J/A+A/696/A130         Dwarf galaxy candidates detection           (Yang+, 2025)

An automatic detection method of small size dwarf galaxy candidates. Yang H.-F., Zhang B.-Y., Cai J.-H., Qu H., Zheng A.-Y., Hao J., Chen X., Zhao X., Xun Y. <Astron. Astrophys. 696, A130 (2025)> =2025A&A...696A.130Y 2025A&A...696A.130Y (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Galaxy catalogs ; Redshifts ; Photometry, SDSS Keywords: methods: data analysis - techniques: image processing - survey - galaxies: dwarf Abstract: The missing satellites problem remains a core issue of the {LAMBDA}CDM model. On small-scale, the number of observed dwarf galaxies is still fewer than the number predicted by existing theories. Therefore, finding fainter dwarf galaxies in deeper images is crucial for refining the existing theoretical framework. In this study, we propose an end-to-end automatic identification scheme for small size and faint dwarf galaxies based on DESI photometric images and provide a batch of dwarf galaxy candidates. We develop a dwarf galaxy automatic detection model, YOLO-DG, based on the YOLOv7 framework, achieving a precision of 88.2% and a recall of 89.1% on the test set. We identify 742251 dwarf galaxy candidates across the entire DESI DR9 footprint using YOLO-DG, with their spectral redshifts concentrated in the range of 0 to 0.1. The faintest dwarf galaxy candidates detected by YOLO-DG have magnitudes of 31.61mag, 27.62mag, and 32.78mag in the g, r, and z bands, respectively. We identify 95230 local volume dwarf galaxy candidates, 33 of which are identified based on spectral redshift. The half-light radius of the smallest local volume dwarf galaxy candidate is 0.31 arcsec. Finally, we provide a complete catalog of local volume dwarf galaxy candidates. Description: This catalog contains all the samples analyzed in our paper, including local volume dwarf galaxy candidates, high-confidence sources in subsequent analysis, and complete detection results. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog1.dat 122 95197 Local volume dwarf galaxy candidates identified based on photometric redshift catalog2.dat 121 33 Local volume dwarf galaxy candidates identified based on spectral redshift catalog3.dat 55 650 Targets too faint to be clearly distinguished by the naked eye catalog4.dat 101 26 Targets that were clearly observed to be actual astronomical object through visual inspection but were not identified by DESI catalog5.dat 101 746899 All sources detected by YOLO-DG -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Index Index 7- 26 A20 --- Name Unique name for each candidate based on position, DHHMMSS.ss_DDMMSS.ss 28- 31 I4 --- release Camera and filter settings 36- 41 I6 --- brickid Brick ID 44- 51 A8 --- brickname Name of brick 54- 58 I5 --- objid Catalog object number within this brick 60- 67 F8.4 deg RAdeg Right ascension at equinox J2000 69- 76 F8.4 deg DEdeg Declination at equinox J2000 78- 82 F5.2 mag gmag g-band magnitude 84- 88 F5.2 mag rmag r-band magnitude 90- 94 F5.2 mag zmag ?=99 z-band magnitude 96-100 F5.2 arcsec rhl Half-light radius of galaxy model for galaxy type 114-122 F9.6 --- zph Photometric redshift -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Index Index 7- 26 A20 --- Name Unique name for each candidate based on position, DHHMMSS.ss_DDMMSS.ss 28- 31 I4 --- release Camera and filter settings 36- 41 I6 --- brickid Brick ID 44- 51 A8 --- brickname Name of brick 54- 58 I5 --- objid Catalog object number within this brick 60- 67 F8.4 deg RAdeg Right ascension at equinox J2000 69- 76 F8.4 deg DEdeg Declination at equinox J2000 78- 82 F5.2 mag gmag g-band magnitude 84- 88 F5.2 mag rmag r-band magnitude 90- 94 F5.2 mag zmag z-band magnitude 96-100 F5.2 arcsec rhl Half-light radius of galaxy model for galaxy type 114-121 F8.6 --- z Spectral redshift -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.4 deg RAdeg Right ascension at equinox J2000 (1) 10- 17 F8.4 deg DEdeg Declination at equinox J2000 (1) 19- 26 F8.4 deg XWORLD Barycenter position along world x axis 28- 35 F8.4 deg YWORLD Barycenter position along world y axis 37- 43 F7.4 mag magAUTO Kron-like elliptical aperture magnitude 46- 55 F10.4 pix FluxRad Radius enclosing a specified fraction of the flux -------------------------------------------------------------------------------- Note (1): This position is obtained through model detection. -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.4 deg RAdeg Right ascension at equinox J2000 (1) 10- 17 F8.4 deg DEdeg Declination at equinox J2000 (1) 19- 26 F8.4 deg RASdeg Right ascension at equinox J2000 from SDSS 28- 35 F8.4 deg DESdeg Declination at equinox J2000 from SDSS 37- 40 I4 --- run Run number 42- 44 I3 --- rerun Rerun number 48 I1 --- camcol Camera column 55- 57 I3 --- Field Field number 61- 64 I4 --- objId The object id within a field 66- 71 A6 --- Type Type classification of the object 73- 77 F5.2 mag umag Model magnitude in u-band 79- 83 F5.2 mag gmag Model magnitude in g-band 85- 89 F5.2 mag rmag Model magnitude in r-band 91- 95 F5.2 mag imag Model magnitude in i-band 97-101 F5.2 mag zmag Model magnitude in z-band -------------------------------------------------------------------------------- Note (1): This position is obtained through model detection -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.6 deg RAdeg Right ascension at equinox J2000 (1) 12- 21 F10.6 deg DEdeg Declination at equinox J2000 (1) 23- 26 I4 --- release the camera and filter set used (1) 31- 36 I6 --- brickid Brick ID (1) 39- 46 A8 --- brickname Name of brick (1) 49- 53 I5 --- objid Catalog object number within this brick (1) 55- 57 A3 --- Type Morphological model (1) 60- 72 A13 3.63uJy Fg Model flux in g, in nanomaggy units (1) 74- 86 A13 3.63uJy Fr Model flux in r, in nanomaggy units (1) 88-100 A13 3.63uJy Fz Model flux in z, in nanomaggy units (1) -------------------------------------------------------------------------------- Note (1): All properties are available from the DESI DR9 Tractor catalog. -------------------------------------------------------------------------------- History: From Jiang-Hui Cai, Jianghui(at)tyust.edu.cn Acknowledgements: The work is supported by the National Natural Science Foundation of China (Grant Nos. 12473105, 12473106, 62272336), Projects of Science and Technology Cooperation and Exchange of Shanxi Province (Grant Nos. 202204041101037, 202204041101033), The central government guides local funds for science and technology development (YDZJSX2024D049), the science research grant from the China Manned Space Project with No. CMS-CSST-2021-B03, and Guanghe Fund (No. ghfund202407027490). The DESI Legacy Imaging Surveys consist of three individual and complementary projects: the Dark Energy Camera Legacy Survey (DECaLS), the Beijing-Arizona Sky Survey (BASS), and the Mayall z-band Legacy Survey (MzLS). DECaLS, BASS and MzLS together include data obtained, respectively, at the Blanco telescope, Cerro Tololo Inter-American Observatory, NSF's NOIRLab; the Bok telescope, Steward Observatory, University of Arizona; and the Mayall telescope, Kitt Peak National Observatory, NOIRLab. NOIRLab is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. Pipeline processing and analyses of the data were supported by NOIRLab and the Lawrence Berkeley National Laboratory (LBNL). Legacy Surveys also uses data products from the Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE), a project of the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. Legacy Surveys was supported by: the Director, Office of Science, Office of High Energy Physics of the U.S. Department of Energy; the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility; the U.S. National Science Foundation, Division of Astronomical Sciences; the National Astronomical Observatories of China, the Chinese Academy of Sciences and the Chinese National Natural Science Foundation. LBNL is managed by the Regents of the University of California under contract to the U.S. Department of Energy. The complete acknowledgments can be found at https://www.legacysurvey.org/acknowledgment/. The Photometric Redshifts for the Legacy Surveys (PRLS) catalog used in this paper was produced thanks to funding from the U.S. Department of Energy Office of Science, Office of High Energy Physics via grant DE-SC0007914.
(End) Patricia Vannier [CDS] 07-Mar-2025
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line