Thank you to AAS Nova for highlighting the recent SDSS-V overview paper! Check out their article (and the overview paper!) to learn how SDSS is expanding our view of the universe through panoptic, spectroscopic mapping of the night sky. 🌌
A New View of the Spectroscopic Universe
The Sloan Digital Sky Survey fundamentally changed the way modern astronomy research is done. The collaboration recently released their summary of the fifth generation of their landmark survey. https://t.co/oSVsZeqtk8
All Black Hole Mapper science programs are available here, https://t.co/Vmufbc3iJc, and they include time domain programs such AQMES (All-Quasar Multi-Epoch Spectroscopy and reverberation mapping, X-ray follow-up programs.
We are releasing several new Jupyter Notebook style tutorials to help you use the new SDSS-V DR19 data: https://t.co/dqBVXal0BC https://t.co/yKApBtfRMO
We are releasing a total of ~380,000 BOSS spectra in DR19 for ~120,000 distinct objects primarily targeted for spectroscopy by BHM, an order of magnitude expansion vs. DR18. https://t.co/vIRBTS4bRq https://t.co/Wu2irPqKzF
Today is a big day for us: it's DATA RELEASE DAY!!! And to celebrate our nineteenth data release, we have not one, but two papers for you to read all about our data: we have a DR19 paper (https://t.co/aprwTYIzuA) and an SDSS-V Overview paper (https://t.co/ne5rOFEO6f) #DR19
about the BLR structure and how they change based on the luminosity state of the quasar. This has implications for the use of reverberation mapping in this source to measure a black hole mass, and more! (3/3)
This week's BHM science paper highlight is "The SDSS-V Black Hole Mapper Reverberation Mapping Project: A Kinematically Variable Broad-Line Region and Consequences for Masses of Luminous Quasars", by @loganfries Fries et al. (2024). (1/3) https://t.co/2NpEtElImM
This paper presents a velocity-resolved analysis of reverberation mapping data of the quasar SDSS-RM 160, which is a hypervariable quasar found to display odd/interesting behavior in its BLR. The team uses reverberation mapping techniques to uncover details (2/3)
They use this sample to look for and report on trends in various properties of AGN that show this behavior, such as accretion rate, and examine the behavior of different emission lines.
This week's BHM paper highlight is "Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results" by Zeltyn et al. (2024). The paper can be found here: https://t.co/00jweGSgEP
This work reports the results of a large-scale search for changing-look AGN (AGN that show dramatic variability and/or changes in "type") with first-year SDSS-V BHM spectroscopy. They found 116 changing-look AGN, the largest number of changing-look AGN ever reported!
Accelerating quasar winds have been reported before, but with 130 observations from SDSS spread over 8 years, researchers were able to show the acceleration at high confidence. These results were also reported by several news outlets: For example, see https://t.co/Erdr6TIi6n
This week's BHM paper highlight is "The SDSS-V Black Hole Mapper Reverberation Mapping Project: CIV BAL Acceleration in the Quasar SBS 1408+544" by Wheatley et al. (2024). The paper can be found here: https://t.co/nMYAUtw86Q
This paper reports an investigation of variability in a broad absorption-line quasar that was observed by the BHM program. Researchers discovered that a prominent absorption line, which indicates a wind being launched off the quasar accretion disk, is accelerating.
This paper analyzes the X-ray (eROSITA) and optical (SDSS and other) properties of the X-ray sources found and is meant as a demonstration of what is to come with the full eROSITA all-sky survey data that may come in future years.
This week's BHM paper highlight is "The eROSITA Final Equatorial Depth Survey (eFEDS): The Hard X-ray Selected Sample" by K. Nandra et al (2024). The paper can be found here: https://t.co/jB3eCeIJ8E
This paper presents a sample of hard X-ray sources detected by the eROSITA satellite, focusing specifically on extragalactic sources, which primarily include AGN. These sources were targeted in the optical by SDSS-V as a part of the BHM program!