An Infrared Survey of Brightest Cluster...

Redshift histogram giving the number of clusters in our sample in redshift bins.

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

Each row shows one BCG. From left to right are shown the IRAC Band 1 (3.6 μm), the IRAC ...

An Infrared Survey of Brightest Cluster...

SEDs of the BCG. We have grouped them by 5.5/8.0 μm color. The fluxes are normalized to ...

An Infrared Survey of Brightest Cluster...

SEDs of the BCG. We have grouped them by 5.5/8.0 μm color. The fluxes are normalized to ...

An Infrared Survey of Brightest Cluster...

Infrared color‐color plot. Each axis is the ratio of the fluxes at the listed wavelength...

Spitzer IRS Spectra and Envelope Models...

IRS SL, LL, SH, and LH slit positions (only one of the two nod positions is shown) super...

Spitzer IRS Spectra and Envelope Models...

IRS spectra of Class I objects in Taurus.

Spitzer IRS Spectra and Envelope Models...

IRS spectra of Class I objects in Taurus.

Spitzer IRS Spectra and Envelope Models...

IRS spectra of Class I objects in Taurus.

Spitzer IRS Spectra and Envelope Models...

IRS spectra of Class I objects in Taurus.

Spitzer IRS Spectra and Envelope Models...

IRS spectra of Class I objects in Taurus.

Spitzer IRS Spectra and Envelope Models...

SED plots of the Class I objects in our sample, ordered alphabetically by their name. Op...

Spitzer IRS Spectra and Envelope Models...

SED plots of the Class I objects in our sample, ordered alphabetically by their name. Op...

Spitzer IRS Spectra and Envelope Models...

SED plots of the Class I objects in our sample, ordered alphabetically by their name. Op...

Spitzer IRS Spectra and Envelope Models...

SED plots of the Class I objects in our sample, ordered alphabetically by their name. Op...

Spitzer IRS Spectra and Envelope Models...

Sketch of an envelope model as described in § 4.1.

Spitzer IRS Spectra and Envelope Models...

IRS spectrum and photometric data of 04016+2610 and an envelope model fit with ﹩L=4.5﹩ L...

Spitzer IRS Spectra and Envelope Models...

IRS spectra of both components of the 21﹩\arcsec﹩ binary IRAS 04108+2803, plotted on the...

Spitzer IRS Spectra and Envelope Models...

IRS spectrum and photometric data of 04108+2803B and an envelope model fit with ﹩L=0.7﹩ ...

Spitzer IRS Spectra and Envelope Models...

IRS spectrum and photometric data of 04154+2823 and an envelope model fit with ﹩L=0.35﹩ ...