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EROS microlensing survey home page

EROS stands for 'Expérience pour la Recherche d'Objets Sombres'. And has known 2 observational phases :. The list of available papers. Related to the EROS experiment is there. Supernovae SN1987a Light Echoes. Monitored by EROS2. ( NEW. Photos de la journée du 23 mai 2003. Eros is financed jointly by CEA. One image before, and the other, two years latter during the maximum of amplification :. 6 New Magellanic R Coronae Borealis stars. New Beat Cepheids found in the Magellanic Clouds. Limit on Machos :.

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EROS microlensing survey home page | eros.in2p3.fr Reviews
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EROS stands for 'Expérience pour la Recherche d'Objets Sombres'. And has known 2 observational phases :. The list of available papers. Related to the EROS experiment is there. Supernovae SN1987a Light Echoes. Monitored by EROS2. ( NEW. Photos de la journée du 23 mai 2003. Eros is financed jointly by CEA. One image before, and the other, two years latter during the maximum of amplification :. 6 New Magellanic R Coronae Borealis stars. New Beat Cepheids found in the Magellanic Clouds. Limit on Machos :.
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2 eros 1
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9 la silla
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EROS microlensing survey home page | eros.in2p3.fr Reviews

https://eros.in2p3.fr

EROS stands for 'Expérience pour la Recherche d'Objets Sombres'. And has known 2 observational phases :. The list of available papers. Related to the EROS experiment is there. Supernovae SN1987a Light Echoes. Monitored by EROS2. ( NEW. Photos de la journée du 23 mai 2003. Eros is financed jointly by CEA. One image before, and the other, two years latter during the maximum of amplification :. 6 New Magellanic R Coronae Borealis stars. New Beat Cepheids found in the Magellanic Clouds. Limit on Machos :.

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eros.in2p3.fr eros.in2p3.fr
1

Presentation of Eros

http://eros.in2p3.fr/presentation.html

Gravitational lensing and micro-lensing. Microlensing and brown dwarfs. Other fields covered by EROS. Back to home page. Gravitational lensing and micro-lensing. Einstein demonstrated that light rays are bent in a gravitational field. This was first evidenced in 1919 by observing small displacements in the apparent positions of stars that happened to lie near the Sun during the total solar eclipse of May 29th of that year. Microlensing and brown dwarfs. Other fields covered by EROS. The EROS experiment m...

2

EROS2 : R Coronae Borealis - Large Magellanic Clouds

http://eros.in2p3.fr/Variables/RCB/RCB-LMC.html

EROS2 - LMC SMC Fields. New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connection between RCBs, DYPers and ordinary carbon stars" (Article: Astro-ph. RCBs description and Data. Approximate position of the Magellanic RCB stars. EROS2 confirmed Magellanic RCB stars :. 151; Ascii Data file : Red. 151; Ascii Data file : Red. 151; Ascii Data file : Red. 151; Ascii Data file : Red. 151; Ascii Data file : Red. 151; Ascii Data file : Red. 151; Ascii Data file : Red.

3

EROS2 : R Coronae Borealis - SMC

http://eros.in2p3.fr/Variables/RCB/RCB-SMC.html

EROS-2 photometry of probable R Coronae Borealis Stars in the Small Magellanic Cloud" (Article: Astro-ph. Approximate position of the 5 EROS2 RCB stars with the 10 SMC fields observed during 7 years. RCB identifiers and J H K magnitudes. We present, for each RCB candidate, the EROS2 ligthcurves (V. During the seven observing years and the finding charts. It is possible to download the image in gif or fits format and an ASCII file to obtain these raw data, organised as followed:. 00:37:47.07 ;. Http:/ mor...

4

Publications d'EROS

http://eros.in2p3.fr/publications.html

Here is a list of available papers about the EROS experiment :. Authors: P.Tisserand, et al. (EROS collaboration) New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connection between RCBs, DYPers and ordinary carbon stars. Accepted in A&A, ( Web site. Authors: J.B.Marquette, et al. (EROS collaboration) The beat Cepheids in the Magellanic Clouds: an analysis from the EROS-2 database. Published in A&A : 2009A&A.495.249M. Published in A&A : 2007A&A.469.387T. Recherc...

5

Eros 18/11/2002

http://eros.in2p3.fr/latestCG/index.html

We present a new EROS-2 measurement of the microlensing optical depth toward the Galactic Bulge. Light curves of 5.6 &times 10. Clump-giant stars distributed over 66 deg. Of the Bulge were monitored during seven Bulge seasons. 120 events were found with apparent amplifications greater than 1.6 and Einstein radius crossing times in the range. 5 d &lt t. Lt 400 d. This is the largest existing sample of clump-giant events and the first to include northern Galactic fields. Lightcurves.120.ps.gz.

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LINKS TO THIS WEBSITE

araucaria.camk.edu.pl araucaria.camk.edu.pl

Classical Cepheid in eclipsing binary OGLE LMC562.05-9009

https://araucaria.camk.edu.pl/p/cep9009

The Araucaria Project: Discovery and study of the classical Cepheid in the eclipsing binary system OGLE LMC562.05-9009 in the Large Magellanic Cloud. Photometry data that were used in the paper:. V-band data from the OGLE. 143 points) and the MACHO. Ic-band data from the OGLE. 588 points) and the EROS. Rc-band data from the MACHO. V-band data from the OGLE. 96 points) project and the MACHO. Ic-band data from the OGLE. 521 points) project and the EROS. Rc-band data from the MACHO. 222 points) project .

eros.web.lal.in2p3.fr eros.web.lal.in2p3.fr

EROS home page

http://eros.web.lal.in2p3.fr/erosa.html

Our web site has been moved to : http:/ eros.in2p3.fr/. Clickez ici voir voir la version francaise. Server - Work in progress . Accesses since Jan. 06 1997. Our main topic is the search for microlensing events induced by brown dwarfs located in our galaxy on stars from the Large Magelanic Cloud. You will eventually find in this server :. Our results toward Galactic Spiral Arms and the variable stars catalogue in these directions. Sorry, in french.). Or in gzipped PostScript. Or in gzipped PostScript.

araucaria.camk.edu.pl araucaria.camk.edu.pl

Physical parameters of the OGLE-LMC-CEP-0227

https://araucaria.camk.edu.pl/p/cep2532

The Araucaria Project: The FO Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-2532. B Pilecki, D. Graczyk, W. Gieren, G. Pietrzyński, I. B. Thompson, R. Smolec, A. Udalski, I. Soszyński, P. Konorski, M. Taormina, A. Gallenne, D. Minniti and M. Catelan. Photometry data that were used in the paper:. V-band data from the OGLE. 230 points) and the MACHO. Ic-band data from the OGLE. 1322 points) and the EROS. Rc-band data from the MACHO. V-band data from the OGLE. Ic-band data from the OGLE.

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eros.gen.tr eros.gen.tr

Eros.Gen.Tr - Eros, Eros Geciktirici Sprey, Eros Krem, Eros Geciktiriciler, Eros Tablet, Spreyler, Ürün, Ürünler, Çeşitleri

eros.group.shef.ac.uk eros.group.shef.ac.uk

EROS Research Group

Emotion Regulation of Others and Self. General overview of the EROS project. EROS People - Researchers. EROS consists of a large number of researchers collaborating across five universities. Find out more about us here. EROS People - Advisory Board. Some text about the advisory board. The EROS project is divided into six core projects. To read more about these please select one of the projects below. This project investigates the brain areas implicated in emotion regulation. View photos of the EROS team.

eros.hu eros.hu

Erős Kft - Burkolóanyag, szaniter, szerelvény.

GÖRGESSEN LE VAGY KATTINTSON. 1107 Budapest, Száva utca 12. TEL: 36 1 260-4380,. 36 1 262 5945,. 36 70 702-0727,. 36 70 702-0728,. E-MAIL: szaniter.plaza@eros.hu. TEL: 36 1 263-1902. MOBIL: 36 70 702-0715. FAX: 36 1 263-2939. 1037 Budapest, Bécsi út 256. TEL: 36 1 439-4480,. 36 1 439-4481,. 36 70 702-0726,. 36 70 702-0716,. 36 70 702-0714,. 36 70 702-0708,. 36 70 702-0734,. FAX: 36 1 256-8925. Termékcsoportok - Erős Kft. Burkolóanyag, szaniter, szerelvények. Az ERŐS név szinte mindenki számára ismert, ak...

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eros.in2p3.fr eros.in2p3.fr

EROS microlensing survey home page

EROS stands for 'Expérience pour la Recherche d'Objets Sombres'. And has known 2 observational phases :. The list of available papers. Related to the EROS experiment is there. Supernovae SN1987a Light Echoes. Monitored by EROS2. ( NEW. Photos de la journée du 23 mai 2003. Eros is financed jointly by CEA. One image before, and the other, two years latter during the maximum of amplification :. 6 New Magellanic R Coronae Borealis stars. New Beat Cepheids found in the Magellanic Clouds. Limit on Machos :.

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