Zobrazeno 1 - 10
of 436
pro vyhledávání: '"Jarvis, Matt J"'
Autor:
Debski, Maya H., Zeimann, Gregory R., Hill, Gary J., Schneider, Donald P., Morabito, Leah, Dalton, Gavin, Jarvis, Matt J., Cooper, Erin Mentuch, Ciardullo, Robin, Gawiser, Eric, Jurlin, Nika
We combine the power of blind integral field spectroscopy from the Hobby-Eberly Telescope (HET) Dark Energy Experiment (HETDEX) with sources detected by the Low Frequency Array (LOFAR) to construct the HETDEX-LOFAR Spectroscopic Redshift Catalog. Sta
Externí odkaz:
http://arxiv.org/abs/2411.08974
Autor:
Pan, Hengxing, Jarvis, Matt J., Zhu, Ming, Ma, Yin-Zhe, Santos, Mario G., Ponomareva, Anastasia A., Heywood, Ian, Jing, Yingjie, Xu, Chen, Liu, Ziming, Chandola, Yogesh, Jing, Yipeng
We present a deep HI survey at L-band conducted with the Five-hundred-meter Aperture Spherical radio Telescope (FAST) over the COSMOS field. This survey is strategically designed to overlap with the MIGHTEE COSMOS field, aiming to combine the sensiti
Externí odkaz:
http://arxiv.org/abs/2408.16597
Autor:
Wang, Lingyu, La Marca, Antonio, Gao, Fangyou, Pearson, William J., Margalef-Bentabol, Berta, Béthermin, Matthieu, Bing, Longji, Donnellan, James, Hurley, Peter D., Oliver, Seb J., Hale, Catherine L., Jarvis, Matt J., Marchetti, Lucia, Vaccari, Mattia, Whittam, Imogen H.
Publikováno v:
A&A 688, A20 (2024)
Single-dish far-infrared (far-IR) and sub-millimetre (sub-mm) point source catalogues and their connections with catalogues at other wavelengths are of paramount importance. However, due to the large mismatch in spatial resolution, cross-matching gal
Externí odkaz:
http://arxiv.org/abs/2405.18290
Autor:
Cook, Robin H. W., Davies, Luke J. M., Rhee, Jonghwan, Hale, Catherine L., Bellstedt, Sabine, Thorne, Jessica E., Delvecchio, Ivan, Collier, Jordan D., Dodson, Richard, Driver, Simon P., Holwerda, Benne W., Jarvis, Matt J., Knowles, Kenda, Lagos, Claudia, Maddox, Natasha, Meyer, Martin, Robotham, Aaron S. G., Roychowdhury, Sambit, Rozgonyi, Kristof, Seymour, Nicholas, Siudek, Malgorzata, Whiting, Matthew, Whittam, Imogen
The tight relationship between infrared luminosity (L$_\mathrm{TIR}$) and 1.4 GHz radio continuum luminosity (L$_\mathrm{1.4GHz}$) has proven useful for understanding star formation free from dust obscuration. Infrared emission in star-forming galaxi
Externí odkaz:
http://arxiv.org/abs/2405.00337
Autor:
Sinigaglia, Francesco, Rodighiero, Giulia, Elson, Ed, Bianchetti, Alessandro, Vaccari, Mattia, Maddox, Natasha, Ponomareva, Anastasia A., Frank, Bradley S., Jarvis, Matt J., Catinella, Barbara, Cortese, Luca, Roychowdhury, Sambit, Baes, Maarten, Collier, Jordan D., Ilbert, Olivier, Khostovan, Ali A., Kurapati, Sushma, Pan, Hengxing, Prandoni, Isabella, Rajohnson, Sambatriniaina H. A., Salvato, Mara, Sekhar, Srikrishna, Sharma, Gauri
We present the first measurement of HI mass of star-forming galaxies in different large scale structure environments from a blind survey at $z\sim 0.37$. In particular, we carry out a spectral line stacking analysis considering $2875$ spectra of colo
Externí odkaz:
http://arxiv.org/abs/2403.00734
Autor:
Deane, Roger P., Radcliffe, Jack F., Njeri, Ann, Akoto-Danso, Alexander, Bernardi, Gianni, Smirnov, Oleg M., Beswick, Rob, Garrett, Michael A., Jarvis, Matt J., Whittam, Imogen H., Bourke, Stephen, Paragi, Zsolt
The past decade has seen significant advances in wide-field cm-wave very long baseline interferometry (VLBI), which is timely given the wide-area, synoptic survey-driven strategy of major facilities across the electromagnetic spectrum. While wide-fie
Externí odkaz:
http://arxiv.org/abs/2401.12298
Autor:
Jarvis, Matt J., Heywood, Ian, Jewell, Sophie M., Deane, Roger P., Klöckner, H. -R., Ponomareva, Anastasia A., Maddox, Natasha, Baker, Andrew J., Bianchetti, Alessandro, Hess, Kelley M., Roberts, Hayley, Rodighiero, Giulia, Ruffa, Ilaria, Sinigaglia, Francesco, Varadaraj, R. G., Whittam, I. H., Adams, Elizabeth A. K., Baes, Maarten, Murphy, Eric J., Pan, Hengxing, Vaccari, Mattia
We present the discovery of the most distant OH megamaser to be observed in the main lines, using data from the MeerKAT International Giga-Hertz Tiered Extragalactic Exploration (MIGHTEE) survey. At a newly measured redshift of $z = 0.7092$, the syst
Externí odkaz:
http://arxiv.org/abs/2312.04345
Autor:
Martin-Alvarez, Sergio, Lopez-Rodriguez, Enrique, Dacunha, Tara, Clark, Susan E., Borlaff, Alejandro S., Beck, Rainer, Montero, Francisco Rodríguez, Jung, S. Lyla, Devriendt, Julien, Slyz, Adrianne, Roman-Duval, Julia, Ntormousi, Evangelia, Tahani, Mehrnoosh, Subramanian, Kandaswamy, Dale, Daniel A., Marcum, Pamela M., Tassis, Konstantinos, del Moral-Castro, Ignacio, Tram, Le Ngoc, Jarvis, Matt J.
The structure of magnetic fields in galaxies remains poorly constrained, despite the importance of magnetism in the evolution of galaxies. Radio synchrotron and far-infrared (FIR) polarization and polarimetric observations are the best methods to mea
Externí odkaz:
http://arxiv.org/abs/2311.06356
Autor:
Pinjarkar, Siddhant, Hardcastle, Martin J., Harwood, Jeremy J., Lal, Dharam V., Hatfield, Peter W., Jarvis, Matt J., Randriamanakoto, Zara, Whittam, Imogen H.
Jets of energetic particles, as seen in FR type-I and FR type-II sources, ejected from the center of Radio-Loud AGN affect the sources surrounding intracluster medium/intergalactic medium. Placing constraints on the age of such sources is important i
Externí odkaz:
http://arxiv.org/abs/2305.07561
Autor:
Ponomareva, Anastasia A., Jarvis, Matt J., Pan, Hengxing, Maddox, Natasha, Jones, Michael G., Frank, Bradley S., Rajohnson, Sambatriniaina H. A., Mulaudzi, Wanga, Meyer, Martin, Adams, Elizabeth A. K., Baes, Maarten, Hess, Kelley M., Kurapati, Sushma, Prandoni, Isabella, Sinigaglia, Francesco, Spekkens, Kristine, Tudorache, Madalina, Heywood, Ian, Collier, Jordan D., Sekhar, Srikrishna
We present the first measurement of the HI mass function (HIMF) using data from MeerKAT, based on 276 direct detections from the MIGHTEE Survey Early Science data covering a period of approximately a billion years ($0 \leq z \leq 0.084 $). This is th
Externí odkaz:
http://arxiv.org/abs/2304.13051