DARTS/Astro Query System - SQL Search -

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total 1

No.
observation_id
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
exposure
awarded_exposure
resolve_exposure
xtend_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
xtend_data_mode1
xtend_data_mode2
processing_count
remarks
1 300062010 Tycho_N 6.33397 64.19052 5.63363 63.91371 42.904 53.78968 120.0949 1.46264 184.87293 60391.14519 2024-03-22 03:29:04 60392.22296 2024-03-23 05:21:04 53.447 20.000 53.447 50.351 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 50.351 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-21 00:26:08 2025-08-31 00:00:00 2024-04-20 09:50:31 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000088 Tycho s SNR is one of the best studied Type Ia remnants in the sky, yet there remains much we do not know, such as ion temperatures of the ejecta species, abundances of rare elements like Cr and Mn (sensitive discriminators of the progenitor model), and the doppler velocities of elements beyond Si. We propose here for observations of both the center of the remnant and the SE Fe-rich knot for 75 ks each as a minimal observation goal. Ideally, we would map the remnant with a series of pointings, determining the spatial distribution of the ion temperature for various elements, and go even deeper on the Fe-rich knot in the SE to pull out any faint features. SUPERNOVA REMNANTS 3 C XRISM Collaboration JAP 0 NOR XRISM OBSERVATIONS OF TYCHO'S SUPERNOVA REMNANT archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300062010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '300062010'

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