New dwarf galaxy candidates in the M106, NGC3521, and UGCA127 groups with the Hyper Suprime Camera
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| Main Authors: | , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866912330686660608 |
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| author | Müller, Oliver Jerjen, Helmut Taibi, Salvatore Heesters, Nick Crosby, Ethan Pawlowski, Marcel S. |
| author_facet | Müller, Oliver Jerjen, Helmut Taibi, Salvatore Heesters, Nick Crosby, Ethan Pawlowski, Marcel S. |
| contents | The local universe is still full of hidden dwarf galaxies to be discovered using deep imaging campaigns. Here we present the third paper in a series to search for low-surface brightness dwarf galaxies around nearby isolated luminous host galaxies with the Subaru Hyper Suprime Camera. Based on visual inspection, we found 11, 0, 4, and 6 dwarf galaxy candidates around M106, NGC2903, NGC3521, and UGCA127, respectively. This adds to the 40 candidates around M104 and 4 candidates around NGC2683 found in the previous papers. Artificial galaxy experiments show that we are complete down to a mean effective surface brightness of 26 mag/arcsec$^2$. The new dwarf galaxy candidates follow known scaling relation in size, surface brightness and luminosity, making them good candidates based on their morphology and photometric properties. We trace the luminosity function of these galaxies down to magnitude of $\approx-$9 in the V band for all galaxies targeted in our survey footprint so far. While the most massive galaxy (M104) has a significant higher abundance of dwarfs, NGC3521, NGC2903, and NGC2683 have a similar luminosity function as the Milky Way. These latter three galaxies also have a similar stellar mass and might be considered Milky Way analogs. UGCA127 is a low-mass galaxy but almost reaches the same number of dwarfs as the Milky Way at our limiting magnitude. We have searched for hints of lopsidedness in the satellite distributions, but found none to be significant. The next step will be to confirm these members through either distance or velocity measurements. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2504_11608 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | New dwarf galaxy candidates in the M106, NGC3521, and UGCA127 groups with the Hyper Suprime Camera Müller, Oliver Jerjen, Helmut Taibi, Salvatore Heesters, Nick Crosby, Ethan Pawlowski, Marcel S. Astrophysics of Galaxies The local universe is still full of hidden dwarf galaxies to be discovered using deep imaging campaigns. Here we present the third paper in a series to search for low-surface brightness dwarf galaxies around nearby isolated luminous host galaxies with the Subaru Hyper Suprime Camera. Based on visual inspection, we found 11, 0, 4, and 6 dwarf galaxy candidates around M106, NGC2903, NGC3521, and UGCA127, respectively. This adds to the 40 candidates around M104 and 4 candidates around NGC2683 found in the previous papers. Artificial galaxy experiments show that we are complete down to a mean effective surface brightness of 26 mag/arcsec$^2$. The new dwarf galaxy candidates follow known scaling relation in size, surface brightness and luminosity, making them good candidates based on their morphology and photometric properties. We trace the luminosity function of these galaxies down to magnitude of $\approx-$9 in the V band for all galaxies targeted in our survey footprint so far. While the most massive galaxy (M104) has a significant higher abundance of dwarfs, NGC3521, NGC2903, and NGC2683 have a similar luminosity function as the Milky Way. These latter three galaxies also have a similar stellar mass and might be considered Milky Way analogs. UGCA127 is a low-mass galaxy but almost reaches the same number of dwarfs as the Milky Way at our limiting magnitude. We have searched for hints of lopsidedness in the satellite distributions, but found none to be significant. The next step will be to confirm these members through either distance or velocity measurements. |
| title | New dwarf galaxy candidates in the M106, NGC3521, and UGCA127 groups with the Hyper Suprime Camera |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2504.11608 |