The edge-on Galaxies in the Pan-STARRS survey (EGIPS). Issue 2 (29th January 2022)

• Record Type: Journal Article
• Authors: Makarov, D; Savchenko, S; Mosenkov, A; Bizyaev, D; Reshetnikov, V; Antipova, A; Tikhonenko, I; Usachev, P; Borisov, S; Makarova, L; Kautsch, S; Marchuk, A; Rubtsov, E
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 511:Issue 2(2022)
• Page Start: 3063
• Page End: 3075
• Publication Date: 2022-01-29
• Subjects: astronomical data bases -- catalogues -- galaxies: photometry -- galaxies: statistics; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac227
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present a catalogue of 16 551 edge-on galaxies created using the public DR2 data of the Pan-STARRS survey. The catalogue covers the three quarters of the sky above Dec. = −30°. The galaxies were selected using a convolutional neural network, trained on a sample of edge-on galaxies identified earlier in the SDSS survey. This approach allows us to dramatically improve the quality of the candidate selection and perform a thorough visual inspection in a reasonable amount of time. The catalogue provides homogeneous information on astrometry, SExtractor photometry, and non-parametric morphological statistics of the galaxies. The photometry is reliably for objects in the 13.8–17.4 r -band magnitude range. According to the HyperLeda data base, redshifts are known for about 63 per cent of the galaxies in the catalogue. Our sample is well separated into the red sequence and blue cloud galaxy populations. The edge-on galaxies of the red sequence are systematically Δ( g − i ) ≈ 0.1 mag redder than galaxies oriented at an arbitrary angle to the observer. We found a variation of the galaxy thickness with the galaxy colour. The red sequence galaxies are thicker than the galaxies of the blue cloud. In the blue cloud, on average, thinner galaxies turn out to be bluer. In the future, based on this catalogue it is intended to explore the three-dimensional structure of galaxies of different morphologies, as well as to study the scaling relations for discs and bulges.