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A STRANGE intergalactic force is drawing our Milky Way galaxy inward. We don’t know what, or why. But a hidden swarm of hundreds of nearby galaxies just discovered by Australian astronomers may help reveal the identity of the ‘Great Attractor’.
This pack of galaxies has been spotted by astronomers using CSIRO’s Parkes Observatory in NSW. The international study involved researchers from Australia, South Africa, the US and the Netherlands, and was published today in Astronomical Journal.
Despite being ‘just next door’ in astronomical terms — a mere 250 million light years away — these galaxies have remained hidden from view because they are on the opposite side of our own.

The intensity of stars and dust crowded together along the plane of the Milky Way is directly in the line of sight — masking everything behind it from view.
That something must be there has been known for some time.
Its immense gravitational pull — the equivalent of a million billion Suns — has been observed through calculations of strange deviations in the flight path of nearby galaxies.
And our own.
Full report:
http://www.news.com.au/technology/science/hidden-cluster-of-galaxies-reveals-the-dark-force-drawing-in-the-milky-way/news-story/bfee4995edf310dce4c16686de6da089
Technical article on arxiv from year 2000 about techniques in all wavelength bands for seeing galaxies in the great attractor.
http://arxiv.org/ps/astro-ph/0006199v1
Abstract from most recent paper.
THE PARKES H I ZONE OF AVOIDANCE SURVEY
L. Staveley-Smith1,2, R. C. Kraan-Korteweg3, A. C. Schröder4, P. A. Henning5, B. S. Koribalski6, I. M. Stewart7, and G. Heald8,9
Published 2016 February 9 • © 2016. The American Astronomical Society. All rights reserved. • The Astronomical Journal, Volume 151, Number 3
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Abstract
A blind H i survey of the extragalactic sky behind the southern Milky Way has been conducted with the multibeam receiver on the 64 m Parkes radio telescope. The survey covers the Galactic longitude range $212^\circ \lt {\ell }\lt 36^\circ $ and Galactic latitudes $| b| \lt 5^\circ $ to an rms sensitivity of 6 mJy per beam per 27 km s−1 channel and yields 883 galaxies to a recessional velocity of 12,000 km s−1. The survey covers the sky within the H i Parkes All-Sky Survey (HIPASS) area to greater sensitivity, finding lower H i mass galaxies at all distances, and probing more completely the large-scale structures at and beyond the distance of the Great Attractor. Fifty-one percent of the H i detections have an optical/near-infrared (NIR) counterpart in the literature. A further 27% have new counterparts found in existing, or newly obtained, optical/NIR images. The counterpart rate drops in regions of high foreground stellar crowding and extinction, and for low H i mass objects. Only 8% of all counterparts have a previous optical redshift measurement. The H i sources are found independently of Galactic extinction, although the detection rate drops in regions of high Galactic continuum. The survey is incomplete below a flux integral of approximately 3.1 Jy km s−1 and mean flux density of approximately 21 mJy, with 75% and 81% of galaxies being above these limits, respectively. Taking into account dependence on both flux and velocity width, and constructing a scaled dependence on the flux integral limit with velocity width (w0.74), completeness limits of 2.8 Jy km s−1 and 17 mJy are determined, with 92% of sources above these limits. A notable new galaxy is HIZOA J1353−58, a possible companion to the Circinus galaxy. Merging this catalog with the similarly conducted northern extension, large-scale structures are delineated, including those within the Puppis and Great Attractor regions and the Local Void. Several newly identified structures are revealed here for the first time. Three new galaxy concentrations (NW1, NW2, and NW3) are key in confirming the diagonal crossing of the Great Attractor Wall between the Norma Cluster and the CIZA J1324.7–5736 cluster. Further contributors to the general mass overdensity in that area are two new clusters (CW1 and CW2) in the nearer Centaurus Wall, one of which forms part of the striking 180° ($100\;{h}^{-1}$Mpc) long filament that dominates the southern sky at velocities of ~3000 km s−1, and the suggestion of a further wall at the Great Attractor distance at slightly higher longitudes.