Next, prepare the planting hole. Dig the hole three times as large and deep as the root ball. Once the dirt is dug out, break up the chunks and return it all to the hole. Then dig another hole in the loosened soil about the size of the root ball.
Dig a trench around the mature avocado tree. Keep digging deeper, expanding the hole if necessary to accommodate the entire root ball. When you can slip your shovel under the root ball, remove the tree and place it in a tarp. Get help to lift it if necessary. Moving an avocado tree is sometimes easier with two people.
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Dogs and cats are not herbivores like cows, horses and goats. Manure from omnivorous animals may carry harmful parasites that can cause disease in people. It is best bury this material in a hole in your backyard 12 inches deep, covered with 6 inches of soil, in a non-food growing area of the yard. This material is also NOT allowed in the food waste/yard debris bin.
One of the most surprising results from our previous Spitzer observations is the discovery of a class of quasars at z 6 without detectable hot dust emission in the mid-IR. These objects have the narrowest emission lines at z 6 with FWHM 1600 km/s, but share all other characteristics of normal type-1 quasars in their broad-band SEDs from X-ray to radio. Based on virial mass estimates, they have relatively small black hole (BH) masses and high Eddington luminosity ratios. The existence of such objects may indicate strong evolution in dust properties at early epochs; alternatively, it could be an orientation effect and challenge the standard AGN unification model. No such narrow-line type-1 quasars without hot dust emission have been found at low redshift. However, these objects are very rare, counting for only one percent of the quasar population at z < 5, and none of them have been observed at the Spitzer sensitivity. Therefore, we propose to carry out four band Spitzer photometry of a sample of 15 luminous narrow-line type-1 quasars at z = 1 - 5 selected from the SDSS quasar catalog. All objects have excellent optical spectroscopy and BH mass measurements. The Spitzer photometry will be used to directly measure the mid-IR hot dust emission in these objects. Combined with Spitzer observations of broad-line quasars and low-redshift Narrow-line Seyfert 1 galaxis, the new Spitzer data will allow us to answer the following questions: (1) How does the fraction of hot-dust-free quasars evolve with redshift; do hot-dust-free quasars only exist at the earliest epochs, or are they common among mature quasars as well (2) How is the hot dust emission in narrow-line type-1 quasars related to BH mass, accretion rate, luminosity, line of sight obscuration, and emission line wind The proposed observations will provide crucial probes to the evolution of dust structures in quasars and its relation to BH growth in the early universe.
Clusters of galaxies are the largest structures in the Universe that are held together by gravity. Astronomers expect these clusters to grow through time and hence that massive clusters would be rare in the early Universe. Although even more distant clusters have been seen, they appear to be young clusters in the process of formation and are not settled mature systems.
Once the team knew the distance to this very rare object they looked carefully at the component galaxies using both the NASA/ESA Hubble Space Telescope and ground-based telescopes, including the VLT. They found evidence suggesting that most of the galaxies in the cluster were not forming stars, but were composed of stars that were already about one billion years old. This makes the cluster a mature object, similar in mass to the Virgo Cluster, the nearest rich galaxy cluster to the Milky Way. 59ce067264