activity
20102025
most citedYSOVAR: the first sensitive, wide-area, mid-IR photometric monitoring of the ONC

234 citations · 985 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2025

A New Spectral Class of Brown Dwarfs at the Bottom of the IMF in IC 348

K. L. Luhman, C. Alves de Oliveira

In a previous study, we used JWST to identify three new brown dwarfs in the center of a nearby star-forming cluster, IC 348. The faintest object had an estimated mass of 3-4 $M_{\r…

astro-ph.SR2024

Medium Resolution 0.97-5.3 micron spectra of Very Young Benchmark Brown Dwarfs with NIRSpec onboard the James Webb Space Telescope

Elena Manjavacas, Pascal Tremblin, Stephan Birkmann +7

Spectra of young benchmark brown dwarfs with well-known ages are vital to characterize other brown dwarfs, for which ages are in general not known. These spectra are also crucial t…

astro-ph.SR2023

JWST/NIRSpec Observations of the Coldest Known Brown Dwarf

K. L. Luhman, P. Tremblin, C. Alves de Oliveira +6

We present 1-5um spectroscopy of the coldest known brown dwarf, WISE J085510.83-071442.5 (WISE 0855), performed with the Near-Infrared Spectrograph (NIRSpec) on board the James Web…

astro-ph.SR2023★ 9 cited

On the origin of planetary-mass objects in NGC1333

Richard J. Parker, Catarina Alves de Oliveira

The dominant formation mechanism of brown dwarfs and planetary mass objects in star-forming regions is presently uncertain. Do they form like stars, via the collapse and fragmentat…

astro-ph.EP2023★ 42 cited

JWST/NIRSpec Observations of the Planetary Mass Companion TWA 27B

K. L. Luhman, P. Tremblin, S. M. Birkmann +8

We present 1-5um spectroscopy of the young planetary mass companion TWA 27B (2M1207B) performed with NIRSpec on board the James Webb Space Telescope. In these data, the fundamental…

astro-ph.IM2023★ 183 cited

In-orbit Performance of the Near-Infrared Spectrograph NIRSpec on the James Webb Space Telescope

T. Böker, T. L. Beck, S. M. Birkmann +47

The Near-Infrared Spectrograph (NIRSpec) is one of the four focal plane instruments on the James Webb Space Telescope. In this paper, we summarize the in-orbit performance of NIRSp…

astro-ph.SR2023

Discovery of dusty sub-solar mass young stellar objects in NGC 346 with JWST/NIRCam

Olivia C. Jones, Conor Nally, Nolan Habel +23

JWST observations of NGC 346, a star-forming region in the metal-poor Small Magellanic Cloud, reveal a substantial population of sub-solar mass young stellar objects (YSOs) with IR…

astro-ph.EP2022★ 2 cited

ESA-Ariel Data Challenge NeurIPS 2022: Inferring Physical Properties of Exoplanets From Next-Generation Telescopes

Kai Hou Yip, Ingo P. Waldmann, Quentin Changeat +11

The study of extra-solar planets, or simply, exoplanets, planets outside our own Solar System, is fundamentally a grand quest to understand our place in the Universe. Discoveries i…

astro-ph.GA2017★ 33 cited

Dynamical histories of the IC348 and NGC1333 star-forming regions in Perseus

Richard J. Parker, Catarina Alves de Oliveira

We present analyses of the spatial distributions of stars in the young (1 - 3 Myr) star-forming regions IC348 and NGC1333 in the Perseus Giant Molecular Cloud. We quantify the spat…

astro-ph.IM2016★ 46 cited

A model-based approach to the spatial and spectral calibration of NIRSpec onboard JWST

Bernhard Dorner, Giovanna Giardino, Pierre Ferruit +8

Context: The NIRSpec instrument for the James Webb Space Telescope (JWST) can be operated in multiobject (MOS), long-slit, and integral field (IFU) mode with spectral resolutions f…

astro-ph.SR2014★ 101 cited

Young Stellar Object Variability (YSOVAR): Long Timescale Variations in the Mid-Infrared

L. M. Rebull, A. M. Cody, K. R. Covey +32

The YSOVAR (Young Stellar Object VARiability) Spitzer Space Telescope observing program obtained the first extensive mid-infrared (3.6 & 4.5 um) time-series photometry of the Orion…

astro-ph.GA2014★ 77 cited

Herschel's view of the large-scale structure in the Chamaeleon dark clouds

C. Alves de Oliveira, N. Schneider, B. Merín +17

The Chamaeleon molecular cloud complex is one of the nearest star-forming sites encompassing three molecular clouds with a different star-formation history, from quiescent (Cha III…

astro-ph.GA2013★ 27 cited

Herschel survey of brown dwarf disks in Rho Ophiuchi

C. Alves de Oliveira, P. Ábrahám, G. Marton +6

Recent observations of the Rho Ophiuchi cluster with the Herschel Space Observatory allow us to probe the spectral energy distribution (SED) of the brown dwarf population in the fa…

astro-ph.SR2013

The Herschel Gould Belt Survey in Chamaeleon II - Properties of cold dust in disks around young stellar objects

L. Spezzi, N. L. J. Cox, T. Prusti +14

We report on the Herschel Gould Belt survey (HGBS) of ChaII, focusing on the detection of Class I to III young stellar objects (YSOs). We aim at characterizing the circumstellar ma…

astro-ph.EP2013★ 17 cited

Identification of transitional disks in Chamaeleon with Herschel

Á. Ribas, B. Merín, H. Bouy +11

Transitional disks are circumstellar disks with inner holes that in some cases are produced by planets and/or substellar companions in these systems. For this reason, these disks a…

astro-ph.SR2013★ 18 cited

A molecular outflow driven by the brown dwarf binary FU Tau

J. -L. Monin, E. Whelan, B. Lefloch +2

We report the detection of a molecular outflow driven by the brown dwarf binary FU Tau. Using the IRAM 30 m telescope we observed the CO(2-1) (CO) emission in the vicinity o…

astro-ph.SR2012★ 17 cited

Searching for planetary-mass T-dwarfs in the core of Serpens

L. Spezzi, C. Alves de Oliveira, E. Moraux +5

We searched for isolated planetary-mass T-dwarfs in the 3Myr old Serpens Core cluster. We performed a deep imaging survey of the central part of this cluster using the WIRCam camer…

astro-ph.GA2012★ 27 cited

A search for mass segregation of stars and brown dwarfs in ρ Ophiuchi

Richard J. Parker, Thomas Maschberger, Catarina Alves de Oliveira

We apply two different algorithms to search for mass segregation to a recent observational census of the rho Ophiuchi star forming region. Firstly, we apply the Lambda_MSR method,…

astro-ph.SR2012★ 13 cited

An unusual very low-mass high-amplitude pre-main sequence periodic variable

Maria V. Rodriguez-Ledesma, Reinhard Mundt, Mansur Ibrahimov +5

We have investigated the nature of the variability of CHS7797, an unusual periodic variable in the Orion Nebula Cluster. An extensive I-band photometric data set of CHS7797 was com…

astro-ph.SR2012★ 9 cited

The dusty environment of HD 97300 as seen by Herschel and Spitzer

Á. Kóspál, T. Prusti, N. L. J. Cox +9

Aims. We analyze the surroundings of HD 97300, one of two intermediate-mass stars in the Chamaeleon I star-forming region. The star is known to be surrounded by a conspicuous ring…

astro-ph.GA2012★ 76 cited

Spectroscopy of new brown dwarf members of rho Ophiuchi and an updated initial mass function

C. Alves de Oliveira, E. Moraux, J. Bouvier +1

To investigate the universality hypothesis of the initial mass function in the substellar regime, the population of the rho Ophiuchi molecular cloud is analysed by including a new…

astro-ph.SR2011★ 234 cited

YSOVAR: the first sensitive, wide-area, mid-IR photometric monitoring of the ONC

M. Morales-Calderón, J. R. Stauffer, L. A. Hillenbrand +33

We present initial results from time series imaging at infrared wavelengths of 0.9 sq. degrees in the Orion Nebula Cluster (ONC). During Fall 2009 we obtained 81 epochs of Spitzer…

astro-ph.GA2010★ 54 cited

The low-mass population of the Rho Ophiuchi molecular cloud

C. Alves de Oliveira, E. Moraux, J. Bouvier +3

Star formation theories are currently divergent regarding the fundamental physical processes that dominate the substellar regime. Observations of nearby young open clusters allow t…