The AstroSat UV Deep Field North: Direct determination of the UV Luminosity Function and its evolution from z~0.8-0.4
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| Format: | Preprint |
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2023
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| _version_ | 1866909230821277696 |
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| author | Bhattacharya, Souradeep Saha, Kanak Mondal, Chayan |
| author_facet | Bhattacharya, Souradeep Saha, Kanak Mondal, Chayan |
| contents | We characterize the evolution of the rest-frame 1500 $\unicode{xC5}$ UV luminosity Function (UVLF) from AstroSat/UVIT F154W and N242W imaging in the Great Observatories Origins Survey North (GOODS-N) field. With deep FUV observations, we construct the UVLF for galaxies at z$<0.13$ and subsequently characterise it with a Schechter function fit. The fitted parameters are consistent with previous determinations. With deep NUV observations, we are able to construct the UVLF in seven redshift bins in the range z $\sim$ 0.8 - 0.4, with galaxies identified till $\sim$2 mag fainter than previous surveys, owing to the high angular-resolution of UVIT. The fitted Schechter function parameters are obtained for these UVLFs. At z $\sim$ 0.8 - 0.7, we also utilize Hubble Space Telescope (HST) F275W observations in the GOODS-N field to construct the UVLF in 2 redshift bins, whose fitted Schechter function parameters are then found to be consistent with that determined from UVIT at z $\sim$ 0.75. We thus probe the variation of the fitted UVLF parameters over z $\sim$ 0.8 - 0.4, a span of $\sim$2.7 Gyr in age. We find that the slope of the Schechter function, $α$, is at its steepest at z $\sim$ 0.65, implying highest star-formation at this instant with galaxies being relatively more passive before and after this time. We infer that this may be a short-lived instance of increased cosmic star-formation even though cosmic star-formation may be winding-down over longer timespan at this redshift range. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2310_01903 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | The AstroSat UV Deep Field North: Direct determination of the UV Luminosity Function and its evolution from z~0.8-0.4 Bhattacharya, Souradeep Saha, Kanak Mondal, Chayan Astrophysics of Galaxies We characterize the evolution of the rest-frame 1500 $\unicode{xC5}$ UV luminosity Function (UVLF) from AstroSat/UVIT F154W and N242W imaging in the Great Observatories Origins Survey North (GOODS-N) field. With deep FUV observations, we construct the UVLF for galaxies at z$<0.13$ and subsequently characterise it with a Schechter function fit. The fitted parameters are consistent with previous determinations. With deep NUV observations, we are able to construct the UVLF in seven redshift bins in the range z $\sim$ 0.8 - 0.4, with galaxies identified till $\sim$2 mag fainter than previous surveys, owing to the high angular-resolution of UVIT. The fitted Schechter function parameters are obtained for these UVLFs. At z $\sim$ 0.8 - 0.7, we also utilize Hubble Space Telescope (HST) F275W observations in the GOODS-N field to construct the UVLF in 2 redshift bins, whose fitted Schechter function parameters are then found to be consistent with that determined from UVIT at z $\sim$ 0.75. We thus probe the variation of the fitted UVLF parameters over z $\sim$ 0.8 - 0.4, a span of $\sim$2.7 Gyr in age. We find that the slope of the Schechter function, $α$, is at its steepest at z $\sim$ 0.65, implying highest star-formation at this instant with galaxies being relatively more passive before and after this time. We infer that this may be a short-lived instance of increased cosmic star-formation even though cosmic star-formation may be winding-down over longer timespan at this redshift range. |
| title | The AstroSat UV Deep Field North: Direct determination of the UV Luminosity Function and its evolution from z~0.8-0.4 |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2310.01903 |