheric phase. Second, mid-IR observations suffer less from effects of interstellar extinction. Third, and perhaps most important, the mid-IR traces dust formation and circumstellar interaction at late times (>100 days) after the radioactive ejecta component fades. The Spitzer Space Telescope has provided substantial mid-IR observations of SNe since its launch in 2003. More than 200 SNe have been targeted, but there are even more SNe that have been observed serendipitously. Here we present the results of a comprehensive study based on archival Spitzer/IRAC images of more than 1100 SN positions; from this sample, 119 SNe of various subclasses have been detected, including 45 SNe with previously unpublished mid-IR photometry. The photometry reveals significant amounts of warm dust in some cases. We perform an in-depth analysis to constrain the origin and heating mechanism of the dust, and present the resulting statistics. Description: Here we presented a comprehensive study of all SNe (discovered before 2015) observed with Spitzer/IRAC, both targeted and untargeted. In total, we increased the published sample of Spitzer SNe by a factor of ∼5x (from ∼200 to ∼1100), including nearly ∼2x more detections (∼70 to ∼120). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 91 113 Basic parameters of the studied SNe with positive Spitzer detection table5.dat 89 77 Mid-IR fluxes of SNe with previously unreported Spitzer photometry table6.dat 70 335 3.6 and 4.5um absolute Vega magnitudes of all SNe positively detected by Spitzer/IRAC refs.dat 69 149 References -------------------------------------------------------------------------------- See also: B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-) J/ApJ/663/320 : IR-through-UV extinction curve (Fitzpatrick+, 2007) J/A+A/538/A120 : A unified supernova catalogue (Lennarz+, 2012) J/ApJ/756/173 : Photometry of SNe II 2005ip & 2006jd (Stritzinger+, 2012) J/MNRAS/433/1312 : SN2009ip UBVRI, UVOT and JHK light curves (Fraser+, 2013) J/ApJ/778/L19 : SN 2011dh (type IIb) 3.6 & 4.5um LCs (Helou+, 2013) J/other/Nat/494.65 : SN 2010mc outburst before explosion (Ofek+, 2013) J/ApJ/782/42 : Panchromatic observations of PTF11qcj (Corsi+, 2014) J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014) J/A+A/580/A142 : SN 2011dh. The first two years (Ergon+, 2015) J/MNRAS/464/2672 : ASAS-SN bright SN catalog 2013-2014 (Holoien+, 2017) J/ApJ/839/88 : IR transients with Spitzer (SPRITEs) (Kasliwal+, 2017) http://www.cbat.eps.harvard.edu/lists/Supernovae.html : The CBAT list of SNe http://sne.space/ : The Open Supernova Catalog home page http://sha.ipac.caltech.edu/applications/Spitzer/SHA/ : Spitzer archive on IRSA Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- f_ID [*] Flag on ID (G1) 3- 11 A9 --- ID Object identifier 13- 19 A7 --- Type SN type 21- 25 I5 d MJD [49074/56950] Modified Julian Date of discovery 27- 39 A13 --- Host Host Galaxy identifier 41- 42 I2 h RAh Hour of Right Ascension (J2000) 44- 45 I2 min RAm Minute of Right Ascension (J2000) 47- 51 F5.2 s RAs Second of Right Ascension (J2000) 53 A1 --- DE- Sign of the Declination (J2000) 54- 55 I2 deg DEd Degree of Declination (J2000) 57- 58 I2 arcmin DEm Arcminute of Declination (J2000) 60- 64 F5.2 arcsec DEs Arcsecond of Declination (J2000) 66- 70 F5.1 Mpc Dist [3.3/280] Distance 71 A1 --- f_Dist [d] d = Distance calculated from redshift 73- 76 F4.1 Mpc e_Dist [0.2/24.0]? Uncertainty in Dist 79- 82 F4.2 mag E(B-V) [0.01/0.36] The (B-V) color excess 84- 91 A8 --- Ref Reference code(s) (see refs.dat file) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- n_ID [I] Note on ID (1) 3 A1 --- f_ID [*] Flag on ID (G1) 5- 13 A9 --- ID Object identifier 15- 17 A3 --- Meth Photometric methods used on ID (2) 19- 25 A7 --- Type SN type 27- 31 I5 d MJD [53047/57285] Modified Julian Date of the observation 33- 44 A12 --- PID Program identifier of the observation (3) 46- 49 I4 d Epoch [8/1735] Days since discovery 51- 54 I4 uJy F3.6 [5/3640]? Spitzer/IRAC 3.6um band flux density 55 A1 --- f_F3.6 [n] Flag on F3.6 (G2) 57- 59 I3 uJy e_F3.6 [5/112]? Uncertainty in F3.6 61- 64 I4 uJy F4.5 [5/2903]? Spitzer/IRAC 4.5um band flux density 65 A1 --- f_F4.5 [n] Flag on F4.5 (G2) 67- 68 I2 uJy e_F4.5 [4/96]? Uncertainty in F4.5 70- 72 I3 uJy F5.8 [14/481]? Spitzer/IRAC 5.8um band flux density 73 A1 --- f_F5.8 [n] Flag on F5.8 (G2) 75- 76 I2 uJy e_F5.8 [8/50]? Uncertainty in F5.8 78- 80 I3 uJy F8.0 [54/859]? Spitzer/IRAC 8.0um band flux density 81 A1 --- f_F8.0 [n] Flag on F8.0 (G2) 83- 85 I3 uJy e_F8.0 [14/105]? Uncertainty in F8.0 87- 89 A3 --- Targ SN-targeted? ("Yes", 41 occurrences; or "No") -------------------------------------------------------------------------------- Note (1): I = The image subtraction can not be applied (in all these cases, measured fluxes can be handled only as upper limits). Note (2): Methods as follows: a = aperture photometry on the original images; b = photometry after subtracting a very late-time image + flux differences c = photometry after subtracting a pre-explosion image + flux differences; d = "Fox+11 method" (2011ApJ...741....7F 2011ApJ...741....7F). Note (3): Program identifier as follows: e = 3641 (PI van Dyk); f = 159 (PI Kennicutt); g = 20256 (PI Meikle); h = 69 (PI Fazio); i = 3672 (PI Mazzarella); j = 80072 (PI Tully); k = 30292 (PI Meikle); m = 40619 (PI Kotak); n = 50111 (PI McGaugh); o = 80089 (PI Sanders); p = 61060 (PI Sheth); q = 30496 (PI Fisher); r = 80254 (PI Stern); s = 61065 (PI Sheth); t = 61003 (PI Freedman); u = 61009 (PI Freedman); v = 60166 (PI Garnavich); w = 11053 (PI Fox); x = 70008 (PI Andrews); y = 80131 (PI Andrews); z = 70038 (PI Sanders); ε = 10139 (PI Fox); ζ = 90137 (PI Fox); α = 61066 (PI Sheth); β = 61062 (PI Sheth); γ = 10046 (PI Sanders); δ = 80023 (PI Fox); ϕ = 90178 (PI Andrews); η = 80069 (PI Beygu); ϑ = 10152 (PI Kasliwal); ι = 10136 (PI Kasliwal); κ = 800025 (PI van Zee); µ = 80196 (PI Kasliwal); ν = 11063 (PI Kasliwal). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- n_ID [I] Note on ID (1) 3- 11 A9 --- ID Object identifier 13 A1 --- f_ID [D] Flag on ID (2) 15- 21 A7 --- Type SN type 23- 27 I5 d MJD [52948/57855] Modified Julian Date of the observation 29 A1 --- f_MJD Flag on MJD (3) 31- 34 I4 d Epoch [2/7746] Days since discovery 36- 41 F6.2 mag 3.6Mag [-22.3/-10.4]? Absolute Spitzer/IRAC 3.6um band magnitude 42 A1 --- f_3.6Mag [n] Flag on 3.6Mag (G2) 44- 47 F4.2 mag e_3.6Mag [0.05/1.51]? Uncertainty in 3.6Mag 49- 54 F6.2 mag 4.5Mag [-22.9/-10.7]? Absolute Spitzer/IRAC 4.5um band magnitude 55 A1 --- f_4.5Mag [n] Flag on 4.5Mag (G2) 57- 60 F4.2 mag e_4.5Mag [0.06/1.4]? Uncertainty in 4.5Mag 62- 70 A9 --- Ref Source for fluxes, distances, epochs and E(B-V) values (see refs.dat file) -------------------------------------------------------------------------------- Note (1): I = The image subtraction can not be applied. Note (2): D = In the case of SN 2009ip, epochs are given regarding the SN-like outburst observed in 2012. Data marked with italic denote cases where image subtraction can not be applied. Note (3): Sources of new data of previously known positive Spitzer targets (PID): a = 90174 (PI Fox); b = 10139 (PI Fox); c = 11053 (PI Fox); d = 12099 (PI Fraser); e = 13053 (PI Kasliwal); f = 11063 (PI Kasliwal). -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref Reference code 5- 23 A19 --- BibCode Bibcode of the reference 25- 45 A21 --- Auth First author's name(s) 47- 69 A23 --- Comm Comment -------------------------------------------------------------------------------- Global notes: Note (G1): * = Positive detection based on single-epoch imaging, see text for details. Note (G2): D = no point source at the position of the SN in this band. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 29-Nov-2019
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