B. Schulz

Hi-GAL, the Herschel infrared Galactic Plane Survey: Photometric maps and compact source catalogues: First data release for the inner Milky Way: +68° ≥ l ≥ -70°

ALMA OBSERVATIONS OF WARM DENSE GAS IN NGC 1614—BREAKING OF THE STAR FORMATION LAW IN THE CENTRAL KILOPARSEC

The HerMES submillimetre local and low-redshift luminosity functions

Herschel Multitiered Extragalactic Survey: clusters of dusty galaxies uncovered by Herschel★ and Planck†

Calibration of the Herschel SPIRE Fourier Transform Spectrometer★

HerMES: point source catalogues from Herschel-SPIRE observations II★

The Herschel★ PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4

Detection of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>B</mml:mi></mml:math>-Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope

EXPLAINING THE [C II]157.7 μm DEFICIT IN LUMINOUS INFRARED GALAXIES—FIRST RESULTS FROM A<i>HERSCHEL</i>/PACS STUDY OF THE GOALS SAMPLE

MID-INFRARED PROPERTIES OF NEARBY LUMINOUS INFRARED GALAXIES. I. <i>SPITZER</i> INFRARED SPECTROGRAPH SPECTRA FOR THE GOALS SAMPLE

HerMES: COSMIC INFRARED BACKGROUND ANISOTROPIES AND THE CLUSTERING OF DUSTY STAR-FORMING GALAXIES

The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3

HerMES: CANDIDATE HIGH-REDSHIFT GALAXIES DISCOVERED WITH<i>HERSCHEL</i>/SPIRE,

HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHS

A COSMIC MICROWAVE BACKGROUND LENSING MASS MAP AND ITS CORRELATION WITH THE COSMIC INFRARED BACKGROUND

The<i>Herschel</i>Multi-tiered Extragalactic Survey: HerMES

HerMES: deep number counts at 250 <i>μ</i>m, 350 <i>μ</i>m and 500 <i>μ</i>m in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background

The suppression of star formation by powerful active galactic nuclei

THE<i>HERSCHEL</i>EXPLOITATION OF LOCAL GALAXY ANDROMEDA (HELGA). II. DUST AND GAS IN ANDROMEDA

HerMES: unveiling obscured star formation – the far-infrared luminosity function of ultraviolet-selected galaxies at z ∼ 1.5