papers

Publications (49)

astro-ph.SR2018

J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX

D. D. Whitten, V. M. Placco, T. C. Beers +24

We present a new methodology for the estimation of stellar atmospheric parameters from narrow- and intermediate-band photometry of the Javalambre Photometric Local Universe Survey…

astro-ph.CO2010

PACS and SPIRE photometer maps of M33: First results of the Herschel M33 extended survey (HERM33ES)

C. Kramer, C. Buchbender, E. M. Xilouris +37

Within the framework of the HERM33ES key project, we are studying the star forming interstellar medium in the nearby, metal-poor spiral galaxy M33, exploiting the high resolution a…

astro-ph.SR2025

Nickel- and iron-rich clumps in planetary nebulae: New discoveries and emission-line diagnostics

K. Bouvis, S. Akras, H. Monteiro +7

Integral field spectroscopy (IFS) offers a distinct advantage for studying extended sources by enabling spatially resolved emission maps for several emission lines without the need…

astro-ph.GA2009

A long trail behind the planetary nebula HFG1 (PK 136+05) and its precataclysmic binary central star V664 Cas

P. Boumis, J. Meaburn, M. Lloyd +1

A deep wide-field image in the light of the Halpha+[N II] emission lines, of the planetary nebula HFG1 which surrounds the precataclysmic binary system V664 Cas, has revealed a tai…

astro-ph.GA2019

The S-PLUS: a star/galaxy classification based on a Machine Learning approach

M. V. Costa-Duarte, L. Sampedro, A. Molino +32

We present a star/galaxy classification for the Southern Photometric Local Universe Survey (S-PLUS), based on a Machine Learning approach: the Random Forest algorithm. We train the…

astro-ph.SR2017

Multi-band polarimetry of post-asymptotic giant branch stars stars. Optical measurements

S. Akras, J. C. Ramirez Velez, N. Nanouris +4

We present new optical broad-band (UBVRI) aperture polarimetric observations of 53 post-asymptotic giant branch (AGB) stars selected to exhibit a large near-infrared excess. 24 out…

astro-ph.SR2025

The planetary nebula NGC 3132 revisited: high definition 3D photoionization model

H. Monteiro, C. Mendes de Oliveira, P. Amram +6

We present a detailed 3D photoionization model of the planetary nebula NGC 3132, constrained by the latest observations. Using the MOCASSIN code, the model incorporates integrated…

astro-ph.GA2022

Deep optical study of the mixed-morphology supernova remnant G 132.7+1.3 (HB3)

P. Boumis, A. Chiotellis, V. Fragkou +8

We present optical ccd images of the large supernova remnant (SNR) G132.71.3 (HB3) covering its full extent for the first time, in the emission lines of H[N II], [S II] and…

astro-ph.SR2016

Modelling the structure and kinematics of the Firework nebula: The nature of the GK Persei nova shell and its jet-like feature

E. Harvey, M. P. Redman, P. Boumis +1

To gain a more complete understanding of the dynamics of the GK Per (1901) remnant faint-object high-resolution echelle spectroscopic observations and imaging were undertaken cover…

astro-ph.SR2022

The miniJPAS survey: White dwarf science with 56 optical filters

C. López-Sanjuan, P. -E. Tremblay, A. Ederoclite +21

We analyze the white dwarf population in miniJPAS, the first square degree observed with 56 medium-band, 145 A in width optical filters by the Javalambre Physics of the acceleratin…

astro-ph.GA2019

The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

C. Mendes de Oliveira, T. Ribeiro, W. Schoenell +142

The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 m robotic telescope, the T80-So…

astro-ph2006

Photometric study of selected cataclysmic variables

C. Papadaki, H. M. J. Boffin, C. Sterken +5

We present time-resolved photometry of five relatively poorly-studied cataclysmic variables: V1193 Ori, LQ Peg, LD 317, V795 Her, and MCT 2347-3144. The observations were made usin…

astro-ph.SR2016

Observations and Analysis of the GK Persei Nova Shell and its "Jet-like" Feature

E. Harvey, M. P. Redman, P. Boumis +1

GK Persei (1901, the 'Firework Nebula') is an old but bright nova remnant that offers a chance to probe the physics and kinematics of nova shells. The kinematics in new and archiva…

astro-ph.SR2023

H molecular gas in the old planetary nebula NGC 3587

G. Ramos-Larios, M. A. Guerrero, J. A. Toalá +2

The acquisition of high-quality deep images of planetary nebulae (PNe) has allowed the detection of a wealth of small-scale features, which highlight the complexity of the formatio…

astro-ph.GA2025

Dissecting NGC 3132: Tracing the mass-loss history of the southern ring planetary nebula

K. Bouvis, S. Akras, H. Monteiro +7

Central to our understanding of stellar evolution and its impact on processes in our Galaxy and across the Universe is the study of mass loss. While the general framework is well e…

astro-ph.SR2016

The circumstellar environment of pre-SN Ia systems

E. Harvey, M. P. Redman, P. Boumis +4

Here we explore the possible preexisting circumstellar debris of supernova type Ia systems. Classical, symbiotic and recurrent novae all accrete onto roughly solar mass white dwarf…

astro-ph.GA2024

ALMA detection of Masers and Dasars in the Hydrogen Recombination Lines of the Planetary Nebula Mz3

Z. Abraham, P. P. B. Beaklini, I. Aleman +5

The hydrogen recombination lines H30, H40, H42, H50 and H57 and the underlying bremsstrahlung continuum emission were detected with ALMA in the bipolar nebula M…

astro-ph.SR2023

Planetary nebulae hosting accreting white dwarfs: A possible solution for the mysterious cut-off of Planetary Nebula Luminosity Function?

D. Souropanis, A. Chiotellis, P. Boumis +2

Many binary companions to the central stars of planetary nebulae (PNe) are found to be inflated, perhaps indicating that accretion onto the central star might occur during the PN p…

astro-ph.CO2012

Cool and warm dust emission from M33 (HerM33es)

E. M. Xilouris, F. S. Tabatabaei, M. Boquien +24

We study the far-infrared emission from the nearby spiral galaxy M33 in order to investigate the dust physical properties such as the temperature and the luminosity density across…

astro-ph.SR2015

Evidence for a [WR] or WEL-type binary nucleus in the bipolar planetary nebula Vy 1-2

S. Akras, P. Boumis, J. Meaburn +3

We present high-dispersion spectroscopic data of the compact planetary nebula Vy 1-2, where high expansion velocities up to 100 km/s are found in the Ha, [N II] and [O III] emissio…

astro-ph.GA2018

J-PLUS: 2-D analysis of the stellar population in NGC 5473 and NGC 5485

I. San Roman, P. Sánchez-Blázquez, A. J. Cenarro +23

The spatial variations of stellar population properties within a galaxy are intimately related to their formation process. Therefore, spatially resolved studies of galaxies are ess…

astro-ph.SR2020

Two New Nova Shells associated with V4362 Sagittarii and DO Aquilae

E. J. Harvey, M. P. Redman, P. Boumis +8

A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The material ejected from the white dwarf surface generally forms an axisymmetric she…

astro-ph.GA2021

On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2

L. Nakazono, C. Mendes de Oliveira, N. S. T. Hirata +25

This paper provides a catalogue of stars, quasars, and galaxies for the Southern Photometric Local Universe Survey Data Release 2 (S-PLUS DR2) in the Stripe 82 region. We show that…

astro-ph.GA2023

Detection of optical emission from the supernova remnant G7.7-3.7

V. Domček, J. V. Hernández Santisteban, A. Chiotellis +6

We present the first optical study of the supernova remnant (SNR) G7.7-3.7, with the aim of determining its evolutionary phase since it has been suggested to be the remnant of SN 3…

astro-ph2008

Photometric study of selected cataclysmic variables II. Time-series photometry of nine systems

C. Papadaki, H. M. J. Boffin, V. Stanishev +3

We present time-series photometry of nine cataclysmic variables: EI UMa, V844Her, V751 Cyg, V516 Cyg, GZ Cnc, TY Psc, V1315 Aql, ASAS J002511+1217.12, V1315 Aql and LN UMa. The obs…

astro-ph2006

New Planetary Nebulae in the Galactic Bulge region with l>0deg - II

P. Boumis, S. Akras, E. M. Xilouris +4

The presentation of new results from an [O III] 5007 A survey in a search for planetary nebulae (PNe) in the galactic bulge is continued. A total of 60 objects, including 19 new PN…

astro-ph.SR2022

Spectroscopic Analysis Tool for intEgraL fieLd unIt daTacubEs (satellite): Case studies of NGC 7009 and NGC 6778 with MUSE

S. Akras, H. Monteiro, J. R. Walsh +11

Integral field spectroscopy (IFS) provides a unique capability to spectroscopically study extended sources over a 2D field of view, but it also requires new techniques and tools. I…

astro-ph.GA2019

J-PLUS: Tools to identify compact planetary nebulae in the Javalambre and southern photometric local universe surveys

L. A. Gutiérrez-Soto, D. R. Gonçalves, S. Akras +28

From the approximately 3,500 planetary nebulae (PNe) discovered in our Galaxy, only 14 are known to be members of the Galactic halo. Nevertheless, a systematic search for hal…

astro-ph.SR2019

RAMSES II - RAMan Search for Extragalactic Symbiotic Stars. Project concept, commissioning, and early results from the science verification phase

R. Angeloni, D. R. Gonçalves, S. Akras +16

Symbiotic stars (SySts) are long-period interacting binaries composed of a hot compact star, an evolved giant star, and a tangled network of gas and dust nebulae. They represent un…

astro-ph.SR2022

The miniJPAS survey: stellar atmospheric parameters from 56 optical filters

H. -B. Yuan, L. Yang, P. Cruz +29

With a unique set of 54 overlapping narrow-band and two broader filters covering the entire optical range, the incoming Javalambre-Physics of the Accelerating Universe Astrophysica…

astro-ph.SR2022

Linking the properties of accreting white dwarfs with the ionization state of their ambient medium

D. Souropanis, A. Chiotellis, P. Boumis +5

Steadily accreting white dwarfs (WDs) are efficient sources of ionization and thus, are able to create extended ionized nebulae in their vicinity. These nebulae represent ideal too…

astro-ph.GA2025

Low-ionization structures in planetary nebulae -- IV. The molecular hydrogen counterpart

M. B. Mari, S. Akras, D. R. Gonçalves

Context. Low-ionization structures (LISs), found in all morphological types of planetary nebulae (PNe), are small-scale features prominent in emission from low-ionization species s…

astro-ph.GA2022

Photometric redshifts for the S-PLUS Survey: is machine learning up to the task?

E. V. R. Lima, L. Sodré, C. R. Bom +14

The Southern Photometric Local Universe Survey (S-PLUS) is a novel project that aims to map the Southern Hemisphere using a twelve filter system, comprising five broad-band SDSS-li…

astro-ph.SR2025

Integral field spectroscopy of the planetary nebula NGC 3242 and the puzzling nature of its low ionization structures

L. Konstantinou, S. Akras, J. Garcia-Rojas +7

The physico-chemical properties of the planetary nebula (PN) NGC 3242 are investigated in both 1D and 2D, using Integral Field Unit (IFU) data. This PN has a complex morphology wit…

astro-ph.SR2022

Discovery of an optical cocoon tail behind the runaway HD 185806

Z. T. Spetsieri, P. Boumis, A. Chiotellis +6

Studies on the circumstellar structures around evolved stars provide vital information on the evolution of the parent star and the properties of the local interstellar medium. In t…

astro-ph.GA2024

Stellar atmospheric parameters and chemical abundances of about 5 million stars from S-PLUS multi-band photometry

C. E. Ferreira Lopes, L. A. Gutiérrez-Soto, V. S. Ferreira Alberice +30

Context. Spectroscopic surveys like APOGEE, GALAH, and LAMOST have significantly advanced our understanding of the Milky Way by providing extensive stellar parameters and chemical…

astro-ph.HE2017

Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

M. C. Díaz, L. M. Macri, D. Garcia Lambas +52

We present the results of prompt optical follow-up of the electromagnetic counterpart of the gravitational-wave event GW170817 by the Transient Optical Robotic Observatory of the S…

astro-ph2006

New Planerary Nebulae towards the Galactic bulge

P. Boumis, S. Akras, P. A. M. van Hoof +3

New Planetary Nebulae (PNe) were discovered through an [O III] 5007 A emission line survey in the Galactic bulge region with l>0 deg. We detected 240 objects, including 44 new PNe.…

astro-ph.SR2016

Deciphering the bipolar planetary nebula Abell 14 with 3D ionization and morphological studies

S. Akras, N. Clyne, P. Boumis +4

Abell 14 is a poorly studied object despite being considered a born again planetary nebula. We performed a detailed study of its 3D morphology and ionization structure using the SH…

astro-ph.SR2012

3-D modelling of the collimated bipolar outflows of compact planetary nebulae with WR-type central stars

S. Akras, J. A. López

We present high-resolution, long-slit spectroscopic observations of five compact ( 10 arcsec) planetary nebulae located close to the galactic bulge region and for which no hi…

astro-ph.GA2025

Mapping H-Excess Candidate Point Sources in the Southern Hemisphere Using S-PLUS Data

L. A. Gutiérrez-Soto, R. Lopes de Oliveira, S. Akras +18

Context. We use the Southern Photometric Local Universe Survey (S-PLUS) Fourth Data Release (DR4) to identify and classify H-excess point sources in the Southern Sky, combining…

astro-ph.GA2019

Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case

A. Molino, M. V. Costa-Duarte, L. Sampedro +42

In this paper we present a thorough discussion about the photometric redshift (photo-z) performance of the Southern Photometric Local Universe Survey (S-PLUS). This survey combines…

astro-ph.GA2018

J-PLUS: measuring emission line fluxes in the nearby universe

R. Logroño-García, G. Vilella-Rojo, C. López-Sanjuan +29

In the present paper we aim to validate a methodology designed to extract the Halpha emission line flux from J-PLUS photometric data. J-PLUS is a multi narrow-band filter survey ca…

astro-ph.SR2022

THA 15-31: Discovery with VLT/X-Shooter and Swift/UVOT of a new symbiotic star of the accreting-only variety

U. Munari, J. K. AlcalÃ, A. Frasca +4

We report the discovery and characterization of a new symbiotic star of the accreting-only variety, which we observed in the optical/near-infrared (NIR) with VLT/X-Shooter and in t…

astro-ph.CO2020

The miniJPAS survey: a preview of the Universe in 56 colours

S. Bonoli, A. Marín-Franch, J. Varela +166

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will soon start to scan thousands of square degrees of the northern extragalactic sky with a unique…

astro-ph.SR2018

The interaction of the halo around the butterfly planetary nebula NGC650-1 with the interstellar medium

G. Ramos-Larios, M. A. Guerrero, A. Nigoche-Netro +7

With its bright and wide equatorial waist seen almost edge-on (the butterfly body) and the faint and broad bipolar extensions (the butterfly wings), NGC650-1 is the archetypical ex…

astro-ph.SR2012

"Distance mapping" and the 3-D structure of BB +30 3639

S. Akras, W. Steffen

BD +30 3639 is a member of a group of uncommon planetary nebula with Wolf-Rayet central star and higher expansion velocities in [O III] than in [N II] lines. Images and high-resolu…

astro-ph.GA2018

J-PLUS: The Javalambre Photometric Local Universe Survey

A. J. Cenarro, M. Moles, D. Cristóbal-Hornillos +119

J-PLUS is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern hemisphere from the dedicated JAST/T80 telescope at the Observatorio…

astro-ph2007

Deep optical observations of the interaction of the SS 433 microquasar jet with the W 50 radio continuum shell

P. Boumis, J. Meaburn, J. Alikakos +6

Four mosaics of deep, continuum-subtracted, CCD images have been obtained over the extensive galactic radio continuum shell, W 50, which surrounds the remarkable stellar system SS…