activity
20012025
most citedLow Temperature Opacities

1.3k citations · 2.7k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2025

Observation of CHOH and CHOH in Orion KL: A New Tool to Study Star-Formation History

Yoshimasa Watanabe, Takahiro Oyama, Akemi Tamanai +2

Methanol is a seed species of complex organic molecules that is of fundamental importance in astrochemistry. Although various isotopologues of CHOH have been detected in the in…

astro-ph.EP2024★ 29 cited

Dust mineralogy and variability of the inner PDS 70 disk

Hyerin Jang, Rens Waters, Till Kaeufer +17

The inner disk of the young star PDS 70 may be a site of rocky planet formation, with two giant planets detected further out. Solids in the inner disk may inform us about the origi…

astro-ph.IM2021★ 7 cited

Spectrometer Using superconductor MIxer Receiver (SUMIRE) for Laboratory Submillimeter Spectroscopy

Yoshimasa Watanabe, Yutaro Chiba, Takeshi Sakai +3

Recent spectroscopic observations by sensitive radio telescopes require accurate molecular spectral line frequencies to identify molecular species in a forest of lines detected. To…

astro-ph.SR2020★ 1 cited

Non-stoichiometric amorphous magnesium-iron silicates in circumstellar dust shells. Dust growth in outflows from supergiants

Hans-Peter Gail, Akemi Tamanai, Annemarie Pucci +1

We investigate the dust growth in oxygen-rich stellar outflows for a set of nine well-observed massive supergiants with optically thin dust shells. Models of the infrared emission…

astro-ph.SR2017★ 12 cited

Optical properties of non-stoichiometric amorphous silicates with application to circumstellar dust extinction

Akemi Tamanai, Annemarie Pucci, Ralf Dohmen +1

Optical constants of non-stoichiometric amorphous magnesium-iron silicates are determined. It is demonstrated that these can well reproduce the observed mid-infrared emission spect…

astro-ph.SR2013★ 19 cited

The twofold debris disk around HD 113766 A - Warm and cold dust as seen with VLTI/Midi and Herschel/Pacs

Johan Olofsson, Thomas Henning, Markus Nielbock +5

Warm debris disks are a sub-sample of the large population of debris disks, and display excess emission in the mid-IR. Around solar-type stars, very few objects show emission featu…