1. Home
  2. Search Results

Search options

Orientation
Colour

Display options

View

Print

To print search results, use print friendly version of this page.

2497570 Search Results

Clamart intercommunal cemetery in the Hauts de Seine.
Clamart intercommunal cemetery in the Hauts de Seine.

TEC4650788: Clamart intercommunal cemetery in the Hauts de Seine. / Bridgeman Images

ID: TEC4650788

Clamart intercommunal cemetery in the Hauts de Seine.

Rue Maurice Arnoult in Montrouge in the Hauts de Seine.
Rue Maurice Arnoult in Montrouge in the Hauts de Seine.

TEC4650939: Rue Maurice Arnoult in Montrouge in the Hauts de Seine. / Bridgeman Images

ID: TEC4650939

Rue Maurice Arnoult in Montrouge in the Hauts de Seine.

Rue Ernest Renan in Malakoff in the Hauts de Seine.
Rue Ernest Renan in Malakoff in the Hauts de Seine.

TEC4651067: Rue Ernest Renan in Malakoff in the Hauts de Seine. / Bridgeman Images

ID: TEC4651067

Rue Ernest Renan in Malakoff in the Hauts de Seine.

Rue Danton a Vanves in the Hauts de Seine.
Rue Danton a Vanves in the Hauts de Seine.

TEC4651143: Rue Danton a Vanves in the Hauts de Seine. / Bridgeman Images

ID: TEC4651143

Rue Danton a Vanves in the Hauts de Seine.

Courbevoie in the Hauts de Seine. Photography 01/10/95.
Courbevoie in the Hauts de Seine. Photography 01/10/95.

TEC4651286: Courbevoie in the Hauts de Seine. Photography 01/10/95. / Bridgeman Images

ID: TEC4651286

Courbevoie in the Hauts de Seine. Photography 01/10/95.

Post office in Puteaux in the Hauts de Seine.
Post office in Puteaux in the Hauts de Seine.

TEC4651339: Post office in Puteaux in the Hauts de Seine. / Bridgeman Images

ID: TEC4651339

Post office in Puteaux in the Hauts de Seine.

Puteaux in the Hauts de Seine. Photography 01/10/95.
Puteaux in the Hauts de Seine. Photography 01/10/95.

TEC4651345: Puteaux in the Hauts de Seine. Photography 01/10/95. / Bridgeman Images

ID: TEC4651345

Puteaux in the Hauts de Seine. Photography 01/10/95.

Courbevoie in the Hauts de Seine. Photography 01/10/95.
Courbevoie in the Hauts de Seine. Photography 01/10/95.

TEC4651568: Courbevoie in the Hauts de Seine. Photography 01/10/95. / Bridgeman Images

ID: TEC4651568

Courbevoie in the Hauts de Seine. Photography 01/10/95.

Ile de la Jatte in the Hauts de Seine. The island of la Jatte, formerly called the island of Grande Jatte, is an island on the Seine, located between Neuilly sur Seine and Levallois Perret on its right bank, Courbevoie and the business district of La Defense on its left bank. Photography 01/10/95.
Ile de la Jatte in the Hauts de Seine. The island of la Jatte, formerly called the island of Grande Jatte, is an island on the Seine, located between Neuilly sur Seine and Levallois Perret on its right bank, Courbevoie and the business district of La Defense on its left bank. Photography 01/10/95.

TEC4651615: Ile de la Jatte in the Hauts de Seine. The island of la Jatte, formerly called the island of Grande Jatte, is an island on the Seine, located between Neuilly sur Seine and Levallois Perret on its right bank, Courbevoie and the business district of La Defense on its left bank. Photography 01/10/95. / Bridgeman Images

ID: TEC4651615

Ile de la Jatte in the Hauts de Seine. The island of la Jatte, formerly called the island of Grande Jatte, is an island on the Seine, located between Neuilly sur Seine and Levallois Perret on its right bank, Courbevoie and the business district of La Defense on its left bank. Photography 01/10/95.

Social housing in Gennevilliers (Hauts de Seine).
Social housing in Gennevilliers (Hauts de Seine).

TEC4651684: Social housing in Gennevilliers (Hauts de Seine). / Bridgeman Images

ID: TEC4651684

Social housing in Gennevilliers (Hauts de Seine).

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200
Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

PIX4651695: Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200 / Bridgeman Images

ID: PIX4651695

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200
Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

PIX4651720: Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200 / Bridgeman Images

ID: PIX4651720

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

21/01/00: Calern Observatory (CERGA): interferometer GI2T - Calern observatory (CERGA): the GI2T/Regain interferometer
21/01/00: Calern Observatory (CERGA): interferometer GI2T - Calern observatory (CERGA): the GI2T/Regain interferometer

PIX4652108: 21/01/00: Calern Observatory (CERGA): interferometer GI2T - Calern observatory (CERGA): the GI2T/Regain interferometer / Bridgeman Images

ID: PIX4652108

21/01/00: Calern Observatory (CERGA): interferometer GI2T - Calern observatory (CERGA): the GI2T/Regain interferometer

The Soirdete interferometer observes cool stars at infrared wavelengths.: Observatory of Calern (CERGA): interferometer Soirdete - Calern observatory (CERGA): the Soirdete interferometer
The Soirdete interferometer observes cool stars at infrared wavelengths.: Observatory of Calern (CERGA): interferometer Soirdete - Calern observatory (CERGA): the Soirdete interferometer

PIX4652194: The Soirdete interferometer observes cool stars at infrared wavelengths.: Observatory of Calern (CERGA): interferometer Soirdete - Calern observatory (CERGA): the Soirdete interferometer / Bridgeman Images

ID: PIX4652194

The Soirdete interferometer observes cool stars at infrared wavelengths.: Observatory of Calern (CERGA): interferometer Soirdete - Calern observatory (CERGA): the Soirdete interferometer

Basin of L'Octagon, transformed by Andre le Notre. Parc du chateau de Sceaux (Hauts de Seine). The park and its gardens were designed by Andre Le Notre in 1673 for Colbert. It was enlarged by the Marquis de Seignelay, the son of Colbert, who in particular had the Grand Canal excavated.
Basin of L'Octagon, transformed by Andre le Notre. Parc du chateau de Sceaux (Hauts de Seine). The park and its gardens were designed by Andre Le Notre in 1673 for Colbert. It was enlarged by the Marquis de Seignelay, the son of Colbert, who in particular had the Grand Canal excavated.

ITR4652263: Basin of L'Octagon, transformed by Andre le Notre. Parc du chateau de Sceaux (Hauts de Seine). The park and its gardens were designed by Andre Le Notre in 1673 for Colbert. It was enlarged by the Marquis de Seignelay, the son of Colbert, who in particular had the Grand Canal excavated. / Bridgeman Images

ID: ITR4652263

Basin of L'Octagon, transformed by Andre le Notre. Parc du chateau de Sceaux (Hauts de Seine). The park and its gardens were designed by Andre Le Notre in 1673 for Colbert. It was enlarged by the Marquis de Seignelay, the son of Colbert, who in particular had the Grand Canal excavated.

Plateau de Chajnantor et voie lactee - Chajnantor plateau and milky way - Réseau Alma. Chajnantor Plateau, 5100 m altitude, Chile. June 2008 Alma network, Chajnantor plateau in Atacama Desert, Chile. June 2008
Plateau de Chajnantor et voie lactee - Chajnantor plateau and milky way - Réseau Alma. Chajnantor Plateau, 5100 m altitude, Chile. June 2008 Alma network, Chajnantor plateau in Atacama Desert, Chile. June 2008

PIX4652289: Plateau de Chajnantor et voie lactee - Chajnantor plateau and milky way - Réseau Alma. Chajnantor Plateau, 5100 m altitude, Chile. June 2008 Alma network, Chajnantor plateau in Atacama Desert, Chile. June 2008 / Bridgeman Images

ID: PIX4652289

Plateau de Chajnantor et voie lactee - Chajnantor plateau and milky way - Réseau Alma. Chajnantor Plateau, 5100 m altitude, Chile. June 2008 Alma network, Chajnantor plateau in Atacama Desert, Chile. June 2008

ALMA - Plateau de Chajnantor - 2011 - Chajnantor plateau and starry sky - Alma Reseau. The Moon shines in the center of the lactee lane. Chajnantor Plateau, 5100 m altitude, Chile. October 2011. ALMA under the Moon in Milky Way. Chajnantor plateau in Atacama Desert, Chile. October 2011
ALMA - Plateau de Chajnantor - 2011 - Chajnantor plateau and starry sky - Alma Reseau. The Moon shines in the center of the lactee lane. Chajnantor Plateau, 5100 m altitude, Chile. October 2011. ALMA under the Moon in Milky Way. Chajnantor plateau in Atacama Desert, Chile. October 2011

PIX4652301: ALMA - Plateau de Chajnantor - 2011 - Chajnantor plateau and starry sky - Alma Reseau. The Moon shines in the center of the lactee lane. Chajnantor Plateau, 5100 m altitude, Chile. October 2011. ALMA under the Moon in Milky Way. Chajnantor plateau in Atacama Desert, Chile. October 2011 / Bridgeman Images

ID: PIX4652301

ALMA - Plateau de Chajnantor - 2011 - Chajnantor plateau and starry sky - Alma Reseau. The Moon shines in the center of the lactee lane. Chajnantor Plateau, 5100 m altitude, Chile. October 2011. ALMA under the Moon in Milky Way. Chajnantor plateau in Atacama Desert, Chile. October 2011

Chateau de Sceaux (Hauts de Seine). The Musee de l'Ile de France is located on the ground floor of the chateau and opened its doors in 1937.
Chateau de Sceaux (Hauts de Seine). The Musee de l'Ile de France is located on the ground floor of the chateau and opened its doors in 1937.

ITR4652335: Chateau de Sceaux (Hauts de Seine). The Musee de l'Ile de France is located on the ground floor of the chateau and opened its doors in 1937. / Bridgeman Images

ID: ITR4652335

Chateau de Sceaux (Hauts de Seine). The Musee de l'Ile de France is located on the ground floor of the chateau and opened its doors in 1937.

Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimeter antennas Alma located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile
Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimeter antennas Alma located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile

PIX4652596: Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimeter antennas Alma located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile / Bridgeman Images

ID: PIX4652596

Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimeter antennas Alma located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile

Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimetric antennas ALMA (Atacama Large Millimeter Array) located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile
Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimetric antennas ALMA (Atacama Large Millimeter Array) located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile

PIX4652609: Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimetric antennas ALMA (Atacama Large Millimeter Array) located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile / Bridgeman Images

ID: PIX4652609

Radiotelescopes ALMA - The Atacama Large Millimeter Array (ALMA) - Artwork - Artist's view of the European network of submilimetric antennas ALMA (Atacama Large Millimeter Array) located in the Atacama Desert, Chile. The Atacama Large Millimeter Array (ALMA), one of the largest ground - based astronomy projects of the next decade, is a major new facility for world astronomy. ALMA will be comprised of a giant array of 12 - m submillimetre quality antennas, with baselines of several kilometers. An additional, compact array of 7 - m and 12 - m antennas is also foreseen. Construction of ALMA started in 2003 and will be completed in 2010. The ALMA project is an international collaboration between Europe, Japan and North America in cooperation with the Republic of Chile

Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope
Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

PIX4652988: Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope / Bridgeman Images

ID: PIX4652988

Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view
Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view

PIX4653068: Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view / Bridgeman Images

ID: PIX4653068

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to

Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg
Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

PIX4653323: Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg / Bridgeman Images

ID: PIX4653323

Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

Housing building, 11 rue Agar in Paris 75016. Architect Hector Guimard (1867-1942), 1911.
Housing building, 11 rue Agar in Paris 75016. Architect Hector Guimard (1867-1942), 1911.

TEC4653725: Housing building, 11 rue Agar in Paris 75016. Architect Hector Guimard (1867-1942), 1911. / Bridgeman Images

ID: TEC4653725

Housing building, 11 rue Agar in Paris 75016. Architect Hector Guimard (1867-1942), 1911.

Hotel Guimard, 122 avenue Mozart in Paris 75016. Architect Hector Guimard (1867-1942), 1910-1913. Following his marriage in 1909, with the painter Adeline Oppenheim, Hector Guimard built a hotel for his home and his architect agency: 90 square meters on the ground on six levels with an elevator and an internal staircase. Following his deces, Adeline Oppenheim proposed to the State to transform the hotel on Avenue Mozart into a museum. She was refused. The furniture was scattered and the archives destroyed.
Hotel Guimard, 122 avenue Mozart in Paris 75016. Architect Hector Guimard (1867-1942), 1910-1913. Following his marriage in 1909, with the painter Adeline Oppenheim, Hector Guimard built a hotel for his home and his architect agency: 90 square meters on the ground on six levels with an elevator and an internal staircase. Following his deces, Adeline Oppenheim proposed to the State to transform the hotel on Avenue Mozart into a museum. She was refused. The furniture was scattered and the archives destroyed.

TEC4653758: Hotel Guimard, 122 avenue Mozart in Paris 75016. Architect Hector Guimard (1867-1942), 1910-1913. Following his marriage in 1909, with the painter Adeline Oppenheim, Hector Guimard built a hotel for his home and his architect agency: 90 square meters on the ground on six levels with an elevator and an internal staircase. Following his deces, Adeline Oppenheim proposed to the State to transform the hotel on Avenue Mozart into a museum. She was refused. The furniture was scattered and the archives destroyed. / Bridgeman Images

ID: TEC4653758

Hotel Guimard, 122 avenue Mozart in Paris 75016. Architect Hector Guimard (1867-1942), 1910-1913. Following his marriage in 1909, with the painter Adeline Oppenheim, Hector Guimard built a hotel for his home and his architect agency: 90 square meters on the ground on six levels with an elevator and an internal staircase. Following his deces, Adeline Oppenheim proposed to the State to transform the hotel on Avenue Mozart into a museum. She was refused. The furniture was scattered and the archives destroyed.

Immeuble Jassede 142 avenue de Versailles and 1 rue Lancret - Paris 16th arrondissement. Architect Hector Guimard (1867-1942), 1910-1913.
Immeuble Jassede 142 avenue de Versailles and 1 rue Lancret - Paris 16th arrondissement. Architect Hector Guimard (1867-1942), 1910-1913.

TEC4653769: Immeuble Jassede 142 avenue de Versailles and 1 rue Lancret - Paris 16th arrondissement. Architect Hector Guimard (1867-1942), 1910-1913. / Bridgeman Images

ID: TEC4653769

Immeuble Jassede 142 avenue de Versailles and 1 rue Lancret - Paris 16th arrondissement. Architect Hector Guimard (1867-1942), 1910-1913.

Aerial view of Dusseldorf, 1990 - Photography
Aerial view of Dusseldorf, 1990 - Photography

LRI4653826: Aerial view of Dusseldorf, 1990 - Photography / Bridgeman Images

ID: LRI4653826

Aerial view of Dusseldorf, 1990 - Photography

Aerial view of city with the castle on Neckar river, 1990 - Photography
Aerial view of city with the castle on Neckar river, 1990 - Photography

LRI4653871: Aerial view of city with the castle on Neckar river, 1990 - Photography / Bridgeman Images

ID: LRI4653871

Aerial view of city with the castle on Neckar river, 1990 - Photography

Aerial view of the city and the canal, 1990 - Photography
Aerial view of the city and the canal, 1990 - Photography

LRI4653880: Aerial view of the city and the canal, 1990 - Photography / Bridgeman Images

ID: LRI4653880

Aerial view of the city and the canal, 1990 - Photography

Aerial view of RWE Power plant in Essen, 1990 - Photography
Aerial view of RWE Power plant in Essen, 1990 - Photography

LRI4654091: Aerial view of RWE Power plant in Essen, 1990 - Photography / Bridgeman Images

ID: LRI4654091

Aerial view of RWE Power plant in Essen, 1990 - Photography

Telescope Swope - Las Campanas Observatory - Swope telescope - Las Campanas Observatory - Cupola du telescope de 1 metre Swope, Observatory of Las Campanas, Chile. Dome of the 1 meter Swope telescope, Las Campanas observatory, Chile
Telescope Swope - Las Campanas Observatory - Swope telescope - Las Campanas Observatory - Cupola du telescope de 1 metre Swope, Observatory of Las Campanas, Chile. Dome of the 1 meter Swope telescope, Las Campanas observatory, Chile

PIX4654098: Telescope Swope - Las Campanas Observatory - Swope telescope - Las Campanas Observatory - Cupola du telescope de 1 metre Swope, Observatory of Las Campanas, Chile. Dome of the 1 meter Swope telescope, Las Campanas observatory, Chile / Bridgeman Images

ID: PIX4654098

Telescope Swope - Las Campanas Observatory - Swope telescope - Las Campanas Observatory - Cupola du telescope de 1 metre Swope, Observatory of Las Campanas, Chile. Dome of the 1 meter Swope telescope, Las Campanas observatory, Chile

Aerial view of Luisenthal coal mine and Arbed steel factories, 1990 - Photography
Aerial view of Luisenthal coal mine and Arbed steel factories, 1990 - Photography

LRI4654117: Aerial view of Luisenthal coal mine and Arbed steel factories, 1990 - Photography / Bridgeman Images

ID: LRI4654117

Aerial view of Luisenthal coal mine and Arbed steel factories, 1990 - Photography

La Palma Observatory: The HEGRA Gamma - Ray Telescope - HEGRA (High - Energy - Gamma - Ray Astronomy) is a telescope located at the Roque de los Muchachos de La Palma Observatory, in the Canary Islands. After making gamma observations until 2002, it was replaced by the MAGIC telescopes. In the background, the GTC dome. HEGRA (High - Energy - Gamma - Ray Astronomy), was an atmospheric Cherenkov telescope for Gamma - ray astronomy. HEGRA took data between 1987 and 2002, at which point it was dismantled in order to build its successor, MAGIC, at the same site. GTC dome is in background
La Palma Observatory: The HEGRA Gamma - Ray Telescope - HEGRA (High - Energy - Gamma - Ray Astronomy) is a telescope located at the Roque de los Muchachos de La Palma Observatory, in the Canary Islands. After making gamma observations until 2002, it was replaced by the MAGIC telescopes. In the background, the GTC dome. HEGRA (High - Energy - Gamma - Ray Astronomy), was an atmospheric Cherenkov telescope for Gamma - ray astronomy. HEGRA took data between 1987 and 2002, at which point it was dismantled in order to build its successor, MAGIC, at the same site. GTC dome is in background

PIX4654563: La Palma Observatory: The HEGRA Gamma - Ray Telescope - HEGRA (High - Energy - Gamma - Ray Astronomy) is a telescope located at the Roque de los Muchachos de La Palma Observatory, in the Canary Islands. After making gamma observations until 2002, it was replaced by the MAGIC telescopes. In the background, the GTC dome. HEGRA (High - Energy - Gamma - Ray Astronomy), was an atmospheric Cherenkov telescope for Gamma - ray astronomy. HEGRA took data between 1987 and 2002, at which point it was dismantled in order to build its successor, MAGIC, at the same site. GTC dome is in background / Bridgeman Images

ID: PIX4654563

La Palma Observatory: The HEGRA Gamma - Ray Telescope - HEGRA (High - Energy - Gamma - Ray Astronomy) is a telescope located at the Roque de los Muchachos de La Palma Observatory, in the Canary Islands. After making gamma observations until 2002, it was replaced by the MAGIC telescopes. In the background, the GTC dome. HEGRA (High - Energy - Gamma - Ray Astronomy), was an atmospheric Cherenkov telescope for Gamma - ray astronomy. HEGRA took data between 1987 and 2002, at which point it was dismantled in order to build its successor, MAGIC, at the same site. GTC dome is in background

CFHT dome - Mauna Kea Observatory - Hawaii - CFHT dome - Mauna Kea Observatory - Hawaii - Mauna Kea Observatory, 4200 metres, altitude, Hawaii, USA. The 3.60 m CFHT telescope (Canada - France - Hawaii) with the rear lights of a car
CFHT dome - Mauna Kea Observatory - Hawaii - CFHT dome - Mauna Kea Observatory - Hawaii - Mauna Kea Observatory, 4200 metres, altitude, Hawaii, USA. The 3.60 m CFHT telescope (Canada - France - Hawaii) with the rear lights of a car

PIX4654930: CFHT dome - Mauna Kea Observatory - Hawaii - CFHT dome - Mauna Kea Observatory - Hawaii - Mauna Kea Observatory, 4200 metres, altitude, Hawaii, USA. The 3.60 m CFHT telescope (Canada - France - Hawaii) with the rear lights of a car / Bridgeman Images

ID: PIX4654930

CFHT dome - Mauna Kea Observatory - Hawaii - CFHT dome - Mauna Kea Observatory - Hawaii - Mauna Kea Observatory, 4200 metres, altitude, Hawaii, USA. The 3.60 m CFHT telescope (Canada - France - Hawaii) with the rear lights of a car

Telescope Gemini North - Gemini North Telescope - The 8.2 meter Gemini North telescope, at the Mauna Kea Observatory, Hawaii. Mauna Kea observatory, Hawaii, USA. The 8,2m Gemini North telescope
Telescope Gemini North - Gemini North Telescope - The 8.2 meter Gemini North telescope, at the Mauna Kea Observatory, Hawaii. Mauna Kea observatory, Hawaii, USA. The 8,2m Gemini North telescope

PIX4655055: Telescope Gemini North - Gemini North Telescope - The 8.2 meter Gemini North telescope, at the Mauna Kea Observatory, Hawaii. Mauna Kea observatory, Hawaii, USA. The 8,2m Gemini North telescope / Bridgeman Images

ID: PIX4655055

Telescope Gemini North - Gemini North Telescope - The 8.2 meter Gemini North telescope, at the Mauna Kea Observatory, Hawaii. Mauna Kea observatory, Hawaii, USA. The 8,2m Gemini North telescope

Telescope CFHT - Telescope Canada - France - Hawaii - The 3.60 m CFHT telescope (Canada - France - Hawaii) installs at an altitude of 4200 m, Mauna Kea observatory. The shadow of the volcano is projected on the sea of clouds. 200
Telescope CFHT - Telescope Canada - France - Hawaii - The 3.60 m CFHT telescope (Canada - France - Hawaii) installs at an altitude of 4200 m, Mauna Kea observatory. The shadow of the volcano is projected on the sea of clouds. 200

PIX4655064: Telescope CFHT - Telescope Canada - France - Hawaii - The 3.60 m CFHT telescope (Canada - France - Hawaii) installs at an altitude of 4200 m, Mauna Kea observatory. The shadow of the volcano is projected on the sea of clouds. 200 / Bridgeman Images

ID: PIX4655064

Telescope CFHT - Telescope Canada - France - Hawaii - The 3.60 m CFHT telescope (Canada - France - Hawaii) installs at an altitude of 4200 m, Mauna Kea observatory. The shadow of the volcano is projected on the sea of clouds. 200


Back to top