Search Results - "COMPANY, M"

SDSS-IV DR17: final release of MaNGA PyMorph photometric and deep-learning morphological catalogues by Domínguez Sánchez, H, Margalef, B, Bernardi, M, Huertas-Company, M

“…ABSTRACT We present the MaNGA PyMorph photometric Value Added Catalogue (MPP-VAC-DR17) and the MaNGA Deep Learning Morphological VAC (MDLM-VAC-DR17) for the…”
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Improving galaxy morphologies for SDSS with Deep Learning by Domínguez Sánchez, H, Huertas-Company, M, Bernardi, M, Tuccillo, D, Fischer, J L

“…Abstract We present a morphological catalogue for ∼670 000 galaxies in the Sloan Digital Sky Survey in two flavours: T-type, related to the Hubble sequence,…”
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The massive end of the luminosity and stellar mass functions: dependence on the fit to the light profile by Bernardi, M., Meert, A., Sheth, R. K., Vikram, V., Huertas-Company, M., Mei, S., Shankar, F.

“…In addition to the large systematic differences arising from assumptions about the stellar mass-to-light ratio, the massive end of the stellar mass function is…”
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Deep learning for galaxy surface brightness profile fitting by Tuccillo, D, Huertas-Company, M, Decencière, E, Velasco-Forero, S, Domínguez Sánchez, H, Dimauro, P

“…Abstract Numerous ongoing and future large area surveys (e.g. Dark Energy Survey, EUCLID, Large Synoptic Survey Telescope, Wide Field Infrared Survey…”
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Deep Learning Identifies High-z Galaxies in a Central Blue Nugget Phase in a Characteristic Mass Range by Huertas-Company, M., Primack, J. R., Dekel, A., Koo, D. C., Lapiner, S., Ceverino, D., Simons, R. C., Snyder, G. F., Bernardi, M., Chen, Z., Domínguez-Sánchez, H., Lee, C. T., Margalef-Bentabol, B., Tuccillo, D.

“…We use machine learning to identify in color images of high-redshift galaxies an astrophysical phenomenon predicted by cosmological simulations. This…”
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Systematic effects on the size–luminosity relations of early- and late-type galaxies: dependence on model fitting and morphology by Bernardi, M., Meert, A., Vikram, V., Huertas-Company, M., Mei, S., Shankar, F., Sheth, R. K.

“…We quantify the systematics in the size–luminosity relation of galaxies in the Sloan Digital Sky Survey main sample (i.e. at z ∼ 0.1) which arise from fitting…”
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CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts by Yang, G., Caputi, K. I., Papovich, C., Arrabal Haro, P., Bagley, M. B., Behroozi, P., Bell, E. F., Bisigello, L., Buat, V., Burgarella, D., Cheng, Y., Cleri, N. J., Davé, R., Dickinson, M., Elbaz, D., Ferguson, H. C., Finkelstein, S. L., Grogin, N. A., Hathi, N. P., Hirschmann, M., Holwerda, B. W., Huertas-Company, M., Hutchison, T. A., Iani, E., Kartaltepe, J. S., Kirkpatrick, A., Kocevski, D. D., Koekemoer, A. M., Kokorev, V., Larson, R. L., Lucas, R. A., Pérez-González, P. G., Rinaldi, P., Shen, L., Trump, J. R., de la Vega, A., Yung, L. Y. A., Zavala, J. A.

“…Abstract Mid-infrared (mid-IR) observations are powerful in identifying heavily obscured active galactic nuclei (AGN) that have weak emission in other…”
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Effectiveness of mandibular advancement appliances in treating obstructive sleep apnea syndrome: A systematic review by Serra-Torres, Sara, Bellot-Arcís, Carlos, Montiel-Company, José M., Marco-Algarra, Jaime, Almerich-Silla, José M.

“…Objectives/Hypothesis Mandibular advancement devices are an alternative to continuous positive airway pressure for patients with mild or moderate obstructive…”
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The evolution of the mass-size relation for early-type galaxies from z ∼ 1 to the present: dependence on environment, mass range and detailed morphology by Huertas-Company, M., Mei, S., Shankar, F., Delaye, L., Raichoor, A., Covone, G., Finoguenov, A., Kneib, J. P., Le, Fèvre O., Povic, M.

“…We study the dependence of the galaxy size evolution on morphology, stellar mass and large-scale environment for a sample of 298 group and 384 field quiescent…”
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Structural and stellar-population properties versus bulge types in Sloan Digital Sky Survey central galaxies by Luo, Yifei, Faber, S M, Rodríguez-Puebla, Aldo, Woo, Joanna, Guo, Yicheng, Koo, David C, Primack, Joel R, Chen, Zhu, Yesuf, Hassen M, Lin, Lin, Barro, Guillermo, Fang, Jerome J, Pandya, Viraj, Huertas-Company, M, Mao, Shude

“…ABSTRACT This paper studies pseudo-bulges (P-bulges) and classical bulges (C-bulges) in Sloan Digital Sky Survey (SDSS) central galaxies using the new bulge…”
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The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation by Varma, S, Huertas-Company, M, Pillepich, A, Nelson, D, Rodriguez-Gomez, V, Dekel, A, Faber, S M, Iglesias-Navarro, P, Koo, D C, Primack, J

“…ABSTRACT We study how mock-observed stellar morphological and structural properties of massive galaxies are built up between $z$ = 0.5 and $z$ = 3 in the TNG50…”
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The massive end of the luminosity and stellar mass functions and clustering from CMASS to SDSS: evidence for and against passive evolution by Bernardi, M., Meert, A., Sheth, R. K., Huertas-Company, M., Maraston, C., Shankar, F., Vikram, V.

“…We describe the luminosity function, based on Sérsic fits to the light profiles, of CMASS galaxies at z ∼ 0.55. Compared to previous estimates, our…”
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Ask the machine: systematic detection of wind-type outflows in low-mass X-ray binaries by Mata Sánchez, D, Muñoz-Darias, T, Casares, J, Huertas-Company, M, Panizo-Espinar, G

“…ABSTRACT The systematic discovery of outflows in the optical spectra of low-mass X-ray binaries opened a new avenue for the study of the outburst evolution in…”
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Mass assembly and morphological transformations since z ∼ 3 from CANDELS by Huertas-Company, M., Bernardi, M., Pérez-González, P. G., Ashby, M. L. N., Barro, G., Conselice, C., Daddi, E., Dekel, A., Dimauro, P., Faber, S. M., Grogin, N. A., Kartaltepe, J. S., Kocevski, D. D., Koekemoer, A. M., Koo, D. C., Mei, S., Shankar, F.

“…We quantify the evolution of the stellar mass functions (SMFs) of star-forming and quiescent galaxies as a function of morphology from z ∼ 3 to the present…”
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THE MORPHOLOGIES OF MASSIVE GALAXIES FROM z ∼ 3-WITNESSING THE TWO CHANNELS OF BULGE GROWTH by Huertas-Company, M., Pérez-González, P. G., Mei, S., Shankar, F., Bernardi, M., Daddi, E., Barro, G., Cabrera-Vives, G., Cattaneo, A., Dimauro, P., Gravet, R.

“…ABSTRACT We quantify the morphological evolution of massive galaxies ( ) from in the 5 CANDELS fields. The progenitors are selected using abundance matching…”
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The size function of massive satellites from the R e– R h and M star– M h relations: constraining the role of environment by Zanisi, L, Shankar, F, Bernardi, M, Mei, S, Huertas-Company, M

“…ABSTRACT In previous work, we showed that a semi-empirical model in which galaxies in host dark matter haloes are assigned stellar masses via a stellar…”
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Identification of tidal features in deep optical galaxy images with convolutional neural networks by Sánchez, H Domínguez, Martin, G, Damjanov, I, Buitrago, F, Huertas-Company, M, Bottrell, C, Bernardi, M, Knapen, J H, Vega-Ferrero, J, Hausen, R, Kado-Fong, E, Población-Criado, D, Souchereau, H, Leste, O K, Robertson, B, Sahelices, B, Johnston, K V

“…ABSTRACT Interactions between galaxies leave distinguishable imprints in the form of tidal features, which hold important clues about their mass assembly…”
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NO EVIDENCE FOR A DEPENDENCE OF THE MASS-SIZE RELATION OF EARLY-TYPE GALAXIES ON ENVIRONMENT IN THE LOCAL UNIVERSE by Huertas-Company, M, Shankar, F, Mei, S, Bernardi, M, Aguerri, J A L, Meert, A, Vikram, V

“…The early-type galaxy (ETG) mass-size relation has largely been studied to understand how these galaxies assembled their mass. One key observational result of…”
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The accelerated build-up of the red sequence in high-redshift galaxy clusters by Cerulo, P., Couch, W. J., Lidman, C., Demarco, R., Huertas-Company, M., Mei, S., Sánchez-Janssen, R., Barrientos, L. F., Muñoz, R. P.

“…We analyse the evolution of the red sequence in a sample of galaxy clusters at redshifts 0.8 < z < 1.5 taken from the HAWK-I Cluster Survey (HCS). The…”
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A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view by Avirett-Mackenzie, M S, Villforth, C, Huertas-Company, M, Wuyts, S, Alexander, D M, Bonoli, S, Lapi, A, Lopez, I E, Ramos Almeida, C, Shankar, F

“…ABSTRACT Supermassive black holes require a reservoir of cold gas at the centre of their host galaxy in order to accrete and shine as active galactic nuclei…”
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