Sample

The Table below lists 22 galaxies in the MAGNHIFFIC sample. Green colors mark sources observed with MeerKAT open-time, orange colors mark sources observed by MHONGOOSE while blue cells show galaxies in the Fornax Cluster (i.e. observed by the MeerKAT Fornax Survey). The sample is divided between ra diative AGN and jetted AGN . The latter form a volume-flux limited sample in the nearby Universe (e.g. Ekers 1989, Ruffa et al. 2019).

Name	Ra [J2000]	Dec [J2000]	DL [Mpc]	Galaxy Type	AGN Type	Environment
NGC 1433	03h42m01.55s	-47d13m19.5s	14.9	SBb	Seyfert 2	group (N1434)
NGC 1386	03h36m46.18s	-35d59m57.87s	15.6	Sb	Seyfert 2	Fornax
NGC 5643	14h32m40.74s	-44d10m27.86s	17.3	Sc	Seyfert 2	Galaxy pair
NGC 1566	04h20m00.42s	-54d56m16.1s	17.6	Sc	Seyfert 1.5	group (Dorado)
NGC 1365	03h33m36.37s	-36d08m25.45s	18.6	Sc	Seyfert 1.8	Fornax
NGC 1672	04h45m42.50s	-59d14m49.85s	18.1	SBc	Seyfert 2	group (Dorado)
ESO 358-G063	03h46m19.01s	-34d56m36.8s	20.2	Sd	Seyfert	in Fornax
NGC 1371	03h35m01.34s	-24d55m59.64s	20.4	Sa	Seyfert	group (Eridanus)
NGC 0289	00h50m17.67s	-31d28m38.30s	22.9	Sb	Seyfert	group (N0134)
ESO 428-G14	03h42m01.55s	-47d13m19.51s	23.3	Sa	Seyfert 2	group
Centaurus A	13h25m27.62s	-43d01m08.81s	3.8	S0	RL restarted	BGG of group
NGC 1399	03h38m29.026s	-35d27m02.36s	19.7	E	RL / FRI	BCG Fornax
Fornax A	03h22m41.718s	-37d12m29.62s	20.8	S0	RL restarted	BGG of group
IC 1459	22h57m10.61s	-36d27m44.00s	25.9	E	RL / FRI	group
NGC 3100	10h00m40.8368s	-31d39m52.35s	38.0	S0	RF / FRI	BGG of group
NGC 3557	11h09m57.642s	-37d32m20.96s	44.5	E	RL / FRI	Poor group
IC 4296	13h36m39.03s	-33d57m57.00s	53.9	E	RL / FRI	BCG of A3537
PKS 1718-649	17h23m41.03s	-65d00m36.62s	62.4	S0	RL / GPS	Isolated
ESO 443-G024	13h01m00.79s	-32d26m28.70s	73.9	SA0	RL / FRI	in A3536
NGC 7075	21h31m32.98s	-38d37m04.50s	80.3	E	RL / FRI	Galaxy pair
IC 1531	00h09m35.577s	-32d16m37.22s	112	SAB0	RL / FRI	Isolated
NGC 612	01h33m57.74s	-36d29m35.70s	130	SA0	RL / FRI	Galaxy pair

The following surveys / projects provide the multi-wavelenght ancillary observations for MAGNIFFIC:

Radiative AGN

Jetted AGN

Reasons Why Zara Is So Successful

1. Really Fast Fashion

Supply chain management is the key to Zara’s success and much of it relies on the fact that they refresh collections almost twice a week — that’s a total of one hundred and four collections annually.

2. Vertical Integration

In a supply chain there are four main phases; sourcing, manufacturing, distribution and retail. A company vertically integrates when it controls two or more of these stages. This operating model enables brands to change collections

3. Cashing In On Trends

The millennial and Gen Z shoppers are frugal, value-minded and demand quick, on-trend fashion. Instead of spending money on research and development in an aim to be the next trendsetter or innovator

4. Limited Exclusivity

Most retailers and brands are used to working with a six month lead time — a tried-and-tested formula at that, but not without risk. By the time the stock rolls out, its at a higher risk of the trend turning outdated. With Zara’s on trend delivery