J/ApJ/943/L15     SN 2021zby optical light curves and spectra     (Wang+, 2023)

Revealing the progenitor of SN 2021zby through analysis of the TESS shock- cooling light curve. Wang Q., Armstrong P., Zenati Y., Ridden-Harper R., Rest A., Arcavi I., Kilpatrick C.D., Foley R.J., Tucker B.E., Lidman C., Killestein T.L., Shahbandeh M., Anderson J.P., Angulo R., Ashall C., Burke J., Chen T.-W., von Coelln S., Dalrymple K.A., Davis K.W., Fulton M.D., Galbany L., Gonzalez E.P., Gao B., Gromadzki M., Howell D.A., Ihanec N., Jencson J.E., Jones D.O., Lyman J.D., McCully C., Muller-Bravo T.E., Newsome M., Nicholl M., O'Neill D., Pellegrino C., Rest S., Smartt S.J., Smith K., Srivastav S., Terreran G., Tinyanont S., Young D.R., Zenteno A. <Astrophys. J., 943, L15 (2023)> =2023ApJ...943L..15W 2023ApJ...943L..15W
ADC_Keywords: Supernovae; Photometry; Optical; Spectra, optical; Spectra, infrared Keywords: Core-collapse supernovae ; Supernovae Abstract: We present early observations and analysis of the double-peaked Type IIb supernova (SN IIb) SN 2021zby. TESS captured the prominent early shock-cooling peak of SN 2021zby within the first ∼10 days after explosion with a 30 minute cadence. We present optical and near-infrared spectral series of SN 2021zby, including three spectra during the shock-cooling phase. Using a multiband model fit, we find that the inferred properties of its progenitor are consistent with a red supergiant or yellow supergiant, with an envelope mass of ∼0.30-0.65M and an envelope radius of ∼120-300R. These inferred progenitor properties are similar to those of other SNe IIb with a double-peaked feature, such as SNe 1993J, 2011dh, 2016gkg, and 2017jgh. This study further validates the importance of the high cadence and early coverage in resolving the shape of the shock-cooling light curve, while the multiband observations, particularly UV, are also necessary to fully constrain the progenitor properties. Description: ATLAS observed SN 2021zby throughout the preexplosion and double-peaked stage in the o band, and also in the postpeak stage in both o and c bands. We also obtained ground-based photometric follow-up in the postpeak stage with DECam on the Cerro Tololo Inter-American Observatory (CTIO) 4-m Blanco telescope in the r and i bands. TESS observed SN 2021zby in full-frame images (FFIs) for sectors 42, 43, and 44, at a 10 minute cadence. In addition, we obtained optical spectra from multiple ground-based observatories including the Wide-Field Spectrograph (WiFeS) on the 2.3m telescope at Siding Spring Observatory (SSO), the IDS long-slit spectrograph on the 2.5m Isaac Newton Telescope (INT), the Kast spectrograph on the 3m Shane Telescope at Lick Observatory, the ESO Faint Object Spectrograph and Camera (EFOSC2) on the ESO New Technology Telescope (NTT, as part of the ePESSTO+ survey; Smartt+ 2015, J/A+A/579/A40), the Spectrograph for the Rapid Acquisition of Transients (SPRAT) on the Liverpool Telescope, and the Las Cumbres Observatory FLOYDS spectrographs mounted on the 2-meter Faulkes Telescope North (FTN) and South (FTS) at Haleakala Observatory and SSO, respectively, through the Global Supernova Project. We obtained an NIR spectrum of SN 2021zby on 2021 September 25 using the SpeX spectrograph on the NASA InfraRed Telescope Facility (IRTF). We used the low-resolution prism mode with the 0.8" slit, providing a resolving power of R∼75 with a simultaneous coverage between 0.7 and 2.5um. Objects: ---------------------------------------------------------- RA (ICRS) DE Designation(s) ---------------------------------------------------------- 03 00 35.62 +11 50 29.7 SN 2021zby = SN 2021zby ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 114 13 Log of spectroscopic observations of SN 2021zby atlas.dat 134 163 ATLAS light curve of SN 2021zby (data behind Figure 1) decam.dat 98 42 CTIO/DECam light curve of SN 2021zby (data behind Figure 1) tess.dat 109 3396 Unbinned TESS light curve of SN 2021zby (data behind Figure 1) tess-bin.dat 97 94 Binned TESS light curve of SN 2021zby (data behind Figure 1) fig1/* . 4 TESS (binned and unbinned), ATLAS and CTIO/DECam light curves in MRT format of SN 2021zby fig2/* . 13 Individual spectra in MRT format of SN 2021zby -------------------------------------------------------------------------------- See also: IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017) VIII/77 : HI spectral properties of galaxies (Springob+, 2005) J/ApJ/742/L18 : Follow-up photometry of the SN IIb PTF 11eon (Arcavi+, 2011) J/ApJ/741/97 : Light curves of Ibc supernovae (Drout+, 2011) J/other/Sci/337.444 : RV curves of Galactic massive O stars (Sana+, 2012) J/ApJ/795/44 : PS1 SNe Ia (0.02<z<0.7) griz light curves (Rest+, 2014) J/MNRAS/438/L101 : First month on SN 2013ej (Valenti+, 2014) J/A+A/580/A142 : SN 2011dh. The first two years (Ergon+, 2015) J/A+A/579/A40 : PESSTO catalog (Smartt+, 2015) J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016) J/ApJ/870/L1 : K2 obs. of type Ia supernova SN 2018oh (Dimitriadis+, 2019) J/A+A/656/A61 : SN Ib nebular phase properties (Dessart+, 2021) J/ApJ/908/51 : TESS early LCs of type Ia Supernovae (Fausnaugh+, 2021) J/ApJ/913/143 : Opt. light curves of the type Ic SN 2019stc (Gomez+, 2021) J/ApJ/923/167 : SN 2018agk spectra and NIR-UV light curves (Wang+, 2021) J/ApJ/938/19 : Opt. phot. and sp. monitoring of SN 2019esa (Andrews+, 2022) J/ApJ/924/15 : Final moments. I. Type II SN 2020tlf (Jacobson-Galan+, 2022) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.3 d MJD [59476.7/59543.3] Modified Julian Date 11- 15 F5.2 d Phase-t0 [2.29/67.1] Phase relative to t0 17- 22 F6.2 d Phase-tpk [-21.7/43.1] Phase relative to tpeak 24- 37 A14 --- Tel Telescope / Instrument 39- 42 I4 --- Range1 [3256/6848] Wavelength lower range 43 A1 --- --- [-] 44- 48 I5 --- Range2 [7994/25378] Wavelength upper range 50- 114 A65 --- FileName Name of the MRT file in subdirectory "fig2"; column added by CDS -------------------------------------------------------------------------------- Byte-by-byte Description of file: atlas.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 F12.6 d MJD [59461.5/59532.4] Modified Julian date of observation (JD-2400000.5) 14- 20 F7.3 mag mag [-25.1/23.4] Observed magnitude in Filt 22- 27 F6.3 mag e_mag [0.03/30] Uncertainty in mag 29- 33 I5 uJy Flux [-217/11718] Flux in Filt 35- 39 I5 uJy e_Flux [8/14100] Uncertainty in Flux 41 A1 --- Filt [co] Filter 43 I1 --- err [0] err (always "0") 45- 48 F4.2 --- chi/N [0.49/3.2] chi/N 50- 57 F8.5 deg RAdeg Right Ascension (J2000) 59- 66 F8.5 deg DEdeg Declination (J2000) 68- 75 F8.2 pix xpixel xpixel 77- 84 F8.2 pix ypixel ypixel 86- 89 F4.2 --- maj [1.74/3.85] maj 91- 94 F4.2 --- min [1.65/3.32] min 96- 100 F5.1 --- phi [-87/88] phi 102- 107 F6.3 --- apfit [-0.55/-0.32] apfit 109- 113 F5.2 mag mag5sig [14.2/19.8] mag5sig 115- 119 F5.2 --- Sky [14.77/21.56] Sky 121- 134 A14 --- Obs Observation identifier -------------------------------------------------------------------------------- Byte-by-byte Description of file: decam.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.5 d MJD [59498.2/59603.1] Modified Julian date of observation (JD-2400000.5) 13- 30 F18.15 mag mag [17/22]? Observed magnitude in Filt 32- 50 F19.17 mag e_mag [0.06/4]? Uncertainty in mag 52 A1 --- Filt [ri] Filter 54- 75 E22.6 uJy Flux [6e-06/0.0006]? Flux in Filt 77- 98 E22.6 uJy e_Flux [3.8e-06/4.6e-05]? Uncertainty in Flux -------------------------------------------------------------------------------- Byte-by-byte Description of file: tess.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.12 d MJD [59473.6/59498.4] Modified Julian date of observation (JD-2400000.5) 20- 43 F24.19 --- Flux [-513/1451]? Flux 45- 65 F21.17 --- e_Flux [0.2/154]? Uncertainty in Flux 67- 84 F18.15 mag Tmag [15.99/29.54]? TESS magnitude 86- 109 F24.19 mag e_Tmag [0.0008/9255]? Uncertainty in mag -------------------------------------------------------------------------------- Byte-by-byte Description of file: tess-bin.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.12 d MJD [59473.7/59498.2] Modified Julian date of observation (JD-2400000.5) 20- 38 F19.15 --- Flux [-9/608]? Flux 40- 57 F18.14 --- e_Flux [55/378]? Uncertainty in Flux 59- 76 F18.15 mag Tmag [16.94/20.57]? TESS magnitude 78- 97 F20.17 mag e_Tmag [0.14/13]? Uncertainty in mag -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 13-Jan-2025
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