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papers

Publications (23)

astro-ph.GA2017

A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations

Robbert Verbeke, Emmanouil Papastergis, Anastasia A. Ponomareva +2

astro-ph.CO2017

Hints against the cold and collisionless nature of dark matter from the galaxy velocity function

Aurel Schneider, Sebastian Trujillo-Gomez, Emmanouil Papastergis +2

astro-ph.GA2017

Testing core creation in hydrodynamical simulations using the HI kinematics of field dwarfs

Emmanouil Papastergis, Anastasia A. Ponomareva

astro-ph.CO2011

The Arecibo Legacy Fast ALFA Survey: The alpha.40 HI Source Catalog, its Characteristics and their Impact on the Derivation of the HI Mass Function

Martha P. Haynes, Riccardo Giovanelli, Ann M. Martin +21

astro-ph.GA2017

From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation

Anastasia A. Ponomareva, Marc A. W. Verheijen, Emmanouil Papastergis +2

astro-ph.GA2016

Environmental dependence of the HI mass function in the ALFALFA 70% catalogue

Michael G. Jones, Emmanouil Papastergis, Martha P. Haynes +1

astro-ph.CO2013

The clustering of ALFALFA galaxies: dependence on HI mass, relationship to optical samples & clues on host halo properties

Emmanouil Papastergis, Riccardo Giovanelli, Martha P. Haynes +2

astro-ph.GA2015

When is Stacking Confusing?: The Impact of Confusion on Stacking in Deep HI Galaxy Surveys

Michael G. Jones, Martha P. Haynes, Riccardo Giovanelli +1

astro-ph.CO2012

Gas-Bearing Early-Type Dwarf Galaxies in Virgo: Evidence for Recent Accretion

Gregory Hallenbeck, Emmanouil Papastergis, Shan Huang +7

astro-ph.CO2011

The velocity width function of galaxies from the 40% ALFALFA survey: shedding light on the cold dark matter overabundance problem

Emmanouil Papastergis, Ann M. Martin, Riccardo Giovanelli +1

astro-ph.GA2016

An assessment of the "too big to fail" problem for field dwarf galaxies in view of baryonic feedback effects

Emmanouil Papastergis, Francesco Shankar

astro-ph.CO2012

A direct measurement of the baryonic mass function of galaxies & implications for the galactic baryon fraction

Emmanouil Papastergis, Andrea Cattaneo, Shan Huang +2

astro-ph.GA2018

The contribution of HI-bearing ultra-diffuse galaxies to the cosmic number density of galaxies

Michael G. Jones, Emmanouil Papastergis, Viraj Pandya +5

astro-ph.CO2017

Another baryon miracle? Testing solutions to the "missing dwarfs" problem

Sebastian Trujillo-Gomez, Aurel Schneider, Emmanouil Papastergis +2

astro-ph.CO2010

The Arecibo Legacy Fast ALFA Survey: X. The HI Mass Function and Omega_HI From the 40% ALFALFA Survey

Ann M. Martin, Emmanouil Papastergis, Riccardo Giovanelli +3

astro-ph.GA2018

The Arecibo Legacy Fast ALFA Survey: The ALFALFA Extragalactic HI Source Catalog

Martha P. Haynes, Riccardo Giovanelli, Brian R. Kent +22

astro-ph.GA2015

Spectroscopic Confusion: Its Impact on Current and Future Extragalactic HI Surveys

Michael G. Jones, Emmanouil Papastergis, Martha P. Haynes +1

astro-ph.GA2015

Is there a "too big to fail" problem in the field?

Emmanouil Papastergis, Riccardo Giovanelli, Martha P. Haynes +1

astro-ph.GA2018

The $HI$- and $H_{2}$-to-stellar mass correlations of late- and early-type galaxies and their consistency with the observational mass functions

A. R. Calette, Vladimir Avila-Reese, Aldo Rodríguez-Puebla +2

astro-ph.GA2017

HI in Virgo's "Red and Dead" Dwarf Ellipticals - A Tidal Tail and Central Star Formation

Gregory Hallenbeck, Rebecca Koopmann, Riccardo Giovanelli +4

astro-ph.GA2014

The ALFALFA "Almost Darks" Campaign: Pilot VLA HI Observations of Five High Mass-to-Light Ratio Systems

John M. Cannon, Charlotte P. Martinkus, Lukas Leisman +13

astro-ph.CO2014

Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies

Andrea Cattaneo, Paolo Salucci, Emmanouil Papastergis

astro-ph.GA2017

How to Reconcile the Observed Velocity Function of Galaxies with Theory

Alyson M. Brooks, Emmanouil Papastergis, Charlotte R. Christensen +4