Hey r/astronomy!

I've been learning to analyze astronomical data and just completed my first systematic quasar analysis. I wanted to share what I found!

The Object: SDSS J150513.83+151010.4

Redshift: z = 4.991

Lookback time: 12.6 billion years (Universe was only 1.2 Gyr old!)

Distance: ~155 billion light-years (comoving)

What I found:

Using the SDSS DR19 spectrum and photometry, I estimated the central supermassive black hole mass using the Shen et al. (2011) virial method:

Black hole mass: ~580 million M☉ (0.58 billion solar masses)

Schwarzschild radius: ~11.4 AU (would engulf most of our inner solar system!)

Eddington ratio: ~0.22 (actively accreting)
Accretion rate: ~2.8 M☉/year

Why this is interesting:

This is a relatively massive black hole existing when the Universe was incredibly young. The big question in astrophysics is: How did supermassive black holes grow so massive so quickly after the Big Bang?

I checked NASA ADS and SIMBAD – while the object is catalogued, there are no dedicated papers studying it. So this might be one of the first detailed analyses of this particular quasar!

My methodology:

  1. Used SDSS SQL search to find high-z quasars (z > 3.5)
  2. Downloaded spectrum and photometry data
  3. Applied virial black hole mass estimator (CIV-based for z~5)
  4. Calculated physical properties using standard cosmology (Planck 2018)

For comparison, I previously analyzed a z=2.003 quasar with a ~217 million M☉ black hole. This z=5 quasar is 2.7× more massive but formed 1.9 billion years earlier in cosmic history!

I'm planning to analyze 4 more z~5 quasars I found to build a small comparative sample. Open to feedback and suggestions!

Tools used: SDSS DR19, Python (matplotlib, numpy), standard virial BH mass relations

Any astrophysicists here – am I doing this right? 😅

by AutomaticBlueMonster

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