J/A+A/684/A104 J-PLUS SN Normalized Cumulative Rank (Gonzalez-Diaz+, 2024)
Supernova environments in J-PLUS. Normalized cumulative-rank distributions and
stellar-population synthesis combining narrow- and broad-band filters.
Gonzalez-Diaz R., Galbany L., Kangas T., Garcia-Benito R., Anderson P.J.,
Lyman J., Varela J., Oltra L., Logrono Garcia R., Vilella Rojo G.,
Lopez-Sanjuan C., Perez-Torres M.A., Rosales-Ortega F., Mattila S.,
Kuncarayakti H., James P., Habergham S., Vilchez J.M., Alcaniz J.,
Angulo E.R., Cenarro J., Cristobal-Hornillos D., Dupke R., Ederoclite A.,
Hernandez-Monteagudo C., Marin-Franch A., Moles M., Sodre L.Jr,
Vazquez Ramio H.
<Astron. Astrophys. 684, A104 (2024)>
=2024A&A...684A.104G 2024A&A...684A.104G (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, nearby ; Supernovae ; Redshifts ; Photometry, H-alpha ;
Optical ; Ultraviolet ; Energy distributions
Keywords: methods: observational - methods: statistical -
techniques: photometric - supernovae: general - galaxies: general -
galaxies: photometry
Abstract:
We investigate the local environmental properties of 418 supernovae
(SNe) of all types using data from the Javalambre Photometric Local
Universe Survey (J-PLUS), which includes five broad- and seven
narrow-band imaging filters. Our study involves two independent
analyses: 1) the Normalized Cumulative Rank (NCR) method, which
utilizes all 12 single bands along with five continuum-subtracted
narrow-band emission and absorption bands, and 2) simple stellar
population (SSP) synthesis, where we build spectral energy
distributions (SED) of the surrounding 1kpc2 SN environment using
the 12 broad- and narrow-band filters. Improvements over previous
works include: (i) the extension of the NCR technique to other filters
(broad and narrow) and using a set of homogeneous data (same
telescope/instrument); (ii) a correction for extinction to all bands
based on the relation between the g-i color and the color excess
E(B-V); and (iii) a correction for the contamination of the [NII]
λ6583 line that falls within the Hα filter. All
NCR distributions in the broad-band filters, tracing the overall light
distribution in each galaxy, are similar to each other. The main
difference is that type Ia, II and IIb SNe are preferably located in
redder environment than the other SN types. The radial distribution of
the SNe shows that type IIb SNe seem to have a preference for
occurring in the inner regions of galaxies, whereas other types of SNe
occur throughout the galaxy without a distinct preference for a
specific location. For the Hα filter we recover the sequence
from SNe Ic with the highest NCR to SNe Ia with the lowest, which is
interpreted as a sequence in progenitor mass and age. All
core-collapse SN types are strongly correlated to the [OII] emission,
which also traces SFR, following the same sequence as in Hα. The
NCRdistributions of the CaII triplet show a clear division between
II/IIb/Ia and Ib/Ic/IIn subtypes, which is interpreted as a difference
in the environmental metallicity. Regarding the SSP synthesis, we
found that including the seven J-PLUS narrow filters in the fitting
process has a more significant effect for the core-collapse SN
environmental parameters than for SNe Ia, shifting their values
towards more extincted, younger, and more star-forming environments,
due to the presence of strong emission-lines and stellar absorptions
in those narrow-bands.
Description:
We built 418 3D datacubes of SN host galaxies from image cutouts of
the 12 (+5) J-PLUS photometric filters. With the datacubes we perform
the NCR for every single image of the cube and for every galaxy. We
also perform SED fitting for every SN to obtain the main four
parameters of the fitting: local extinction Av, star formation rate
(SFR), specific SFR (sSFR) and average stellar age (<t*>).
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
tablea1.dat 132 418 SN sample informations
taba234.dat 408 421 Normalized Cumulative Rank (NCR) values for
every filter and SN (tables A2, A3 and A4)
tablea5.dat 95 418 Av, SFR, sSFR and <t*> for every SN
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Byte-by-byte Description of file: tablea1.dat
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Bytes Format Units Label Explanations
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1- 38 A38 --- Tile Tile of the J-PLUS field
40- 60 A21 --- Name Supernova name
62- 68 A7 --- Type Supernova type
70- 81 F12.8 deg RAdeg Right ascension of the SN (J2000)
83- 94 F12.8 deg DEdeg Declination of the SN (J2000)
96-105 F10.6 deg RAHdeg Right ascension of the host galaxy (J2000)
107-117 F11.7 deg DEHdeg Declination of the host galaxy (J2000)
119-122 I4 --- side Size of the cutout (side*side)
124-132 E9.2 --- z Heliocentric redshift of the SN
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Byte-by-byte Description of file: taba234.dat
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Bytes Format Units Label Explanations
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1- 21 A21 --- Name Supernova name
23- 29 A7 --- Type Supernova type
31- 40 F10.8 --- uJAVA Normalized Cumulative Rank (NCR)
in uJAVA (348.5nm) band
42- 52 E11.6 --- e_uJAVA Error of the Normalized Cumulative Rank (NCR)
in the uJAVA band
54- 63 F10.8 --- J0378 Normalized Cumulative Rank (NCR)
in J0378 (378.5nm) band
65- 75 F11.9 --- e_J0378 Error of the Normalized Cumulative Rank (NCR)
in the J0378 band
77- 86 F10.8 --- J0395 Normalized Cumulative Rank (NCR)
in J0395 (395.0nm) band
88- 98 F11.9 --- e_J0395 Error of the Normalized Cumulative Rank (NCR)
in the J0395 band
100-109 F10.8 --- J0410 Normalized Cumulative Rank (NCR)
in J0410 (410.0nm) band
111-120 F10.8 --- e_J0410 Error of the Normalized Cumulative Rank (NCR)
in the J0410 band
122-131 F10.8 --- J0430 Normalized Cumulative Rank (NCR)
in J0430 (430.0nm) band
133-143 F11.9 --- e_J0430 Error of the Normalized Cumulative Rank (NCR)
in the J0430 band
145-154 F10.8 --- gSDSS Normalized Cumulative Rank (NCR)
in gSDSS (480.3nm) band
156-165 F10.8 --- e_gSDSS Error of the Normalized Cumulative Rank (NCR)
in the gSDSS band
167-176 F10.8 --- J0515 Normalized Cumulative Rank (NCR)
in J0515 (515.0nm) band
178-188 F11.9 --- e_J0515 Error of the Normalized Cumulative Rank (NCR)
in the J0515 band
190-198 F9.7 --- rSDSS Normalized Cumulative Rank (NCR)
in rSDSS (625.4nm) band
200-209 F10.8 --- e_rSDSS Error of the Normalized Cumulative Rank (NCR)
in the rSDSS band
211-220 F10.8 --- J0660 Normalized Cumulative Rank (NCR)
in J0660 (660.0nm) band
222-232 F11.9 --- e_J0660 Error of the Normalized Cumulative Rank (NCR)
in the J0660 band
234-243 F10.8 --- iSDSS Normalized Cumulative Rank (NCR)
in iSDSS (766.8nm) band
245-255 F11.9 --- e_iSDSS Error of the Normalized Cumulative Rank (NCR)
in the iSDSS band
257-266 F10.8 --- J0861 Normalized Cumulative Rank (NCR)
in J0861 (861.0nm) band
268-278 F11.9 --- e_J0861 Error of the Normalized Cumulative Rank (NCR)
in the J0861 band
280-289 F10.8 --- zSDSS Normalized Cumulative Rank (NCR)
in zSDSS (911.4nm) band
291-301 F11.9 --- e_zSDSS Error of the Normalized Cumulative Rank (NCR)
in the zSDSS band
303-311 F9.7 --- Ha+[NII] Normalized Cumulative Rank (NCR)
in H-alpha+[NII] emission
313-322 F10.8 --- e_Ha+[NII] Error of the Normalized Cumulative Rank (NCR)
of H-alpha+[NII] emission
324-332 F9.7 --- [OII] Normalized Cumulative Rank (NCR)
in [OII] emission continuum subtracted
334-343 F10.8 --- e_[OII] Error of the Normalized Cumulative Rank (NCR)
of [OII] emission
345-353 F9.7 --- CaIIT Normalized Cumulative Rank (NCR)
in CaII triplet absorption
continuum subtracted
355-365 E11.6 --- e_CaIIT Error of the Normalized Cumulative Rank (NCR)
of CaII triplet absorption
367-375 F9.7 --- Ha Normalized Cumulative Rank (NCR)
in H-alpha emission
377-386 F10.8 --- e_Ha Error of the Normalized Cumulative Rank (NCR)
of H-alpha emission
388-396 F9.7 --- [NII] Normalized Cumulative Rank (NCR)
in [NII] emission
398-408 F11.9 --- e_[NII] Error of the Normalized Cumulative Rank (NCR)
of the [NII] emission
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Byte-by-byte Description of file: tablea5.dat
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Bytes Format Units Label Explanations
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1- 21 A21 --- Name Supernova name
23- 29 A7 --- Type Supernova Type
31- 35 F5.2 [yr] log<t*> log of the average stellar age
37- 40 F4.2 [yr] E_log<t*> Positive deviation of the average stellar age
43- 46 F4.2 [yr] e_log<t*> Negative deviation of the average stellar age
48- 50 F3.1 mag AV Local extinction
52- 55 F4.2 mag E_AV Positive deviation of the local extinction
57- 61 F5.2 mag e_AV Negative deviation of the local extinction
63- 68 F6.2 [Msun/yr] logSFR log of the star formation rate
70- 73 F4.2 [Msun/yr] E_logSFR Positive deviation of the star formation rate
76- 79 F4.2 [Msun/yr] e_logSFR Negative deviation of the star formation rate
81- 84 F4.2 [Msun] logM log of the specific star formation rate
86- 89 F4.2 [Msun] E_logM Positive deviation of the
specific star formation rate
92- 95 F4.2 [Msun] e_logM Negative deviation of the
specific star formation rate
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Acknowledgements:
Raul Gonzalez Diaz, rgonzalez(at)inaoep.mx, raulghuelma(at)gmail.com,
Raul.GonzalezD(at)autonoma.cat
(End) Patricia Vannier [CDS] 25-Jan-2024