Differential attenuation in star-forming galaxies at 0.3 $\lesssim$ $z$ $\lesssim$ 1.5 in the SHARDS/CANDELS field Article Swipe

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L. Rodríguez-Muñoz , G. Rodighiero , Pablo G. Pérez‐González , M. Talia , Ivano Baronchelli , L. Morselli , A. Renzini , Annagrazia Puglisi , A. Grazian , Anita Zanella , C. Mancini , A. Feltre , Michael Romano , Alba Vidal-García , A. Franceschini , Belén Alcalde Pampliega , P. Cassata , Luca Costantin , H. Domínguez Sánchez , Néstor Espino-Briones , Edoardo Iani , Anton M. Koekemoer , A. Lumbreras-Calle , J. M. Rodríguez-Espinosa ·

YOU? · · 2021 · Open Access · · DOI: https://doi.org/10.48550/arxiv.2112.01885

We use a sample of 706 galaxies, selected as [OII]$λ$3727 ([OII]) emitters in the Survey for High-$z$ Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to study the differential attenuation of the nebular emission with respect to the stellar continuum. The sample includes only galaxies with a counterpart in the infrared and $\mathrm{log}_{10}(M_{*}/\mathrm{M}_{\odot})$ $>$ 9, over the redshift interval 0.3 $\lesssim$ $z$ $\lesssim$ 1.5. Our methodology consists in the comparison of the star formation rates inferred from [OII] and H$α$ emission lines with a robust quantification of the total star-forming activity (${SFR}_{\mathrm{TOT}}$) that is independently estimated based on both infrared and ultraviolet (UV) luminosities. We obtain $f$$=$$E(B-V)_{\mathrm{stellar}}$/$E(B-V)_{\mathrm{nebular}}$ $=$ 0.69$^{0.71}_{0.69}$ and 0.55$^{0.56}_{0.53}$ for [OII] and H$α$, respectively. Our resulting $f$-factors display a significant positive correlation with the UV attenuation and shallower or not-significant trends with the stellar mass, the $SFR_{\mathrm{TOT}}$, the distance to the main sequence, and the redshift. Finally, our results favour an average nebular attenuation curve similar in shape to the typical dust curve of local starbursts.

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Physics Redshift Astrophysics Galaxy Star formation Stellar mass Attenuation Infrared Photometric redshift Lambda Astronomy Optics

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Type: preprint
Language: en
Landing Page: https://doi.org/10.48550/arxiv.2112.01885
OA Status: green
Related Works: 10
OpenAlex ID: https://openalex.org/W4200633286

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DOI: https://doi.org/10.48550/arxiv.2112.01885

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Title: Differential attenuation in star-forming galaxies at 0.3 $\lesssim$ $z$ $\lesssim$ 1.5 in the SHARDS/CANDELS field

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Type: preprint

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Language: en

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Publication year: 2021

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Publication date: 2021-12-03

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Authors: L. Rodríguez-Muñoz, G. Rodighiero, Pablo G. Pérez‐González, M. Talia, Ivano Baronchelli, L. Morselli, A. Renzini, Annagrazia Puglisi, A. Grazian, Anita Zanella, C. Mancini, A. Feltre, Michael Romano, Alba Vidal-García, A. Franceschini, Belén Alcalde Pampliega, P. Cassata, Luca Costantin, H. Domínguez Sánchez, Néstor Espino-Briones, Edoardo Iani, Anton M. Koekemoer, A. Lumbreras-Calle, J. M. Rodríguez-Espinosa

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Landing page: https://doi.org/10.48550/arxiv.2112.01885

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Concepts: Physics, Redshift, Astrophysics, Galaxy, Star formation, Stellar mass, Attenuation, Infrared, Photometric redshift, Lambda, Astronomy, Optics

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abstract_inverted_index.and	19, 53, 80, 102, 111, 115, 130, 147
abstract_inverted_index.for	15, 113
abstract_inverted_index.our	151
abstract_inverted_index.the	13, 24, 29, 33, 39, 51, 58, 70, 73, 89, 127, 136, 139, 141, 144, 148, 163
abstract_inverted_index.use	1
abstract_inverted_index.(UV)	104
abstract_inverted_index.1.5.	65
abstract_inverted_index.Dead	20
abstract_inverted_index.both	100
abstract_inverted_index.dust	165
abstract_inverted_index.from	78
abstract_inverted_index.main	145
abstract_inverted_index.only	45
abstract_inverted_index.over	57
abstract_inverted_index.star	74
abstract_inverted_index.that	94
abstract_inverted_index.with	36, 47, 84, 126, 135
abstract_inverted_index.H$α$	81
abstract_inverted_index.[OII]	79, 114
abstract_inverted_index.based	98
abstract_inverted_index.curve	158, 166
abstract_inverted_index.lines	83
abstract_inverted_index.local	168
abstract_inverted_index.mass,	138
abstract_inverted_index.rates	76
abstract_inverted_index.shape	161
abstract_inverted_index.study	28
abstract_inverted_index.total	90
abstract_inverted_index.$>$	55
abstract_inverted_index.H$α$,	116
abstract_inverted_index.Survey	14
abstract_inverted_index.favour	153
abstract_inverted_index.field,	26
abstract_inverted_index.obtain	107
abstract_inverted_index.robust	86
abstract_inverted_index.sample	3, 43
abstract_inverted_index.trends	134
abstract_inverted_index.([OII])	10
abstract_inverted_index.Sources	21
abstract_inverted_index.average	155
abstract_inverted_index.display	121
abstract_inverted_index.nebular	34, 156
abstract_inverted_index.respect	37
abstract_inverted_index.results	152
abstract_inverted_index.similar	159
abstract_inverted_index.stellar	40, 137
abstract_inverted_index.typical	164
abstract_inverted_index.(SHARDS)	22
abstract_inverted_index.Finally,	150
abstract_inverted_index.High-$z$	16
abstract_inverted_index.activity	92
abstract_inverted_index.consists	68
abstract_inverted_index.distance	142
abstract_inverted_index.emission	35, 82
abstract_inverted_index.emitters	11
abstract_inverted_index.galaxies	46
abstract_inverted_index.includes	44
abstract_inverted_index.inferred	77
abstract_inverted_index.infrared	52, 101
abstract_inverted_index.interval	60
abstract_inverted_index.positive	124
abstract_inverted_index.redshift	59
abstract_inverted_index.selected	7
abstract_inverted_index.estimated	97
abstract_inverted_index.formation	75
abstract_inverted_index.galaxies,	6
abstract_inverted_index.redshift.	149
abstract_inverted_index.resulting	119
abstract_inverted_index.sequence,	146
abstract_inverted_index.shallower	131
abstract_inverted_index.$\lesssim$	62, 64
abstract_inverted_index.Absorption	17
abstract_inverted_index.comparison	71
abstract_inverted_index.continuum.	41
abstract_inverted_index.$f$-factors	120
abstract_inverted_index.attenuation	31, 129, 157
abstract_inverted_index.correlation	125
abstract_inverted_index.counterpart	49
abstract_inverted_index.methodology	67
abstract_inverted_index.significant	123
abstract_inverted_index.starbursts.	169
abstract_inverted_index.ultraviolet	103
abstract_inverted_index.differential	30
abstract_inverted_index.star-forming	91
abstract_inverted_index.[OII]$λ$3727	9
abstract_inverted_index.independently	96
abstract_inverted_index.luminosities.	105
abstract_inverted_index.respectively.	117
abstract_inverted_index.quantification	87
abstract_inverted_index.CANDELS/GOODS-N	25
abstract_inverted_index.not-significant	133
abstract_inverted_index.0.55$^{0.56}_{0.53}$	112
abstract_inverted_index.0.69$^{0.71}_{0.69}$	110
abstract_inverted_index.$SFR_{\mathrm{TOT}}$,	140
abstract_inverted_index.(${SFR}_{\mathrm{TOT}}$)	93
abstract_inverted_index.$\mathrm{log}_{10}(M_{*}/\mathrm{M}_{\odot})$	54
abstract_inverted_index.$f$$=$$E(B-V)_{\mathrm{stellar}}$/$E(B-V)_{\mathrm{nebular}}$	108
cited_by_percentile_year
countries_distinct_count	0
institutions_distinct_count	24
citation_normalized_percentile.value	0.19075768
citation_normalized_percentile.is_in_top_1_percent	False
citation_normalized_percentile.is_in_top_10_percent	False