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 NGC 4945 196.3636 -49.4659 195.633608 -49.198211 217.017818 -38.639251 305.27160994 13.34216317 120.2557 55590.0873842593 2011-01-29 02:05:50 55591.1182175926 2011-01-30 02:50:14 705047050 46.1076 40 46.1076 46.1076 0 46.1076 2 2 0 2 1 0 0 54.0907 54.0907 89.0518 0 PROCESSED 57600.8100810185 2016-07-31 19:26:31 55969 2012-02-12 00:00:00 55602.2238194445 2011-02-10 05:22:18 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051442 We propose five 40 ks observations of the Compton-thick AGN in NGC 4945, with the aim of monitoring possible variations of the X-ray source, and correlate the intrinsic variations seen above 10~keV with the variations in the reflected spectrum below 10~keV. This campaign is unique in two respects: NGC 4945 is the only object suitable for an investigation of possible variations of a Compton-thick AGN, which would set the first constraints on the structure and dimensions of the absorber/reflector in these objects, and the proposed observations are a clear "ideal case" for Suzaku, making full use of its unique properties, i.e. the high-energy spectral capabilities and the simultaneous availability of the full 1-100~keV spectral interval. EXTRAGALACTIC COMPACT SOURCES 7 B GUIDO RISALITI USA 5 AO5 HARD X-RAY MONITORING OF THE COMPTON-THICK AGN IN NGC 4945 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705047050/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '705047050'

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