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 MCG -5-23-16 146.9445 -30.9023 146.395049 -30.669659 162.619875 -41.096298 262.72964912 17.28396386 118.3849 53711.9526388889 2005-12-07 22:51:48 53714.4939699074 2005-12-10 11:51:19 700002010 95.6774 100 95.6774 95.7174 95.7174 95.6854 2 2 2 2 1 0 0 85.5647 85.5647 219.5251 3 PROCESSED 57532.4508680556 2016-05-24 10:49:15 54247 2007-05-27 00:00:00 54039.1988310185 2006-10-31 04:46:19 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001006 We request a 100ks Suzaku observation of the bright Seyfert galaxy, MCG -5-23-16 simultaneously with approved XMM-Newton and Chandra HETG observations in December 2005. MCG -5-23-16 has one of the best known examples of a relativistically broadened iron K line. With a Swift-BAT flux of 1.6e-10 cgs (15-100 keV), it is one of the brightest AGN above 10 keV. The simultaneous observations will allow us to determine the shape of the broad relativistic Fe line after subtracting the narrow line components measured by HETG. Importantly, Suzaku's wide bandpass will accurately measure the broad-band continuum and reflection component of MCG -5-23-16, essential for constraining the broad iron line. These observations will also allow us to determine the temperature of the high energy cut-off. EXTRAGALACTIC COMPACT SOURCES 7 A JAMES REEVES JAP 0 SWG PROBING THE BROAD IRON LINE AND HIGH ENERGY CONTINUUM OF MCG -5-23-16 SIMULTANEOUSLY WITH SUZAKU, XMM-NEWTON AND CHANDRA HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700002010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '700002010'

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