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 | ARP220 | 233.7664 | 23.5658 | 233.223657 | 23.731386 | 223.777121 | 41.366844 | 36.73879852 | 53.01919685 | 114.8377 | 53742.3490856482 | 2006-01-07 08:22:41 | 53744.9654398148 | 2006-01-09 23:10:14 | 700006010 | 98.5506 | 100 | 98.5586 | 98.5506 | 98.5586 | 98.5586 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 93.3623 | 93.3623 | 226.0419 | 2 | PROCESSED | 57532.6850925926 | 2016-05-24 16:26:32 | 54247 | 2007-05-27 00:00:00 | 54040.0356597222 | 2006-11-01 00:51:21 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001033 | We propose a 100 ks observation of the nearest ultraluminous infrared galaxy (ULIG) Arp220. The major objective is to search for evidence of heavily obscured nuclei. First detection of a Compton-thick source may be possible with the HXD's sensitivity, if a powerful nucleus is present, leading to a major discovery. The good quality XIS spectrum can be decisive for the origin of the strong Fe K line, barely detected with the previous XMM-Newton observation. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | KAZUSHI IWASAWA | JAP | 0 | SWG | HARD X-RAY EMISSION FROM THE NEAREST ULTRALUMINOUS INFRARED GALAXY ARP220 | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700006010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '700006010'
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