Results 21 to 30 of about 5,123 (230)
Review: Far-infrared instrumentation and technological development for the next decade [PDF]
, 2019 Far-infrared astronomy has advanced rapidly since its inception in the late 1950s, driven by a maturing technology base and an expanding community of researchers.Staguhn, Johannes, Smith, John-David, Ardila, D, Bradford, Charles M., Lis, DC, Enrique, LR, Rinehart, Stephen A., Carey, S, Sanders, D, Leisawitz, D, Farrah, Duncan, Smith, KE, Kamenetzky, Julia R., Murphy, Eric J., Kamenetzky, J, Kamenetzky, Julia, Rhodes, Alan, Mills, Elisabeth, Lacy, Mark D., Lis, Dariusz C., Sankrit, Ravi, Mills, E, Bartlett, J, Murphy, EJ, Lacy, M, Nikola, Thomas, Stierwalt, S, Carey, Sean, MacGregor, Meredith, Savini, Giorgio, John-David, S, Dipirro, M, Locke, L, Sanders, David, Rangwala, N, Sankrit, R, Rhodes, A, Bartlett, James, DiPirro, Michael J., Glenn, J, Ferkinhoff, Carl, Locke, Lisa, Staguhn, J, Moseley, SH, Savini, G, Zemcov, M, Fischer, WJ, Lopez-Rodriguez, Enrique, Carey, Sean J., Ferkinhoff, C, Goldsmith, Paul, Farrah, D, Zmuidzinas, J, Leisawitz, David, Nikola, T, Rigopoulou, Dimitra, Stierwalt, Sabrina, Zemcov, Michael, Goldsmith, Paul F., Zmuidzinas, Jonas, MacGregor, M, Dipirro, Michael, Leisawitz, David T., Richter, Matthew J., Goldsmith, P, Ardila, David, Staguhn, Johannes G., Fischer, William J., Kartaltepe, J, Moseley, Samuel H., Rigopoulou, D, Rangwala, Naseem, Bradford, CM, Lacy, Mark, Rinehart, SA, Richter, Matt, Glenn, Jason, Locke, Lisa S., Sanders, David B., Kartaltepe, Jeyhan, Smith, Kimberly Ennico, Richter, M +81 morecore +3 more sourcesCross-slot metal-mesh bandpass filters for far-infrared astronomy
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, 2022 The far-infrared (IR) region is rich with information needed to characterize interstellar dust and to investigate the cold outer planets of the solar system and their icy moons. The proposed sub-orbital observatory the Balloon Experiment for Galactic INfrared Science (BEGINS) will utilize cryogenic instruments to map spectral energy distributions (SEDs)Perido, Joanna, Denis, Kevin, Glenn, Jason, Cothard, Nicholas F., Quijada, Manuel, Patel, Jessica, Wollack, Edward, Hewagama, Tilak, Aslam, Shahid, Day, Peter K. +9 moreopenaire +2 more sourcesHow Accurately Can Obscured Galaxy Luminosities Be Measured Using Spectral Energy Distribution Fitting of Near- through Far-infrared Observations?
The Astrophysical JournalInfrared-luminous galaxies are important sites of stellar and black hole mass assembly at most redshifts. Their luminosities are often estimated by fitting spectral energy distribution (SED) models to near- to far-infrared data, but the dependence of ...Duncan Farrah, Kiana Ejercito, Andreas Efstathiou, David Leisawitz, Athena Engholm, Irene Shivaei, Matteo Bonato, David L. Clements, Sara Petty, Lura. K. Pitchford, Charalambia Varnava, Jose Afonso, Carlotta Gruppioni, Evanthia Hatziminaoglou, Andrew Hoffman, Mark Lacy, Brenda C. Matthews, Conor Nixon, Chris Pearson, Berke Vow Ricketti, Dimitra Rigopoulou, Loren Robinson, Locke D. Spencer, Lingyu Wang, David B. Sanders, Gerard van Belle +25 moredoaj +1 more sourceTailoring Phonon‐Driven Responses in α‐MoO3 through Isotopic Enrichment
Advanced Materials, EarlyView.ABSTRACT
The implementation of polaritonic materials into nanoscale devices requires selective tuning of parameters to realize desired spectral or thermal responses. One robust material, α‐MoO3, an orthorhombic crystal boasting three distinct phonon dispersions, provides three polaritonic dispersions of hyperbolic phonon polaritons (HPhPs) across the ...Thiago S. Arnaud, Ryan W. Spangler, Johnathan D. Georgaras, Jonah B. Haber, Daniel Hirt, Maximilian Obst, Gonzalo Álvarez‐Pérez, Mackey Long III, Felix G. Kaps, Jakob Wetzel, Courtney Ragle, John E. Buchner, Youngji Kim, Aditha S. Senarath, Richarda Niemann, Mingze He, Giulia Carini, Unai Arregui‐Leon, Akash C. Behera, Ramachandra Bangari, Nihar Sahoo, Niels C. Brumby, J. Michael Klopf, Martin Wolf, Lukas M. Eng, Susanne C. Kehr, Thomas G. Folland, Alexander Paarmann, Patrick E. Hopkins, Felipe Jornada, Jon‐Paul Maria, Joshua D. Caldwell +31 morewiley +1 more sourceHerMES : SPIRE galaxy number counts at 250, 350, and 500 μm [PDF]
, 2010 Emission at far-infrared wavelengths makes up a significant fraction of the total light detected from galaxies over the age of Universe. Herschel provides an opportunity for studying galaxies at the peak wavelength of their emission.M Vaccari, Franceschini, A., Glenn J, Xu, C.K., R. Ward, Schulz B, S√°nchez Portal, M, Sánchez Portal, M, Maffei, B., B. Schulz, Babbedge, T., E. Valiante, Ibar, E., Seymour N, Pérez-Fournon, I, M Zemcov, Castro-Rodríguez, N, Fox, M., C D Dowell, M Pohlen, Vaccari M, Dwek, E., E Dwek, S. J. Oliver, S. Madden, Eales, S, D. Rizzo, Smith, AJ, Hatziminaoglou, E., Tugwell, K.E., D. L. Clements, Babbedge, T, N. Lu, M J Page, Clements, D L, S. Eales, Arumugam V, Wang, L., Smith AJ, P√©rez-Fournon, I, Dowell, CD, Nguyen, H T, Valiante E, Madden, S, B Altieri, M Sánchez Portal, M. Pohlen, M. Fox, M. Zemcov, N Seymour, Auld R, Cooray, A, A Papageorgiou, R Ward, Stevens, J. A., Shupe DL, M. Rowan-Robinson, Page, M. J., Panuzzo, P, Blain A, Lagache G, A. Franceschini, Mortier, AMJ, Griffin M, Smith, A J, O'Halloran, B, I. Valtchanov, Oliver SJ, Papageorgiou, A., J A Stevens, Franceschini A, Glenn, J, Altieri, B, Dwek E, G. Wright, Raymond, G, Dowell, C. D., Gear W, Franceschini, A, Rigopoulou D, Valiante, E, Halpern, M., Valiante, E., et al (16046813), Aussel, H., Levenson, L, D Elbaz, A J Smith, Page, M J, Mainetti G, Papageorgiou A, K Isaak, A Cava, Arumugam, V, Gear, W, S Eales, D Rigopoulou, D Rizzo, Griffin, M., J. Glenn, Castro-Rodríguez, N., C K Xu, Pohlen, M., Ivison, R.J., Roseboom, IG, Page, M.J., Nguyen, HT, Rizzo, D., Zemcov, M., Ivison RJ, A. Cava, Blain, A. W. (Andrew W.), Trichas, M., A M J Mortier, Fox M, Shupe, D L, Cooray, Asantha, Pearson CP, Vigroux L, Pohlen, M, E Valiante, L Vigroux, P Chanial, Conley, A., I Pérez-Fournon, Symeonidis, M., Eales S, Roseboom, I. G., Eales, S., Hatziminaoglou E, Clements, D. L., Auld, R, Rowan-Robinson M, Mitchell-Wynne K, A. Blain, B. O'Halloran, G Wright, Elbaz, D., K. Mitchell-Wynne, D. Rigopoulou, V Arumugam, Tugwell KE, Scott, D, A Cooray, M Symeonidis, Arumugam, V., Seymour, N, Omont A, Omont, A., Xu CK, Maffei, B, M. Trichas, Rawlings, J.I., Conversi, L., Perez-Fournon I, Oliver, S J, A. Omont, Altieri, B., Symeonidis, M, Eales, Stephen Anthony, M. Vaccari, Madden, S., Mitchell-Wynne, K, Rizzo, D, C. P. Pearson, Tugwell, KE, D. Elbaz, Cava, A, P. Panuzzo, Burgarella, D., G. Raymond, Dowell, C D, W Gear, E Hatziminaoglou, Vigroux, L., Castro-Rodriguez N, E Ibar, Smith, A. J., Nguyen, H.T., H. T. Nguyen, Gear, Walter Kieran, H Aussel, Buat V, Ivison, R. J., T Babbedge, Roseboom IG, Valtchanov, I., O'Halloran, B., D Burgarella, Pohlen M, A. Conley, Wright, G., Mainetti, G, Zemcov, M, J I Rawlings, Isaak K, Savage, R, Bock, J, Levenson, L., Ward R, Ivison, RJ, V Buat, Marchetti L, Xu, CK, V. Buat, H. Aussel, B. Altieri, R Savage, L. Conversi, Xu, C. K., Cooray A, Mainetti, G., I Roseboom (16061063), Rigopoulou, D, M. J. Page, Tugwell, K. E., J. A. Stevens, Xu, C K, K Mitchell-Wynne, Glenn, J., J. Bock, Pearson, C.P., Stevens, J A, Boselli, A, Omont, A, Savage, Richard S., M Fox, E. Ibar, E. Hatziminaoglou, R Auld, Pearson, C. P., A. Cooray, Wright G, Auld, R., Boselli, A., Castro-Rodr√≠guez, N, Amblard, A, Conversi, L, K. E. Tugwell, Nguyen HT, G. Lagache, Blain, A., Levenson L, Pearson, CP, Rawlings, J. I., Dowell, C.D., M Halpern, Panuzzo P, Schulz, B, L Wang (5323634), Rizzo D, Page, MJ, B. Maffei, Pearson, C P, G Raymond, Eales, Stephen, M Trichas, Zemcov M, Wang, L, Dwek, Eli, Cava, A., Clements, David L., I. G. Roseboom, J. D. Vieira, Bock, J., A Franceschini, Cava A, L Marchetti, Lagache, Guilaine, Rawlings, JI, R. Auld, L. Vigroux, Lagache, G., Seb Oliver (4460809), Rowan-Robinson, M, Chanial, P, Valtchanov, I, M Rowan-Robinson, Isaak, Kate Gudrun, Halpern M, Conley, A, A Omont, A. Papageorgiou, Savage R, K. Isaak, Valtchanov I, J D Vieira, J. I. Rawlings, Bock J, Boselli A, Scott, D., K E Tugwell, Wright, G, Mortier, A M J, N. Seymour, Aussel, H, Chanial, P., M. Halpern, Buat, V., Shupe, DL, Cooray, A., Vieira JD, Scott D, T. Babbedge, N Castro-Rodríguez, Symeonidis M, A. Amblard, Oliver, SJ, Raymond G, Sanchez Portal M, Clements, DL, R. Savage, A Boselli, Aussel H, L. Wang, Marchetti, L, M. Griffin, Maffei B, I. Pérez-Fournon, L Conversi, Ibar E, L Wang, Rawlings JI, Papageorgiou, A, A. M. J. Mortier, Trichas M, Elbaz D, S J Oliver, Rowan-Robinson, Michael, Schulz, B., Stevens JA, Omont, Alain, D. Scott, D. Burgarella, Portal, M. Sanchez, B O'halloran, Lu, N., A J Smith (7985102), Mortier AMJ, Raymond, Gwenifer, Roseboom, I.G., H T Nguyen, Chanial P, Conversi L, L. Levenson, A Blain, C. K. Xu, Oliver, S. J., Amblard, A., Griffin, M, Vieira, JD, J Glenn, Rawlings, J I, Buat, V, C P Pearson, Burgarella D, Ivison, R J, Wright, Gavin, A. J. Smith, Elbaz, D, Vieira, J D, I Valtchanov, Isaak, K, Valiante, Elisabetta, Stevens, JA, Trichas, M, Vaccari, M., C. D. Dowell, Vieira, J. D., D. L. Shupe, D Scott, Mitchell-Wynne, K., Tugwell, K E, Hatziminaoglou, E, Savage, R., Babbedge T, M. Symeonidis, Raymond, G., B Schulz, Gear, W., Shupe, D. L., Lu, N, Clements DL, G. Mainetti, Ward, R, Roseboom, I G, Trichas, Markos, P Panuzzo, J Bock, L. Marchetti, M. Sánchez Portal, Conley A, N. Castro-Rodríguez, Ibar, E, Fox, M, A Amblard, Wang L, Stevens, Jason, A. Boselli, Vaccari, M, Madden S, Isaak, K., Blain, A, E. Dwek, O’Halloran, B., A Conley, Sánchez Portal, M., Auld, Robbie Richard, Papageorgiou, Andreas, Vigroux, L, Scott, Douglas, Halpern, Mark, Lu N, D L Clements, Seymour, N., Dowell CD, R. J. Ivison, Pérez-Fournon, I., Rowan-Robinson, M., M Griffin, P. Chanial, Mortier, A. M. J., Lagache, G, V. Arumugam, Ward, R., I G Roseboom, Halpern, M, Griffin, Matthew Joseph, W. Gear, Panuzzo, P., Altieri B, Dwek, E, Burgarella, Denis, Amblard A, Marchetti, L., Nguyen, H. T., Rigopoulou, D., Pohlen, Michael, D L Shupe, Burgarella, D, Page MJ, O'Halloran B +441 morecore +1 more source
