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
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'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏