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 PG 1211+143 183.6045 14.1097 182.967898 14.387617 177.569786 14.352789 267.53559231 74.37841457 120.7913 53698.7348263889 2005-11-24 17:38:09 53701.3397453704 2005-11-27 08:09:14 700009010 96.3241 100 96.59 97.5802 96.3241 96.3241 3 2 3 3 1 0 0 84.0087 84.0087 225.0438 2 PROCESSED 57528.1616203704 2016-05-20 03:52:44 54247 2007-05-27 00:00:00 54038.7422106482 2006-10-30 17:48:47 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001041 A 100ks Suzaku observation of the NLS1, PG 1211+143 is proposed. Previous XMM-Newton and Chandra observation claimed both blue-shifted (0.1c) and redshifted (0.26c-0.40c) iron Kalpha absorption lines. The redshifted iron K lines may originate from matter falling onto the supermassive black hole. The high effective area and low background of Suzaku XIS above 5 keV will enable us to measure these relativistically shifted iron lines in PG 1211+143 with great accuracy. Constraining the time variability of the lines will allow us to determine the physical origins of the absorption, e.g. failed jet/outflow or gravitational redshift from a Kerr black hole. The excellent broadband capabilities of Suzaku will accurately determine the continuum, essential for modeling the iron K band. EXTRAGALACTIC COMPACT SOURCES 7 A JAMES REEVES JAP 0 SWG EXPLORING THE RELATIVISTICALLY SHIFTED IRON LINES IN PG 1211+143 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700009010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '700009010'

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