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In this study I present new K and L$'$-band infrared photometry and 2-4$\mu$m spectra of ten Class I and flat spectrum stars forming within the Taurus dark cloud complex. Nine sources have H$_2$ {\it v}=0-1 S(1) emission, and some show…

Astrophysics · Physics 2008-11-26 Tracy L. Beck

The combination of the AKARI and WISE infrared all-sky surveys provides an unique opportunity to identify and characterize the most highly dust obscured AGNs in the universe. Dust-obscured AGNs are not easily detectable and potentially…

Astrophysics of Galaxies · Physics 2018-08-06 Anson Lam , Matthew A. Malkan , Edward L. Wright

We present near-infrared spectra of three low-luminosity protostars and one background star in the Perseus molecular cloud, acquired using the Infrared Camera (IRC) onboard the \textit{AKARI} space telescope. For the comparison with…

Breakthrough direct detections of planetary companions orbiting A-type stars confirm the existence of massive planets at relatively large separations, but dedicated surveys are required to estimate the frequency of similar planetary…

Earth and Planetary Astrophysics · Physics 2015-06-05 A. Vigan , J. Patience , C. Marois , M. Bonavita , R. J. De Rosa , B. Macintosh , I. Song , R. Doyon , B. Zuckerman , D. Lafrenière , T. Barman

We present near-infrared spectral measurements of Themis family asteroid (379) Huenna (D~98 km) and its 6 km satellite using SpeX on the NASA IRTF. The companion was farther than 1.5" from the primary at the time of observations and was…

We carried out low-resolution optical spectroscopy of 51 main-belt asteroids, most of which have highly-inclined orbits. They are selected from D-type candidates in the SDSS-MOC 4 catalog. Using the University of Hawaii 2.2 m telescope and…

Earth and Planetary Astrophysics · Physics 2020-06-03 Aya Iwai , Yoichi Itoh , Tsuyoshi Terai , Ranjan Gupta , Asoke Sen , Jun Takahashi

Near-Earth asteroids Ryugu and Bennu, were visited, characterised, and sampled by the Hayabusa2 and OSIRIS-REx missions: remote sensing data and sample return analysis showed that both asteroids have primitive, hydrated and organic-rich…

Earth and Planetary Astrophysics · Physics 2023-12-06 Marco Delbo , Chrysa Avdellidou , Kevin J. Walsh

With the plentiful information available in the Gaia BP/RP spectra, there is significant scope for applying discriminative models to extract stellar atmospheric parameters and abundances. We describe an approach to leverage an `Uncertain…

Solar and Stellar Astrophysics · Physics 2024-05-20 Connor P. Fallows , Jason L. Sanders

The AKARI Deep Field South (ADF-S) is a ~12 sq. deg. region near the South Ecliptic Pole that has been observed with deep scans in the far-infrared by the AKARI satellite. As such it is becoming one of the key extragalactic survey fields.…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 D. L. Clements , G. Bendo , C. Pearson , Sophia A. Khan , S. Matsuura , M. Shirahata

We present the first Spitzer Infrared Spectrograph (IRS; The IRS was a collaborative venture between Cornell University and Ball Aerospace Corporation funded by NASA through the Jet Propulsion Laboratory and the Ames Research Center.)…

Context. The sizes of many asteroids, especially slowly rotating, low-amplitude targets, remain poorly constrained due to selection effects. These biases limit the availability of high-quality data, leaving size estimates reliant on…

Earth and Planetary Astrophysics · Physics 2025-05-16 A. Choukroun , A. Marciniak , J. Ďurech , J. Perła , W. Ogłoza , R. Szakats , L. Molnar , A. Pal , F. Monteiro , I. Mieczkowska , W. Beisker , D. Agnetti , C. Anderson , S. Andersson , D. Antuszewicz , P. Arcoverde , R. -L. Aubry , P. Bacci , R. Bacci , P. Baruffetti , L. Benedyktowicz , M. Bertini , D. Blazewicz , R. Boninsegna , Zs. Bora , M. Borkowski , E. Bredner , J. Broughton , M. Butkiewicz - Bąk , N. Carlson , G. Casalnuovo , F. Casarramona , Y. -J. Choi , S. Cikota , M. Collins , B. Cseh , G. Csörnyei , H. De Groot , P. Delincak , P. Denyer , R. Dequinze , M. Dogramatzidis , M. Drozdz , R. Duffard , D. Eisfeldt , M. Eleftheriou , C. Ellington , S. Fauvaud , M. Fauvaud , M. Ferrais , M. Filipek , P. Fini , M. Frits , B. Gährken , G. Galli , D. Gault , S. Geier , B. Gimple , J. Golonka , L. Grazzini , J. Grice , K. Guhl , W. Hanna , M. Harman , W. Hasubick , T. Haymes , D. Herald , D. Higgins , R. Hirsch , J. Horbowicz , A. Horti - David , B. Ignacz , E. Jehin , A. Jones , R. Jones , D. Dunham , Cs. Kalup , K. Kaminski , M. K. Kaminska , P. Kankiewicz , M. Kaplan , A. Karagiannidis , B. Kattentidt , S. Kidd , B. Kirpluk , D. -H. Kim , M. -J. Kim , I. Konstanciak , G. Krannich , M. Kretlow , J. Kubanek , V. Kudak , P. Kulczak , M. Lecossois , R. Leiva , M. Libert , J. Licandro , P. Lindner , R. Liu , Y. Liu , G. Lyzenga , M. Maestripieri , C. Malagon , P. Maley , A. Manna , S. Messner , O. Michniewicz , M. A. Miftah , M. Mizutani , N. Morales , M. Murawiecka , J. Nadolny , T. Nemoto , J. Newman , V. Nikitin , P. Nosal , P. Nosworthy , M. O'Connell , J. Oey , A. M. Ortiz-Ochoa , A. Ossola , D. Oszkiewicz , E. Pakstiene , M. Pawlowski , V. Perig , E. Petrescu , F. Pilcher , E. Podlewska-Gaca , M. Polacek , J. Polak , T. Polakis , M. Polinska , A. Popowicz , V. Reddy , J. -J. Rives , M. Rottenborn , N. Ruocco , A. Rutkowski , K. Saci , T. Santana-Ros , K. Sarneczky , O. Schreurs , V. Sempronio , B. Skiff , J. Skrzypek , D. Smith , K. Sobkowiak , E. Sonbas , S. Sposetti , C. Stewart , W. Stewart , T. Swift , M. Szkudlarek , K. Szyszka , N. Takacs , L. Tychoniec , M. Uno , S. Urakawa , K. Vida , C. Weber , N. Wünsche , H. Yamamura , H. Yoshihara , M. Zawilski , P. Zeleny , S. Zola , M. Zejmo , K. Zukowski

We have studied several color-color infrared diagrams of the 276 late type stars of the BIS catalog. For 95 of these stars we derived spectral classification from our slit spectroscopy. From the 2MASS color diagram we derive that none of…

Solar and Stellar Astrophysics · Physics 2017-08-16 S. Gaudenzi , S. Gaudenzi , R. Nesci , C. Rossi , S. Sclavi , K. S. Gigoyan , A. M. Mickaelian

There is significant scientific value to be gained from combining AKARI fluxes with data at other far-IR wavelengths from the IRAS and Herschel missions. To be able to do this we must ensure that there are no systematic differences between…

We report the results of a search for emission features from interstellar deuterated polycyclic aromatic hydrocarbons (PAHs) in the 4um region with the Infrared Camera (IRC) onboard AKARI. No significant excess emission is seen in 4.3-4.7um…

Astrophysics of Galaxies · Physics 2015-06-17 Takashi Onaka , Tamami I. Mori , Itsuki Sakon , Ryou Ohsawa , Hidehiro Kaneda , Yoko Okada , Masahiro Tanaka

The amount of deuterium locked up in polycyclic aromatic hydrocarbons (PAHs) has to date been an uncertain value. We present a near-infrared (NIR) spectroscopic survey of HII regions in the Milky Way, Large Magellanic Cloud (LMC), and Small…

Astrophysics of Galaxies · Physics 2016-01-27 Kirstin D. Doney , Alessandra Candian , Tamami Mori , Takashi Onaka , A. G. G. M. Tielens

Spitzer Space Telescope IRAC 3-8 micron and AKARI IRC 2-4 micron photometry are reported for ten white dwarfs with photospheric heavy elements; nine relatively cool stars with photospheric calcium, and one hotter star with a peculiar high…

Earth and Planetary Astrophysics · Physics 2015-03-13 J. Farihi , M. Jura , J. -E. Lee , B. Zuckerman

We present a supervised, probabilistic taxonomic classification of asteroid reflectance spectra from Gaia Data Release 3 (DR3). Using high-quality Gaia DR3 spectra and a reference set of spectra from the literature consisting exclusively of…

Earth and Planetary Astrophysics · Physics 2026-03-02 Marco Delbo , Thomas Dyer , Ullas Bhat , Chrysa Avdellidou , Laurent Galluccio , Amelia Milton

We present a far-infrared all-sky atlas from a sensitive all-sky survey using the Japanese $AKARI$ satellite. The survey covers $> 99$% of the sky in four photometric bands centred at 65 $\mu$m, 90 $\mu$m, 140 $\mu$m, and 160 $\mu$m with…

Comet C/2007 N3 (Lulin) was observed with the Japanese infrared satellite AKARI in the near-infrared at a post-perihelion heliocentric distance of 1.7 AU. Observations were performed with the spectroscopic (2.5--5.0 micron) and imaging…

Spectroscopic observations from the ultraviolet to the mid-infrared have revealed new and diagnostic differences among primitive asteroids. We review the spectral characteristics of these asteroids and their inferred compositional and…

Earth and Planetary Astrophysics · Physics 2018-09-06 Humberto Campins , Julia de Leon , Javier Licandro , Amanda Hendrix , Juan A. Sanchez , Victor Ali-Lagoa