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 AWM7 43.631 41.5933 42.82175 41.390486 53.723626 23.815753 146.34082925 -15.61629549 90.4997 53954.2348842593 2006-08-07 05:38:14 53954.71625 2006-08-07 17:11:24 801035010 18.9858 20 18.9858 18.9858 18.9858 18.9858 2 2 2 2 1 0 0 17.5542 17.5542 41.588 0 PROCESSED 57535.2434953704 2016-05-27 05:50:38 54422 2007-11-18 00:00:00 54020.7471759259 2006-10-12 17:55:56 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010076 The bright elongated cluster AWM7 is likely to be the place of gas infall along the large-scale filament of the Pisces-Perseus supercluster. We propose to probe the gas motion by measuring the energy shift and line broadening of Fe-K line based on the good energy resolution and low background of the XIS instrument. The motion of 1000 km/s is a reliably detectable level and we can directly measure the cluster formation process and its relation with the large-scale filament for the first time. If no gas motion is found, then secular asymmetric structure of the dark matter halo is implied. EXTRAGALACTIC DIFFUSE SOURCES 8 B TAKAYA OHASHI JAP 1 AO1 SIGNATURE OF LARGE-SCALE GAS MOTION IN AWM7 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801035010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801035010'

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