DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | COMA RADIO HALO | 194.9267 | 27.9061 | 194.323466 | 28.175433 | 181.517491 | 31.325949 | 56.39742233 | 88.00849705 | 295.2687 | 53886.8435300926 | 2006-05-31 20:14:41 | 53890.7439699074 | 2006-06-04 17:51:19 | 801097010 | 178.6572 | 180 | 178.6892 | 178.6572 | 178.7132 | 178.6892 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 167.4506 | 167.4506 | 336.9758 | 7 | PROCESSED | 57534.5953472222 | 2016-05-26 14:17:18 | 54401 | 2007-10-28 00:00:00 | 53926.6760416667 | 2006-07-10 16:13:30 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 014446 | We will observe the central regions of the Coma cluster with the HXD/PIN to detect and characterize the nonthermal Inverse Compton (IC) emission from the radio halo. Coma has the best-studied and brightest radio halo, which makes it the best case to detect IC and the most useful one for testing theories for the origin of radio halos. Previous detections with BeppoSAX and RXTE are controversial. Suzaku is more sensitive, will avoid contamination by nearby AGNs including X Comae, and will detect IC even if it is fainter than the claimed BeppoSAX detection. The HXD/PIN data will allow the cluster magnetic field, and nonthermal energy and pressure to be derived. The XIS observations will be used to determine accurate abundances and gradients in Coma, and to test theories for ICM enrichment. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | CRAIG SARAZIN | KYOKO MATSUSHITA | USJ | 1 | AO1 | NAILING DOWN THE HARD X-RAY INVERSE COMPTON EMISSION FROM THE RADIO HALO IN THE COMA CLUSTER | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801097010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801097010'
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