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OBSID:
27617
 Title:
X-RAY SURVEYING RADIO-LOUD ACTIVE GALAXIES AND THEIR LARGE-SCALE ENVIRONMENTS 
Investigator:
Massaro
 Observer:
Paggi, Alessandro
 Phone:
390116707462
 Email:
alessandro.paggi@gmail.com
Target Name:
B2.2 1334+27
 Sequence Number:
704895
 Instrument:
ACIS-S
 Grating:
NONE
 SI Mode:
TE_005C6B
 Raster Scan:
N
 Annotated DOT:
DEC2622a

Proposal Number:
20701064
 Right Ascension:
204.172
 Declination:
27.0621
 Status:
archived
 Start Date:
2023-01-08 07:13:25
Category:
ACTIVE GALAXIES AND QUASARS
 Type:
CCT
 AO Cycle:
20
 Dither Flag:
Y
 Y Offset:
0
 Z Offset:
0
Est. Count Rate:
0.01
 Order-1 Count Rate:

 Exposure Time:
16
 Time Remaining:
16.110
 Reqd Start Time:

 Reqd Stop Time:
Period:

 Epoch:

 Start of Period:

 End of Period:

 PS Margin:

 PE Margin:

 Max Segments:
0

ACIS Mode:
TE
 Standard?:
No
 BEP Mode:
VF
On-Chip Summing?:
No
 Row Sum:

 Column Sum:

 Frame Time:
Subarray Mode:
NONE
 Starting Row:
0
 Row Count:
1023
 Subarray Frame Time:

Duty Cycle?:
No
 Cycle Count:
0
 Primary Exp Time:

 Secondary Exp Time:
Event Filter?:
No
 Filter Threshold:

 Filter Range:

 Bias Requested?:
No
 Bias Frequency:

 Bias After?:
No
 Spatial Window?:
No

Abstract:
Surveying radio-loud active galaxies (AGNs) in the X-rays is a challenging task which difficulties are mainly driven by their low sky density (i.e. number of sources per square degree) in comparison with other AGN classes. On the other hand, discoveries achieved in the last two decades, based on Chandra observations, allowed us to study many aspects of their evolution. Given the observational evidence that radio-loud AGNs tend to live in galaxy-rich large-scale environments (i.e., galaxy groups or clusters), their X-ray observations are crucial to shed a light on the feedback mechanism. The main objective of this white paper is to highlight the importance of results achieved thanks to X-ray snapshot observations of radio-loud AGNs, in particular on the revised Third Cambridge catalog (3CR), to propose a selected sample of radio sources listed in the Bologna Sky Survey at 408 MHz (B2CAT), as cool-attitude targets for the Chandra mission. The 3CR Chandra snapshot survey represents a perfect example of how short-exposure X-ray observations can provide great discoveries.

Remarks:
N/A

psci Run:
29
 Processing Date:
Jan 18 2023
 psci Directory:
/nfs/maaxnew/r3/fi/acis123a/acis123.log
OBSID:
27617
 SIM Mode:
ACIS-S
 OTG Mode:
NONE
 Seq Number:
704895
 Target Name:
B2.2_1334+27
 AO:
20
Start VCDU:
73330:112
 Start Time (UTC):
008:26830.207
 Stop Time (UTC):
008:42953.156
 Kilosecs:
16.1
 % Frames:
100.0
 # CCDs:
S3
# Frames:
5133
 # Events:
330016
 Events/sec:
20
 PSCI errors:
0
 % drops:
0.0
 Bias Errs:
1
 FP Temp:
-111.0
Parameter Block:
0x005c6024
 Window Block:
-
 # Windows:
0
 FEP Mode:
Te5x5
 BEP Mode:
F
 Start Row:
0
 # Rows:
1024
Primary Exposure:
31
 Secondary Exposure:
0
 Duty Cycle:
0
 Summing?:
No
 Bias?:
Yes
 Trickle?:
Yes
 Bias Run:
29

pgf@space.mit.edu Mon Mar 31 10:36:39 EST 2025