You Didn\u27t Want Me When I Wanted You : I\u27m Somebody Else\u27s Now

https://digitalcommons.library.umaine.edu/mmb-vp/5212/thumbnail.jp

Oh! Tennessee : You\u27ve Won The Heart Of Me

https://digitalcommons.library.umaine.edu/mmb-vp/4282/thumbnail.jp

When I Come Back To You : We\u27ll Have A Yankee-Doodle Wedding

https://digitalcommons.library.umaine.edu/mmb-vp/2952/thumbnail.jp

Turkestan

https://digitalcommons.library.umaine.edu/mmb-vp/6386/thumbnail.jp

I\u27D Give Everything For You

https://digitalcommons.library.umaine.edu/mmb-vp/1736/thumbnail.jp

Turkestan

Illustration of woman with a hand fanhttps://scholarsjunction.msstate.edu/cht-sheet-music/5457/thumbnail.jp

While You Were Making Believe

Illustration of woman with pearl necklacehttps://scholarsjunction.msstate.edu/cht-sheet-music/10992/thumbnail.jp

Rhythm Of The Rain

No cover arthttps://scholarsjunction.msstate.edu/cht-sheet-music/10219/thumbnail.jp

We\u27re Going to Celebrate The End Of War in Ragtime (Be Sure That Woodrow Wilson Leads The Band)

Illustration of man conducting band and photo or woman in hathttps://scholarsjunction.msstate.edu/cht-sheet-music/5076/thumbnail.jp

The Mid-Infrared Environments of High-Redshift Radio Galaxies

Taking advantage of the impressive sensitivity of Spitzer to detect massive galaxies at high redshift, we study the mid-infrared environments of powerful, high-redshift radio galaxies at 1.2<z<3. Galaxy cluster member candidates were isolated using a single Spitzer/IRAC mid-infrared color criterion, [3.6]-[4.5]>-0.1 (AB), in the fields of 48 radio galaxies at 1.2<z<3. This simple IRAC color selection is effective at identifying galaxies at z>1.2. Using a counts-in-cell analysis, we identify a field as overdense when 15 or more red IRAC sources are found within 1arcmin (i.e.,~0.5Mpc at 1.2<z<3) of the radio galaxy to the 5sigma flux density limits of our IRAC data (f3.6=11.0uJy, f4.5=13.4uJy). We find that radio galaxies lie preferentially in medium to dense regions, with 73% of the targeted fields denser than average. Our (shallow) 120s data permit the rediscovery of previously known clusters and protoclusters associated with radio galaxies as well as the discovery of new promising galaxy cluster candidates at z>1.2.Comment: 14 pages, 7 figures, 3 tables, accepted for publication in Ap