Vincent Minier

Submm/FIR astronomy in Antarctica: Potential for a large telescope facility (2008)

Minier, Vincent, Minier, V., Olmi, L., Spinoglio, L., Durand, G.A., ...

Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500 micron regime, i.e. for far-infrared (FIR) and...

Submm/FIR astronomy in Antarctica: Potential for a large telescope facility (2008)

Minier, Vincent, Minier, V., Olmi, L., Spinoglio, L., Durand, G.A., ...

Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500 micron regime, i.e. for far-infrared (FIR) and...

Submm/FIR astronomy in Antarctica: Potential for a large telescope facility (2008)

Minier, Vincent, Minier, V., Olmi, L., Spinoglio, L., Durand, G. A., ...

Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500 micron regime, i.e. for far-infrared (FIR) and...

Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)

Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...

Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out...

Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)

Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...

Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out...

Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array (2007)

Minier, Vincent, Durand, Gilles, Lagage, Pierre-Olivier, Talvard, Michel, Travouillon, Tony, Busso, Maurizio, ...

Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out...

A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)

Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...

We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...

A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)

Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...

We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...

A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)

Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...

We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...

A search for propylene oxide and glycine in Sagittarius B2 (LMH) and Orion (2007)

Cunningham, Maria R., Jones, Paul A., Godfrey, Peter D., Cragg, Dinah M., Bains, Indra, Burton, Michael G., ...

We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected either species, but have...

Molecular line mapping of the giant molecular cloud associated with RCW 106 I : 13 (CO) (2006)

Bains, Indra, Wong, Tony H., Cunningham, Maria R., Sparks, Patricia A., Brisbin, D., Calisse, Paolo G., ...

We present the first paper in a series detailing the results of (CO)-C-13 observations of a similar to 1 deg(2) region of the giant molecular cloud (GMC) complex associated with the H II region RCW...

A CH3CN and HCO+ survey towards southern methanol masers associated with star formation (2006)

Purcell, Cormac R., Balasubramanyam, Ramesh, Burton, Michael G., Walsh, Andrew J., Minier, Vincent, Hunt-Cunningham, Maria R., ...

We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected massive star-forming regions. Here, we report observations of the J Combining double low line 5-4 and...

Molecular line mapping of the giant molecular cloud associated with RCW 106 I : 13 (CO) (2006)

Bains, Indra, Wong, Tony H., Cunningham, Maria R., Sparks, Patricia A., Brisbin, D., Calisse, Paolo G., ...

We present the first paper in a series detailing the results of (CO)-C-13 observations of a similar to 1 deg(2) region of the giant molecular cloud (GMC) complex associated with the H II region RCW...

A CH3CN and HCO+ survey towards southern methanol masers associated with star formation (2006)

Purcell, Cormac R., Balasubramanyam, Ramesh, Burton, Michael G., Walsh, Andrew J., Minier, Vincent, Hunt-Cunningham, Maria R., ...

We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected massive star-forming regions. Here, we report observations of the J Combining double low line 5-4 and...

Molecular line mapping of the giant molecular cloud associated with RCW 106 I : 13 (CO) (2006)

Bains, Indra, Wong, Tony H., Cunningham, Maria R., Sparks, Patricia A., Brisbin, D., Calisse, Paolo G., ...

We present the first paper in a series detailing the results of (CO)-C-13 observations of a similar to 1 deg(2) region of the giant molecular cloud (GMC) complex associated with the H II region RCW...

A CH3CN and HCO+ survey towards southern methanol masers associated with star formation (2006)

Purcell, Cormac R., Balasubramanyam, Ramesh, Burton, Michael G., Walsh, Andrew J., Minier, Vincent, Hunt-Cunningham, Maria R., ...

We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected massive star-forming regions. Here, we report observations of the J Combining double low line 5-4 and...

Molecular line mapping of the giant molecular cloud associated with RCW 106 I : 13 (CO) (2006)

Bains, Indra, Wong, Tony H., Cunningham, Maria R., Sparks, Patricia A., Brisbin, D., Calisse, Paolo G., ...

We present the first paper in a series detailing the results of (CO)-C-13 observations of a similar to 1 deg(2) region of the giant molecular cloud (GMC) complex associated with the H II region RCW...

A CH3CN and HCO+ survey towards southern methanol masers associated with star formation (2006)

Purcell, Cormac R., Balasubramanyam, Ramesh, Burton, Michael G., Walsh, Andrew J., Minier, Vincent, Hunt-Cunningham, Maria R., ...

We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected massive star-forming regions. Here, we report observations of the J Combining double low line 5-4 and...

Millimetre continuum observations of southern massive star formation regions - II. SCUBA observations of cold cores and the dust grain emissivity index (beta) (2006)

Thompson, M, Pierce-Price, D, ...

We report the results of a submillimetre continuum emission survey targeted towards 78 star formation regions, 72 of which are devoid of methanol maser and UC H II regions, identified in the Swedish...

Millimetre continuum observations of southern massive star formation regions - II. SCUBA observations of cold cores and the dust grain emissivity index (beta) (2006)

Thompson, M, Pierce-Price, D, ...

We report the results of a submillimetre continuum emission survey targeted towards 78 star formation regions, 72 of which are devoid of methanol maser and UC H II regions, identified in the Swedish...

Investigating the Nature of the Dust Emission around Massive Protostar NGC 7538 IRS 1: Circumstellar Disk and Outflow? (2005)

De Buizer, James M., Minier, Vincent

We have obtained high resolution mid-infrared images of the high mass protostar NGC 7538 IRS 1 using Michelle on Gemini North and find that the circumstellar dust associated with this source is...

Science programs for a 2-m class telescope at Dome C, Antarctica : PILOT, the pathfinder for an international large optical telescope (2005)

Ashley, Michael C., Bailey, Jeremy A., Bedding, Timothy R., Blake, Christopher J., Bland-Hawthorn, Jonathan, Bond, I. A., ...

The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....

Science programs for a 2-m class telescope at Dome C, Antarctica: PILOT, the pathfinder for an international large optical telescope (2005)

Burton, Michael G., Lawrence, J. S., Ashley, M. C. B., Bailey, J. A., Blake, Chris, Bedding, T. R., ...

The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....

Science programs for a 2-m class telescope at Dome C, Antarctica : PILOT, the pathfinder for an international large optical telescope (2005)

Ashley, Michael C., Bailey, Jeremy A., Bedding, Timothy R., Blake, Christopher J., Bland-Hawthorn, Jonathan, Bond, I. A., ...

The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....

Science programs for a 2-m class telescope at Dome C, Antarctica : PILOT, the pathfinder for an international large optical telescope (2005)

Ashley, Michael C., Bailey, Jeremy A., Bedding, Timothy R., Blake, Christopher J., Bland-Hawthorn, Jonathan, Bond, I. A., ...

The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....