activity
20002021
most citedComplex organic molecules in comets C/2012 F6 (Lemmon) and C/2013 R1 (Lovejoy): detection of ethylene glycol and formamide

131 citations · 750 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.EP2021★ 37 cited

Molecular composition of comet 46P/Wirtanen from millimetre-wave spectroscopy

N. Biver, D. Bockelée-Morvan, J. Boissier +11

We present the results of a molecular survey of comet 46P/Wirtanen undertaken with the IRAM 30-m and NOEMA radio telescopes in December 2018. Observations at IRAM 30-m during the 1…

astro-ph.IM2019★ 6 cited

Design, operation and performance of the PAON4 prototype transit interferometer

R. Ansari, J. E Campagne, D. Charlet +14

PAON4 is an L-band (1250-1500 MHz) small interferometer operating in transit mode deployed at the Nançay observatory in France, designed as a prototype instrument for Intensity Map…

astro-ph.IM2018★ 5 cited

Progress in the Construction and Testing of the Tianlai Radio Interferometers

Santanu Das, Christopher J. Anderson, Reza Ansari +44

The Tianlai Pathfinder is designed to demonstrate the feasibility of using a wide field of view radio interferometers to map the density of neutral hydrogen in the Universe after t…

astro-ph.EP2016★ 11 cited

Comets at radio wavelengths

Jacques Crovisier, Dominique Bockelée-Morvan, Pierre Colom +1

Comets are considered as the most primitive objects in the Solar System. Their composition provides information on the composition of the primitive solar nebula, 4.6 Gyr ago. The r…

astro-ph.EP2016★ 103 cited

Isotopic ratios of H, C, N, O, and S in comets C/2012 F6 (Lemmon) and C/2014 Q2 (Lovejoy)

N. Biver, R. Moreno, D. Bockelée-Morvan +15

The apparition of bright comets C/2012 F6 (Lemmon) and C/2014 Q2 (Lovejoy) in March-April 2013 and January 2015, combined with the improved observational capabilities of submillime…

astro-ph.EP2015

Ethyl alcohol and sugar in comet C/2014Q2 (Lovejoy)

Nicolas Biver, Dominique Bockelée-Morvan, Raphaël Moreno +7

The presence of numerous complex organic molecules (COMs; defined as those containing six or more atoms) around protostars shows that star formation is accompanied by an increase o…

astro-ph.GA2014★ 7 cited

OH and H2O maser variations in W33B

P. Colom, E. E. Lekht, M. I. Pashchenko +1

The active star-forming region W33B is a source of OH and H2O maser emission located in distinct zones around the central object. The aim was to obtain the complete Stokes pattern…

astro-ph.EP2014★ 131 cited

Complex organic molecules in comets C/2012 F6 (Lemmon) and C/2013 R1 (Lovejoy): detection of ethylene glycol and formamide

N. Biver, D. Bockelée-Morvan, V. Debout +9

A spectral survey in the 1 mm wavelength range was undertaken in the long-period comets C/2012 F6 (Lemmon) and C/2013 R1 (Lovejoy) using the 30 m telescope of the Institut de radio…

astro-ph.EP2013★ 23 cited

Gas and dust productions of comet 103P/Hartley 2 from millimetre observations: interpreting rotation-induced time variations

J. Boissier, D. Bockelée-Morvan, N. Biver +7

Comet 103P/Hartley 2 made a close approach to the Earth in October 2010. It was the target of an extensive observing campaign and was visited by the Deep Impact spacecraft (mission…

astro-ph.EP2013★ 8 cited

Millimetre continuum observations of comet C/2009 P1 (Garradd)

J. Boissier, D. Bockelée-Morvan, O. Groussin +7

Little is known about the physical properties of the nuclei of Oort cloud comets. Measuring the thermal emission of a nucleus is one of the few means for deriving its size and cons…

astro-ph.CO2012★ 20 cited

BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures

Réza Ansari, Jean-Eric Campagne, Pierre Colom +5

3D mapping of matter distribution in the universe through the 21 cm radio emission of atomic hydrogen HI is a complementary approach to optical surveys for the study of the Large S…

astro-ph.GA2012★ 4 cited

The Source of Maser Emission W33C (G12.8-0.2)

P. Colom, E. E. Lekht, M. I. Pashchenko +1

Results of observations of the maser sources toward the W33C region (G12.8-0.2) carried out on the 22-m radio telescope of the Pushchino Radio Astronomy Observatory in the 1.35-cm…

astro-ph.EP2012★ 12 cited

Observations of the 18-cm OH lines of comet 103P/Hartley 2 at Nançay in support to the EPOXI and Herschel missions

Jacques Crovisier, Pierre Colom, Nicolas Biver +2

The 18-cm radio lines of the OH radical were observed in comet 103P/Hartley 2 with the Nançay radio telescope in support to its flyby by the EPOXI mission and to observations with…

astro-ph.CO2011★ 51 cited

21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction

R. Ansari, J. E. Campagne, P. Colom +6

Large Scale Structures (LSS) in the universe can be traced using the neutral atomic hydrogen HI through its 21cm emission. Such a 3D matter distribution map can be used to test the…

astro-ph.IM2011★ 1 cited

BAORadio : Cartographie 3D de la distribution de gaz H dans l'Univers

R. Ansari, J. E. Campagne, P. Colom +5

3D mapping of matter distribution in the universe through the 21 cm radio emission of atomic hydrogen is a complementary approach to optical surveys for the study of the Large Scal…

astro-ph.HE2011★ 39 cited

HESS J1943+213: a candidate extreme BL Lacertae object

H. E. S. S. Collaboration, :, A. Abramowski +200

We report on a newly detected point-like source, HESS J1943+213 located in the Galactic plane. This source coincides with an unidentified hard X-ray source IGR J19443+2117, which w…

astro-ph.EP2011★ 29 cited

Molecular investigations of comets C/2002 X5 (Kudo-Fujikawa), C/2002 V1 (NEAT), and C/2006 P1 (McNaught) at small heliocentric distances

N. Biver, D. Bockelée-Morvan, P. Colom +4

We present unique spectroscopic radio observations of comets C/2002 X5 (Kudo-Fujikawa), C/2002 V1 (NEAT), and C/2006 P1 (McNaught), which came within $r_h ~ 0.2 AU of the Sun in 20…

astro-ph.EP2011★ 14 cited

Earth-based detection of the millimetric thermal emission of the nucleus of comet 8P/Tuttle

J. Boissier, O. Groussin, L. Jorda +7

Little is known about the physical properties of cometary nuclei. Apart from space mission targets, measuring the thermal emission of a nucleus is one of the few means to derive it…

astro-ph.EP2009★ 16 cited

Interferometric imaging of carbon monoxide in comet C/1995 O1 (Hale-Bopp): evidence for a strong rotating jet

D. Bockelée-Morvan, F. Henry, N. Biver +6

Observations of the CO J(1-0) 115 GHz and J(2-1) 230 GHz lines in comet C/1995 O1 (Hale-Bopp) were performed with the IRAM Plateau de Bure interferometer on 11 March, 1997. The obs…

astro-ph.EP2009★ 48 cited

The chemical diversity of comets

J. Crovisier, N. Biver, D. Bockelée-Morvan +3

A fundamental question in cometary science is whether the different dynamical classes of comets have different chemical compositions, which would reflect different initial conditio…

astro-ph2008★ 39 cited

Radio observations of Jupiter-family comets

J. Crovisier, N. Biver, D. Bockelée-Morvan +1

Radio observations from decimetric to submillimetric wavelengths are now a basic tool for the investigation of comets. Spectroscopic observations allow us i) to monitor the gas pro…

astro-ph2008★ 125 cited

Large excess of heavy nitrogen in both hydrogen cyanide and cyanogen from comet 17P/Holmes

D. Bockelée-Morvan, N. Biver, E. Jehin +15

From millimeter and optical observations of the Jupiter-family comet 17P/Holmes performed soon after its huge outburst of October 24, 2007, we derive 14 N/15N = 139 +/- 26 in HCN,…

astro-ph2006★ 20 cited

Radio observations of comet 9P/Tempel 1 before and after Deep Impact

N. Biver, D. Bockelée-Morvan, J. Boissier +14

Comet 9P/Tempel 1 was the target of a multi-wavelength worldwide investigation in 2005. The NASA Deep Impact mission reached the comet on 4.24 July 2005, delivering a 370 kg impact…

astro-ph2000★ 1 cited

A ridge of recent massive star formation between Sgr B2M and Sgr B2N

P. de Vicente, J. Martin-Pintado, R. Neri +1

We present single dish and interferometric maps of several rotational transitions of HC3N vibrationally excited levels towards Sgr B2. The single dish maps show, for the first time…