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 4151 182.642 39.4132 182.010684 39.69131 164.095796 36.629182 155.04475012 75.06022062 134.3454 56242.8428472222 2012-11-11 20:13:42 56245.9599537037 2012-11-14 23:02:20 707024010 150.2669 150 150.2829 150.2669 0 150.2829 2 2 0 2 1 0 0 150.5465 150.5465 269.2897 4 PROCESSED 57608.0679861111 2016-08-08 01:37:54 56702 2014-02-14 00:00:00 56330.6348032407 2013-02-07 15:14:07 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071417 We propose simultaneous NuSTAR/Suzaku observations of NGC 4151 and IC 4329A. These pointings will achieve three goals: (1) They will provide the best-ever broad-band X-ray spectra of two of the brightest Seyfert galaxies in the 0.5-80 keV band; (2) They will enable broad-band, time-resolved X-ray spectroscopy of these fascinating and variable sources; (3) They will serve as invaluable calibration targets for the two observatories. The spectral coverage and sensitivity will enable the continuum, absorption and reflection components of each spectrum to be conclusively disentangled, allowing us to determine whether inner disk reflection signatures are present. We will also be able to break the degeneracy between the coronal temperature and optical depth in both AGN. EXTRAGALACTIC COMPACT SOURCES 7 A LAURA BRENNEMAN USA 7 AO7 SHEDDING NEW LIGHT ON THE BROAD-BAND X-RAY SPECTRA OF NGC 4151 AND IC 4329A XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707024010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '707024010'

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