CG4 Current Research Activities - Revision history

Hoette at 22:50, 18 January 2011

2011-01-18T22:50:28Z

Hoette at 22:45, 18 January 2011

2011-01-18T22:45:36Z

Rebull at 00:33, 4 January 2011

2011-01-04T00:33:12Z

Rebull at 00:32, 4 January 2011

2011-01-04T00:32:24Z

CJohnson: /* Previously Known Objects in Puppis region (Reipurth and Pettersson 1993) */

2010-11-23T19:00:12Z

Previously Known Objects in Puppis region (Reipurth and Pettersson 1993)

Hoette: /* Edu poster 1 */

2010-09-30T18:59:01Z

Edu poster 1

Hoette: /* Edu poster 1 */

2010-09-29T22:09:04Z

Edu poster 1

Hoette: /* Edu poster 1 */

2010-09-29T22:06:26Z

Edu poster 1

CJohnson at 22:03, 29 September 2010

2010-09-29T22:03:29Z

CJohnson at 22:00, 29 September 2010

2010-09-29T22:00:59Z

@@ Line 116: / Line 116: @@
 NEW! See email...
-=[[CG4 AAS 2010 Meeting]]=
+=[[CG4 AAS 2011 Meeting]]=
 ''Pictures and more''

← Older revision		Revision as of 22:45, 18 January 2011
Line 115:		Line 115:
	=[[CG4 Winter Mini-Workshop]]=		=[[CG4 Winter Mini-Workshop]]=
	NEW! See email...		NEW! See email...
		+
		+	=[[CG4 AAS 2010 Meeting]]=
		+	''Pictures and more''

← Older revision		Revision as of 00:33, 4 January 2011
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	=[[CG4 Abstracts]]=		=[[CG4 Abstracts]]=
	''Now pulled off to their own page.''		''Now pulled off to their own page.''
		+
		+	=[[CG4 Winter Mini-Workshop]]=
		+	NEW! See email...

@@ Line 110: / Line 110: @@
 =[[CG4 Fall Work]]=
-==Science Abstract==
+=[[CG4 Abstracts]]=
-First draft of Science Abstract:
+''Now pulled off to their own page.''

@@ Line 18: / Line 18: @@
 Subject to change! Includes agenda for Summer visit.
-=Previously Known Objects in Puppis region (Reipurth and Pettersson 1993)=
+=Previously Known Objects in Puppis region (Reipurth and Pettersson 1993)...''fixed CG-Halpha4''=
 {| border="1"
 |Star
@@ Line 54: / Line 54: @@
 |CG-Halpha 4
 |07 31 21.92
-| -46 59 45.14
+| -46 '''''57''''' 45.14 **
 |14.59
 |1.40

← Older revision		Revision as of 18:59, 30 September 2010
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	This poster tracks our work with an SSC scientist during the spring, summer, and fall of 2010. The group coauthored another AAS poster on finding Young Stellar Objects (YSO) in the CG4 Nebula in Puppis. During the project, the students, scientists and teachers developed a number of techniques for learning the necessary science as well as doing the required data acquisition and analysis. Collaborations were formed between students with disabilities and their non-disabled peers to create multi-media projects. Ultimately, the projects created for our work with NITARP will be disseminated through our professional connections in order to ignite a passion for astronomy in all students - with and without disabilities. This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by NASA Astrophysics Data Program and Archive Outreach funds.		This poster tracks our work with an SSC scientist during the spring, summer, and fall of 2010. The group coauthored another AAS poster on finding Young Stellar Objects (YSO) in the CG4 Nebula in Puppis. During the project, the students, scientists and teachers developed a number of techniques for learning the necessary science as well as doing the required data acquisition and analysis. Collaborations were formed between students with disabilities and their non-disabled peers to create multi-media projects. Ultimately, the projects created for our work with NITARP will be disseminated through our professional connections in order to ignite a passion for astronomy in all students - with and without disabilities. This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by NASA Astrophysics Data Program and Archive Outreach funds.
		+
		+	I think that maybe ewe should change
		+	Yerkes Observatory scientists, along with educators
		+	to
		+	Educators and students from Yerkes Observatory, Wisconsin School for the Deaf, etc.
		+
		+	same number of words... Viv on Thurs Sept. 30th
		+

@@ Line 179: / Line 179: @@
-Connie's suggested edits (still 296 words)
+Connie/Viv/Chelen leading to final version here:
-Individuals with disabilities - specifically individuals who are deaf or hard of hearing (DHH) and/or blind and visually-impaired (BVI) - have traditionally been underrepresented in the fields of Science, Technology, Engineering, and Math (STEM).  The low incidence rate of these populations, coupled with geographic isolation, creates limited opportunities for students to work with and receive mentoring by professionals who not only have specialty knowledge in disability areas but also work in STEM fields. For this reason, Yerkes Observatory scientists, along with educators from the Wisconsin School for the Deaf, the Wisconsin Center for the Blind and Visually Impaired, Breck School, and Oak Park and River Forest High School, are engaged in active research with a Spitzer Science Center (SSC) scientist. Our ultimate goals are threefold; to engage DHH and BVI students with equal success as their sighted and hearing peers, to share our techniques to make astronomy more accessible to DHH and BVI youth, and to generate a life-long interest which will lead our students to STEM careers.
+Individuals with disabilities - specifically individuals who are deaf or hard of hearing (DHH) and/or blind and visually-impaired (BVI) - have traditionally been underrepresented in the fields of Science, Technology, Engineering, and Math (STEM).  The low incidence rate of these populations, coupled with geographic isolation, creates limited opportunities for students to work with and receive mentoring by professionals who not only have specialty knowledge in disability areas but also work in STEM fields. Yerkes Observatory scientists, along with educators from the Wisconsin School for the Deaf, the Wisconsin Center for the Blind and Visually Impaired, Breck School, and Oak Park and River Forest High School, are engaged in active research with a Spitzer Science Center (SSC) scientist. Our ultimate goals are threefold; to engage DHH and BVI students with equal success as their sighted and hearing peers, to share our techniques to make astronomy more accessible to DHH and BVI youth, and to generate a life-long interest which will lead our students to STEM careers.
 This poster tracks our work with an SSC scientist during the spring, summer, and fall of 2010.  The group coauthored another AAS poster on finding Young Stellar Objects (YSO) in the CG4 Nebula in Puppis.  During the project, the students, scientists and teachers developed a number of techniques for learning the necessary science as well as doing the required data acquisition and analysis.  Collaborations were formed between students with disabilities and their non-disabled peers to create multi-media projects.  Ultimately, the projects created for our work with NITARP will be disseminated through our professional connections in order to ignite a passion for astronomy in all students - with and without disabilities.  This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by NASA Astrophysics Data Program and Archive Outreach funds.

← Older revision		Revision as of 22:03, 29 September 2010
Line 121:		Line 121:
	rationale for my changes: occasional missing words/wordsmithing. the stuff about radially pointing is indeed true, but not strictly relevant to the abstract (tho' it's appropriate for the main body of the poster in the introduction). 'we will use' = lingering sentence left over i think from editing, since it is redundant with prior sentence. stuff about separating YSOs from contaminants absolutely true, but is implicit in the statement that we've identified YSO candidates -- of course we've attempted to weed out contaminants. there should be some text on that in the main body of the poster, though, for sure.		rationale for my changes: occasional missing words/wordsmithing. the stuff about radially pointing is indeed true, but not strictly relevant to the abstract (tho' it's appropriate for the main body of the poster in the introduction). 'we will use' = lingering sentence left over i think from editing, since it is redundant with prior sentence. stuff about separating YSOs from contaminants absolutely true, but is implicit in the statement that we've identified YSO candidates -- of course we've attempted to weed out contaminants. there should be some text on that in the main body of the poster, though, for sure.

−	~~Final version (as submitted to AAS):~~
−	We used archival Spitzer infrared data to look for new young stellar objects (YSOs) in Cometary Globule 4 (CG4) in Puppis. CG4 is approximately 1300 parsecs away and one of about 30 cometary globules in the Gum Nebula, many of which are known to be forming stars. CG4 is dramatic in appearance, and that has brought it to the attention of both scientists and the public. Our team used archival Spitzer InfraRed Array Camera (IRAC) and Multiband Imaging Photometer for Spitzer (MIPS) data, combined with 2 Micron All Sky Survey (2MASS) data as well as optical data obtained by collaborators. We used infrared excess to investigate the properties of previously known YSOs in this region and identify additional new candidate YSOs in this region. This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by NASA Astrophysics Data Program and Archive Outreach funds.

		+	Final version (as submitted to AAS): ''We used archival Spitzer infrared data to look for new young stellar objects (YSOs) in Cometary Globule 4 (CG4) in Puppis. CG4 is approximately 1300 parsecs away and one of about 30 cometary globules in the Gum Nebula, many of which are known to be forming stars. CG4 is dramatic in appearance, and that has brought it to the attention of both scientists and the public. Our team used archival Spitzer InfraRed Array Camera (IRAC) and Multiband Imaging Photometer for Spitzer (MIPS) data, combined with 2 Micron All Sky Survey (2MASS) data as well as optical data obtained by collaborators. We used infrared excess to investigate the properties of previously known YSOs in this region and identify additional new candidate YSOs in this region. This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by NASA Astrophysics Data Program and Archive Outreach funds.''

	--[[User:CJohnson\|CJohnson]] 17:00, 29 September 2010 (CDT)		--[[User:CJohnson\|CJohnson]] 17:00, 29 September 2010 (CDT)

← Older revision		Revision as of 22:00, 29 September 2010
Line 121:		Line 121:
	rationale for my changes: occasional missing words/wordsmithing. the stuff about radially pointing is indeed true, but not strictly relevant to the abstract (tho' it's appropriate for the main body of the poster in the introduction). 'we will use' = lingering sentence left over i think from editing, since it is redundant with prior sentence. stuff about separating YSOs from contaminants absolutely true, but is implicit in the statement that we've identified YSO candidates -- of course we've attempted to weed out contaminants. there should be some text on that in the main body of the poster, though, for sure.		rationale for my changes: occasional missing words/wordsmithing. the stuff about radially pointing is indeed true, but not strictly relevant to the abstract (tho' it's appropriate for the main body of the poster in the introduction). 'we will use' = lingering sentence left over i think from editing, since it is redundant with prior sentence. stuff about separating YSOs from contaminants absolutely true, but is implicit in the statement that we've identified YSO candidates -- of course we've attempted to weed out contaminants. there should be some text on that in the main body of the poster, though, for sure.

		+	Final version (as submitted to AAS):
		+	We used archival Spitzer infrared data to look for new young stellar objects (YSOs) in Cometary Globule 4 (CG4) in Puppis. CG4 is approximately 1300 parsecs away and one of about 30 cometary globules in the Gum Nebula, many of which are known to be forming stars. CG4 is dramatic in appearance, and that has brought it to the attention of both scientists and the public. Our team used archival Spitzer InfraRed Array Camera (IRAC) and Multiband Imaging Photometer for Spitzer (MIPS) data, combined with 2 Micron All Sky Survey (2MASS) data as well as optical data obtained by collaborators. We used infrared excess to investigate the properties of previously known YSOs in this region and identify additional new candidate YSOs in this region. This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by NASA Astrophysics Data Program and Archive Outreach funds.
		+
		+
		+	--[[User:CJohnson\|CJohnson]] 17:00, 29 September 2010 (CDT)