Over half of the far-infrared background light comes from galaxies at z ≥ 1.2

Devlin et al.

Nature 458 (2009)
arXiv:0904.1201

	BLAST GOODS-South (BGS) Maps: [README]
	250 μm:	Reduced	Noise	Hits	Decon	DeconNoise	Smooth	SmoothNoise	Filter
	350 μm:	Reduced	Noise	Hits	Decon	DeconNoise	Smooth	SmoothNoise	Filter
	500 μm:	Reduced	Noise	Hits	Decon	DeconNoise	Smooth	SmoothNoise	Filter

NOTE: On 4 May, 2009 our team realized that we had accidentally posted earlier versions of the 'Smooth' and 'SmoothNoise' maps. We have now replaced these maps with the correct versions, and apologise for any confusion this may have caused users who downloaded the earlier versions.

BLAST: The Mass Function, Lifetimes, and Properties of Intermediate Mass Cores from a 50 Square Degree Submillimeter Galactic Survey in Vela (ℓ = 265°)

Netterfield et al.

Submitted to the Astrophysical Journal
arXiv:0904.1207

A Bright Submillimeter Source in the Bullet Cluster (1E0657-56) Field Detected with BLAST

Rex et al.

Submitted to the Astrophysical Journal
arXiv:0904.1203

The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) 2006: Calibration and Flight Performance

Truch et al.

Submitted to the Astrophysical Journal
arXiv:0904.1202

BLAST: Resolving the Cosmic Submillimeter Background

Marsden et al.

Submitted to the Astrophysical Journal
arXiv:0904.1205

See BGS maps above

BLAST: A Far-Infrared Measurement of the History of Star Formation

Pascale et al.

Submitted to the Astrophysical Journal
arXiv:0904.1206

See BGS maps above

BLAST: Correlations in the Cosmic Far-Infrared Background at 250, 350, and 500 µm Reveal Clustering of Star-Forming Galaxies

Viero et al.

Submitted to the Astrophysical Journal
arXiv:0904.1200

See BGS maps above

Radio and Mid-Infrared Identification of BLAST Source Counterparts in the Chandra Deep Field South

Dye et al.

Submitted to the Astrophysical Journal
arXiv:0904.1204

See BGS maps above
Machine (and human) readable tables:
Table 1 Table 2 Table 3

Submillimeter Number Counts From Statistical Analysis of BLAST Maps

Patanchon et al.

Submitted to the Astrophysical Journal
arXiv:0906.0981

See BGS maps above

The Balloon-Borne Large Aperture Submillimeter (BLAST) 2005: Calibration and Targeted Sources

Truch et al.

Astrophys.J. 681 (2008) 415-427
arXiv:0804.0003

Note: Most of the structure seen in the maps at right are due to the PSF of BLAST05, not the source itself. See the appropriate README for more info.

The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 4 deg² Galactic Plane Survey in Vulpecula (ℓ = 59°)

Chapin et al.

Astrophys.J. 681 (2008) 428-452
arXiv:0711.3461

SANEPIC: A Map-Making Method for Timestream Data from Large Arrays

Patanchon et al.

Astrophys.J. 681 (2008) 708-725
arXiv:0711.3462

The Balloon-Borne Large Aperture Submillimeter Telescope: BLAST

Pascale et al.

Astrophys.J. 681 (2008) 400-414
arXiv:0711.3465