activity
20012015
most citedThe Infrared Astronomical Mission AKARI

842 citations · 1.6k across the 14 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2015★ 98 cited

The Far-Infrared All-Sky Survey Maps

Yasuo Doi, Satoshi Takita, Takafumi Ootsubo +15

We present a far-infrared all-sky atlas from a sensitive all-sky survey using the Japanese satellite. The survey covers % of the sky in four photometric bands centred…

astro-ph.GA2011★ 16 cited

The Stellar Content of Obscured Galactic Giant HII Regions. VII. W3

F. Navarete, E. Figueredo, A. Damineli +3

Spectrophotometric distances in the K band have been reported by different authors for a number of obscured Galactic HII regions. Almost 50% of them show large discrepancies compar…

astro-ph.SR2010★ 83 cited

Spectrophotometric Distances to Galactic H\,{\sc{ii}} Regions

A. P. Moisés, A. Damineli, E. Figuerêdo +3

We present a near infrared study of the stellar content of 35 H\,{\sc{ii}} regions in the Galactic plane. In this work, we have used the near infrared domain , and $K_{s}-…

astro-ph2008★ 6 cited

Timeline analysis and wavelet multiscale analysis of the AKARI All-Sky Survey at 90 micron

Lingyu Wang, Michael Rowan-Robinson, Issei Yamamura +17

We present a careful analysis of the point source detection limit of the AKARI All-Sky Survey in the WIDE-S 90 m band near the North Ecliptic Pole (NEP). Timeline Analysis is us…

astro-ph2008★ 28 cited

High Spatial Resolution Spectroscopy of W51 IRS2E and IRS2W: Two Very Massive Young Stars in Early Formation Stages

C. L. Barbosa, R. D. Blum, P. S. Conti +2

We present -band spectra of the near infrared counterparts to IRS2E and IRS2W which is associated with the ultracompact HII region W51d, both of them embedded sources in the Gal…

astro-ph2008

The Stellar Content of Obscured Galactic Giant HII Regions. VI: W51A

E. Figueredo, R. D. Blum, A. Damineli +2

We present K-band spectra of newly born OB stars in the obscured Galactic giant H II region W51A and ~ 0.8'' angular resolution images in the J, H and K_S-bands. Four objects have…