The Large Magellanic Cloud LRGB From "Down Under" (Tom Peter AKA Astrovetteman)

Please note: The following tables are updated every 24 hours.

Distribution of astrophotographers

This table shows the number of distinct astrophotographers who have been assigned and IOTD/TP award compared to the total number of images awarded.
	Distinct awarded users	Total awarded images
Image of the day
Top picks
Top pick nominations

Distribution of subject types

This table shows the distribution of awards per subject type, compared to the popularity of images of that subject type.
	Image of the day	Top pick	Top pick nominations	Total submitted
Deep sky
Solar system
Extremely wide field
Star trails
Northern lights
Noctilucent clouds
Landscape
Artificial satellite

Distribution of data sources

This table shows the distribution of awards per data source, compared to the popularity of images acquired from that data source.
	Image of the day	Top pick	Top pick nominations	Total submitted
Backyard
Traveller
Own remote observatory
Amateur hosting facility
Public amaeteur data
Professional, scientific grade data
Mix of multiple sources
Other
Unknown

The “AstroBin Image of the Day and Top Picks”, or IOTD/TP, is a long-running system to promote beautiful, interesting, peculiar, or otherwise amazing astrophotographs, with a focus on technical excellence. Learn more.

Submitted The date and time when you submitted this image for IOTD/TP consideration.	...
Views by Submitters (available since September 19th, 2023) Every image is assigned to 50% of available Submitters. In the event that at least 80% of them don't view the image before its time in the IOTD/TP process expires, it's assigned to the other 50% of Submitters and the process begins anew.
Promotions by Submitters When 3 distinct Submitters promote the image, it moves on to the next stage of the process: evaluation for Top Pick status. This requirement, in addition to anonymization of images and distribution to only a subset of them, prevents biases and ensures that the best images are selected.
Promotions by Reviewers When 3 distinct Reviewers promote the image, it moves on to the next stage of the process: evaluation for IOTD status.
Early dismissal Staff members have a lot of images to inspect on a daily basis, and they can dismiss images if they believe they don't meet the requirements for IOTD/TP selection. If an image is dismissed 5 times, it's removed from the process. This streamlines the process and ensures that any bias present in promotions could be overruled by other staff members.

30 Dor Cluster · IC 2117 · IC 2128 · IC 2145 · NGC 1737 · NGC 1743 · NGC 1745 · NGC 1749 · NGC 1751 · NGC 1754 · NGC 1755 · NGC 1756 · NGC 1764 · NGC 1766 · NGC 1767 · NGC 1768 · NGC 1770 · NGC 1772 · NGC 1774 · NGC 1775 · NGC 1782 · NGC 1786 · NGC 1789 · NGC 1791 · NGC 1793 · NGC 1795 · NGC 1801 · NGC 1804 · NGC 1806 · NGC 1809 · NGC 1813 · NGC 1814 · NGC 1815 · NGC 1816 · NGC 1820 · NGC 1823 · NGC 1825 · NGC 1828 · NGC 1829 · NGC 1830 · NGC 1833 · NGC 1835 · NGC 1836 · NGC 1837 · NGC 1838 · NGC 1839 · NGC 1840 · NGC 1842 · NGC 1844 · NGC 1845 · NGC 1846 · NGC 1847 · NGC 1848 · NGC 1850 · NGC 1852 · NGC 1854 · NGC 1856 · NGC 1858 · NGC 1860 · NGC 1861 · NGC 1863 · NGC 1864 · NGC 1865 · NGC 1869 · NGC 1870 · NGC 1871 · NGC 1872 · NGC 1873 · NGC 1874 · NGC 1877 · NGC 1878 · NGC 1881 · NGC 1885 · NGC 1890 · NGC 1894 · NGC 1895 · NGC 1897 · NGC 1898 · NGC 1899 · NGC 1901 · NGC 1903 · NGC 1905 · NGC 1910 · NGC 1913 · NGC 1914 · NGC 1916 · NGC 1917 · NGC 1918 · NGC 1921 · NGC 1922 · NGC 1926 · NGC 1928 · NGC 1929 · NGC 1934 · NGC 1936 · NGC 1937 · NGC 1938 · NGC 1939 · NGC 1940 · NGC 1943 · NGC 1949 · NGC 1950 · NGC 1953 · NGC 1955 · NGC 1958 · NGC 1959 · NGC 1962 · NGC 1965 · NGC 1967 · NGC 1968 · NGC 1969 · NGC 1970 · NGC 1971 · NGC 1972 · NGC 1974 · NGC 1983 · NGC 1984 · NGC 1986 · NGC 1987 · NGC 1994 · NGC 2000 · NGC 2001 · NGC 2004 · NGC 2005 · NGC 2009 · NGC 2010 · NGC 2011 · NGC 2014 · NGC 2015 · NGC 2016 · NGC 2018 · NGC 2019 · NGC 2020 · NGC 2021 · NGC 2025 · NGC 2028 · NGC 2030 · NGC 2031 · NGC 2032 · NGC 2033 · NGC 2035 · NGC 2036 · NGC 2037 · NGC 2038 · NGC 2040 · NGC 2042 · NGC 2044 · NGC 2046 · NGC 2047 · NGC 2048 · NGC 2050 · NGC 2051 · NGC 2052 · NGC 2053 · NGC 2055 · NGC 2056 · NGC 2057 · NGC 2059 · NGC 2060 · NGC 2065 · NGC 2066 · NGC 2069 · NGC 2070 · NGC 2072 · NGC 2074 · NGC 2075 · NGC 2078 · NGC 2079 · NGC 2081 · NGC 2083 · NGC 2084 · NGC 2085 · NGC 2088 · NGC 2091 · NGC 2092 · NGC 2093 · NGC 2094 · NGC 2095 · NGC 2096 · NGC 2098 · NGC 2100 · NGC 2102 · NGC 2103 · NGC 2107 · NGC 2108 · NGC 2109 · NGC 2111 · NGC 2113 · NGC 2114 · NGC 2116 · NGC 2117 · NGC 2118 · NGC 2121 · NGC 2122 · NGC 2125 · NGC 2127 · NGC 2133 · NGC 2134 · NGC 2136 · NGC 2137 · NGC 2145 · Tarantula Nebula · The star βMen · The star θDor · bet Men · tet Dor

Status	Advanced success
Started	...
PixInsight job	2PQA6STR9VQB9H0R02M3L09W0A46VC5M
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	05h23m37s.99
RA (top/left)	05h58m41s.60
RA (top/right)	05h51m38s.97
RA (bottom/right)	04h56m36s.48
RA (bottom/left)	04h47m38s.25

Dec (center)	-69°45′42″.8
Dec (top/left)	-72°18′29″.3
Dec (top/right)	-66°57′18″.6
Dec (bottom/right)	-66°52′37″.7
Dec (bottom/left)	-72°12′42″.5

AstroBin

AstroBin

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