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19972023
most citedSpitzer 70-micron Source Counts in GOODS-North

127 citations · 1k across the 25 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 45 cited

Two stripped envelope supernovae with circumstellar interaction -- but only one really shows it

J. Sollerman, C. Fransson, C. Barbarino +23

We present SN 2019tsf (ZTF19ackjszs) and SN 2019oys (ZTF19abucwzt). These two stripped envelope Type Ib supernovae suddenly showed a (re-)brightening in their late light curves. We…

astro-ph.HE2020★ 21 cited

SN 2020bqj: a Type Ibn supernova with a long lasting peak plateau

E. C. Kool, E. Karamehmetoglu, J. Sollerman +31

Context: Type Ibn supernovae are a rare class of stripped envelope supernovae interacting with a helium-rich CSM. The majority of the SNe Ibn reported display a surprising homogene…

astro-ph.GA2020★ 122 cited

The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]

M. Dessauges-Zavadsky, M. Ginolfi, F. Pozzi +32

The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity,…

astro-ph.GA2020★ 125 cited

The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8

Yoshinobu Fudamoto, P. A. Oesch, A. Faisst +34

We present dust attenuation properties of spectroscopically confirmed star forming galaxies on the main sequence at a redshift of ~4.4-5.8. Our analyses are based on the far infrar…

astro-ph.HE2020★ 57 cited

SN2020bvc: a Broad-lined Type Ic Supernova with a Double-peaked Optical Light Curve and a Luminous X-ray and Radio Counterpart

A. Y. Q. Ho, S. R. Kulkarni, D. A. Perley +34

We present optical, radio, and X-ray observations of SN2020bvc (=ASASSN20bs; ZTF20aalxlis), a nearby (; =114 Mpc) broad-lined (BL) Type Ic supernova (SN). Our observat…

astro-ph.GA2020★ 46 cited

The ALPINE-ALMA [CII] survey: Small Lya-[CII] velocity offsets in main-sequence galaxies at 4.4 < z < 6

P. Cassata, L. Morselli, A. Faisst +30

The Lya line in the UV and the [CII] line in the FIR are widely used tools to identify galaxies and to obtain insights into ISM properties in the early Universe. By combining data…