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| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2512.03695 |
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| _version_ | 1866912940371738624 |
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| author | Phan, Kim Galbany, Lluís Müller-Bravo, Tomás E. Bose, Subhash Burns, Christopher R. Stritzinger, Maximilian D. Sørensen, Camilla T. G. Ashall, Chris Castander, Francisco J. Palau, Cristina Jiménez Johansson, Joel Anderson, Joseph P. Chambers, Ken. C. Gromadzki, Mariusz Pessi, Priscila J. Chen, Ting-Wan |
| author_facet | Phan, Kim Galbany, Lluís Müller-Bravo, Tomás E. Bose, Subhash Burns, Christopher R. Stritzinger, Maximilian D. Sørensen, Camilla T. G. Ashall, Chris Castander, Francisco J. Palau, Cristina Jiménez Johansson, Joel Anderson, Joseph P. Chambers, Ken. C. Gromadzki, Mariusz Pessi, Priscila J. Chen, Ting-Wan |
| contents | Type Ia supernovae (SNe Ia) provide the most robust means of measuring extragalactic distances. While most of the effort has focused on increasing the number of SNe Ia observed in the optical, near-infrared (NIR) observations remain scarce despite their advantages, that is, reduced dust extinction and a more intrinsic standard candle behavior, requiring little to no empirical corrections. Here, we present ASNOS (ANDICAM-SOFI Near-infrared and Optical type Ia Supernova), a dataset with sample size of 1,482 epochs in the $BVRIYJH$ filters from the ANDICAM instrument on the 1.3-meter SMARTS telescope at Cerro Tololo Inter-American Observatory, along with 125 $JHK$ epochs from the SOFI instrument on the 3.58-meter New Technology Telescope on the La Silla Observatory. Additionally, we incorporate optical forced photometry from the Zwicky Transient Facility and the Asteroid Terrestrial-impact Last Alert System. The sample comprises 41 SNe Ia in total, including 29 normal events, eight 1991T-like objects, and four peculiar subtypes, all located at redshifts $z < 0.085$. This paper provides a detailed overview of the ASNOS sample selection, data reduction, SN photometry, host-galaxy spectral energy distribution construction, both global and local, and SN light-curve fitting using three methods: SALT3-NIR, SNooPy, and BayeSN. A companion paper will present the cosmological analysis. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_03695 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The ANDICAM-SOFI Near-infrared and Optical type Ia Supernova (ASNOS) sample: Description and data release Phan, Kim Galbany, Lluís Müller-Bravo, Tomás E. Bose, Subhash Burns, Christopher R. Stritzinger, Maximilian D. Sørensen, Camilla T. G. Ashall, Chris Castander, Francisco J. Palau, Cristina Jiménez Johansson, Joel Anderson, Joseph P. Chambers, Ken. C. Gromadzki, Mariusz Pessi, Priscila J. Chen, Ting-Wan Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena Type Ia supernovae (SNe Ia) provide the most robust means of measuring extragalactic distances. While most of the effort has focused on increasing the number of SNe Ia observed in the optical, near-infrared (NIR) observations remain scarce despite their advantages, that is, reduced dust extinction and a more intrinsic standard candle behavior, requiring little to no empirical corrections. Here, we present ASNOS (ANDICAM-SOFI Near-infrared and Optical type Ia Supernova), a dataset with sample size of 1,482 epochs in the $BVRIYJH$ filters from the ANDICAM instrument on the 1.3-meter SMARTS telescope at Cerro Tololo Inter-American Observatory, along with 125 $JHK$ epochs from the SOFI instrument on the 3.58-meter New Technology Telescope on the La Silla Observatory. Additionally, we incorporate optical forced photometry from the Zwicky Transient Facility and the Asteroid Terrestrial-impact Last Alert System. The sample comprises 41 SNe Ia in total, including 29 normal events, eight 1991T-like objects, and four peculiar subtypes, all located at redshifts $z < 0.085$. This paper provides a detailed overview of the ASNOS sample selection, data reduction, SN photometry, host-galaxy spectral energy distribution construction, both global and local, and SN light-curve fitting using three methods: SALT3-NIR, SNooPy, and BayeSN. A companion paper will present the cosmological analysis. |
| title | The ANDICAM-SOFI Near-infrared and Optical type Ia Supernova (ASNOS) sample: Description and data release |
| topic | Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2512.03695 |