2025RNAAS...9....5J


Query : 2025RNAAS...9....5J

2025RNAAS...9....5J - Research Notes of the AAS, 9, 5 (2025/January-0)

An Updated Detection Pipeline for Precursor Emission in Type II Supernova 2020tlf.

JACOBSON-GALAN W.V., GONZALEZ S., PATEL S., DESSART L., JONES D.O., COPPEJANS D.L., DIMITRIADIS G., FOLEY R.J., KILPATRICK C.D., MATTHEWS D.J., REST S., TERRERAN G., ALEO P.D., AUCHETTL K., BLANCHARD P.K., COULTER D.A., DAVIS K.W., DE BOER T.J.L., DEMARCHI L., DROUT M.R., EARL N., GAGLIANO A., GALL C., HJORTH J., HUBER M.E., IBIK A.L., MILISAVLJEVIC D., PAN Y.-C., REST A., RIDDEN-HARPER R., ROJAS-BRAVO C., SIEBERT M.R., SMITH K.W., TAGGART K., TINYANONT S., WANG Q. and ZENATI Y.

Abstract (from CDS):

We present a new photometric pipeline for the detection of pre-supernova (pre-SN) emission in the Young Supernova Experiment (YSE) sky survey. The method described is applied to SN 2020tlf, a type II SN with precursor emission in the last ∼100 days before first light. We re-analyze the YSE griz-band light curves of SN 2020tlf and provide revised pre-explosion photometry that includes a robust list of confident detection and limiting magnitudes. Compared to the results of W. V. Jacobson-Galán et al., this new analysis yields fewer total r/i/z-band pre-SN detections at phases >-100 days. Furthermore, we discourage the use of the blackbody modeling of the pre-explosion spectral energy distribution, the pre-SN bolometric light curve and the blackbody model parameters presented in W. V. Jacobson-Galán et al. Nevertheless, binned photometry of SN 2020tlf confirms a consistent progenitor luminosity of ∼1040 erg s–1 before explosion.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Supernovae - Sky surveys

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 2020tlf SN* 14 40 10.030 +42 46 39.64           SNII(n) 55 0

Query : 2025RNAAS...9....5J

Basic data :
SN 2020tlf -- SuperNova
Other object types:
otypes_help
ev (AT,ATLAS), SN* (SN)
ICRS coord. (ep=J2000) :
14 40 10.030 +42 46 39.64 [ ] D 2020ATel14024....1D
FK4 coord. (ep=B1950 eq=1950) :
14 38 15.982 +42 59 29.39 [ ]
Gal coord. (ep=J2000) :
075.382041 +62.971933 [ ]
Radial velocity / Redshift / cz :
V(km/s) 2389 [~] / z(~) 0.008 [~] / cz 2398 [~]
   D 2020ATel14024....1D
Spectral type:
SNII(n) C 2020ATel14024....1D
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Identifiers (3) :
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SN 2020tlf AT 2020tlf ATLAS 20bbft

References (55 between 1850 and 2026) (Total 55)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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