Sökning: WFRF:(Folatelli Gaston) > THE CARNEGIE SUPERN...
Fältnamn | Indikatorer | Metadata |
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000 | 03378naa a2200601 4500 | |
001 | oai:DiVA.org:su-70909 | |
003 | SwePub | |
008 | 120124s2011 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-709092 URI |
024 | 7 | a https://doi.org/10.1088/0004-6256/142/5/1562 DOI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Stritzinger, Maximilianu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)mstri |
245 | 1 0 | a THE CARNEGIE SUPERNOVA PROJECT :b SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE |
264 | c 2011-10-03 | |
264 | 1 | b American Astronomical Society,c 2011 |
338 | a print2 rdacarrier | |
500 | a authorCount :23 | |
520 | a The Carnegie Supernova Project (CSP) was a five-year observational survey conducted at Las Campanas Observatory that obtained, among other things, high-quality light curves of similar to 100 low-redshift Type Ia supernovae (SNe Ia). Presented here is the second data release of nearby SN Ia photometry consisting of 50 objects, with a subset of 45 having near-infrared follow-up observations. Thirty-three objects have optical pre-maximum coverage with a subset of 15 beginning at least five days before maximum light. In the near-infrared, 27 objects have coverage beginning before the epoch of B-band maximum, with a subset of 13 beginning at least five days before maximum. In addition, we present results of a photometric calibration program to measure the CSP optical (uBgVri) bandpasses with an accuracy of similar to 1%. Finally, we report the discovery of a second SN Ia, SN 2006ot, similar in its characteristics to the peculiar SN 2006bt. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a galaxies: distances and redshifts | |
653 | a supernovae: general | |
700 | 1 | a Phillips, M. M.4 aut |
700 | 1 | a Boldt, Luis N.4 aut |
700 | 1 | a Burns, Chris4 aut |
700 | 1 | a Campillay, Abdo4 aut |
700 | 1 | a Contreras, Carlos4 aut |
700 | 1 | a Gonzalez, Sergio4 aut |
700 | 1 | a Folatelli, Gaston4 aut |
700 | 1 | a Morrell, Nidia4 aut |
700 | 1 | a Krzeminski, Wojtek4 aut |
700 | 1 | a Roth, Miguel4 aut |
700 | 1 | a Salgado, Francisco4 aut |
700 | 1 | a DePoy, D. L.4 aut |
700 | 1 | a Hamuy, Mario4 aut |
700 | 1 | a Freedman, Wendy L.4 aut |
700 | 1 | a Madore, Barry F.4 aut |
700 | 1 | a Marshall, J. L.4 aut |
700 | 1 | a Persson, Sven E.4 aut |
700 | 1 | a Rheault, Jean-Philippe4 aut |
700 | 1 | a Suntzeff, Nicholas B.4 aut |
700 | 1 | a Villanueva, Steven4 aut |
700 | 1 | a Li, Weidong4 aut |
700 | 1 | a Filippenko, Alexei V.4 aut |
710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Astronomical Journald : American Astronomical Societyg 142:5, s. 156-q 142:5<156-x 0004-6256x 1538-3881 |
856 | 4 | u https://oaktrust.library.tamu.edu/bitstream/1969.1/179186/1/document-1.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-70909 |
856 | 4 8 | u https://doi.org/10.1088/0004-6256/142/5/156 |
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