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PUBLICATIONS

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First author

Galaxy properties as revealed by MaNGA - III. Kinematic profiles and stellar population gradients in S0s

Domínguez Sánchez, H.;​ Bernardi, M.;​ Nikakhtar, F.;​ Margalef-Bentabol, B.;​ Sheth, R. K.;  2020; MNRAS, 495, Issue 3, pp.2894-2908

Galaxy properties as revealed by MaNGA. I. Constraints on Initial Mass Function and M/L gradients in ellipticals

Domínguez Sánchez, H.; Bernardi, M.; Brownstein, J. R.; Drory, N.; Sheth, R. K.; 2019, MNRAS, 489, Issue 4, p.5612-5632

Transfer learning for galaxy morphology from one survey to another

Domínguez Sánchez, H.; Huertas Company, M.; Bernardi, M. et al.; 2019; MNRAS, 484, Issue 1, p.93-100

 

Improving galaxy morphologies for SDSS with Deep Learning

Domínguez Sánchez, H.; Huertas Company, M.; Bernardi, M. et al.; 2018; MNRAS, 476, Issue 3, p.3661-3676

Pathways to quiescence: SHARDS view on the Star Formation Histories of massive quiescent galaxies at 1.0 < z < 1.5

Domínguez Sánchez, H.; Pérez González, P.G. et al.; 2016; MNRAS, 457, Issue 4, p.3743-3768

 

Herschel FIR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate Estimates

Domínguez Sánchez, H., Bongiovani, A. et al.; 2014; MNRAS, 441, Issue 1, p.2-23

 

Comparison of Star Formation Rates from Halpha and infrared luminosities as seen by Herschel

Domínguez Sánchez, H.; Mignoli, M. et al.; 2012; MNRAS, 426, Issue 1, pp. 330-341

 

The evolution of quiescent galaxies at high z (z > 1.4)

Domínguez Sánchez, H., Pozzi F.; Gruppioni, C., Cimatti, A. et al.; 2011; MNRAS, 417, Issue 2, pp. 900-915

SECOND author

Pushing automated morphological classifications to their limits with the Dark Energy Survey

Vega-Ferrero J., Domínguez Sánchez, H;  Bernardi M., Huertas-Company, M and the DES collaboration; 2021; arXiv:2012.07858

Hidden AGN in dwarf galaxies revealed by MaNGA: light echoes, o-nuclear wanderers, and a new broad-line AGN

Mezcua M. and Domínguez Sánchez, H.; ApJL, 898, 2

The stellar mass Fundamental Plane: the virial relation and a very thin plane for slow rotators  

Bernardi, M.;​ Domínguez Sánchez, H.;​ Margalef-Bentabol, B.;​ Nikakhtar, F.;​ Sheth, R. K.;  2020; MNRAS, 494, Issue 4, pp.5148-5160

Galaxy properties as revealed by MaNGA. II. Differences in stellar populations of slow and fast rotator ellipticals and dependence on environment

Bernardi, M.; Domínguez Sánchez, H.; Brownstein, J. R.; Drory, N.; Sheth, R. K.; 2019, MNRAS, 489, Issue 4, p.5633-5652

SDSS-IV MaNGA PyMorph Photometric and Deep Learning Morphological Catalogues and implications for bulge properties and stellar angular momentumt

Fischer J.L.; Domínguez Sánchez, H.; Bernardi, M.;  2019, MNRAS, 483, Issue 4, p.2057-2077

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