| dc.contributor.author | Guha, Labanya Kumar | |
| dc.contributor.author | Srianand, R | |
| dc.contributor.author | Dutta, Rajeshwari | |
| dc.date.accessioned | 2026-10-05T05:33:03Z | |
| dc.date.available | 2026-10-05T05:33:03Z | |
| dc.date.issued | 2026-09-10 | |
| dc.identifier.citation | The Astrophysical Journal, Vol. 1008, No. 2, 259 | en_US |
| dc.identifier.issn | 1538-4357 | |
| dc.identifier.uri | http://hdl.handle.net/2248/9060 | |
| dc.description | Open Access | en_US |
| dc.description | Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. h | |
| dc.description.abstract | We present the largest catalogue to date of Galaxies On Top Of Quasars (GOTOQs)---systems where the sight line to a background quasar passes directly through or very close to a foreground galaxy. Using ~1.1 million quasar spectra from the SDSS-DR16 and DESI Early Data Release, we identify 1345 unique GOTOQs over 0.0045 <= z <= 1.09, more than quadrupling the number previously known. The catalogue combines both absorption-agnostic and absorption-selected searches, enabling a robust characterisation of gas in galaxies at projected separations of D ≲ 20 kpc. The GOTOQ emission-line ratios indicate that their host galaxies are predominantly normal, star-forming disks with typical dust extinctions of AV ≃ 0.5 mag. We measure the Mg II covering fraction at D ≲ 20 kpc and find it to be remarkably high, fc=98.2-4.5+1.3 %, indicating that these systems trace gas-rich, metal-enriched regions at the disk-halo interface. The median colour excess towards the quasar line of sight of E(B - V) = 0.087 is significantly higher than that of typical Mg II absorbers, underscoring the dust-rich nature of GOTOQ sight lines. From a high signal-to-noise composite spectrum, we report the first statistical detection of the diffuse interstellar band at λ4428 (Wr = 0.055 ± 0.011 Å) and at λ5780 (Wr = 0.051 ± 0.012 Å), revealing the presence of complex organic molecules at the disk-halo interface. This catalogue provides a powerful reference sample for future multiwavelength studies of gas flows, cold gas, and dust evolution in the inner circumgalactic medium. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | American Astronomical Society | en_US |
| dc.relation.uri | ttps://doi.org/10.3847/1538-4357/ae99c6 | |
| dc.rights | © 2026. The Author(s) | |
| dc.subject | Quasar absorption line spectroscopy | en_US |
| dc.subject | Quasar-galaxy pairs | en_US |
| dc.subject | Galaxy evolution | en_US |
| dc.subject | Circumgalactic medium | en_US |
| dc.subject | Interstellar medium | en_US |
| dc.subject | Interstellar dust | en_US |
| dc.subject | Catalogs | en_US |
| dc.title | Cosmic chance superpositions: Largest catalog of quasar-galaxy pairs at a projected separation of D ≲ 20 kpc | en_US |
| dc.type | Article | en_US |