Zobrazeno 1 - 10
of 25
pro vyhledávání: '"D. L. Shupe"'
Autor:
A. Gal-Yam, R. Bruch, S. Schulze, Y. Yang, D. A. Perley, I. Irani, J. Sollerman, E. C. Kool, M. T. Soumagnac, O. Yaron, N. L. Strotjohann, E. Zimmerman, C. Barbarino, S. R. Kulkarni, M. M. Kasliwal, K. De, Y. Yao, C. Fremling, L. Yan, E. O. Ofek, C. Fransson, A. V. Filippenko, W. Zheng, T. G. Brink, C. M. Copperwheat, R. J. Foley, J. Brown, M. Siebert, G. Leloudas, A. L. Cabrera-Lavers, D. Garcia-Alvarez, A. Marante-Barreto, S. Frederick, T. Hung, J. C. Wheeler, J. Vinkó, B. P. Thomas, M. J. Graham, D. A. Duev, A. J. Drake, R. Dekany, E. C. Bellm, B. Rusholme, D. L. Shupe, I. Andreoni, Y. Sharma, R. Riddle, J. van Roestel, N. Knezevic
Publikováno v:
Gal-Yam, A, Bruch, R, Schulze, S, Yang, Y, Perley, D A, Irani, I, Sollerman, J, Kool, E C, Soumagnac, M T, Yaron, O, Strotjohann, N L, Zimmerman, E, Barbarino, C, Kulkarni, S R, Kasliwal, M M, De, K, Yao, Y, Fremling, C, Yan, L, Ofek, E O, Fransson, C, Filippenko, A V, Zheng, W, Brink, T G, Copperwheat, C M, Foley, R J, Brown, J, Siebert, M, Leloudas, G, Cabrera-Lavers, A L, Garcia-Alvarez, D, Marante-Barreto, A, Frederick, S, Hung, T, Wheeler, J C, Vinkó, J, Thomas, B P, Graham, M J, Duev, D A, Drake, A J, Dekany, R, Bellm, E C, Rusholme, B, Shupe, D L, Andreoni, I, Sharma, Y, Riddle, R, van Roestel, J & Knezevic, N 2022, ' A WC/WO star exploding within an expanding carbon–oxygen–neon nebula ', Nature, vol. 601, no. 7892, pp. 201-204 . https://doi.org/10.1038/s41586-021-04155-1
The final explosive fate of massive stars, and the nature of the compact remnants they leave behind (black holes and neutron stars), are major open questions in astrophysics. Many massive stars are stripped of their outer hydrogen envelopes as they e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea2f603c0b66036933e12b0d0c8e214b
https://orbit.dtu.dk/en/publications/9223735d-26fb-451d-a220-2392fd9e5b72
https://orbit.dtu.dk/en/publications/9223735d-26fb-451d-a220-2392fd9e5b72
Autor:
M Deckers, K Maguire, M R Magee, G Dimitriadis, M Smith, A Sainz de Murieta, A A Miller, A Goobar, J Nordin, M Rigault, E C Bellm, M Coughlin, R R Laher, D L Shupe, M Graham, M Kasliwal, R Walters
Publikováno v:
MNRAS
In the new era of time-domain surveys, Type Ia supernovae are being caught sooner after explosion, which has exposed significant variation in their early light curves. Two driving factors for early-time evolution are the distribution of 56Ni in the e
Autor:
B. O'Halloran, Mat Page, Michael Pohlen, P. Popesso, David J. Rosario, C. K. Xu, S. J. Lilly, Chris Pearson, Peter Capak, E. Le Floc'h, Matthew Joseph Griffin, E. Giovannoli, Duncan Farrah, D. Rigopoulou, Georgios E. Magdis, Jason Glenn, L. Riguccini, V. Arumugam, Ho Seong Hwang, Ismael Perez-Fournon, Evanthia Hatziminaoglou, Alberto Franceschini, S. Berta, Edo Ibar, Mattia Vaccari, Stijn Wuyts, Lucia Marchetti, Michael Rowan-Robinson, Dieter Lutz, David L. Clements, Lian-Tao Wang, Asantha Cooray, Andreas Papageorgiou, O. Ilbert, Seb Oliver, Benjamin Magnelli, Anthony J. Smith, Benjamin L. Schulz, D. L. Shupe, L. Conversi, Isaac Roseboom, A. Boselli, C. D. Dowell, Douglas Scott, A. Conley, Nick Seymour, Francesca Pozzi, Mara Salvato, Rob Ivison, H. Patel, Herve Aussel, Alain Omont, H. T. Nguyen, Ivan Valtchanov, M. Symeonidis, Michael Zemcov, Raanan Nordon, V. Buat, J. Kartaltepe, James J. Bock
Publikováno v:
Symeonidis, M, Vaccari, M, Berta, S, Page, M J, Lutz, D, Arumugam, V, Aussel, H, Bock, J, Boselli, A, Buat, V, Capak, P L, Clements, D L, Conley, A, Conversi, L, Cooray, A, Dowell, C D, Farrah, D, Franceschini, A, Giovannoli, E, Glenn, J, Griffin, M, Hatziminaoglou, E, Hwang, H-S, Ibar, E, Ilbert, O, Ivison, R J, Floc'h, E L, Lilly, S, Kartaltepe, J S, Magnelli, B, Magdis, G, Marchetti, L, Nguyen, H T, Nordon, R, O'Halloran, B, Oliver, S J, Omont, A, Papageorgiou, A, Patel, H, Pearson, C P, Pérez-Fournon, I, Pohlen, M, Popesso, P, Pozzi, F, Rigopoulou, D, Riguccini, L, Rosario, D, Roseboom, I G, Rowan-Robinson, M, Salvato, M, Schulz, B, Scott, D, Seymour, N, Shupe, D L, Smith, A J, Valtchanov, I, Wang, L, Xu, C K, Zemcov, M & Wuyts, S 2013, ' The Herschel census of infrared SEDs through cosmic time ', Monthly Notices of the Royal Astronomical Society, vol. 431, no. 3, pp. 2317-2340 . https://doi.org/10.1093/mnras/stt330
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 431 (3), pp.2317--2340. ⟨10.1093/mnras/stt330⟩
Monthly Notices of the Royal Astronomical Society, 2013, 431 (3), pp.2317--2340. ⟨10.1093/mnras/stt330⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 431 (3), pp.2317--2340. ⟨10.1093/mnras/stt330⟩
Monthly Notices of the Royal Astronomical Society, 2013, 431 (3), pp.2317--2340. ⟨10.1093/mnras/stt330⟩
Using Herschel data from the deepest SPIRE and PACS surveys (HerMES and PEP) in COSMOS and GOODS (N+S), we examine the dust properties of IR-luminous (L_IR>10^10 L_sun) galaxies at 0.145K) SEDs and cold (T
Comment: 27 pages, 23 figures, 2 tables
Comment: 27 pages, 23 figures, 2 tables
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::87bed8ee548a81019332eaa201cb0e4b
https://ora.ox.ac.uk/objects/uuid:19130c46-dd55-4750-b812-779b4894e131
https://ora.ox.ac.uk/objects/uuid:19130c46-dd55-4750-b812-779b4894e131
Autor:
V. Arumugam, Ismael Perez-Fournon, M. Bethermin, Andreas Papageorgiou, Alberto Franceschini, Mattia Vaccari, A. M. Pérez García, Lucia Pozzetti, G. Wright, B. O'Halloran, P. Chanial, Giulia Rodighiero, Pierluigi Monaco, P. Popesso, E. Zucca, Michael Pohlen, Benjamin Magnelli, K. G. Isaak, Lucia Marchetti, Eckhard Sturm, Bruno Maffei, Michael Rowan-Robinson, Matthew Joseph Griffin, Michael Zemcov, Marco Scodeggio, C. K. Xu, Lian-Tao Wang, Antonio Cava, O. Le Fevre, K. E. Tugwell, M. Magliocchetti, Dimitra Rigopoulou, Albrecht Poglitsch, S. C. Madden, Bruno Altieri, Raanan Nordon, M. Carollo, Rob Ivison, Alexandre Amblard, N. Castro-Rodríguez, R. Genzel, James J. Bock, Vincenzo Mainieri, Linda J. Tacconi, Alvio Renzini, Anthony J. Smith, Francesca Pozzi, David J. Rosario, Chris Pearson, Mark Sargent, A. Boselli, Denis Burgarella, G. Mainetti, Edo Ibar, C. D. Dowell, Ivan Delvecchio, H. Aussel, A. Conley, Benjamin L. Schulz, Simon J. Lilly, Jamie Stevens, H. T. Nguyen, V. Buat, Guilaine Lagache, D. Elbaz, Nick Seymour, Asantha Cooray, Alessandro Cimatti, Douglas Scott, M. J. Page, Louis Levenson, M. Sánchez-Portal, Evanthia Hatziminaoglou, David L. Clements, Nanyao Y. Lu, M. Symeonidis, S. Berta, L. Riguccini, L. Vigroux, Ivan Valtchanov, Emanuele Daddi, Roberto Maiolino, Eli Dwek, J. Cepa, Stephen Anthony Eales, H. Dominguez-Sanchez, G. Zamorani, Dieter Lutz, P. Panuzzo, S. Bardelli, D. L. Shupe, Carlotta Gruppioni, E. Le Floc'h, Isaac Roseboom, Seb Oliver, Ángel Bongiovanni, P. Andreani, Alvaro Iribarrem, Thierry Contini, N. M. Foerster Schreiber, Jason Glenn, Markos Trichas, O. Ilbert
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
We exploit the deep and extended far infrared data sets (at 70, 100 and 160 um) of the Herschel GTO PACS Evolutionary Probe (PEP) Survey, in combination with the HERschel Multi tiered Extragalactic Survey (HerMES) data at 250, 350 and 500 um, to deri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c5d7cc70c7ac7880301e3887ab85057c
Autor:
Eli Dwek, Bruno Maffei, Giulia Rodighiero, Duncan Farrah, Mat Page, Julie Wardlow, Hien Nguyen, Michael Zemcov, A. Amblard, David L. Clements, Matthew Joseph Griffin, Antonio Cava, C. K. Xu, Stephen Anthony Eales, Edo Ibar, N. Lu, Rob Ivison, Pasquale Panuzzo, David Elbaz, Pierre Chanial, Ivan Valtchanov, G. Marsden, Kate Gudrun Isaak, J. I. Rawlings, D. Rizzo, S. C. Madden, L. R. Levenson, Anthony J. Smith, Thomas R. Greve, G. Mainetti, Lucia Marchetti, Michael Rowan-Robinson, Gillian S. Wright, Asantha Cooray, Robbie Richard Auld, Edward L. Chapin, N. Castro-Rodríguez, Glenn Morrison, Drew Brisbin, Nick Seymour, Gwenifer Raymond, Andrew Blain, James J. Bock, Markos Trichas, A. Conley, Joaquin Vieira, Mark Halpern, Marco P. Viero, Bernhard Schulz, Guilaine Lagache, V. Arumugam, Denis Burgarella, J. S. Dunlop, D. L. Shupe, L. Conversi, Herve Aussel, Isaac Roseboom, Lian-Tao Wang, Alain Omont, Jamie Stevens, Evanthia Hatziminaoglou, C. P. Pearson, A. M. J. Mortier, Andreas Papageorgiou, Douglas Scott, Scott Chapman, B. O'Halloran, Jason Glenn, C. D. Dowell, M. Symeonidis, Ismael Perez-Fournon, Alberto Franceschini, Dimitra Rigopoulou, Mattia Vaccari, Alessandro Boselli, Matthieu Béthermin, K. E. Tugwell, Michael Pohlen, V. Buat, S. J. Oliver, L. Vigroux
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 419:2758-2773
We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500 {\mu}m by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm-sources with
Autor:
Bruno Maffei, Guilaine Lagache, Lucia Marchetti, Andreas Papageorgiou, Michael Rowan-Robinson, Stephen Anthony Eales, L. Vigroux, G. Marsden, Ivan Valtchanov, Pierre Chanial, Charles D. Dowell, Michael Pohlen, Matthew Joseph Griffin, Bruno Altieri, Mat Page, P. Panuzzo, Lian-Tao Wang, Asantha Cooray, G. Mainetti, Michael Zemcov, Nick Seymour, Gillian S. Wright, C. P. Pearson, D. Rizzo, C. K. Xu, A. Amblard, Ismael Perez-Fournon, David Elbaz, Suzanne C. Madden, Alberto Franceschini, Dimitra Rigopoulou, Joaquin Vieira, S. J. Oliver, Mattia Vaccari, Alain Omont, V. Buat, Alessandro Boselli, Jason Glenn, Matthieu Béthermin, A. Conley, Kate Gudrun Isaak, Walter Kieran Gear, K. E. Tugwell, Hien Nguyen, David L. Clements, A. J. Smith, M. Sanchez Portal, T. Babbedge, Timothy P. Ellsworth-Bowers, V. Arumugam, B. O'Halloran, D. L. Shupe, Eli Dwek, Glenn Laurent, L. Conversi, Isaac Roseboom, Robyn L. Ward, Rob Ivison, Antonio Cava, Markos Trichas, Douglas Scott, Herve Aussel, N. Castro-Rodríguez, Evanthia Hatziminaoglou, Andrew Blain, Nanyao Y. Lu, James J. Bock, M. Symeonidis, Mark Halpern, M. Fox, Edo Ibar, L. R. Levenson, Benjamin L. Schulz, Jamie Stevens
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:109-121
Dusty, star forming galaxies contribute to a bright, currently unresolved cosmic far-infrared background. Deep Herschel-SPIRE images designed to detect and characterize the galaxies that comprise this background are highly confused, such that the bul
Autor:
Marc Sauvage, Woong-Seob Jeong, V. Buat, Koryo Okumura, E. Le Floc'h, Amélie Saintonge, Edo Ibar, G. Mainetti, Ángel Bongiovanni, Herve Aussel, Eli Dwek, Antonio Cava, D. L. Shupe, Lian-Tao Wang, H. Dominguez, M. Sanchez Portal, Carlotta Gruppioni, L. Conversi, Isaac Roseboom, H. M. Lee, Guilaine Lagache, Robbie Richard Auld, Evanthia Hatziminaoglou, Lucia Marchetti, Michael Rowan-Robinson, Paola Popesso, Nick Seymour, L. R. Levenson, Alessandro Boselli, Stephen Anthony Eales, Michael Pohlen, A. J. Smith, James Dunlop, Andrea Cimatti, Benjamin L. Schulz, K. E. Tugwell, Matthew Joseph Griffin, M. Symeonidis, P. Panuzzo, Giulia Rodighiero, J. Cepa, Jamie Stevens, C. K. Xu, Jonathan Rawlings, Suzanne C. Madden, Myung Gyoon Lee, Kate Gudrun Isaak, S. J. Oliver, Ranga-Ram Chary, Ivan Valtchanov, Emanuele Daddi, Roberto Maiolino, Mark Dickinson, Georgios E. Magdis, Joaquin Vieira, Albrecht Poglitsch, Edward L. Chapin, Jason Glenn, Helmut Dannerbauer, Andreas Papageorgiou, Markos Trichas, A. M. J. Mortier, Asantha Cooray, Walter Kieran Gear, T. Babbedge, N. M. Förster Schreiber, Douglas Scott, Paola Santini, B. O'Halloran, Lijing Shao, N. Lu, Reinhard Genzel, E. Sturm, Benjamin Magnelli, Denis Burgarella, D. Le Borgne, Alain Omont, Ho Seong Hwang, V. Arumugam, Francesca Pozzi, N. Castro-Rodríguez, A. Conley, Jounghun Lee, D. Rizzo, S. Berta, Ismael Perez-Fournon, Andrew Blain, James J. Bock, Alberto Franceschini, Dimitra Rigopoulou, Mattia Vaccari, Bruno Altieri, Mat Page, A. M. Pérez García, M. Fox, Charles D. Dowell, Mark Halpern, Dieter Lutz, Robyn L. Ward, L. Riguccini, Michael Zemcov, Raanan Nordon, Paola Andreani, Bruno Maffei, Linda J. Tacconi, Gillian S. Wright, David Elbaz, Alexandre Amblard, Rob Ivison, C. P. Pearson, Duncan Farrah, Hien Nguyen, David L. Clements, Pierre Chanial, L. Vigroux
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:75-82
We study the dust properties of galaxies in the redshift range 0.1 0.5 with L_IR>5x10^{10} L_\odot, appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities; and the dispersion in T_dust for high-z galaxies incr
Autor:
Herve Aussel, Simon Dye, M. Sanchez Portal, Evanthia Hatziminaoglou, Martin Kunz, V. Buat, Edo Ibar, M. Symeonidis, Bruno Maffei, Markos Trichas, Andreas Papageorgiou, J.-S. Huang, L. R. Levenson, Lucia Marchetti, Michael Rowan-Robinson, Jason Glenn, Benjamin L. Schulz, A. J. Smith, Ismael Perez-Fournon, Drew Brisbin, Jamie Stevens, Antonio Cava, Alberto Franceschini, Walter Kieran Gear, Matthew Joseph Griffin, T. Babbedge, Dimitra Rigopoulou, Pasquale Panuzzo, Mattia Vaccari, V. Arumugam, B. O'Halloran, D. L. Shupe, N. Lu, Suzanne C. Madden, Edward L. Chapin, L. Conversi, Isaac Roseboom, C. K. Xu, Michael Zemcov, Lian-Tao Wang, A. Conley, Rob Ivison, Seb Oliver, N. Castro-Rodríguez, D. Rizzo, Duncan Farrah, Denis Burgarella, David Elbaz, Alexandre Amblard, G. Wright, C. P. Pearson, Hien Nguyen, Mark Halpern, David L. Clements, Eli Dwek, Kate Gudrun Isaak, H. Patel, Robbie Richard Auld, Michael Pohlen, Robyn L. Ward, E. A. González Solares, Nick Seymour, Andrew Blain, James J. Bock, Gwenifer Raymond, Guilaine Lagache, G. Marsden, L. Vigroux, A. M. J. Mortier, Douglas Scott, Jonathan Rawlings, M. Fox, Bruno Altieri, Mat Page, Joaquin Vieira, C. D. Dowell, Pierre Chanial, Stephen Anthony Eales, Ivan Valtchanov, Asantha Cooray, Alessandro Boselli, Matthieu Béthermin, G. Mainetti, K. E. Tugwell, Alain Omont, Martin Harwit
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:48-65
We present the cross-identification and source photometry techniques used to process Herschel SPIRE imaging taken as part of the Herschel Multi-Tiered Extragalactic Survey (HerMES). Cross-identifications are performed in map-space so as to minimise s
Autor:
D. Rigopoulou, G. Magdis, R. J. Ivison, A. Amblard, V. Arumugam, H. Aussel, A. Blain, J. Bock, A. Boselli, V. Buat, D. Burgarella, N. Castro-Rodríguez, A. Cava, P. Chanial, D. L. Clements, A. Conley, L. Conversi, A. Cooray, C. D. Dowell, E. Dwek, S. Eales, D. Elbaz, D. Farrah, A. Franceschini, J. Glenn, M. Griffin, M. Halpern, E. Hatziminaoglou, J.-S. Huang, E. Ibar, K. Isaak, G. Lagache, L. Levenson, N. Lu, S. Madden, B. Maffei, G. Mainetti, L. Marchetti, H. T. Nguyen, B. O’Halloran, S. J. Oliver, A. Omont, M. J. Page, P. Panuzzo, A. Papageorgiou, C. P. Pearson, I. Pérez-Fournon, M. Pohlen, D. Rizzo, I. G. Roseboom, M. Rowan-Robinson, B. Schulz, Douglas Scott, N. Seymour, D. L. Shupe, A. J. Smith, J. A. Stevens, M. Symeonidis, M. Trichas, K. E. Tugwell, M. Vaccari, I. Valtchanov, L. Vigroux, L. Wang, G. Wright, C. K. Xu, M. Zemcov
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 409:L7-L12
We present first results of a study of the submillimetre (rest frame far-infrared) properties of z~3 Lyman Break Galaxies (LBGs) and their lower-redshift counterparts BX/BM galaxies, based on Herschel-SPIRE observations of the Northern field of the G
Autor:
M. Rowan-Robinson, I. G. Roseboom, M. Vaccari, A. Amblard, V. Arumugam, R. Auld, H. Aussel, T. Babbedge, A. Blain, J. Bock, A. Boselli, D. Brisbin, V. Buat, D. Burgarella, N. Castro-Rodriguez, A. Cava, P. Chanial, D. L. Clements, A. Conley, L. Conversi, A. Cooray, C. D. Dowell, E. Dwek, S. Dye, S. Eales, D. Elbaz, D. Farrah, M. Fox, A. Franceschini, W. Gear, J. Glenn, E. A. González Solares, M. Griffin, M. Halpern, E. Hatziminaoglou, J. Huang, E. Ibar, K. Isaak, R. J. Ivison, G. Lagache, L. Levenson, N. Lu, S. Madden, B. Maffei, G. Mainetti, L. Marchetti, A. M. J. Mortier, H. T. Nguyen, B. O'Halloran, S. J. Oliver, A. Omont, M. J. Page, P. Panuzzo, A. Papageorgiou, H. Patel, C. P. Pearson, I. Perez Fournon, M. Pohlen, J. I. Rawlings, G. Raymond, D. Rigopoulou, D. Rizzo, B. Schulz, Douglas Scott, N. Seymour, D. L. Shupe, A. J. Smith, J. A. Stevens, M. Symeonidis, M. Trichas, K. E. Tugwell, I. Valtchanov, L. Vigroux, L. Wang, R. Ward, G. Wright, C. K. Xu, M. Zemcov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:2-11
We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5-sigma at 250, 350 and 500 mu in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and for AGN dust